Launcher for next space station crew in position for liftoff Friday – Spaceflight Now

A Russian Soyuz rocket made a railroad journey Wednesday to its launch pad in Kazakhstan, two days before blastoff with a crew of three spaceflight veterans from the United States, Italy and Russia heading for the International Space Station.

The three-stage rocket departed an assembly building just after sunrise Wednesday on a special rail car for the journey to Launch Pad No. 1, the same mount from which Russian cosmonaut Yuri Gagarin launched on the first piloted space mission in April 1961.

A hydraulic lift raised the Soyuz vertical before swing arms moved into place around the rocket. The launch structure containing the Soyuz booster then rotated to align with the planned launch azimuth.

Fridays liftoff is scheduled for 1541 GMT (11:41 a.m. EDT; 9:41 p.m. Baikonur time). The three-man crew inside the Soyuz MS-05 capsule will head into orbit on a fast-track pursuit of the space station, with docking set for approximately 2200 GMT (6 p.m. EDT) with the research outposts Rassvet module.

Russian cosmonaut Sergey Ryazanskiy, 42, will occupy the Soyuz spacecrafts center seat during Fridays launch and docking. The Soyuz commander, a biochemist with a career in space medicine before his selection as a cosmonaut in 2003, is making his second trip to the space station after spending 166 days in orbit as a flight engineer on the Expedition 37 and 38 crews.

NASA astronaut Randy Bresnik will be the Soyuz MS-05 spaceships board engineer, assisting Ryazanskiy with cockpit duties during the six-hour voyage from liftoff to docking. The 49-year-old retired Marine Corps fighter pilot hails from Santa Monica, California, and logged nearly 11 days in orbit aboard the space shuttle Atlantis on a 2009 mission to the space station.

Bresnik will take command of the stations Expedition 53 crew in September.

European Space Agency flight engineer Paolo Nespoli has 174 days of space experience on two previous missions, including a flight on the shuttle Discovery in 2007 and a long-duration stay on the space station in 2010 and 2011. Nespoli, 60, is a native of Milan and was a special forces operator in the Italian Army before working on several European space projects as an engineer.

The trio will become part of the space stations Expedition 52 and 53 crews, joining commander Fyodor Yurchikhin and flight engineers Peggy Whitson and Jack Fischer on the orbiting complex. Yurchikhin, Whitson and Fischer are due to depart the station and return to Earth on Sept. 2, and three fresh crew members will launch on the next Soyuz spaceship from Baikonur on Sept. 12.

The space station has been flying with a three-person crew since early June, and Fridays docking will boost the outposts occupancy back to six.

Yurchikhin and Ryazanskiy will conduct a spacewalk Aug. 17 to deploy several small satellites and work outside the Russian segment of the station.

A SpaceX Dragon supply ship launched from NASAs Kennedy Space Center in Florida is expected to arrive at the complex the same week, but its liftoff will have to work around the scheduled Russian spacewalk. Station managers want to ensure the satellites released by the Russian spacewalkers are accurately tracked before committing the Dragon cargo freighter to approach the outpost, minimizing the chance for a collision with one of the small craft.

The Dragon capsule is currently set to launch around Aug. 14, but if it slips more than a day or two, the launch aboard a Falcon 9 rocket could be further delayed until officials are sure the small satellites are well away from the space station. A United Launch Alliance Atlas 5 rocket is also expected to launch the same week, potentially complicating bookings on the U.S. Air Forces Eastern Range, which is responsible for flight safety, communications and tracking support for all missions from Cape Canaveral.

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Launcher for next space station crew in position for liftoff Friday - Spaceflight Now

Commercial lunar mission signs up with Atlas 5 for launch – Spaceflight Now

Credit: Astrobotic illustration of lander

CAPE CANAVERAL In a commercial push to return to the Moon while celebrating the 50th anniversary of Apollo 11, Astrobotic Technology Inc. has contracted with United Launch Alliance to use an Atlas 5 rocket to send the Peregrine lander to the lunar surface in 2019.

Astrobotic is thrilled to select a ULA launch vehicle as the means to get Peregrine to the Moon, said John Thornton, CEO of Astrobotic. By launching with ULA, Astrobotic can rest assured our payload customers will ride on a proven launch vehicle with a solid track record of success. Together, our two organizations will honor the past and trail blaze the lunar future.

This initial Peregrine lunar lander will fly 77 pounds (35 kilograms) of customer payloads from six nations either above or below the spacecrafts deck, depending on specific needs.

The autonomous landing will use cameras, guidance computing and five Aerojet Rocketdyne-made hypergolic engines to set the lander down on four shock-absorbing legs.

It will stand 6 feet tall (1.8 meters) and have a diameter of 8 feet (2.5 meters).

Subsequent missions envision scaling up to payload masses of 585 pounds (265 kilograms). Markets range from scientific instruments to placing mementos on the Moon.

Technical credibility and signed deals remain key differentiators for Astrobotic as a lunar delivery company. Our customers and partners know that our 10 years of lunar lander development work has made us the world leader in this market, said Thornton.

The Pittsburgh-based Astrobotic aims to deliver payloads to the Moon for companies, governments, universities, non-profits and individuals.

We are thrilled that Astrobotic has selected ULA to launch the Peregrine Lander to the Moon, said ULA president and CEO, Tory Bruno. The Moon is the next great frontier, but in a different way than when Neil Armstrong landed there. Enabling technologies like those from Astrobotic will allow people to live and work in the space between here and the Moon and take advantage of all those resources in a way that is sustainable.

The Atlas 5 now has added six high-profile launches to its backlog in the past four months three commercial, two Air Force and one for NASA.

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Commercial lunar mission signs up with Atlas 5 for launch - Spaceflight Now

Orion STA undergoing pre-mission testing in Denver – NASASpaceflight.com

July 27, 2017 by Philip Sloss

With all the structural test articles (STA) of the Orion spacecraft at prime contractor Lockheed Martins Space Systems facility in the Denver area, work is underway to qualify the elements for the Exploration Mission-1 (EM-1) and Exploration Mission-2 (EM-2) missions to the Moon. Testing of different combinations of spacecraft hardware in support of EM-1 and EM-2 will continue into 2019. Current status:

This phase of testing will help characterize the dynamic response of the structures and verify that the design meets the required factor of safety.

The Crew Module STA is currently set up in a loads testing fixture in the Structural Test Lab at Lockheed Martin Space Systems Waterton facility in Littleton, Colorado. It was shipped from the Kennedy Space Center (KSC) in Florida on NASAs Super Guppy cargo aircraft in late April to Buckley Air Force Base near Denver.

The Service Module STA made the same Super Guppy flight a couple of months later after the Crew Module Adapter (CMA) and European Service Module (ESM) STAs were mated at Kennedy.

Weve done tests on two of them so far, Dan Qvale, Orion STA Assembly Test and Launch Operations Lead with Lockheed Martin, said during an interview with NASASpaceflight.com.

The crew module is actually in its second test, the first one was whats called proof pressure we went to 150% percent of the maximum expected internal pressure on the vehicle and validated that it structurally survived. That completed [at] Kennedy before we shipped it to Denver. Now that its here, were running qualification loads testing on the crew module primary and secondary structure.

The launch abort system has been assembled and were also in qualification load testing for it now, its having a test run. And then the service module is being set up for the next roughly one month. The spacecraft adapter cone is being installed, the outer walls on the CMA are going on, and then it will go into a modal test of just the service module. And that will begin about a month from now.

The launch abort system (LAS) STA was assembled with inert motors that simulate the weight and center of gravity of the units that will fly on EM-1 and EM-2.

Everything is on the LAS essentially except for the fact that its [an] inert motor. No antennas, but it has fillets, ogives, it has the MATA truss assembly (Motor Adapter Truss Assembly), [and] it has the inert motor. Structurally it has got all those components the ogives actually provide structural load path for the launch abort system as well.

Types of tests:

The STAs will go through different types of tests in the facilities at Waterton, including modal, loads, shock, and acoustic testing.

The tests are broken up into different types of tests and in many cases they are in multiple configurations, Qvale explained. A modal test is a way we take measurements of the vehicle, its dynamic response, and they use those to validate the numeric models that theyre using to simulate and obtain load data analytically.

They need these modal tests in order to measure the stiffness of the combined joints that connect all of the pieces together. And so you tend to run them in configurations your vehicle is going to be in.

In our case, the first one were going to run is the entire stacked vehicle SM (Service Module), CM, and Launch Abort System all connected so thats obviously a flight configuration on the launch pad and during ascent.

We run a modal test on just the CM alone, which is obviously a configuration it will be on reentry. We do a modal test on just the CM and SM, which is the flight configuration it would be in during the mission. We run one on the launch abort system connected to the crew module the LAV (Launch Abort Vehicle) they call it because that would be the configuration you would be in if you experienced an abort event.

So those tests are for the most part being run in order to validate models for all these different configurations that the vehicle will be in or could be in during a mission.

The second category of tests are loads tests.

Those very much fall into the category of one-time only [tests], Qvale added. What were trying to do is apply loads for the major events the vehicle experiences during the mission to simulate those.

You dont just want the vehicle to survive the maximum predicted event, you want some margin on that some assurances that it can survive and theres margin on top of that. And so what we do there is we try to go to 140% of what the maximum expected load is going to be. For example, right now were testing both the launch abort system and the crew module.

Qvale provided a breakdown of what they are trying to qualify/validate in the loads tests for the different elements, such as the all-important for crew safety Launch Abort System (LAS)

The LAS is basically getting two primary things validated, one is the ascent loads so the compression that happens on the vehicle while youre in nominal ascent. The other is abort loads, so qualification of loads that would be applied in the event that an abort actually happens and now instead of compressive loads you have large tension loads.

The crew module has a whole series of nine different events that were trying to simulate, so those include things like main parachute extraction. (Then) were running LAS load cases that represent the landing of the vehicle or the ascent of the vehicle. Weve already run cases where we simulate the jettison of the forward bay cover.

So its basically case-by-case cases where we take the hydraulic jacks, connect up to the vehicle, and then well apply a load thats intended to simulate what the flight-like the loads would be plus 40%. So as long as the design doesnt change on the vehicle, it has been qualified and theres no need to go revisit these.

As Qvale noted, the initial loads test on the CM articles was done at KSC. Both pressure vessels were proof tested to verify that they would hold pressure up to 140% of the maximum pressure load expected during flight. Qvale noted that the flight article, which is still at KSC being fully outfitted for the EM-1 flight, was pressurized to 140%; however, the STA was taken up to 150%.

The third type of tests are shock tests, to evaluate how well parts of the structure handle pyrotechnic events during flight.

[A] typical first flight vehicle would get protoqual shock tested, Qvale explained, which means you cant make the shock more severe, you cant say we did it plus margin. Its as severe as it ends up being. You cant add additional explosives to make it more severe, so instead what you do is you run it twice.

So the way that Orion is going to be protoqual-ing the shock environment (run it twice) is by number one doing it during the EM-1 mission and number two after EM-1 is recovered, were going in and running it a second time. All this needs to happen before we have a manned mission.

However, Qvale added that the program is starting shock testing on the STAs before EM-1. We dont want to wait until the EM-1 mission to start making sure that this will work properly, he said, so what the STA is doing is we are measuring the shock response on the vehicle from these events.

Were going in and say we have an avionics box [that is] near a shock source. Were putting accelerometers on it, and then were running the shock event and were measuring the response at that avionics box and were comparing that with the screening requirements that we gave the avionics box supplier to design and test the box too. And so this should validate that what we gave them to screen this hardware too is enveloped by the measurements that we just took.

So its essentially validation of the capability of the vehicle to survive shock and the combination of these measurements that were doing on the STA that will be compared with screening requirements that our EM-1 hardware was bought to and then ultimately validation by running the event during the mission and then running it a second time on the EM-1 vehicle post-mission.

The Waterton test facilities are used by Lockheed Martin on all the spacecraft they build and have been part of Orion testing since the early days of the spacecraft.

Both the test fixturing as well as the load control and data acquisition are incredibly specialized skills, and youre applying loads that basically take the vehicle to the limit of what its capable of most likely, Qvale explained. [It] doesnt matter if its Orion or another program, you tend to have the same objective there and its such a specialized area that essentially the Structures Test Lab does qualification loads testing for Lockheed Martin [Space Systems], period.

Space Systems brings them their hardware to run these sorts of tests because its impractical that youd have this expertise on a program, even if that program had hundreds of people on it.

At the time of the interview, Qvale noted that the Service Module was waiting for one of the next generation Global Positioning System (GPS) satellites to finish using a test facility before it could move in.

Test setup/configuration:

Structural test hardware for all the spacecraft elements is there to support the test campaign, with mass simulators for some of the larger moving parts, especially on the Service Module assembly.

We got the spacecraft adapter cone at the base, we have a flight-like OMS-E nozzle, we have a structural representation of the ESM so it has mass sims (simulators) instead of avionics boxes, Qvale explained.

On top of the ESM weve got the crew module adapter, so its made up of similar to the flight-like one it has all the longeron trusses, theyre called. The forward and the aft composite walls, the composite outer walls, mass simulators for all the avionics that goes in the avionics ring.

For the four solar arrays, we dont have any flight-like solar arrays theyre all mass simulators. And then for the SM fairings the SAJs (Spacecraft Adapter Jettisoned panels), theyre called theyre essentially flight like, they have the harnessing on them to run the pyro tests.

In addition, an Orion stage adapter STA also recently hitched a ride on the Super Guppy from the Marshall Space Flight Center in Alabama to Colorado. The stage adapter connects the full spacecraft stack to the launch vehicle upper stage.

Qvale explained that the tests are mostly focused on the spacecraft structure.

**Click here for 100s of Orion News Articles**

For the most part it is just the structural elements. The only electronics that we are putting on the vehicle are harnessing thats used to get to all the pyro-mechanisms, but instead of having an avionics box that fires the pyro-mechanisms we basically take test cables, mate up to the flight-like cables, and then use test equipment to fire the pyros. The only electronics per-se, is just the harnessing on the vehicle in order to run the shock tests. Everything else is structural.

One thing that is important is we want to have similar mass in the right locations on the vehicle to run a lot of these tests and so we have mass simulators that basically have the appropriate weight and the appropriate center of gravity so that when they get bolted onto the vehicle from a structural standpoint it looks like a flight vehicle.

Test campaign supports EM-1 and EM-2, runs into 2019:

Development of Orion was divided into three phases, with each culminating in the scheduled test flights: EFT-1, EM-1, and EM-2.

This round of testing in Colorado will support the two Exploration Mission test flights that first cover the major phases of flight to the Moon and back without a crew and then with a crew.

Right now the end of the campaign is [about the] middle of 2019, Qvale explained. One distinction here is that some of these tests are needed before EM-1 launches, but other tests are not needed until EM-2 launches. So the ones that are happening out in the 2019 time-frame are more the tests like of the LAV the crew module with the launch abort system. [Those tests are] trying to gather data in support of if we had either a pad or an ascent abort on EM-2.

Were predicting that all the prerequisites we need to complete before EM-1 launches are going to be completed by the beginning of November 2018, and thus far if you were to look at the start of the campaign, which we typically measure as the day that the crew module got delivered to Kennedy from MAF at this point, halfway through 2017 were essentially on schedule for all three vehicles.

The SM is on schedule, the launch abort system testing is on schedule and the CM is within two to three days of being on schedule.

Different hardware combinations will go through different tests at the Lockheed Martin facilities and the ordering of the test schedule was built based on multiple factors. In general the philosophy of how we ordered the tests, was number one we had to look at do any of these tests produce data that we need soon?, Qvale explained.

One of the first tests well run when we build the entire vehicle up the full stack is an acoustic test. And similar to what I told you about the shock test, this acoustic test is intended to be similar.

Its only intended to take measurements at specific locations and validate requirements that we are having [the] flight boxes screened to, so obviously it would be a really bad day to find out very late in the flow that we never designed and screened the boxes to the values that theyre going to experience. So for example [placing] a test like that early in the flow so that we can validate [the parameters] that all this hardware for EM-1 is getting designed and built around is a good plan.

Qvale added that the other part that determined the flow was that it takes a lot of time to build the vehicle.

For example, when we put the SM fairing on, thats on the order of twenty shifts of work to get it completed. You dont want to take them back off or youre going to have to go back through another twenty shifts worth of labor to reinstall them. So we ordered the flow so that if we build the vehicle one time, like we will be doing this Fall, we will knock out all the tests that need the vehicle in that configuration.

Theres an acoustic test thats stacked, theres a modal test thats stacked, and then we need to disassemble the vehicle to move it from one facility that has the acoustic chamber to another facility where were going to be running the loads testing. So rather than just dismantle the vehicle, we said lets just run the shock test for the launch abort system. Just run the test, blow the pyros, and thats what will separate the launch abort system and now thats how you take it apart.

So we tried to be smart about ordering things so that we got the maximum bang for the buck every time we had to assemble the vehicle.

There are plans to use at least some of the structural test articles after all the testing in Littleton is complete Qvale noted plans to use the crew module STA in a water impact test at NASAs Langley Research Center prior to the EM-2 flight. Given those future plans and the extensive testing that will be done during the test campaign, the health of the hardware will be closely monitored.

Lets go back to the loads test for example. The requirement may be that the vehicle needs to survive 140 percent [of] the limit load. In the case of the crew module, maybe survive means not rupture but it could be bent basically when youre done.

For our purposes that doesnt work because we cant destroy the vehicle we need to use it for the next year and a half. So during these tests, they monitor the health of the vehicle and if we believe were bumping up on the ultimate capability and we could damage it, then we curtail things and say OK, lets put completion of this test back on the shelf.

Well revisit it in a year and say were we close enough did we get to 138 percent and thats good enough? Or do we need to 140 percent and lets put the vehicle back in there and well bend things on it to verify that it doesnt rupture.

Thus far, every single test weve run has essentially gotten to the 140 percent limit load with no adverse effects. So I think well get the majority of these done the first time around and hopefully well end the campaign and the vehicle will have seen some extreme loading, but it will still be completely viable to go use for another mission.

Post EM-1 tests with returning Crew Module:

As noted earlier, the crew module that flies the EM-1 mission will also take part in gathering test data.

When we launch EM-1, the launch abort system isnt coming back, the service module not coming back, the fairings are not coming back the only thing were getting back is the crew module, Qvale said.

The first environmental test data set collected with the EM-1 crew module will occur as it flies the uncrewed mission to lunar orbit and then returns to Earth for entry, descent, and landing.

The reason most spacecraft go through environments testing is to verify that they work after theyre exposed to the environment, so thats acoustics and thermal and shock, he added. In the case of the EM-1 mission, theres one environment that its not going to experience and thats abort.

And so part of what well be doing with this post EM-1 flight testing is not only running the second shock test but exposing the vehicle to abort-level vibration and then validating that oh, by the way, all the mechanisms you need to survive and still operate after that did in fact work.

Part of our plan long term to validate the abort environment is well still have the STA service module and the STA launch abort system and the STA service module fairings. Were going to take all those things, assemble the vehicle with the EM-1 post-flight vehicle, and were going to go back and run these shock events a second time.

(Images: NASA, Lockheed Martin and L2 artist Nathan Koga The full gallery of Nathans (SpaceX Dragon to MCT, SLS, Commercial Crew and more) L2 images can be *found here*))

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Orion STA undergoing pre-mission testing in Denver - NASASpaceflight.com

Mars 160: 6-person crew arrives at arctic station – SpaceFlight Insider

Paul Knightly

July 22nd, 2017

Jonathan Clarke and Anastasiya Stepanova stand next to the Mars Society flag at the Flashline Mars Arctic Research Station. The second phase of the Mars 160 mission began its Mars mission simulation on July 20, 2017. Photo Credit: Mars Society

The second phase of the Mars Societys Mars 160 mission began at the end of June 2017 in the Canadian high arctic. A six-person crew is staying at the organizations Flashline Mars Arctic Research Station (FMARS) for several weeks. However, due to inclement weather, the crew was unable to make it to FMARS until July 17.

The six-person crew will be living under simulated Mars mission constraints for 30 days at FMARS located on the rim of the Haughton Impact Crater on Devon Island in Nunavut, Canada. The arctic mission represents the second half of Mars 160 after the first half concluded in December 2016 at the Mars Desert Research Station (MDRS) in Utah.

The primary goal of Mars 160 is to conduct two nearly identical field analog studies to determine how mission location impacts science return. As space agencies and organizations around the world are setting goals of sending humans to Mars, the metrics and methods used for crew selection and training on Earth increase in importance. Mars 160 also seeks to perform detailed field studies to answer questions about the geology and biology of these unique desert and high arctic environments.

The six-person Mars 160 crew arrives at the Flashline Mars Arctic Research Station on July 17, 2017. From left to right: Yusuke Marakami, Paul Knightly, Anastasiya Stepanova, Anushree Srivastava, Alexandre Mangeot, and Jonathan Clarke. Photo Credit: Mars Society

The location for FMARS was selected for its similarities to the surface of the Red Planet in terms of its analogous geology as well as its relative isolation. Situated on the rim of a well-preserved 39-million-year-old impact crater, periglacial processes near the arctic station are similar to those that have been observed on the Martian surface.

Daily temperatures during the arctic summer hover right around the freezing point of water, which would be considered a warm day at the Martian equator. Its remote location in the arctic has made it well-suited to test the effects of isolation on the 13 crews it has hosted over the last 17 years.

The Mars 160 arctic crew consists of six members representing six nationalities:

The second phase of Mars 160 is being coordinated by two principal investigators:

After performing a necessary refit of the station, the crew entered into simulation (or sim) conditions July 20. That, in part, requires crew members to wear simulated space suits while conducting field science activities. Additional simulation constraints placed on the crew will include limiting communications to the outside world.The Mars 160 mission is expected to run through the middle of August.

For more information and regular updates on the Mars 160 mission, visit http://mars160.marssociety.org/. Additionally, you can follow the mission on Twitter: @MDRSUpdates.

Paul Knightly is serving as a crew geologist for Mars 160 and is also writing for Spaceflight Insider.

Tagged: Flashline Mars Arctic Research Station Mars Mars 160 Mars Society The Range

Paul is currently a graduate student in Space and Planetary Sciences at the University of Akransas in Fayetteville. He grew up in the Kansas City area and developed an interest in space at a young age at the start of the twin Mars Exploration Rover missions in 2003. He began his studies in aerospace engineering before switching over to geology at Wichita State University where he earned a Bachelor of Science in 2013. After working as an environmental geologist for a civil engineering firm, he began his graduate studies in 2016 and is actively working towards a PhD that will focus on the surficial processes of Mars. He also participated in a 2-week simluation at The Mars Society's Mars Desert Research Station in 2014 and remains involved in analogue mission studies today. Paul has been interested in science outreach and communication over the years which in the past included maintaining a personal blog on space exploration from high school through his undergraduate career and in recent years he has given talks at schools and other organizations over the topics of geology and space. He is excited to bring his experience as a geologist and scientist to the Spaceflight Insider team writing primarily on space science topics.

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Videos: Atlas 5 rocket assembled to launch NASA’s TDRS-M bird … – Spaceflight Now

The United Launch Alliance Atlas 5 rocket that will boost NASAs latest communications relay satellite into space is targeting an Aug. 20 liftoff at 7:56 a.m. EDT (1156 GMT).

The Tracking and Data Relay satellite-M, or TDRS-M, will be carried aloft from Complex 41 at Cape Canaveral Air Force Station in Florida, reaching a customized high-perigee geosynchronous transfer orbit nearly two hours after launch.

The mission was delayed from Aug. 3 after a crane incident damaged the crafts Omni antenna in the cleanroom, requiring replacement.

The spacecraft will act like a relay station 22,300 miles above Earth to receive telemetry, voice, video and scientific data from lower orbiting platforms like the International Space Station and Hubble Space Telescope and beam the signals to a central ground hub.

The satellite will become the 12th TDRS placed in space since 1983 and extend the constellation well into the 2020s, providing near continuous connectivity to spacecraft that would otherwise be in range of ground stations 15 percent of each orbit.

The two stages of the Atlas 5 rocket arrived by sea on June 26, sailing into Port Canaveral from the manufacturing plant in Decatur, Alabama, aboard the Delta Mariner cargo ship.

On Wednesday, July 12, United Launch Alliance workers began stacking the launch vehicle, designated AV-074, by erecting the first stage aboard the mobile launch platform parked inside the VIF.

The combined interstage, Centaur upper stage and boattail of the fairing, all pre-integrated together off-site, was hoisted atop the first stage on July 13.

The 191-foot-tall rocket will be wheeled to the pad on Aug. 18 at 9 a.m.

Video courtesy of NASA-KSC TV

Arrival

First stage

Centaur

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Videos: Atlas 5 rocket assembled to launch NASA's TDRS-M bird ... - Spaceflight Now

Newly developed Nanotube Technology could revolutionize spaceflight – SpaceFlight Insider

Michael Cole

July 26th, 2017

A carbon nanotube Composite Overwrap Pressure Vessel (COPV) flew in May 2017 as part of the SubTec-7 mission using a 56-foot (17-meter) tall Black Brant IX rocket launched from NASAs Wallops Flight Facility in Virginia. Shown here is the SubTec7 payload undergoing final testing and evaluation at Wallops Flight Facility. Photo Credit: Berit Bland / NASA

A cold-gas thruster system, partially made from carbon nanotube material, was recently tested aboard a Black Brant IX suborbital sounding rocket, which was launchedon May 16, 2017, at 5:45 a.m. EDT (09:45 GMT) from NASAs Wallops Flight Facility in Virginia. Part of the thruster system was a Composite Overwrapped Pressure Vessel (COPV).

A Black Brant IX sounding rocket carrying SubTec-7 leaves the launch pad at NASAs Wallops Flight Facility. Photo Credit: Chris Perry / NASA

The COPV is an aluminum tank that is wrapped with a composite material to strengthen the tanks ability to hold a fluid or gas under pressure. In the recent test, the overwrap material was a newly developed carbon nanotube yarn that has 200 times the strength and five times the elasticity of steel.

We picked the COPV because the design properties require good tensile strength, Michael Meador, Program Element Manager for Lightweight Materials and Manufacturing at NASA Glenn Research Center in Cleveland, Ohio, told SpaceFlight Insider. But you could think about using these nanotube yarns in other structural components.

Meadors group did trade studies at NASAs Langley Research Center that looked at incorporating nanotube materials with lower structural densities into a cryotank for a notional launch vehicle.

Meador said: What we found out from those trade studies was that if you could reduce the density of the structural material by 25 percent or so, you could reduce the mass of the launch vehicle by 30 percent. So that is a real game-changer. We cant think about any other single technology that would have that much of an impact.

The nanotube fiber yarn used as the overwrap for the COPV in the test was manufactured by a company called Nanocomp Technologies, Inc., in Merrimack, New Hampshire. The company had developed it originally for use in lightweight data cables. Their initial emphasis was on the electrical properties of the yarn, so it was not very strong.

Since then, in collaboration with NASA, Nanocomp has modified their process for making this material. The yarn now has mechanical properties on a per weight basis that are comparable to or even a little bit better than carbon fiber.

Meador said: Our idea in this project was to work with Nanocomp to increase the tensile properties of the fiber, and [] develop techniques to incorporate this into composites.

Meadors project is part of the Game-Changing New Developments program at NASA. Developing a nanotube fiber that can reliably perform its function within the systems of a launch vehicle, while reducing the weight of that launch vehicle by 30 percent, is indeed a game-changer.

Game-changing program is all about maturing technologies and demonstrating them and their suitability for use in a NASA mission, Meador said. That usually involves making hardware, and it usually involves a flight test. We selected the COPV because the tensile properties of the fiber are particularly important for that component. And then we worked with Wallops to design an experiment where we could demonstrate the use of the COPV in a cold gas thruster system. We basically pressurized the COPV with argon and used it to make two maneuvers for the flight test. One was to wiggle the payload back and forth a little bit, and the second one was to spin the payload up prior to descent. They always do that to improve the aerodynamics.

The COPV on the sounding rocket test performed exactly as was expected. The payload was recovered, but Meador and his group have not received the COPV back yet. They intend to do some post-test analysis on it to see if the structural integrity has changed as a result of the flight test.

LEFT: A demonstration flight article is wound with carbon nanotube composites. RIGHT: COPV tank inside the sounding rocket. Photos Credit: NASA

This new carbon nanotube technology could potentially reduce the weight of a launch vehicle by 30 percent. But what, exactly, are carbon nanotubes?

First, one must understand that carbon nanotubes get their strength from the extremely strong bond between carbon atoms.

When you get down to a scale of 1 to 100 nanometers, conventional physics breaks down, and that gives rise to new phenomena, Meador explained. With carbon nanotubes, the aspect ratio, the length divided by the width of the tube, is quite large, and that means it makes a great reinforcement for things like plastics and other materials.

The nanotubes are made in a heated tube furnace by injecting a catalyst and a special mix of gases full of carbon atoms. What they generate is something that looks like black smoke. It is called a nanotube aerogel. That aerogel can be deposited onto a rotating drum to make a nonwoven fabric, or it can be grabbed and twisted and pulled onto a spindle to make a yarn out of it. The yarn is then further manipulated to make it into the material that was used to wrap around the pressure vessel in the recent test.

The nanotube yarn, then, is simply a million or so nanotubes with no binder between them. The yarn is all nanotube in the fiber. The only thing holding the fiber together are twists between the individual nanotubes interlocking between one another.

We got interested in this technology initially in 2000, Emilie Siochi, Research Materials Engineer at NASAs Langley Research Center in Hampton, Virginia, told SpaceFlight Insider. The reason is we thought there were data showing that the mechanical properties of carbon nanotubes far exceed those that are typically used for structural applications in aerospace. Especially for space exploration, we care about mass reduction. The initial analysis of how much mass we could save in large structures like launch vehicles [was] based on what we knew about the properties of carbon nanotubes at that time.

LEFT: Shown here is a Composite Overwrapped Pressure Vessel, or COPV, in a test setup. The aluminum vessel was pressurized to test the overwrapped carbon nanotube yarns ability to strengthen or reinforce the vessel against the internal pressure forces. A number of these burst-tests were conducted to prepare the newly developed carbon nanotube yarn and the COPV for its launch test aboard a sounding rocket launched from NASA Wallops. Photo Credit: NASA Glenn Research Center. RIGHT: A spool of the newly developed carbon nanotube yarn developed in collaboration with NASA by Nanocomp Technologies, Inc. in Merrimack, New Hampshire.Photo Credit: Nanocomp Technologies, Inc.

Siochi and others at Langley did a series of analyses on how much the mechanical properties of the nanotubes would have to be improved in order to use them in spaceflight applications. The analysis told them the nanotube fibers would have to be doubled in strength.

We spent many years trying to work with carbon nanotubes in the form that was available, Siochi said. This changed in 2004 when Nanocomp started making carbon nanotubes not in powder form but in large sheets. These sheets are now in a form that is very similar to what we can use for carbon fiber composites. We started working with them around 2010 because we were evaluating their material for our applications.

The early versions of the carbon nanotube yarn, if looked at under a microscope, would show gaps between the individual nanotubes within the yarn.

They (Nanocomp) have changed the process, and modified the chemicals they use to make the yarn, Meador said. They also did some post-processing techniques on them. To look at a cross section of the current yarn under a microscope, it looks more like a fiber. It is very consolidated and the gaps arent there anymore.

Like any new technology, it takes time to gain acceptance of the technology as reliable for its designed tasks. Further development and testing on the carbon nanotube yarn will determine that acceptance.

There are more improvements that can be made to get the strength up, Meador said. Nanocomp is working on that, and we are continuing to collaborate with them.

Tagged: carbon nanotubes Nanocomp Technologies NASA The Range

Michael Cole is a life-long space flight enthusiast and author of some 36 educational books on space flight and astronomy for Enslow Publishers. He lives in Findlay, Ohio, not far from Neil Armstrongs birthplace of Wapakoneta. His interest in space, and his background in journalism and public relations suit him for his focus on research and development activities at NASA Glenn Research Center, and its Plum Brook Station testing facility, both in northeastern Ohio. Cole reached out to SpaceFlight Insider and asked to join SFI as the first member of the organizations Team Glenn.

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Newly developed Nanotube Technology could revolutionize spaceflight - SpaceFlight Insider

First-ever laser communications terminal to be tested on the Moon – SpaceFlight Insider

Tomasz Nowakowski

July 25th, 2017

Astrobotics Peregrine Lander will deliver a laser communications terminal built by ATLAS to the Moon. Image Credit: Astrobotic

ATLAS Space Operations Inc., a company specializing in cloud-based satellite management and control services, has announced that it will test the first-ever laser communications terminal on the lunar surface. The company has recently signed a contract with Astrobotic Technology Inc., which could see their system fly to the Moon in late 2019.

The terminal, under development by ATLAS, is expected to establish the worlds first laser communication link from the lunar surface. This could mark a significant breakthrough in terms of laser communications for planetary missions.

It is hoped this new system could serve to revolutionize deep space communications. Photo Credit: Mark Usciak / SpaceFlight Insider

Our main goal is to demonstrate the viability of a commercial laser communications capability from the lunar surface. This is a stepping-stone to establishing a permanent infrastructure in support of future lunar activity, Dan Carey, Director of Marketing at ATLAS Space Operations, told SpaceFlight Insider.

The terminal, which will be sent to the Moon on board Astrobotics Peregrine Lander, will carry out first the crucial tests for the development of this potentially ground-breaking technology. This hardware is intended to be a baseline for ATLAS future interplanetary communications technology. Carey noted that the tests on lunar surface will allow us to learn the hard lessons closer to home, on the Moon, before venturing beyond.

By sending its payload to the Moon ATLAS also aims to provide a platform for the public to access a virtual lunar experience. With this technology and lunar capability, the company would be able to provide the rest of humanity an experience that previously has been reserved for an elite class of explorers.

Organizations like NASA and MIT/Lincoln Labs are the ones who have developed the revolutionary technology. ATLAS is taking that technology and commercializing it for the advancement of human interest in space. Our company was founded on the ideal of making space accessible to all, Carey said.

The laser communications terminal is expected to weigh less than 22 pounds (10 kilograms) and will consume less than 60 W for up to 1.0 Gbps of data transfer to Earth. The ground segment of this system will be comprised of Earth Observation Stations, part of the International Laser Ranging Service adapted for this mission, and other commercially-available ground terminal technology previously used for laser communications.

For ATLAS management, the partnership with Astrobotic is considered to be key to showcase its capabilities. Moreover, both companies share the same vision of space exploration and look forward to a long-lasting collaboration.

Astrobotic is progressive and forward thinking. Our companies share a common goal in advancing human interest in lunar and interplanetary exploration. We aim to make the heavens more available and affordable than ever before to all who have similar interests, Carey concluded.

Tagged: Astrobotic Atlas Moon Peregrine lander The Range

Tomasz Nowakowski is the owner of Astro Watch, one of the premier astronomy and science-related blogs on the internet. Nowakowski reached out to SpaceFlight Insider in an effort to have the two space-related websites collaborate. Nowakowski's generous offer was gratefully received with the two organizations now working to better relay important developments as they pertain to space exploration.

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New Horizons team obtains wealth of data from 2014 MU69 occultation – SpaceFlight Insider

Laurel Kornfeld

July 24th, 2017

A 2014 MU69 occultation campaign telescope. Photo Credit: NASA / JHU-APL / SwRI

NASAs New Horizons team captured crucial data on Kuiper Belt Object (KBO) 2014 MU69 the spacecrafts second target during a third organized observation of the KBO occulting a star on Monday, July 17, 2017.

Mission scientists traveled to a remote area in Argentina to catch MU69 pass in front of a star after analysis of observations made with the Hubble Space Telescope and the Gaia satellite determined the location where the KBO would cast a shadow on Earths surface.

Now you see it, now you dont: NASAs New Horizons team trained mobile telescopes on an unnamed star (center) from rural Argentina on July 17, 2017. A Kuiper Belt object 4.1 billion miles from Earth known as 2014 MU69 briefly blocked the light from the background star, in whats called an occultation. The time difference between frames is 200 milliseconds (0.2 seconds). This data helps scientists to better measure the shape, size, and environment around the object; the New Horizons spacecraft will fly by this ancient relic of Solar System formation on Jan. 1, 2019. Animation & Caption Credit: NASA / JHU-APL / SwRI

Led by Marc Buie of the Southwest Research Institute (SwRI), more than 60 scientists braved cold weather and high winds, setting up a line of 24 portable telescopes in Chubut and Santa Cruz, Argentina.

They received support and logistical assistance from Argentinian government officials, scientists, and members of the public, including a two-hour closure of a highway to prevent headlights from impeding the observation.

Located 4.1 billion miles (6.6 billion km) from Earth and one billion miles (1.6 billion km) beyond Pluto, MU69 blocked the light of a bright background star for just 0.2 seconds, but that was enough for at least five observation teams to capture the event.

It was the most historic occultation on the face of the Earth, said NASA director of planetary science Jim Green, who called the team to congratulate them. You pulled it off and made it happen.

Mission co-investigator Amanda Zangari was the first to detect the signature of the 1425 miles (2240 kilometers) wide KBO, which the spacecraft will fly by on January 1, 2019.

MU69 will then be the most distant object to be visited by a spacecraft.

The July 17 event was the last of three stellar occultations by the KBO. The other two occurred on June 3 and July 10. Mission scientists traveled to Argentina and South Africa to observe the June 3 event, then flew above the clouds in NASAs Stratospheric Observatory for Infrared Astronomy (SOFIA) aircraft over the Pacific Ocean from New Zealand for the second one in an effort to study the KBOs environment.

That study centered on detection of any potential hazards near MU69 that could pose a threat to New Horizons.

While it will take scientists weeks to analyze all the data collected during the occultations, that data will play a key role in helping them discover its size, shape, orbit, and environment.

MU69 was detected in 2014 by the Hubble Space Telescope as part of the New Horizons teams search for a second flyby target after Pluto, but it was too remote for any constraint on its size and shape.

Buie praised the Argentinian community of Comodoro Rivadavia for assisting the team by turning off street lights and even parking trucks to act as windbreakers.

The local people were a major team player, he emphasized. He specifically thanked Argentinas National Commission on Space Activities and the Argentinian people for their assistance, noting the effort is an example of space exploration bringing out the best in everyone.

Principal Investigator Alan Stern said: This effort, spanning six months, three spacecraft, 24 portable ground-based telescopes, and NASAs SOFIA airborne observatory was the most challenging stellar occultation in the history of astronomy, but we did it. We spied the shape and size of 2014 MU69 for the first time, a Kuiper Belt scientific treasure we will explore just over 17 months from now.

LEFT: Marc Buie, New Horizons occultation campaign lead, holds up five fingers to represent the number of mobile telescopes in Argentina initially thought to have detected the fleeting shadow of 2014 MU69. The New Horizons spacecraft will fly by the ancient Kuiper Belt object on Jan. 1, 2019. RIGHT: New Horizons Co-Investigator Amanda Zangari was the first occultation campaign scientist to see the telltale signature of MU69 while analyzing data from July 17, saying, We nailed it spectacularly. Credits: NASA / JHU-APL / SwRI / Adriana Ocampo

A video depicting preparations for the July 17 occultation is available for viewing here, and reports on all three occultation observations can be viewed here.

Tagged: KBO 2014 MU69 New Horizons The Range

Laurel Kornfeld is an amateur astronomer and freelance writer from Highland Park, NJ, who enjoys writing about astronomy and planetary science. She studied journalism at Douglass College, Rutgers University, and earned a Graduate Certificate of Science from Swinburne Universitys Astronomy Online program. Her writings have been published online in The Atlantic, Astronomy magazines guest blog section, the UK Space Conference, the 2009 IAU General Assembly newspaper, The Space Reporter, and newsletters of various astronomy clubs. She is a member of the Cranford, NJ-based Amateur Astronomers, Inc. Especially interested in the outer solar system, Laurel gave a brief presentation at the 2008 Great Planet Debate held at the Johns Hopkins University Applied Physics Lab in Laurel, MD.

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New Horizons team obtains wealth of data from 2014 MU69 occultation - SpaceFlight Insider

Our SpaceFlight Heritage: The Shuttle replacement that never was – SpaceFlight Insider

Christopher Paul

July 22nd, 2017

In this artists depiction, NASAs Shuttle C spacecraft opens its payload bay doors. Image Credit: Nathan Koga / SpaceFlight Insider

When the Space Shuttle was first proposed it was meant to be all things to all users, a replacement for all U.S. launch vehicles. All the expendable launchers, Atlas, Titan, and Delta would retire and the shuttle would be responsible for all U.S. launches from its three pads, LC-39A / B at Kennedy Space Center, and SLC-6 at Vandenberg Air Force Base.

The shuttles launch rate was expected to be 100 launches a year. Enormous amounts of money would be saved through the Shuttles reusability.

Unfortunately, this plan fell apart. The shuttle never came close to its predicted launch rate. Officials in the Air Force doubted that a human-rated system would ever save money. However, after the Challenger (STS-51L) disaster, the military almost totally abandoned the shuttle and restored the expendable systems it had nearly abandoned, for its part, as noted by Astronautix, NASA thought the shuttle would only fly about 14 times per year after 1986 (a number of annual flights the agency never came close to reaching).

What was more, the space station that NASA wanted to build was slowly growing in mass. Two modules had already become too heavy for the agencys fleet of orbiters to launch.In the face of these problems, a solution was sought. Shuttle-C was one of the answers proposed.

A NASA Shuttle-C vehicle roars to orbit in this artists depiction. Image Credit: Nathan Koga / SpaceFlight Insider

Shuttle-C was designed as a pure cargo launcher, able to launch much more cargo than the Space Shuttle itself. Since the shuttle was intended to return to Earth with its crew, it necessitated an aerodynamic form, heat shielding for that form, and a crew cabin as well as all of the prerequisites to allow astronauts to live on orbit. Shuttle-C would be an expendable vehicle, enabling much larger cargoes to be delivered to orbit.

The configuration that NASA settled into for Shuttle-C involved an unmodified External Tank and Reusable Solid Rocket Boosters, with a cylindrical cargo container attached to the Shuttles boattail engine housing. Two Space Shuttle Main Engines (SSMEs) would be mounted on the boattail, along with the Shuttles Orbital Maneuvering System.

While SSMEs are expensive and were designed to be reusable, they had a limited life span. NASA usually planned for a maximum of ten flights for each SSME. If Shuttle-C was only launched with engines that already had 9 flights under their belts, no money would be lost in expending them.

NASA also thought about making Shuttle-Cs avionics reusable. By replacing the aerodynamic nose cone over the cylindrical cargo carrier with a Mercury-style reentry vehicle, the avionics could be returned to Earth after launch and reused. NASA studied this system and released a technical report to document this study, entitled, Preliminary design of the Shuttle-C avionics recovery system.

Other versions of Shuttle-C were envisioned, both by internal NASA documents and Martin-Marietta studies. Many included an in-line launch vehicle, with SSMEs mounted under a modified External Tank, and included the option for upper stages. However, NASA disliked these versions, since they required modifications to the External Tank. NASA desired a system that would be a drop-in replacement for their orbiters for cargo-only launches.

Shuttle-C never came into existence. Despite NASAs desire for a heavy-lift cargo launch vehicle, the fusion of Space Station Freedom and Russias Mir-2 station into the International Space Station changed much of the shuttle-station centered planning at NASA.

However, Shuttle-C nearly got another chance at life when NASA started plans to send their fleet of orbiters off on their next mission, as monuments in museums and tourist destinations.

One option presented to the Augustine Committees study of shuttle replacement options in 2009 was Shuttle-C. The proposal was essentially to mount the Orion capsule and its Launch Escape System on top of the Shuttle-C cargo carrier. This would allow both crew and cargo launches to the ISS, and the Shuttle-C cargo carrier had room for both a Delta Cryogenic Second Stage derived upper stage, a J-2X powered Earth Departure Stage as well as additional cargo. This version of Shuttle-C would have mounted three SSMEs and have no additional Orbital Maneuvering System. The proposal suggested an initial cargo-only launch in 2013, and a first crew launch in 2014 after the Shuttles expected retirement in 2010-2011.

Shuttle-C was an often-discussed option, both in and outside of the space agency, though it never came to anything. It might also be considered a symptom of the Shuttle systems success.

However, the independent value of the Shuttle-C system itself is difficult to evaluate in the shadow of NASAs now-retired fleet of shuttle orbiters. It does seem clear in hindsight that a dedicated cargo heavy-lift vehicle would have been a powerful supplement to the orbiter fleet, perhaps enabling a crewed mission to the Moon, or heavier and more-capable robotic missions to other planets, including possibly a dedicated Europa orbiter akin to the Europa Clipper mission now scheduled for an SLS launch.

Regardless of Shuttle-Cs utility or value, NASA is subject to many forces that influence its decision-making, perhaps most potently the whims of elected officials. In the past 13 years, presidents and congresses have come and gone and NASAs directive has been altered several times with many of its programs and efforts rising and falling. Shuttle-C would was joined by other cancelled initiatives, such as Venturestar and Constellation and will, doubtlessly, as new political winds blow in and out of Washington, be joined by others.

Video courtesy of NASA STI

Tagged: NASA Shuttle-C Space Shuttle Main Engine The Range

Christopher Paul has had a lifelong interest in spaceflight. He began writing about his interest in the Florida Tech Crimson. His primary areas of interest are in historical space systems and present and past planetary exploration missions. He lives in Kissimmee, Florida, and also enjoys cooking and photography. Paul saw his first Space Shuttle launch in 2005 when he moved to central Florida to attend classes at the Florida Institute of Technology, studying space science, and has closely followed the space program since. Paul is especially interested in the renewed effort to land crewed missions on the Moon and to establish a permanent human presence there. He has covered several launches from NASA's Kennedy Space Center and Cape Canaveral for space blogs before joining SpaceFlight Insider in mid-2017.

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Our SpaceFlight Heritage: The Shuttle replacement that never was - SpaceFlight Insider

Opportunity rover peers into ‘Perseverance Valley’ Spaceflight Now – Spaceflight Now

Toward the right side of this scene is a broad notch in the crest of the western rim of Endeavour Crater. Wheel tracks in that area were left by NASAs Mars Exploration Rover Opportunity as it observed Perseverance Valley from above in the spring of 2017. The valley is a major destination for the rovers extended mission. It descends out of sight on the inner slope of the rim, extending down and eastward from that notch. Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

NASAs Opportunity rover, now showing nearly 28 miles (45 kilometers) on its odometer since landing on Mars, recorded a panoramic view last month of its next scientific destination, a valley that may have been carved by water, an icy or muddy debris flow, or ancient Martian winds.

Imagery experts stitched together this view from a series of images taken by Opportunitys panoramic camera from June 7 to June 19, according to NASA. The panorama covers three-quarters of a full-circle view.

The rover collected images for the panorama while engineers analyzed a stall on the robots left-front wheel steering actuator.

The wheel was pointed outward more than 30 degrees,prompting the team to call the resulting vista Pancams Sprained Ankle panorama, NASA said in a press release.

Engineers were able to get the wheel pointed straight ahead to resume driving, but Opportunity now uses the steering capability of only its two rear wheels, NASA said. The right-front steering actuator failed in 2006.

Opportunitys tracks lead into notch to the right of an outcrop dubbed Cape Tribulation, and scientists think the dip may have been a spillway through which water, ice or wind flowed into the bed of Endeavour Crater, an expansive 14-mile-wide (22-kilometer) depression the rover has explored for nearly six years.

The mobile robot landed on Mars in January 2004 and studied several smaller craters to find evidence that Mars was once habitable. Opportunity arrived at the rim of Endeavour Crater in 2011 after a cross-country journey from its original landing site, outliving its original three-month design life more than 50 times.

The floor of Endeavour Crater stretches toward the horizon in this panorama.

The wheel tracks visible in the image were created as Opportunity drove to the edge of the crater to look into Perseverance Valley, which lies on the inner slope of the crater rim just beyond the notch. Three-dimensional stereo images will help controllers plot Opportunitys drive into the valley, which sits at a slope of 15 to 17 degrees and extends the length of two football fields, based on observations from orbit.

It is a tantalizing scene, said Ray Arvidson, Opportunitys deputy principal investigator from Washington University in St. Louis. You can see what appear to be channels lined by boulders, and the putative spillway at the top of Perseverance Valley. We have not ruled out any of the possibilities of water, ice or wind being responsible.

The rover is now parked in the upper reaches of the valley.

Opportunity will drive deeper into Perseverance Valley next month once engineers re-establish full communications with the rover. Signals between Earth and spacecraft at Mars are currently blocked as the red planet travels behind the sun, but the rover is collecting a new panorama from its current location.

The valley is the prime target for this phase of Opportunitys mission, which NASA approved last year through at least September 2018. Scientists want to know what created the valley, which is the first such fluid-carved feature to ever be visited by a rover on Mars.

Opportunity will also take measurements of the rocks inside Endeavour Crater to compare their composition to the material on the plains outside the crater, officials said.

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Study teams comb through NASA’s wish list for new telescope – Spaceflight Now

This artists rendition shows a possible design of a potential successor to the Hubble Space Telescope. This conceptual mission, called the Advanced Telescope Large-Aperture Space Telescope (ATLAST), is similar in approach to one of several observatories currently under study by astronomers. Credit: NASA

Scientists outlining four concepts for a powerful new space telescope that could launch in the 2030s this week said improvements in optics, detectors and access to huge new rockets like NASAs Space Launch System could revolutionize the way astronomers observe potentially habitable planets, black holes, and the earliest galaxies in the universe.

It is likely NASA will only be able to afford one of the four proposed flagship observatories, and the space agency will take the advice of an independent review by the National Research Council in 2020 on which type of telescope should receive highest priority.

NASA launched studies last year to look into the scientific benefits, costs and technical challenges of four astronomy missions:

Four teams will produce interim reports on the four mission concepts by the end of this year, then publish their final reports in 2019 as a resource for scientists on the next astrophysics decadal survey panel in 2020, which will rank priorities for future NASA astronomy missions.

The studies will offer only a roadmap for NASAs next leap in astronomy, and officials say any telescope that does reach the launch pad in the 2030s will likely look much different from the concepts currently under investigation. Tough decisions on engineering constraints and cost caps remain ahead, but NASA it needs to start preparing now given the long life cycles of such missions.

The space agency typically follows the decadal surveys advice.

The two last decadal surveys prioritized infrared astronomy. A report from the National Research Council in 2001 led to the approval of the James Webb Space Telescope, which is due for launch next year, and the 2010 decadal survey recommended NASA pursue a mission which became the Wide-Field Infrared Survey Telescope, or WFIRST, scheduled for liftoff in the mid-2020s.

NASA expects to have funding for another advanced flagship-class, multibillion-dollar great observatory to launch some time in the 2030s, once the agency puts behind major spending on JWST and WFIRST.

Astronomers expect breakthroughs with any route prioritized in the next decadal survey.Cost estimates on each of the four mission concepts will come later to help inform the decadal surveys decisions.

The LUVOIR mission concept would be a true successor to Hubble, covering much the same range of wavelengths as NASAs most famous long-lived orbiting telescope. The mission outline is similar in capability to the High Definition Space Telescope, a super-Hubble proposed by astronomers in 2015, and the Advanced Technology Large-Aperture Space Telescope, known by the apt acronym ATLAST.

With LUVOIR, we would be able to study in much greater detail how galaxies assemble their stars, said Debra Fischer, a professor of astronomy at Yale University who co-chairs the LUVOIR study team. The killer app for LUVOIR is actually being able to coronagraph and image pale blue dots around some of the nearest stars, and then once we have those images, to be able to take spectra of them.

Instruments on a mission like LUVOIR could look for signs of water vapor, oxygen, methane and other gases in alien atmospheres that might be habitable, Fischer said in a presentation Thursday to NASAs Astrophysics Advisory Committee.

The size of an observatory like LUVOIR hinges on the volume of launchers that might be available in the 2030s. A primary mirror with multiple segments, similar to the design of JWST, would be folded up for liftoff.

Commercial rockets like United Launch Alliances Delta 4-Heavy and SpaceXs Falcon Heavy come with standard fairings around 5 meters (16 feet) in diameter, while NASAs more costly but more powerful Space Launch System could accommodate payloads as wide as 8.4 meters (28 feet) by the late 2020s.

The dimensions of a telescope like LUVOIR are bracketed by the capabilities of the Delta, Falcon and SLS rocket options, although the Delta 4 rocket is likely to be retired in favor of ULAs next-generation Vulcan booster by the time such a mission is ready for liftoff.

Another rocket that might give future telescopes rides into space is the New Glenn, a methane-powered booster in development by Blue Origin, the space company founded by Amazon.coms Jeff Bezos. The privately-operated New Glenn could make its debut launch by 2020, and it can loft payloads as wide as 7 meters (23 feet).

A rule-of-thumb for deployable telescopes is that a 9 or 10-meter (30-33 foot) primary mirror could tuck inside standard Delta 4-Heavy or Falcon Heavy fairings. The Space Launch Systems nose cone could fit a 16-meter (52-foot) multi-segment mirror folded up origami-style.

None of the proposals under study would need in-space assembly by astronauts, but Fischer said robotic or human servicing might be possible for a mission like LUVOIR.

Fischer identified launch vehicle limitations as one of the top technological risks for the LUVOIR concept, which would likely be sent to an observation post at the L2 Lagrange point a million miles (1.5 million kilometers) from Earth in the direction away from the sun. Other question marks include the readiness of ultraviolet mirror coatings, infrared detector technology, and ultra-stable opto-mechanical systems, Fischer said.

While LUVOIR would be a general purpose observatory best geared for large-scale galactic, dark matter and statistical exoplanet surveys, the smaller HabEx concept would emphasize exoplanet research, focusing on a few nearby stars known to host potentially habitable worlds.

Rather than statistical-based as LUVOIR is, were more exploration-based, said Scott Gaudi, a professor of astronomy at Ohio State University who co-chairs the HabEx study. We want to study nearby planetary systems and just figure out what theyre like.

HabEx could probe up to a dozen potentially Earth-like planets around stars in the suns neighborhood, Gaudi said Thursday.

Our goal is to detect and characterize a handful of potentially habitable planets, and then search for signs of habitability and biosignatures on those planets, he said.

A mission based on the HabEx concept could perhaps distinguish between analogs of Venus, Earth and Mars, which all lie within the suns habitable zone, a region where liquid water could persist on a planets surface under the right conditions. But only Earth has an environment ripe for life.

Gaudi said his team will present at least two HabEx mission concepts to the decadal survey panel, one with a single-piece 4-meter (13-meter) primary mirror with nearly twice the collecting area of Hubble, and another with a 6.5-meter (21-foot) segmented mirror comparable to JWSTs.

HabEx will need help resolving the faint light coming from exoplanets, which can be more than a billion times dimmer than the light coming from their host stars.

One option is to launch a separate starshade, a petal-shaped spacecraft tens of meters (up to 100 feet) wide that would keep formation via laser navigation tens of thousands of miles from a telescope such as HabEx. The idea is to block bright starlight, revealing planets lurking nearby.

A tiny coronagraph embedded inside the telescope could also help detectors register exoplanets, allowing instruments to break up the light into spectra like a prism, telling scientists about the chemicals and gases in their atmospheres.

No space telescope has ever flown with a starshade, and coronagraphs aboard current-era observatories like Hubble and JWST are unable to see planets close to their stars, where temperatures might be favorable for life. The WFIRST mission might carry a coronagraph that works in concert with deformable mirrors and ultra-low-noise cameras, yielding views of potentially habitable worlds, but HabEx would have much better sensitivity thanks to a bigger mirror.

Two other concepts under scrutiny would scan the infrared and X-ray universe.

The Origins Space Telescope will probe the births of stars and planets in the Milky Way galaxy, trace the evolution of galaxies throughout cosmic history, seeing through thick envelopes of dust to study regions invisible to other telescopes.

Building on discoveries expected from JWST and WFIRST both infrared observatories the Origins Space Telescope would be sensitive to lower-energy far-infrared light, a part of the spectrum that reveals some of the coldest parts of the universe.

Beyond JWST, we will still have questions, said Asantha Cooray, a professor at the University of California, Irvine, and co-chair of the Origins Space Telescope study. We will not how those stars came to be. We want to know and we want to understand what mechanics produce what stars.

The far-infrared telescope could be as big as 9 meters (30 feet) in diameter, Cooray said Thursday, a size limit set by the volumes of Delta and Falcon rocket fairings.

The Origins Space Telescope could image pockets of tenuous gas and dust in the interstellar medium, the area between stars. Clumps of cold matter glow in far-infrared light.

We still do not have a probe for the interstellar medium, and thats where the Origins Space Telescope comes in, Cooray said.

He said the infrared observatory would also make observations of exoplanets like LUVOIR and HabEx, and potentially detect biosignatures.

Our science case is broad and covers a wide range of topics, Cooray said. Our aim is to provide a factor of maybe between 5,000 and 10,000 improvement in sensitivity relative to the best we had with (ESAs) Herschel. Thats a large number.

Cooray said a mission based on the Origins Space Telescope approach would have have a factor of 30 better sensitivity than JWST, not just because of its size but because mechanical coolers would chill the observatorys detectors below 5 Kelvin (minus 450 degrees Fahrenheit), just above absolute zero. That will make the future telescope capable of seeing frigid parts of the universe.

We are not trying to take images and improve a little bit, he said. We are really talking about revolutionary astronomy with the Origins Space Telescope.

Astronomers scoping the next potential X-ray telescope are working on the Lynx mission concept.

Billed as a machine for looking back in time to the first billion years after the Big Bang, the Lynx observatory would seek to find the universes first black holes and galaxies. Theories currently govern astronomers understanding of this era, when light from the first stars could escape through an absorbing haze of hydrogen left over from the Big Bang, but Lynx could add hard data to the equation.

We have decided what kind of observatory Lynx should be, how big that observatory should be, said Alexey Vikhlinin, astrophysicist at the Harvard-Smithsonian Center of Astrophysics and co-chair of the Lynx study. We have identified plans for the X-ray optics. We are in the process of making a decision on the (proposed) instrument suite.

Vikhlinin said Thursday the Lynx team has identified the drivers of galaxy formation and the dawn of black holes as two key pillars of the would-be mission.

Lynx would also map the distribution of matter in the cosmic web, the voids, clusters and filaments that tie together the universe. Another target would be the halos of material surrounding galaxies brightest star-filled regions, which astronomers believe plays an important role in a galaxys birth.

Scientists say the Lynx mission would offer a leap in sensitivity two orders of magnitude over Chandra, which launched in 1999, and the planned European-led Athena X-ray telescope due for liftoff in 2028.

But big advances in technology are required to make a mission like Lynx a reality.Vikhlinin said high-resolution lightweight X-ray optics is the area of most concern for us.

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Study teams comb through NASA's wish list for new telescope - Spaceflight Now

On Atlantis’ anniversary, USA’s future space fleet closing in on maiden flights – NASASpaceflight.com

July 21, 2017 by Chris Bergin

The long-awaited return of American astronauts launching on US spacecraft, a capability last seen when Atlantis closed out the Shuttle Program in 2011, is set to return next year. Along with new crew transporters, the Space Shuttles legacy will be honored by the return of a lifting body vehicle, as Dream Chaser makes progress towards her role for uncrewed ISS resupply efforts. Commercial Spacecraft:

Two spacecraft are in a race to launch Americans to the International Space Station (ISS), a capability that has been exclusively conducted by the Russians with a hefty price tag via their Soyuz spacecraft following the 2011 retirement of the Space Shuttle fleet.

The Space Shuttle programs storied 30+ year flight history came to an emotional conclusion six years ago today whenAtlantis dropped from thepre-dawn darkness into the lights illuminating runway 15 at the Kennedy Space Center.

When Atlantis wheels came to a stop just before 5:58am on 21 July 2011, the conclusion of the Shuttle programresulted in a planned crew launch capability gap for the U.S., though few at the time believed the gapwouldlast more than a few years.

Originally, a transition period using the Orion spacecraft in an opening role of launching crew to the ISShad been considered before the demise of the Constellation Program (CxP) created an uncertain future for Orion.

When the SLS program architecture was announced in September 2011, Orion was re-revealed as an exclusivelyBeyond Earth Orbit (BEO) vehicle.

Notably, this change of call sign for Orions future missions was part of a further transition towards handing over Low Earth Orbit (LEO) to the commercial sector, a partnership between NASA and the space launch industry that resulted in the agency contracting out its LEO obligations to commercial companies, all with NASA oversight.

The commercialization of LEO, focused on a supply line to the ISS, began by complementing existing resupply vehicles, such as Russias Progress, Japans HTV and ESAs ATV spacecraft. Joining the resupply team were Orbital ATKs Cygnus and SpaceXs Dragon cargo spacecraft.

Although both vehicles have suffered from a launch vehicle-related failure, the Commercial Resupply Services (CRS) program has proven its worth, paving the way for a second phase, known as CRS2, to continue to provide commercial supply runs into the 2020s.

CRS2 expands the number of flights on the manifest for Cygnus and cargo Dragon whilst also welcoming Dream Chaser to the uncrewed fleet.

A fan favorite in the space flight community, Dream Chaser was one of the main contenders to launch American astronauts to the Station during the Commercial Crew competitionphase.

That crew version of the spacecraft is still technically within NASAs thoughts, as she completes the CCiCAP (Commercial Crew Integrated Capability) element of a NASA contract that was part of the Agencys Commercial Crew Program (CCP) aspirations.

Despite variouslevels of international interest, the crewed version of Dream Chaser faces an uncertain future. However, her new version an uncrewed cargo variant has a lot to look forward to.

As recently noted by SNC, Dream Chaser is currently undergoing a second roundof testing at the Dryden Flight Research Center in California, mirroring the tests conducted in 2013 that resulted in a successful set of milestones, only to be ruined by one of her landing gear gear that was salvaged from a fighter jet failing to deploy during landingthe resulted in the vehicle crashing off the side of the runway.

The spacecraft, a repaired and modified Engineering Test Article (ETA), is currently moving through tow tests ahead of Captive Carry tests and on a date yet to be decided this fall a replay of her free flight and landing that will hopefully conclude the test program with a safe rollout on Edwards Air Force Base runway 22L.

SNC is building two cargo Dream Chasers, each able to fly a total of 30 times over a 10 year lifetime. They, as expected, will be launched by United Launch Alliances Atlas V rocket, with a contract that confirms the partnership signed just this week.

ULA is pleased to partner with Sierra Nevada Corporation to launch its Dream Chaser cargo system to the International Space Station in less than three years, said Gary Wentz, ULA vice president of Human and Commercial Systems, speaking about the deal for the first two launches. We recognize the importance of on time and reliable transportation of crew and cargo to Station and are honored the Atlas V was selected to continue to launch cargo resupply missions for NASA.

Dream Chasers partnership with Atlas V goes back as far as the SpaceDev days, which first provided a fascinating glimpse of the lifting body spacecraft perched on top of the Atlas Vs Centaur upper stage.

The latest version of Dream Chaser is more streamlined and fits inside the large Atlas V fairing. The first launch is expected to take place in 2020.

SNC recognizes the proven reliability of the Atlas V rocket and its availability and schedule performance makes it the right choice for the first two flights of the Dream Chaser, added Mark Sirangelo, corporate vice president of SNCs Space Systems business area.

ULA is an important player in the market and we appreciate their history and continued contributions to space flights and are pleased to support the aerospace community in Colorado and Alabama.

Along with Dream Chasers often-touted dissimilar redundancy by way of being a different type of spacecraft when compared to her capsule based colleagues she will add to NASAs downmass capability, a required element that only Dragon is currently capable of achieving for the CRS program.

This downmass capability which includes time-sensitive science payloads will be returned directly to land, with Dream Chaser utilizing her design by landing on a runway, allowing for quick access to critical experiments.

While Orbital ATKs Cygnus can only look forward to a destructive re-entry at the conclusion of her mission, SpaceXs Dragon returns to a Pacific Ocean splashdown before being shipped back to the Port of Los Angeles and then eventually to Texas for a full mission debrief.

Interestingly, land and sea returns will now be the forward pathfor NASAs two CCP partners, SpaceX and Boeing.

SpaceXs Dragon 2 is nowconfirmed to be returning only to a splashdown in the Pacific, after an anticipatedtransition to a propulsive land landing capability via her SuperDraco thrusters was deleted.

Elon Musk confirmed while noting the related impact on the now-cancelled Red Dragon that propulsive landings are too challenging for the interim, which means Dragon 2 will be heading for water landings via parachutes.

Notably, Dragon 2 was always going to use parachutes, albeit just on the opening crew missions, before transitioning to apropulsive landing.

Regardless of landing style, as previously reported, the first launch of SpaceXs newDragon 2 on an uncrewed demonstration mission to the ISS has now officially slipped into 2018, with the SpX Demo-1 mission now set for February of next year, followed by SpX Demo-2, this time with a crew, in June.

Dragon 2s rival, Boeings Starliner had no plans for propulsive landings, but will interestingly return to land to conclude her crew missions thanks to an invention called airbags, as one Boeing employee cheekily referenced when comparing his spacecraft to other returning vehicles.

Starliner will return under parachutes before inflating itsairbag system at the base of the capsule to allow for a soft touchdown at the landing site. This capability has already been tested during Starliners development program.

The spacecraft like Dream Chaser has partnered with ULA forAtlas V launches en route to the Station.

The first Starliner launch known as the Orbital Flight Test (OFT) is now set to take place in June ahead of a crewed version of themission (the Crewed Flight Test CFT) currently scheduled just two months later in August.

All four missions will be heavily reviewed after each flight prior to NASA working a certification process that will green light the spacecraft for official NASA crew rotation missions.

While Soyuz continues to be contracted for the interim, including an overlap during this initial period as a back-up in case of problems with the commercial vehicles, the ultimate aim is to focus NASA money on American vehicles, as opposed to paying for seats on Soyuz.

(Images: Boeing, SNC, SpaceX, NASA, andL2 artist Nathan Koga The full gallery of Nathans (Starliner to SpaceX Dragon to MCT, SLS, Commercial Crew and more) L2 images can be *found here*)

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On Atlantis' anniversary, USA's future space fleet closing in on maiden flights - NASASpaceflight.com

NanoRacks airlock moving toward 2019 installation on the ISS – SpaceFlight Insider

Jim Siegel

July 21st, 2017

Astronauts test the accessibility of handrails on the NanoRacks airlock mockup in the Neutral Buoyancy Laboratory. Photo Credit: NanoRacks

Five months ago, NanoRacks, LLC announced it would partner with Boeing to build the first private airlock for the International Space Station. That initiative is progressing and recently achieved a design milestone with the successful test of a NASA-built, full-scale mockup at the Johnson Space Center in the Neutral Buoyancy Laboratory (NBL).

The NBL features a 6.2 million gallon indoor pool, which is 10 times larger than a typical Olympic-size swimming pool. It contains full-size mockups of ISS modules and payloads, as well as space station visiting vehicles such as SpaceXs Dragon capsule.

An artists rendering of the NanoRacks airlock attached to the Tranquility module. Image Credit: NanoRacks

The purpose of the NBL, which simulates the weightlessness of working in space, is to prepare for missions involving spacewalks. NASA team members use the NBL to develop flight procedures, verify hardware compatibility, train astronauts, and refine spacewalk procedures during flight that are necessary to ensure mission success.

Recent tests involving the airlock confirmed that spacewalking astronauts will be able to successfully maneuver around the structure and mounted external payloads. Astronauts will be able to do this with the assistance of handrails, which will be strategically placed by the NanoRacks design team.

The test lasted about two to three hours and went so well that we cancelled the additional test time scheduled for the next day, said airlock Project Manager Brock Howe. In particular, we were able to validate the handrail locations.

Howe said all is progressing smoothly with the development of the NanoRacks airlock.

We are still targeting launch in 2019 in a SpaceX Dragon trunk, and were thankful for the hard work involving all of our airlock partners, including our friends at Boeing, ATA Engineering, and Oceaneering, Howe said.

NanoRacks airlock will be the solution to the constraints associated with the stations only airlock system used for deploying CubeSats and other items into space. That current airlock, located on the Japanese Kibo module, can only be opened 10 times per year, with only five of those allocated to NASA and commercial companies. The other five go to the Japan Aerospace Exploration Agency, which owns the airlock. Demand by both NASA and commercial companies now far exceeds that capacity.

The NanoRacks airlock, to be located on the port side of the Tranquility module, will measure roughly 6.6 feet (2 meters) in diameter and 5.9 feet (1.8 meters) long. It will be much larger than the existing Japanese airlock.

The private airlock will be able to discharge five times the volume of payload at a time. Additionally, it will be designed to accept components from outside of the ISS, components that might be in need of repair or adjustment.

ISS astronauts will be able to place payloads inside the airlock, close its hatch, depressurize it, and then detach it from the module using the stations Canadian robotic arm. The arm will extend the airlock aft and 45 degrees down, and the CubeSats and other payloads will be deployed into orbit or tested in the vacuum of space.

Image Credit: NanoRacks

Howe said NASA will provide an air save pump that will recover about 80-90 percent of the air evacuated from the airlock.

There are constraints on the frequency of opening the airlock and deploying payloads, however. Howe said the most significant of these is crew time, followed by the availability of the robotic arm and other activity outside the ISS. At this time, teams are planning for four to six per year, though he added there is talk of as many as 10-12 per year if justified by demand and allowed by crew schedules.

Abby Dickes, NanoRacks director of marketing, communications, and special events, said there is considerable ongoing demand for CubeSat deployment. Over 180 have been launched to date and an additional 30 are scheduled to be included in the manifest for the upcoming SpaceX CRS-12 mission slated for next month.

We are looking pretty full, said Dickes. There are a few slots that are open in the next few launches, but the few that are left are filling fast. We operate on just about every U.S. mission launching to ISS, so there are plenty of new flight opportunities coming up as new customers get signed on.

The fee to deploy a 1U CubeSat going through the NanoRacks CubeSat Deployer is roughly $85,000. Internal payloads start at about $15,000. Dickes estimates that it takes about 12-18 months from the time a customer orders a CubeSat launch until it is deployed.

In addition to internal payloads aboard the ISS and externally-released CubeSats, NanoRacks offers a third alternative to its customers.The NanoRacks External Platform (NREP), manufactured by Airbus, was placed outside the ISS in August 2016.

Our External Platform actually doesnt release CubeSats payloads are however in the CubeSat form factor, Dickes said. The NREP offers a great solution to run a lot of the same systems as a CubeSat but you dont lose the CubeSat to orbit your NREP payload can return to Earth. NREP is robotically maneuvered in and out of station, and then your payload can come home.

The NanoRacks airlock is on track to meet its next project milestones.

We are working through the detailed design and anticipate a critical design review at the end of October, Howe said. The next big milestone will be a Phase II Safety Review with NASA in January or so.

Tagged: International Space Station Johnson Space Center Lead Stories NanoRacks NASA Neutral Buoyancy Laboratory

Jim Siegel comes from a business and engineering background, as well as a journalistic one. He has a degree in Mechanical Engineering from Purdue University, an MBA from the University of Michigan, and executive certificates from Northwestern University and Duke University. Jim got interested in journalism in 2002. As a resident of Celebration, FL, Disneys planned community outside Orlando, he has written and performed photography extensively for the Celebration Independent and the Celebration News. He has also written for the Detroit News, the Indianapolis Star, and the Northwest Indiana Times (where he started his newspaper career at age 11 as a paperboy). Jim is well known around Celebration for his photography, and he recently published a book of his favorite Celebration scenes. Jim has covered the Kennedy Space Center since 2006. His experience has brought a unique perspective to his coverage of first, the space shuttle Program, and now the post-shuttle era, as US space exploration accelerates its dependence on commercial companies. He specializes in converting the often highly technical aspects of the space program into contexts that can be understood and appreciated by average Americans.

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NanoRacks airlock moving toward 2019 installation on the ISS - SpaceFlight Insider

Our Spaceflight Heritage: 48 years since Apollo 11 landed on the Moon – SpaceFlight Insider

Collin Skocik

July 20th, 2017

A photograph of Armstrong near the Apollo 11 LM, taken by Aldrin on the lunar surface; most of the time, Armstrong had the camera. Photo Credit: NASA

On July 20, 196948 years ago todaythe world was changed forever when two human beings walked on the Moon. 38-year-old Neil Armstrong stepped off the ladder of the flimsy, spidery Lunar Module Eagleonto the soft and pliant dust of the Moons Sea of Tranquillity (Mare Tranquillitatis) and spoke the immortal words: Thats one small step for [a] man, one giant leap for mankind.

Apollo 11 launch. Photo Credit: NASA

It was the culmination of a decade of feverish work and the dedication of 500,000 people across the nation,which paved the way for six more crewed lunar missions.

It began in 1957 when the Soviet Union began the Space Race by launching the first satellite, Sputnik. The National Advisory Committee for Aeronautics (NACA) was reorganized into a civilian agency known as the National Aeronautics and Space Administration (NASA). After several failures, NASA succeeded in launching Americas first satellite, Explorer I.

Nonetheless, it was the crewed space race that attracted the most attention. After vetting the highest qualified test pilots in all the armed services, NASA selected seven top pilots as its Mercury Astronautsthe Mercury Seven.

However, the Soviet Union led the way again, launching Yuri Gagarin into space on April 12, 1961. On May 5, Alan Shepard was launched on a fifteen-minute suborbital flight in his tiny Freedom 7 Mercury capsule propelled by a Redstone rocket. That fifteen minutes of space experience was enough to bolster the confidence of young President John F. Kennedy to stand before Congress and ask for the funding to put a man on the Moon by the end of the decade.

Nine more astronauts were selected for the two-man Gemini Program and the upcoming three-man Apollo flights. Five more Mercury missions expanded Americas ability to live, work, and navigate in space.

The ten Gemini flights perfected the skills that would be needed for a successful Moon landingextravehicular activity, rendezvous and docking, measurement of the radioactivity of the Van Allen radiation belts surrounding the Earth, endurance during long missions, integration of spacecraft systems, communications, and many other things.

However, tragedy struck on Jan. 27, 1967, when a fire broke out inside the Apollo One spacecraft during a routine plugs-out test. Astronauts Gus Grissom, Ed White, and Roger Chaffee were killed.

The Apollo Program was shut down for over a year while the spacecraft was disassembled, with each and every piece examined and analyzed. The problem was found and corrected, as were numerous other problems with the Apollo spacecraft.

Finally, on Oct. 11, 1968, the Apollo Program took flight. Wally Schirra, Donn Eisele, and Walt Cunningham were launched aboard Apollo 7 by a Saturn 1B rocket from Cape Canaveral Air Force Stationthe last crewed mission launched from Cape Canaveral. It was a twelve-day orbital flight to test the Apollo Command and Service Module (CSM) in space.

Then, on Dec. 21, NASA launched perhaps the most daring and audacious space mission in history: Apollo 8. Frank Borman, Jim Lovell, and Bill Anders launched on a Saturn Vthe first crewed launch of that massive rocketand, even though the Lunar Module (LM) was not yet ready for flight, set off on a journey all the way to the Moon. Their Christmas Eve broadcast in lunar orbit transmitted the first television images of the lunar surface to the people of Earth.

Apollo 11 LM Eagle in lunar orbit. Photo Credit: NASA

On March 3, 1969, Apollo 9 launched from Kennedy Space Center to test the Lunar Module in Earth orbit. Dave Scott piloted the CSM Gumdrop while Jim McDivitt and Rusty Schweickart put the Lunar Module Spider through its paces.

On May 18, Tom Stafford, John Young, and Gene Cernan flew Apollo 10 to the Moon to test the Lunar Module Snoopy in lunar orbit and to do a full run-through of the first lunar landing.

Finally, on July 16, Apollo 11 launched on the long-awaited first mission to land humans on the Moon and return them safely to the Earth.

Neil Armstrong was a civilian pilot who had flown the Air Forces X-15 to 207,500 feet (63,250 meters), and, on March 16, 1966, had finally beaten the Russians in space by carrying out the first rendezvous and docking in space, docking the Gemini VIII spacecraft with an Agena target vehicleand then saved Gemini VIII when it went into a disastrous spin.

Command Module Pilot (CMP) was Michael Collins, a 38-year-old Air Force pilot and test pilot, and the first astronaut to perform two spacewalks.

Lunar Module Pilot (LMP) was Edwin Buzz Aldrin, a 38-year-old Air Force pilot and Korean War veteran, and the only astronaut at the time to have a Ph.D. Foreseeing the importance of spaceflight in the near future, he had written his doctoral thesis on orbital rendezvous, and had used his skills to dock Gemini XII with an Agena target vehicle when the rendezvous computer failed.

On July 20, 1969, Neil Armstrong and Buzz Aldrin moved from the Command Module Columbia into the Lunar Module Eagle, leaving Collins alone to orbit the Moon in the Apollo CSM. After undocking, Armstrong rotated the Eagle so that Collins could verify that the landing legs were extended and locked into position.

The Apollo 11 plaque on the Moon. (Click to enlarge) Photo Credit: NASA

CAPCOM Charlie Duke, in Mission Control, Houston, talked Armstrong down during powered descent, but Eagle overshot the landing site due to expelled air in the docking mechanism. Seeing that the computer was bringing Eagle into a hazardous, rocky area, Armstrong took manual control and flew Eagle across the lunar surface until he spotted a flat area.

At 4:18 p.m. EDT (20:18 UTC), Armstrong set Eagle down in the Sea of Tranquillity, informing Duke: Houston Tranquillity Base Here. The Eagle has landed.

Armstrong stepped onto the lunar surface at 10:56 EDT (02:56 UTC on July 21). Aldrin followed half an hour later, and the world watched a grainy black-and-white broadcastwith such poor resolution (due to the slow-scan television transmission being incompatible with commercial TV) that Armstrong and Aldrin looked like ghosts as they movedas the two astronauts collected soil and rock samples, set up the experiments of the Early Apollo Scientific Experiments Package (EASEP), and famously planted the American flag.

It was an inspiring mission for the entire world. The plaque on the Eagle, which still sits undisturbed on the lunar surface, reads:

Here men from the planet Earth first set foot upon the Moon, July 1969 A.D. We come in peace for all mankind.

It is an eternal testament to one of humankinds proudest moments, and the one national program ever mounted in the cause of peace and scientific exploration.

Apollo 11, as well as the six Apollo missions that followed, serve as a beacon for the world to follow. Today the future of our space program has never been more uncertain, so full of possibilities and so empty of promise. From here we may go nowhere, or we may conquer the stars. Only timeand the will of the American peoplewill tell.

This photograph of the Lunar Module at Tranquillity Base was taken by Neil Armstrong during the Apollo 11 mission, from the rim of Little West Crater on the lunar surface. Armstrongs shadow and the shadow of the camera are visible in the foreground. When he took this picture, Armstrong was clearly standing above the level of the Lunar Modules footpads. Darkened tracks lead leftward to the deployment area of the Early Apollo Surface Experiments Package (EASEP) and rightward to the TV camera. This is the furthest distance from the Lunar Module traveled by either astronaut while on the Moon. Photo & Caption Credit: NASA

Buzz Aldrin salutes U.S. flag on the Moon. Photo Credit: NASA

Video courtesy of NASA Johnson

Tagged: Apollo 11 Lead Stories Moon NASA

Collin R. Skocik has been captivated by space flight since the maiden flight of space shuttle Columbia in April of 1981. He frequently attends events hosted by the Astronaut Scholarship Foundation, and has met many astronauts in his experiences at Kennedy Space Center. He is a prolific author of science fiction as well as science and space-related articles. In addition to the Voyage Into the Unknown series, he has also written the short story collection The Future Lives!, the science fiction novel Dreams of the Stars, and the disaster novel The Sunburst Fire. His first print sale was Asteroid Eternia in Encounters magazine. When he is not writing, he provides closed-captioning for the hearing impaired. He lives in Atlantic Beach, Florida.

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Our Spaceflight Heritage: 48 years since Apollo 11 landed on the Moon - SpaceFlight Insider

Spaceflight Beeps Inspire Cosmic ‘Quindar’ Music: A Q&A with the Composers – Space.com

Cover for new record from art historian James Merle Thomas and Wilco keyboardist Mikael Jorgensen.

At times, the inexplicable emotions that run though the minds of music creators carries with it the weight of traversing space.

Using technological elements that bring people together over great distances, thus "minimizing" the space and time between them, art historian James Merle Thomas and Wilco keyboardist Mikael Jorgensen have created a musical experience that taps into the history of spaceflight. They dubbed the project "Quindar."

Quindar-Tones are the communication "beeps" between CapCom and spacecraft during NASA's Apollo and other space missions. The purpose of the beeps is to "trigger the ground station transmitters when there is an outgoing transmission from Earth," according to NASA Apollo Lunar Surface Journal contributor Markus Mehring. [Exoplanet Symphony: Listen to TRAPPIST-1 Worlds' Orbital Music]

These tones served as an inspiration for the duo's new record, "Hip Mobility," and they were infused with other NASA audio archives to create the songs, including "Twin-Pole Sunshade for Rusty Schweikart" and "Honeysuckle This Is Houston," which hark back to the Apollo program.

Space.com talked with James Merle Thomas and Mikael Jorgensen of Quindar in an email interview about the record's inspiration and its technical details.

Space.com: In a very novel approach to composing music, you've interwoven space, time and technology into an ethereal experience. How did your interest in spaceflight history and communications technology act as a muse for the record?

James Merle Thomas: Quindar evolved organically out of our shared enthusiasm for histories of art, technology and music, and is directly related to my doctoral research I'm trained as a historian and curator of modern and contemporary art, and am specifically interested in understanding how our notion of what "modern" looks like is related to the technology and politics of the Cold War period. In 2011, while on a Guggenheim fellowship at the National Air and Space Museum, I was researching how NASA designed for space. My research was focused on how the agency's understanding of its own design shifted during the late 1960s/early 1970s, as the Apollo Applications Programs (including Skylab) drew to a close, and as the program reoriented from symbolic exploration to include a narrative about living and working in space, about scientific research in a laboratory setting, etc.

One fascinating aspect of this transitional period is the rich collaboration (and sometimes tensions) between engineers, who were planning for precision and efficiency, and, on the other hand, architects, artists and industrial designers (e.g., Raymond Loewy, who designed the interior of Skylab), who were invested in questions of visual identity, orientation [and] personal space, and who were genuinely interested in matters of aesthetic design and the possibility for personal improvisation.

Mikael Jorgensen: Early on in our collaboration, James suggested that we listen to some of the NASA archival audio materials he'd been gathering as potential source material for the music we were creating. It all made sense in that moment to ingest and remix not only the sounds of the space program but to utilize these recordings to provide narratives to our songs the way lyrics and singing function. Since we were trying to push our own creative sensibilities and sonic possibilities, incorporating this as a fundamental part of our working methodology we didn't see or feel the need to use our own voices. This vast archive of sound would help us figure out what we wanted to say.

The big, heroic, epic stories of spaceflight have been told. There's the endless preparation, calculation, trials, training and tests leading to the blastoff, being in orbit, and then, re-entry. This larger context is the backdrop for what we've been curious about exploring. What is it like to be aggravated in space? Is weightlessness as wonderful as it sounds? (It turns out to be very uncomfortable at times.) In the moments between endless experiments and tasks, is there time to deeply ponder how insane it is to be so unimaginably far away from our planet before a radio crackles and asks for a status report? [Fun in Zero-G: Weightless Photos from Earth and Space]

Quindar tones are 250ms sine waves at 2.525kHz and 2.475kHz which are generated by an analog synthesizer which is housed in a module that would plug into the control panels in mission control. A corresponding Quindar device in the spacecraft would receive a Quindar tone at one frequency and respond with the other. The more we learned about what Quindar tones were and how they functioned, this beautiful metaphor emerged. I like to think of it as a screenplay:

INT. MISSION CONTROL. NIGHT. A vast array of control panels, switches, lights, dials, meters, are busy indicating life-support levels, fuel supplies are attended by men in suits. Large screens in the front of the room display world maps indicating the current position of the spacecraft as it hurtles through space, hundreds of miles above the Earth. The ambient audio of the chatter in the busy room fades out as we zoom in on a single Quindar module in a control panel bank:

Cut to spacecraft:

MISSION CONTROL QUINDAR MODULE: [BEEP] (An indicator lamp lights when the device transmits) Subtitle: Hey, are you there?

SPACECRAFT QUINDAR MODULE: (Lamp lights, confirming receipt of the [BEEP]) Subtitle: I'm here! [BEEP] (Lamp lights when the device transmits) Subtitle: Are you still there?

MISSION CONTROL QUINDAR MODULE: (Lamp lights, confirming receipt of the [BEEP]) Subtitle: I'm here! [BEEP] (An indicator lamp lights when the device transmits) Subtitle: Are you still there?

Cut to Mission Control:

This conversation continues in the background ensuring a consistent communication channel between the astronauts and mission control.

Fade to black.

So this idea that a musical conversation is being transmitted and received by a pair of synthesizers one of which is in space spoke very deeply to us.

Space.com: You're bringing to light a little-known, but really important, component of communications with Quindar. Can you explain how it was applied when composing the record?

Jorgensen: James was pretty quick to take the Quindar tones into the music software Ableton Live, assign them musical values and generate musical textures and chords using the original recordings.

Thomas: I was struck by how a Quindar tone is a focused sonic element, and how, when you slow down the intro/outro tones, their subtle difference becomes more perceptible. For anyone even casually familiar with John Cage, Pierre Schaeffer and a larger artistic tradition of using found sounds in composition, it's a pretty short path to re-imagining an array of Quindar tones as a kind of musical instrument.

Space.com: When you were thinking about what the title of the record should be, how did you decide that "Hip Mobility" was the way to go?

Jorgensen: It's pretty easy to get wrapped up in the seriousness and weight of these unfathomably difficult missions. There were countless problems to solve and challenges to predict with only slide rulers, pencils and brain power. That being said and fully appreciated, we've identified moments that seem unintentionally funny to us. "Hip Mobility" was the title of an excerpt from an industrial film that was depicting the flexibility of a prototype spacesuit and it was just exactly what you'd expect: A man wearing long underwear, in a preposterous aluminum exoskeletal framework, bending and stretching to illustrate the range of motion that this particular spacesuit would provide an astronaut in space. Out of context, "Hip Mobility" sounds like a name for the coolest dance moves or a description of moving into, or out of (not sure which) an up and coming neighborhood. [Evolution of the pacesuit in Pictures (Space Tech Gallery)]

I'd just like to say that we're in no way making fun of these men and women who worked diligently and seriously on these projects, but that we're empathizing with them and hopefully acknowledging some of the ridiculous things that we find ourselves doing in service of some larger goal. It's important to be serious, but not to take yourself too seriously.

Art historian James Merle Thomas and Wilco keyboardist Mikael Jorgensen collaborate to create the 'Quindar' record.

Space.com: Converting phenomena throughout the cosmos, that's usually inaudible by humans, into music has drawn a lot of interested folks to our site. Looking forward, is there another bit of technology, space history or a phenomenon that has been stirring the creative juices?

Jorgensen: There is currently such a wealth of tools and software that exist to make almost any idea a reality. We've been lucky to work with Jeremy Roth, who does stage design and lighting for Wilco, and tap into his expertise when it comes to our live show presentation. We've been using software called Resolume Arena which allows us to cue up video and present it in real time, but also to display multiple channels at once, superimpose video and more. It's been extremely gratifying to build our live show with our synthesizers and laptops and have them communicate with the video software to put this live show together that is at once interactive and responsive to each other.

"Hip Mobility" is available on Amazon. Learn more about Quindar through their website.

Follow Steve Spaleta @stevespaleta. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

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Spaceflight Beeps Inspire Cosmic 'Quindar' Music: A Q&A with the Composers - Space.com

Propulsive landings nixed from SpaceX’s Dragon spaceship – Spaceflight Now

Artists concept of SpaceXs Red Dragon spacecraft. Credit: SpaceX

SpaceXs upgraded Dragon capsules will not return astronauts to Earth for powered landings as originally envisioned, company boss Elon Musk said Wednesday, a design change that raises questions about the space transport firms plans to send commercial landers to the surface of Mars.

Musk cited safety concerns for eliminating plans for propulsive Dragon landings in remarks at the International Space Station Research and Development Conference in Washington. He also said the original Dragon landing concept, in which four landing legs would extend from the base of the capsules heat shield as throttleable SuperDraco thrusters slowed the crafts speed for touchdown, was not as useful as he initially thought for SpaceXs plans to send humans to Mars.

That was a tough decision, Musk said in response to a question on the matter. He added that the human-rated Dragon, which SpaceX is developing with mostly NASA funding, is technically still capable of propulsive landings.

Although youd have to land it on some pretty soft landing pad because weve deleted the little legs that pop out of the heat shield, Musk said.

SpaceX unveiled the design of the next-generation spacecraft in May 2014, when Musk predicted the capsule should be ready to ferry astronauts to and from the International Space Station by the end of 2016. Musk said Wednesday that the spaceship is now scheduled to launch crews by mid-2018, and he described the crew capsule effort as SpaceXs primary focus.

NASA awarded SpaceX a $2.6 billion contract later in 2014 to finish development of the upgraded Dragon spacecraft called Crew Dragon or Dragon 2 and fly up to six crew rotation missions to the space station. Boeing won a similar contract worth $4.2 billion for its CST-100 Starliner spacecraft.

Both programs have been delayed and will miss NASAs goal of having the vehicles certified for piloted missions by the end of 2017, ending U.S. reliance on Russian Soyuz spacecraft to carry astronauts to the space station and return them to Earth.

Boeing says the CST-100 Starliners first orbital test flight with a two-person crew in August 2018.

SpaceX officials said in 2015 that the Crew Dragons first few missions would end with parachute-assisted splashdowns at sea, similar to the way the current Dragon cargo capsules come back to Earth. The crew-capable version is heavier, requiring four main chutes instead of the three flying on station resupply flights.

But engineers continued to plan for propulsive landings once NASA certified the powered descent approach. The Crew Dragon will already have the SuperDraco thrusters needed for a powered descent. The same rocket packs act as the capsules escape booster to whisk astronauts away from a failing launcher.

That is how a 21st century spaceship should land, Musk said in 2014, describing the crew capsules ability to land anywhere on Earth with the accuracy of a helicopter.

SpaceX now favors another type of recovery.

The reason we decided not to pursue (powered landings) heavily is it would have taken a tremendous amount of effort to qualify that for safety, particularly for crew transport, Musk said. And then there was a time when I thought that the Dragon approach to landing on Mars, where youve got a base heat shield and side-mounted thrusters, would be the right way to land on Mars, but now Im pretty confident that is not the right way, and that theres a far better approach.

Musk did not elaborate on the new concept for landing on Mars.

Thats what the next generation of SpaceX rockets and spacecraft is going to do, so just the difficulty of safely qualifying Dragon for propulsive landings, and the fact, from a technology evolution standpoint, it was no longer in line with what we were confident was the optimal way to land on Mars, Musk said. Thats why were not pursuing it.

It could be something that we bring back later, but it doesnt seem like the right way to apply resources right now.

The redesign of the next-generation Dragons landing system will affect SpaceXs plans to send the first in a series of robotic Dragon spacecraft to Mars in 2020. Musk did not address the status of the first so-called Red Dragon mission Wednesday, but the concept involved dispatching a Dragon capsule similar to the ship built for crews to the red planet on top of a huge Falcon Heavy booster.

The Red Dragon would have descended to a powered touchdown on landing legs in a sequence similar to the one envisioned for Crew Dragons on Earth.

Gwynne Shotwell, SpaceXs president and chief operating officer, said in February that the first Red Dragon flight was delayed to mid-2020 from 2018, pushing its arrival at Mars back to early 2021. Launch opportunities to Mars come approximately every 26 months when the planets are favorably aligned.

The Red Dragons would have delivered cargo and experiments to the Martian surface and tested supersonic retro-propulsion in the planets rarefied atmosphere for the first time. NASA engineers say a rocket-braking mechanism like the Dragons SuperDraco thrusters is needed to safely land heavy supply ships and crew vehicles on Mars.

The space agency signed up to support the privately-developed Red Dragon project to gather data on supersonic retro-propulsion officials said NASA would be unable to obtain until at least the late 2020s with a government-managed mission. NASA said it would spend more than $30 million on the effort by providing advisors, navigation, communications and tracking services, and technical analysis.

Musk wrote in a tweet that SpaceX has not abandoned supersonic retro-propulsion at Mars.

Plan is to do powered landings on Mars for sure, but with a vastly bigger ship, he tweeted Wednesday after his remarks in Washington.

Musk said his team at SpaceX is refining how the company could send people to Mars, eventually to settle there. He revealed a Mars transportation architecture in a speech at the 67th International Astronautical Congress in Guadalajara, Mexico, last year, but the outline has since changed.

A vision for gigantic interplanetary transporters Musk presented last year has been downsized, he said.

Its a little smaller, still big, but I think this ones got a shot at being real on the economic front, Musk said, adding that he might present more details at this years International Astronautical Congress in Adelaide, Australia.

Musk said SpaceX is making progress on the Crew Dragon vehicle, which has a different aerodynamic shape than the companys cargo craft. Designers are also adding a life support system, seats, cockpit displays and other equipment for human passengers.

Its been way more difficult than cargo, for sure, Musk said. As soon as people enter the picture, its really a giant step up in making sure things go right. For sure, the oversight from NASA is much tougher. I thought it was tough for cargo, but its really intense for crew.

It can be a bit tough on the men and women at SpaceX, but I know where its coming from, he said. Its the right motivation, and there will be some debates going into next year about some of the technical details is this right or that right? But I think we really want to make everything humanly possible to make sure it goes well and triple check everything.

Crews riding Dragon spacecraft will blast off on SpaceXs Falcon 9 rocket from pad 39A at the Kennedy Space Center in Florida. SpaceX is working on final modifications to the Falcon 9, which it calls the Block 5 configuration, to meet NASA human-rating safety standards.

Musk said there were some small technical bones of contention, but were working through those.

He did not offer details on the disagreements.

Some (of the) the things are really esoteric, really in the weeds of rocket and spacecraft design, he said. But I think its good to have these debates.

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Propulsive landings nixed from SpaceX's Dragon spaceship - Spaceflight Now

Brown dwarf discovered with the help of citizen scientists – SpaceFlight Insider

Ocean McIntyre

July 20th, 2017

This illustration shows the average brown dwarf is much smaller than our Sun and low-mass stars and only slightly larger than the planet Jupiter. Image & Caption Credit: NASAs Goddard Space Flight Center

Sometimes in science, when you search for one thing, you end up finding something completely different. Such is the case with the search for the thus far elusive Planet Nine and the citizen scientists who ended up finding a brown dwarf instead.

Backyard Worlds: Planet 9 is a NASA-funded project sponsored by Zooniverse, and is the group under whose auspices the discovery was made just weeks after its official launch on February 15, 2017. The launch date, which also happened to coincide with the 87th anniversary of the discovery of Pluto, was a tip of the hat to the methodology that is being used to look for the hypothesized planet along with other dim rogue worlds in the far distant outer reaches of the Solar System and beyond.

The newly discovered brown dwarf WISEA J110125.95+540052.8 appears as a moving dot (indicated by the circle) in this animated flipbook from the Backyard Worlds: Planet 9 citizen science project. Image & Caption Credit: NASA / WISE

The search for Planet Nine, also called Planet X by some, has led to several new discoveries, including this brown dwarf designated WISEA 1101+5400.

We realized we could do a much better job identifying Planet 9 if we opened the search to the public, said Marc Kuchner, an astrophysicist at NASAs Goddard Space Flight Center in Greenbelt, Maryland, and lead researcher for the Backyard Worlds project. Along the way, were hoping to find thousands of interesting brown dwarfs.

WISEA 1101+5400 (full name WISEA J110125.95+540052.8) was found with the critical assistance of four citizen scientists, one of whom is Rosa Castro, a therapist, who is credited with nearly 100 classifications as a part of this project.

Backyard Worlds, along with the majority of the other projects under the umbrella of Zooniverse, relies heavily on citizen scientists to sort through huge volumes of data for things that stand out to them. In this case, the project provides participant individuals with flipbooks animated collections of time-lapsed images of the same part of space to review, noting any visible changes in the position or brightness of the pixels within the series of images.

The flipbooks are a collection of the data that was gathered by the Wide-Field Infrared Survey Explorer (WISE) which was launched into space on December 14, 2009.

Originally designed to observe cold objects, as well as those that emit light in the infrared portion of the spectrum (long wavelengths) such as brown dwarfs, WISE was deactivated in 2011 after depleting its source of frozen hydrogen that was needed to cool the sensors, and then reactivated in 2013 as NEOWISE to search for near-Earth objects, or NEOs, which tend to be cold, dark objects easier to locate in the infrared spectrum.

The data that the WISE and NEOWISE missions gathered of the entire sky provides one of the best chances of locating the enigmatic Planet 9 because it may already have been caught in those images. It takes human eyes to be able to look through the noise filled images and be able to recognize these objects, though.

There are a vast number of images, more images than a small team of researchers alone could process in a lifetime, which is why the Backyard Worlds project was created and opened up to the public. What started out as a small group of individuals has grown significantly in the five months it has been in operation. Currently, there are several hundred (or more) citizen scientists looking through the flipbooks for additional objects.

So, whats the deal with WISEA 1101+5400? WISEA1101+5400 isnt exactly local with a location approximately 34 parsecs (111 light-years) from Earth in the constellation Ursa Major. The object is a brown dwarf classified as a spectral T5.5, meaning that its size and mass are too low to sustain fusion as a star and that its temperature runs between 9001,500 K (6301,230 C / 1,1602,240 F).

Artists rendition of a T-class brown dwarf. Image Credit: NASA/JPL-Caltech

Researchers took images of the spectra (light) from the object and found that it was nearly identical to other T dwarfs, containing specific amounts of water, methane, iron hydride, potassium, and molecular hydrogen. If the object were cooler or hotter, the amounts and variety of these molecules in the spectral analysis would be different.

The spectrum of WISEA 1101+5400 in black with another T5.5 brown dwarf in red. Image Credit: Kuchner et al.

In fact, WISEA 1101+5400 is pretty average as far as T dwarfs go. What isnt average is who and how it was discovered. Its unlikely that Rosa Castro, Dan Caselden, or the two other citizen scientists involved with the discovery, had set out to find this cold distant object, but find it they did, and just six days after the start of the project.

Even with WISEA 1101+5400 averageness, the researchers are excited. Kuchner hopes that with enough time and interest, they will be able to locate super small, super-cold brown dwarfs called Y-dwarfs, some of which may be lurking far closer to us than we realize.

Theyre so faint that it takes quite a bit of work to pull them from the images, thats where Kuchners project will help immensely, said Adam Burgasser at the University of California San Diego. Anytime you get a diverse set of people looking at the data, theyll bring unique perspectives that can lead to unexpected discoveries.

Its interesting to note that this isnt the only discovery that Backyard Worlds has made. There are currently 117 additional brown dwarf candidates being vetted all from this citizen science driven project, and Kuchner expects that the Backyard Worlds effort will continue for several years to come allowing more volunteers to get involved.

I am not a professional. Im just an amateur astronomer appreciating the night sky, said Rosa Castro. If I see something odd, Ill admire and enjoy it.

Backyard Worlds: Planet 9 is a collaboration between NASA, UC Berkeley, the American Museum of Natural History in New York, Arizona State University, the Space Telescope Science Institute in Baltimore, and Zooniverse a collaboration of scientists, software developers, and educators who collectively develop and manage citizen science projects on the Internet.

NASAs Jet Propulsion Laboratory (JPL) in Pasadena, California, manages the NEOWISE mission for NASAs Planetary Defense Coordination Office within the Science Mission Directorate in Washington. The Space Dynamics Laboratory in Logan, Utah, built the science instrument. Ball Aerospace & Technologies Corp. of Boulder, Colorado, built the spacecraft. Science operations and data processing take place at the Infrared Processing and Analysis Center at Caltech in Pasadena. Caltech manages JPL for NASA.

For more information, visitBackyard Worlds: Planet 9 and NASAs WISE mission.

Tagged: brown dwarf NASA Planet 9 The Range WISE WISEA 1101+5400

A native of the Greater Los Angeles area, Ocean McIntyre's writing is focused primarily on science (STEM and STEAM) education and public outreach. McIntyre is a NASA/JPL Solar System Ambassador as well as holding memberships with The Planetary Society, Los Angeles Astronomical Society, and is a founding member of SafePlaceForSpace.org. McIntyre is currently studying astrophysics and planetary science with additional interests in astrobiology, cosmology and directed energy propulsion technology. With SpaceFlight Insider seeking to expand the amount of science articles it produces, McIntyre was a welcomed addition to our growing team.

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Soyuz liftoff glimpsed by orbiting observer and launch pad cameras … – Spaceflight Now

The launch of a Russian Soyuz rocket July 14 with more than 70 satellites was captured in multiple views from a sharp-eyed orbiting nanosatellite and cameras positioned around the launch pad at the Baikonur Cosmodrome in Kazakhstan.

The Russian state space corporation, Roscosmos, released a video clip containing imagery of last weeks blastoff from several cameras placed around Launch Pad No. 31 at Baikonur, where the Soyuz rocket soared into space at 0636 GMT (2:36 a.m. EDT; 12:36 p.m. Baikonur time) July 14.

The rocket deployed 73 spacecraft into a range of orbits several hundred miles above Earth, including 48 Dove satellites to grow Planets commercial fleet of Earth-imaging CubeSats to nearly 200 members.

One of the Dove satellites already in space about the size of a toaster oven happened to be flying over Kazakhstan at the time of launch. Planets ground controllers pointed the telescopic camera on the spacecraft toward the launch pad at Baikonur.

To create this animation, we pointed a Dove approximately 50 degrees off-nadir towards the pad, capturing one still image per second of the fixed target as the Dove traveled overhead at an approximate speed of seven kilometers per second (or 15,658 mph), a Planet employee wrote in a post on the companys website. Then our imaging team cropped and stitched the stills together. All in all, this short clip covers about two and a half minutes in real-time including liftoff and flight.

The U.S. company operates the worlds largest fleet of commercial satellites, most of which are about the size of a shoebox and built in-house at the companys San Francisco headquarters.

The Soyuz booster launched last week also sent a Russian satellite into orbit to locate forest fires, eight commercial weather satellites for Spire Global, another San Francisco-based company, and spacecraft owned by institutions and operators in Germany, Norway and Japan.

More photos of the July 14 launch are posted below.

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Pioneering probe for gravitational wave observatory ends mission – Spaceflight Now

Artists illustration of the LISA Pathfinder spacecraft. Credit: ESA

The European Space Agencys LISA Pathfinder spacecraft, now sailing around the sun on a trajectory away from Earth, was deactivated Tuesday after a nearly 18-month mission testing previously-untried lasers, vacuum enclosures, exotic gold-platinum cubes and micro-thrusters needed for a trio of gravitational wave observatories set for launch in the 2030s.

Stefano Vitale, principal investigator of the LISA Pathfinder missions core instruments, sent the long-planned command to passivate the probe at 1800 GMT (2 p.m. EDT) Tuesday from the European Space Operations Center in Darmstadt, Germany.

The end of LISA Pathfinders mission Tuesday marked another turning point in gravitational wave research, a field of astrophysics reinvigorated in the last two years by two major advances, according to Paul McNamara, the missions project scientist at ESA.

First came the launch of LISA Pathfinder on Dec. 3, 2015. Three months later, scientists announced the first confirmed detection of gravitational waves, ripples in the fabric of spacetime produced by the movement of massive objects in space, such as immense supermassive black holes at the centers of galaxies.

The gravitational waves, first predicted more than a century ago by Albert Einstein, were discovered by scientists crunching data gathered in September 2015 from a ground-based observatory called LIGO, which has antennas positioned 1,800 miles (3,000 kilometers) apart in Hanford, Washington, and Livingston, Louisiana.

Gravitational wave research requires huge detectors spread of thousands or millions of miles because the ripples are observed at very low frequencies as they travel through the universe at the speed of flight. Astronomers say the waves, which can be triggered by violent phenomena such as black hole mergers, reveal a new way of studying the cosmos impossible with conventional optical telescopes.

The back-to-back breakthroughs catapulted gravitational waves to the forefront of astronomical journals and space mission planning.

Was it a big step forward? Absolutely, because up to this point there were two doubts, McNamara said in an interview this week with Spaceflight Now. One doubt was gravitational waves dont exist, and then LIGO comes along and detects them.

Then we launched LISA Pathfinder, and we demonstrated the hardware in space, he said. So the two big questions do they exist and can we detect them? both were answered within three months of each other.

LISA Pathfinder was named for a follow-on mission dubbed the Laser Interferometer Space Antenna, which was formally selected by ESAs science planning board June 20 to move into the next phase of mission planning after decades of starts and stops.

With the astonishing success of LISA Pathfinder, we now know how to build a mission like LISA, said Vitale, a researcher at the University of Trento and the National Institute for Nuclear Physics in Italy.

Launched from French Guiana aboard a Vega rocket, the hexagonal space probe is about the size of a small car. LISA Pathfinder reached an operating point at the L1 Lagrange point nearly a million miles (1.5 million kilometers) from Earth in January 2016, lurking near a gravitational balance point between in a direction toward the sun.

In March 2016, on the first day LISA Pathfinder was in full science mode, ground controllers confirmed the mission had already met its minimum success requirements.

Two gold-platinum test cubes launched inside the LISA Pathfinder spacecraft were released from their launch restraints, a complicated procedure involving needle-like appendages that carefully pulled away from the cubes each 1.8 inches (46 millimeters) on a side and with a mass of 4.4 pounds (2 kilograms) to avoid disturbing them with electrostatic forces.

The crux of the mission was to prove the test cubes could be kept in a constant state of nearly perfect free fall during LISA Pathfinders mission.

Two sets of low-impulse thrusters essentially steered the spacecraft around the free-floating test masses suspended inside two vacuum enclosures placed 15 inches (38 centimeters) apart on the satellite.

Accelerometers aboard LISA Pathfinder precisely tracked its movements, and a control computer sent signals to the low-thrust rocket packs outside the probe to continuously correct to keep the test cubes from contacting the walls of their chambers.

A high-precision laser interferometer constantly measured the range between the two test cubes, and that device also exceeded requirements, measuring the relative motion of the test masses with a precision of a femtometer, or one quadrillionth of a meter.

LISA Pathfinder is 10,000 times more stable than any satellite flown on a previous science mission, officials said, demonstrating that it was possible for the test masses to remain virtually motionless with respect to each other.

ESA said the test masses had a relative acceleration of only ten billionths of a billionth of Earths gravity, an achievement made possible by a tedious accounting of every component of the spacecraft that could influence the floating metallic cubes.

Many of the lessons learned from LISA Pathfinder were not in how to build a space-rated gravitational wave detector, but how to operate it, McNamara said. Even the switch-on of a transponder or star tracker added noise to the instrument beyond acceptable limits.

This is such a sensitive instrument that it responds to anything changing whatseover, NcNamara said. Weve learned that, for LISA, we have to assume if you make any changes on-board its going to take you time to recover back into equilibirium. If you turn any unit on, you turn any heater on, or do anything on the spacecraft to put it in a slightly different orientation, itll take you a week to get back to operational status.

Such precision is needed because gravitational waves have an amplitude of a few millionths of a millionth of a meter over a distance of a million kilometers (621,000 miles). Any larger movement of the test masses would mask the gravitational wave.

The LISA Pathfinder mission cost around $630 million, a figure that includes contributions from ESA, NASA and other institutions scattered across Europe.

LISA Pathfinder was conceived to prove a gravitational wave mission was technically feasible.

People just didnt think it was possible, McNamara said. Thats why LISA Pathfinder came into being. It was just to see could we build an instrument which was quiet enough.

The concept for the LISA mission selected by ESA last month calls for three spacecraft similar to LISA Pathfinder to launch in 2034 into an orbit around the sun that trails the Earth.

The LISA spacecraft will fly in a triangular formation more than 1.5 million miles (2.5 million kilometers) apart, linked by lasers to track the exact distances between the nodes, which will each contain two free-floating test masses. Sensors will watch for tiny variations in the range between the craft as gravitational waves pass through the solar system.

With gravitational waves, its a completely new endeavor were taking on, McNamara told Spaceflight Now. This idea of flying three spacecraft separated by millions of kilometers, and you have to be able to measure the distance to a hundredth the size of an atom.

We have exceeded not only the requirements set for LISA Pathfinder, but also the accuracy required for LISA at all frequencies: we are definitely ready to take the next step, said Karsten Danzmann, a LISA Pathfinder co-investigator, the lead proposer of the LISA mission, and director at the Max Planck Institute for Gravitational Physics in Germany.

ESA expects the LISA mission to cost up to $1.2 billion (more than a billion euros), not including support from NASA.

Paul Hertz, director of NASAs astrophysics division, said Wednesday that the U.S. space agency wants to contribute technology and hardware to the LISA mission roughly equivalent to around 20 percent of the missions total cost.

NASA and ESA originally planned a larger, more ambitious LISA mission, but NASA dropped out of the partnership in 2011 due to budget constraints. ESA pressed on with a scaled-back gravitational wave observatory, which received prioritization from the agency in 2013 ahead of the LISA concepts selection last month.

European officials want ESA to lead the LISA mission to avoid falling victim to another failed partnership, but NASA will still be a significant contributor. After discussions in the last few years for NASA to be a 10 percent partner, the U.S. stake in the LISA mission is now likely to be closer to 20 percent.

We are talking about a more substantial contribution than a 10 percent share, Hertz said. ESA has welcomed us as a very major partner.

NASA might develop lasers and telescopes for the LISA observatory, or the missions charge management system. Another potential U.S. addition to the mission could be the micro-thrusters needed to deftly control each of the LISA spacecraft, which will be assembled in Europe.

LISA is third in ESAs Cosmic Vision line of large-class billion-euro space science missions.

A robotic spacecraft that will orbit Jupiter, and then circle Jupiters largest moon Ganymede, is on schedule for launch aboard an Ariane 5 rocket in 2022, followed by liftoff of the Athena X-ray astronomy observatory in 2028.

Then it will be LISAs turn.

Before shutting down LISA Pathfinder, controllers fired its thrusters to nudge it out of its post at the L1 Lagrange point in April to head into a heliocentric orbit around the sun. The maneuver minimized the chance the spacecraft will return to Earths vicinity.

LISA Pathfinders science mission officially ended June 30, and engineers spent the final weeks practicing procedures to recapture the test masses inside their housings, which might be necessary if problems develop on the LISA mission. Other final tasks included monitoring the instruments behavior when the spacecrafts thrusters were turned off, and tracking the test masses response to a coronal mass ejection from the sun.

Scientists were eager to see how the spacecraft responded when it was zapped by ionizing energy from a solar eruption last week. In particular, mission officials wanted to know whether the instrument would still provide useful science data when the test masses were hit by charged particles. Reviews of that data are still ongoing, McNamara said.

The final commands uplinked to LISA Pathfinder turned off the crafts transponder and corrupted the memory files of the probes primary and redundant computers by filling the processors with the names of scientists and engineers who worked on the mission.

This is a celebration, and its certainly not a sad moment, Vitale said moments before sending the order that silenced the spacecraft.

LISA Pathfinder has done everything and more that we could have asked of it, McNamara said. And its allowed LISA to go ahead, so yes, were sad thats going away and its ending, but were very happy LISA is taking off.

Its another 17 years to go before that one launches, so well exercise our patience.

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VASIMR plasma engine: Earth to Mars in 39 days? – SpaceFlight Insider

Collin Skocik

July 19th, 2017

Artists impression of a 200-megawatt VASIMR spacecraft. Images Credit: Ad Astra Rocket Company

In Arthur C. Clarkes classic science fiction novels and movies 2001: A Space Odyssey and 2010: Odyssey Two, the spaceships Discovery and Alexei Leonov make interplanetary journeys using plasma drives. Nuclear reactors heat hydrogen or ammonia to a plasma state thats energetic enough to provide thrust.

In 1983, seven-time Space Shuttle Astronaut Franklin Chang Diaz turned Clarkes speculations into reality with an engine known as the Variable Specific Impulse Magnetoplasma Rocket (VASIMR).

An electric power source ionizes hydrogen, deuterium, or helium fuel into a plasma by stripping away electrons. Magnetic fields then direct the charged gas in the proper direction to provide thrust.

A rocket engine is a canister holding high-pressure gas, Chang Diaz explained. When you open a hole at one end, the gas squirts out and the rocket goes the other way. The hotter the stuff in the canister, the higher the speed it escapes and the faster the rocket goes. But if its too hot, it melts the canister.

The VASIMR engine is different, Chang Diaz explained, because of the fuels electrical charge: When gas gets above 10,000 [kelvins], it changes to plasma an electrically charged soup of particles. And these particles can be held together by a magnetic field. The magnetic field becomes the canister, and there is no limit to how hot you can make the plasma.

Chang Diaz has pointed out that hydrogen would be an advantageous fuel for the VASIMR engine because the spacecraft would not have to lift off carrying all the fuel it needs for the journey.

VASIMR System. Image Credit: Ad Astra Rocket Company

Were likely to find hydrogen pretty much anywhere we go in the Solar System, he said.

A spacecraft using conventional chemical rockets would take eight months to get to Mars during opposition. However, the VASIMR engine would make the journey in as little as 39 days.

Chang Diaz explained: Remember, you are accelerating the first half of the journey the other half youre slowing, so you will reach Mars but not pass it. The top speed with respect to the Sun would be about 32 miles per second [or 51.5 km/s]. But that requires a nuclear power source to heat the plasma to the proper temperature.

The use of nuclear power in space is not without its controversy. In 1997, there was widespread public concern when NASAs Cassini probe, which carried a plutonium battery, made a flyby of Earth to perform a gravity assist. Although NASA denied that the risk to the public, should an accident occur, was no greater thanthat posed every day by other sources of radiation, some scientists, including the popular theoretical physicist Michio Kaku, disagreed.

In April 1970, the Atomic Energy Commission was deeply concerned about the return of Apollo 13 to Earth. Where an Apollo mission would usually leave the lunar modules descent stage on the Moon, the unsuccessful Apollo 13 dropped its lunar module Aquarius, with its plutonium-powered scientific experiments, into the ocean, raising concerns about radioactive contamination.

Elon Musk, CEO of Space Exploration Technologies Corporation (SpaceX), is skeptical about the viability of the VASIMR engine. One reason is the concern about radioactive debris falling to Earth in the event of an accident.

Musk is also skeptical that the VASIMR engine would be a significant improvement over chemical rockets, stating: So people like Franklin basically its a very interesting ion engine hes got there, but it requires a big nuclear reactor. The ion engine is going to help a little bit, but not a lot in the absence of a big nuclear reactor. Musk also points out that the big nuclear reactor would add a lot of weight to a rocket.

Chang Diaz dismisses the concerns about nuclear reactors in space, stating: People are afraid of nuclear power. Chernobyl, Three Mile Island, Fukushima it is a little misunderstood. But if humans are truly going to explore space, we eventually will have to come to grips with the concept.

Another vocal critic of the VASIMR engine is Robert Zubrin, president of The Mars Society, who designed the Mars Direct plan to colonize Mars and wrote the popular book The Case For Mars. He has gone as far as to call the VASIMR engine a hoax.

Zubrin wrote in SpaceNews: To achieve his much-repeated claim that VASIMR could enable a 39-day one-way transit to Mars, Chang Diaz posits a nuclear reactor system with a power of 200,000 kilowatts and a power-to-mass ratio of 1,000 watts per kilogram. In fact, the largest space nuclear reactor ever built, the Soviet[-era] Topaz, had a power of 10 kilowatts and a power-to-mass ratio of 10 watts per kilogram. There is thus no basis whatsoever for believing in the feasibility of Chang Diazs fantasy power system.

Chang Diaz, however, says in his paper: Assuming advanced technologies [emphasis added] that reduce the total specific mass to less than 2 kg/kW, trip times of less than 60 days will be possible with 200 MW of electrical power. One-way trips to Mars lasting less than 39 days are even conceivable using 200 MW of power if technological advances allow the specific mass to be reduced to near or below 1 kg/kW.

LEFT: Artists rendition of a lunar tug with 200 kW solar powered VASIMR. RIGHT: Artists rendition of a human mission to Mars with 10 MW NEP-VASIMR. Images Credit: Ad Astra Rocket Company

In other words, Chang Diaz is allowing for further developments that would enable such a reactor.

Zubrin, however, stated: [T]he fact that the [Obama] administration is not making an effort to develop a space nuclear reactor of any kind, let alone the gigantic super-advanced one needed for the VASIMR hyper drive, demonstrates that the program is being conducted on false premises.

The 2011 NASA research paper Multi-MW Closed Cycle MHD Nuclear Space Power Via Nonequilibrium He/Xe Working Plasma by Ron J. Litchford and Nobuhiro Harada, indicates that such developments are feasible in the near future.

Whether the VASIMR engine is viable or not, in 2015, NASA awarded Chang Diazs firm Ad Astra Rocket Company a three-year, $9 million contract. Up to now, the VASIMR engine has fired at fifty kilowatts for one minute still a long way from Chang Diazs goal of 200 megawatts.

In its current form, the VASIMR engine uses argon for fuel. The first stage of the rocket heats the argon to plasma and injects it into the booster. There, a radio frequency excites the ions in a process called ion cyclotron resonance heating. As they pick up energy, they are spun into a stream of superheated plasma and accelerated out the back of the rocket.

Video courtesy of Ad Astra Rocket Company

Tagged: Ad Astra Rocket Company Chang Diaz Journey to Mars The Range VASIMR

Collin R. Skocik has been captivated by space flight since the maiden flight of space shuttle Columbia in April of 1981. He frequently attends events hosted by the Astronaut Scholarship Foundation, and has met many astronauts in his experiences at Kennedy Space Center. He is a prolific author of science fiction as well as science and space-related articles. In addition to the Voyage Into the Unknown series, he has also written the short story collection The Future Lives!, the science fiction novel Dreams of the Stars, and the disaster novel The Sunburst Fire. His first print sale was Asteroid Eternia in Encounters magazine. When he is not writing, he provides closed-captioning for the hearing impaired. He lives in Atlantic Beach, Florida.

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