Daily Archives: October 25, 2016

Mars One – Wikipedia

Posted: October 25, 2016 at 7:35 am

This article is about the one-way manned trip to Mars proposed for 2026. For the first Soviet spacecraft for Mars, see Mars 1. For other uses, see Mars 1 (disambiguation).

Mars One is an organization based in the Netherlands that has proposed to land the first humans on Mars and establish a permanent human colony there by 2026.[1] The private spaceflight project is led by Dutch entrepreneur Bas Lansdorp, who announced the Mars One project in May 2012.[2] The project's schedule, technical and financial feasibility, and ethics, have been criticized by scientists, engineers and those in the aerospace industry.[3][4][5][6][7][8][9][10]

Mars One's original concept included launching a robotic lander and orbiter as early as 2016 to be followed by a human crew of four in 2022. Organizers plan for the crew to be selected from applicants who paid an administrative fee, to become the first permanent residents of Mars with no plan of returning to Earth. Partial funding options, which have yet to be realized, include a proposed reality television program documenting the journey. In February 2015, the primary contractors on the initial pre-Phase A contracts had completed all studies paid for by Mars One at that time.[11] The current state of the Mission Plan Deliverables (either in the form of Studies or actual Hardware) will be tracked in Table 2 in the Technology section.

The Mars One organization is the controlling stockholder of the for-profit Interplanetary Media Group.

The concept for Mars One began in 2011 with discussions between the two founders, Bas Lansdorp and Arno Wielders.[12]

The Mars One project has no connection with Inspiration Mars, a similarly-timed project to send a married couple on a Mars flyby and return them to Earth over a period of 500 days.[13]

Mars One publicly announced the concept in May 2012 for a one-way trip to Mars, with the intention of an initial robotic precursor mission in 2020 and transporting the first human colonists to Mars in 2024.[14] In a 2015 debate, Bas Lansdrop clarified that "were not going to do, I think, the current design of the mission" and "Mars One's goal is not to send humans to Mars in 2027 with a $6 billion budget and 14 launches. Our goal is to send humans to Mars, period."[15] According to Mars One's website, "It is Mars One's goal to establish a permanent human settlement on Mars."[16]

Notes:

In December 2013, Mars One announced its concept of a robotic precursor mission in 2018, two years later than had been conceptually planned in the 2012 announcements. The robotic lander would be "built by Lockheed Martin based on the design used for NASA's Phoenix and InSight missions, as well as a communications orbiter built by Surrey Satellite Technology Ltd."[26] In February 2015, Lockheed Martin and Surrey Satellite Technology confirmed that contracts on the initial study phase begun in late 2013 had run out and additional contracts had not been received for further progress on the robotic missions. Plans have been disclosed to raise the US$200 million or more needed to support the initial robotic mission,[11][26] but some critics do not find the economic plans to raise money from private investors and exclusive broadcasting rights to be sufficient to support the initial, or follow-on, mission(s).

Mars One selected a second-round pool of astronaut candidates in 2013 of 1058 people"586 men and 472 women from 107 countries"from a larger number of 202,586 who initially showed interest on the Mars One website, although this number is heavily disputed. Former Mars One candidate Dr. Joseph Roche claims the number of initial applicants was only 2,761,[27] which Mars One later conceded via YouTube video.[28]

Mars One announced a partnership with Uwingu on 3 March 2014, stating that the program would use Uwingu's map of Mars in all of their planned missions.[29][30]Kristian von Bengtson began work on Simulation Mars Home for crew on 24 March 2014.

The second-round pool was whittled down to 705 candidates (418 men and 287 women) in the beginning of May 2014. 353 were removed due to personal considerations.[31] After the medical physical requirement, which was similar to a normal FAA exam plus EKG, due either to financial, health or access reasons, only 660 candidates remained.[28] Notably, some applicants were notified of life-threatening conditions such as early-stage cancer and were able to immediately begin treatment.[32] These selected persons will then begin the interview process following which several teams of two men and two women will be compiled. The teams will then begin training full-time for a potential future mission to Mars, while individuals and teams may be selected out during training if they are not deemed suitable for the mission.[31]

On June 2, 2014, Darlow Smithson Productions (DSP) announced it has gained exclusive access to Mars One.[33]

On June 30, 2014, it was made public that Mars One seeks financial investment through a bidding process to send company experiments to Mars. The experiment slots will go to the highest bidder and will include company-related ads, and the opportunity to have the company name on the robotic lander that is proposed to carry the experiments to Mars in 2018.[34]

Mars One selected a third-round pool of astronaut candidates in 2015 of 100 people "50 men and 50 women who successfully passed the second round. The candidates come from all around the world, namely 39 from the Americas, 31 from Europe, 16 from Asia, 7 from Africa, and 7 from Oceania".

In a video posted on 19 of March 2015, Lansdorp said that because of delays in the robotic precursor mission, the first crew will not set down on Mars until 2027.[35] In August 2015, Lansdorp reiterated that their 12-year plan for landing humans on Mars by 2027 is subject to constant improvement and updates.[36]

The Space Review reported in October 2016 that while Mars One was "successful in generating a tremendous amount of publicity as well as enormous excitement about Mars, ... its proposal lacked substance both in mission architecture and in workable funding mechanisms. As such, it has faded from the public consciousness."[37]

According to their schedule as of March 2015, the first crew of four astronauts would arrive on Mars in 2027, after a seven-month journey from Earth. Additional teams would join the settlement every two years, with the intention that by 2035 there would be over twenty people living and working on Mars.[18] The astronaut selection process began on 22 April 2013.[38]

As of July 2015[update], the fourth round astronaut selection process, planned for Sept 2016, by which Mars One will choose six teams of four out of the 100 people selected in the third round, was announced.[39]

In December 2013, mission concept studies for an unmanned Mars mission were contracted with Lockheed Martin and Surrey Satellite Technology for a demonstration mission to be launched in 2017 and land on Mars in 2018. It would be based on the design of the successful 2007 NASA Phoenix lander,[40] and provide proof of concept for a subset of the key technologies for a later permanent human settlement on Mars.[41] Upon submission of Lockheed Martin's Proposal Information Package,[40] Mars One released a Request for Proposals[42] for the various payloads on the lander. The total payload mass of 44kg is divided among the seven payloads as follows:[42]

In 2022, an unmanned rover will be launched to Mars in order to pick a landing site for the 2027 Mars One landing and a site for the Mars One colony. At the same time, a communication satellite will be launched, enabling continuous communication with the Mars One colony.[43]

In 2024, the 6 cargo missions will be launched in close succession, consisting of two living units, two life-support units, and two supply units.[43]

A spacecraft containing four astronauts will be launched from Earth to meet a Transit vehicle bound for Mars.[43]

In 2027, the landing module will land on Mars, containing four astronauts. They will be met by the rover launched in 2020, and taken to the Mars One colony.[43]

The application was available from 22 April 2013 to 31 August 2013.[44][45] This first application consists of applicants general information, a motivational letter, a rsum and a video. More than 200,000 people expressed interest, so Mars One plans to hold several other application periods in the future.

By 9 September 2013, 4,227 applicants[46] had paid their registration fee and submitted public videos in which they made their case for going to Mars in 2023.[47] The application fee varies from US $5 to US $75 (the amount depending on the relative wealth of the applicant's country).[48]

Distribution of the 1,058 applicants selected for Round 2 according to the academic degree[49]

Other (37%)

The results of applicants selected for round 2 were declared on 30 December 2013. A total of 1,058 applicants from 107 countries were selected.[26] The gender split is 586 male (55.4%) and 472 female (44.6%). Among the people that were selected for round 2, 159 have a master's degree, 347 have bachelor's degrees and 29 have Doctor of Medicine (M.D.) degrees. The majority of the applicants are under 36 and well educated.[50][51][52]

Medically cleared candidates were interviewed, and 50 men and 50 women from the total pool of 660 from around the world were selected to move on to the third round of the astronaut selection process:[53][54]

Although initial plans were for the Mars One selection committee to perform regional interviews around the world, applicants were ultimately remotely interviewed and recorded by Mars One over a relatively short Skype/SparkHire call regarding Martian-related orbital, temp/pressure, geological and historical parameters and the specific elements of the Mars One one-way mission.[27][55][56] Dr. Joseph Roche, one of the finalists, has accused the selection process of being based on a point system that is primarily dependent on how much money each individual generated or gave to the Mars One organization, despite many of the round three selectees having not spent any money in the process, apart from the application fee, which varied as a function of each applicant's country GDP.[27][55][56] Lansdorp acknowledges a "gamification" point system but denies that selection is based on money earned.[56] Roche also stated that if paid for interviews, they are asked to donate 75% of the payment to Mars One.[27][56] This was confirmed by Lansdorp.[27][56]

It was originally planned that the pool of roughly one thousand successful applicants would be narrowed through regional contests. These events did not take place, and the above-mentioned group of 100 candidates were selected through the remote interview process and selected directly to round 3 in February 2015.

In late 2013, details of the 2015 selection phases had not been agreed upon due to ongoing negotiations with media companies for the rights to televise the selection processes.[57][needs update]

It was planned that the regional selection may be broadcast on TV and Internet in countries around the world. In each region, plans included 2040 applicants participating in challenges including rigorous simulations, many in team settings, with focus on testing the physical and emotional capabilities of the remaining candidates, with the aim of demonstrating their suitability to become the first humans on Mars. The audience was to select one winner per region, and the experts could select additional participants, if needed, to continue to the international level.[58][59][needs update]

Round three takes place in 2016[needs update], over the course of 5 days. At the start of the event, the candidates organize themselves into groups of 105 men and 5 women of diverse nationalities and age groups.

The Mars One selection committee then sets up group dynamic challenges and provide study materials related to each challenge. This allow them to observe how the candidates work in a group setting and choose candidates for elimination.[39][needs update]

At the end of each day all the teams except the winner lose members; then they reorganize themselves for the following day. At the end 40 candidates remain.

The remaining 40 candidates are spending nine days in an isolation unit. The candidates are observed closely to examine how they act in situations of prolonged close contact with one another. This test is implemented because, during the journey to Mars and upon arrival, the candidates will spend 24 hours a day with each other and during this time the simplest things may start to become bothersome. It takes a specific team dynamic to be able to handle this, and the goal of this selection round is to find those that are best suited for this challenge.

After the isolation round, 30 candidates are chosen to partake in a Mars Settler Suitability Interview.[39]

The Mars Settler Suitability Interview measures suitability for long duration Space missions and Mars settlement and will last approximately 4 hours. 24 candidates are selected after the interview and will be offered full-time employment with Mars One.[39]

From the previous selection series, six groups of four are to become full-time employees of the Mars One astronaut corps, after which they are to train for the mission. Whole teams and individuals might be deselected during training if they prove not to be suitable for the mission. Six to ten[citation needed] teams of four people are to be selected for seven years of full-time training.

Mars One funding comes from private investment (undisclosed), intellectual property (IP) rights, the sale of future broadcasting rights, and astronaut application fees.[48]

Mars One's investment of revenues[60]

Concept design studies (78.3%)

Travel expenses (11.6%)

Legal expenses (3.3%)

Website maintenance (2.4%)

Communications (2.3%)

Office and other (2.1%)

On January 29, 2013, Mars One announced its initial batch of investors[61] from the Netherlands and South Africa. The value of the investment remains undisclosed.

Mars One initially estimated a one-way trip, excluding the cost of maintaining four astronauts on Mars until they die, at 6 billion USD.[62] Lansdorp has declined questions regarding the cost estimate because he believes "it would be very stupid for us to give the prices that have been quoted per component".[63] For comparison, an "austere" manned Mars mission (including a temporary stay followed by a return of the astronauts) proposed by NASA in 2009 had a projected cost of $100 billion USD after an 18-year program, including a NASA-required return component.[64]

Mars One, the not-for-profit foundation, is the controlling stockholder of the for-profit Interplanetary Media Group.[65] A proposed global "reality-TV" media event was intended to provide funds to finance the expedition, however, no such reality TV show has emerged and no contracts have been signed. The astronaut selection process (with some public participation) was to be televised and continue on through the first years of living on Mars.[66][67]

Discussions between Endemol, producers of the Big Brother series, and Mars One ended with Endemol subsidiary Darlow Smithson Productions issuing a statement in February 2015 that they "were unable to reach agreement on the details of the contract" and that the company was "no longer involved in the project."[68] Lansdorp updated plans to no longer include live broadcasts from Mars but instead rely on a documentary-style production, adding "Just like the Olympics, we watch highlights, we don't watch things that athletes do when they're not performing their abilities."[69]

On 31 August 2012, company officials announced that funding from its first sponsors had been received.[62] Corporate sponsorship money will be used mostly to fund the conceptual design studies provided by the aerospace suppliers.[62]

Since the official announcement of their conversion to a Stichting, Mars One has been accepting one-time and regular monthly donations through their website. As of 4 July 2016, Mars One had received $928,888 in donations and merchandise sales.[70] The recent donation update adds the Indiegogo campaign ($313,744) to the private donation and merchandise total.

Over three quarters of the investment is in concept design studies. Mars One states that "income from donations and merchandise have not been used to pay salaries". To date, no financial records have been released for public viewing.[71]

On 10 December 2013, Mars One set up a crowdfunding campaign on Indiegogo to fund their 2018 demonstration mission. The 2018 mission includes a lander and communications satellite, and aims to prove several mission critical technologies in addition to launch and landing. The campaign goal was to raise $400,000 USD by 25 January 2014. Since the ending date was drawing near, they decided to extend the ending date to 9 February 2014. By the end of the campaign, they had received $313,744 in funds. Indiegogo will receive 9% ($28,237) of the $313,744 for the campaign failing to achieve its goal.[72]

Mars One has identified at least one potential supplier for each component of the mission.[73][74] The major components are planned to be acquired from proven suppliers.[75] As of May 2013[update], Mars One has a contract with only one company, Paragon Space Development Corporation, for a preliminary life support study.[76]

The Falcon Heavy from SpaceX was the notional launcher in the early Mars One conceptual plan,[75] which included the notional use of SpaceX hardware for the lander and crew habitat, but, as of May 2013, SpaceX had not yet been contracted to supply mission hardware, and SpaceX has stated that it did "not currently have a relationship with Mars One."[76] By March 2014, SpaceX indicated that they had been contacted by Mars One, and were in discussions, but that accommodating Mars One requirements would require some additional work and that such work was not a part of the current focus of SpaceX.[77][24]

A manned interplanetary spacecraft, which would transport the crew to Mars, would be assembled in low Earth orbit and comprise two propellant modules: a Transit Living Module (discarded just before arrival at Mars) and a lander (see "Human Lander" below).[75][78]

A potential supplier for the Transit living module as of November 2012[update] was Thales Alenia Space.[79][non-primary source needed]

Contract has been signed with Lockheed Martin to build the Demo Lander with the same designs as the Phoenix lander that went to Mars.[21]

In December 2013 Mars One awarded a contract to Surrey Satellite Technology for a study of the satellite technology required to provide 24/7 communication between Earth and the Mars base.[80][81] Mars One proposed at least two satellites, one in areostationary orbit above Mars and a second at the Earth Sun L4 or L5 point to relay the signal when Mars blocks the areosynchronous satellite from line of sight to Earth.[81] It is possible that a third satellite will be required to relay the signal on the rare occasions when the Sun blocks the first relay satellite from line of sight with Earth.[81]

An early notional Mars One lander was shown in concept art as a 5 meters (16ft)-diameter variant of SpaceX's Dragon capsule. SpaceX has not agreed for their technoogy to be used by the Mars One project.[24]

The rover would be unpressurized and support travel distances of 80km (50 miles).[82] A potential supplier for the rover as of November 2012[update] was Astrobotic Technology.[79][non-primary source needed]

The Mars suit would be flexible to allow the settlers to work with both cumbersome construction materials and sophisticated machinery when they are outside the habitat while protecting them from the cold, low pressure and noxious gases of the Martian atmosphere.[83] The likely supplier of the suits is ILC Dover.[84] On 12 March 2013, Paragon Space Development Corporation was contracted to develop concepts for life support and the Mars Surface Exploration Spacesuit System. The Paragon Space Development Corporation study was stated to be finished late summer 2013; Mars One released the results of this (ECLSS portion only) study to the public in June 2015.[85][86] The Mars suit study portion of the original contract has just entered ITAR review, with a publicly accessible copy available once passed through review.

Mars One has received a variety of criticism, mostly relating to medical,[87] technical and financial feasibility. There are also unverified claims that Mars One is a scam designed to take as much money as possible from donors, including reality show contestants.[88][89] Many have criticized the project's US$6 billion budget as being too low to successfully transport humans to Mars, to the point of being delusional.[10][90] A similar project study by NASA estimated the cost of such a feat at US$100 billion, although that included transporting the astronauts back to Earth. Objections have also been raised regarding the reality TV project associated with the expedition. Given the transient nature of most reality TV ventures, many believe that as viewership declines, funding could significantly decrease, thereby harming the entire expedition. Further, TV reality show contestants have reported that they were ranked based on their donations and funds raised.[88][91]

John Logsdon, a space policy expert at George Washington University, criticized the program, saying it appears to be a scam[90] and not "a credible proposition".[92]

Chris Welch, director of Masters Programs at the International Space University, has said "Even ignoring the potential mismatch between the project income and its costs and questions about its longer-term viability, the Mars One proposal does not demonstrate a sufficiently deep understanding of the problems to give real confidence that the project would be able to meet its very ambitious schedule."[93]

Gerard 't Hooft, theoretical physicist and ambassador[94] to Mars One, has stated that he thought both their proposed schedule and budget were off by a factor of ten.[27][95] He said he still supported the project's overall goals.[95]

A space logistics analysis conducted by PhD candidates at the Massachusetts Institute of Technology revealed that the most optimistic of scenarios would require 15 Falcon Heavy launches that would cost approximately $4.5 billion.[96] They concluded that the reliability of Environmental Control and Life Support systems (ECLS), the Technology Readiness Levels (TRL), and in situ resource utilization (ISRU) would have to be improved. Additionally, they determined that if the costs of launch were also lowered dramatically, together this would help to reduce the mass and cost of Mars settlement architecture.[96] The environmental system would result in failure to be able to support human life in 68 days if fire safety standards on over-oxygenation were followed, due to excessive use of nitrogen supplies that would not then be able to be used to compensate leakage of air out of the habitat, leading to a resultant loss in pressurization, ending with pressures too low to support human life.[97] Lansdorp replied that although he has not read all the research, supplier Lockheed Martin says that the technologies were viable.[98]

Another serious concern uncovered in the research conducted by MIT is replacement parts. The PhD candidates estimated the need for spare parts in a Mars colony based on the failure rates of parts on the ISS. They determined that a resupply mission every two years would be necessary unless a large space in the initial launch were to be reserved for extra materials. Lansdorp commented on this saying, "They are correct. The major challenge of Mars One is keeping everything up and running. We don't believe what we have designed is the best solution. It's a good solution."[98]

In March 2015, one of the Mars One finalists, Joseph Roche,[99] stated to media outlets that he believes the mission to be a scam. Roche holds doctorate degrees in physics and astrophysics, and shared many of his concerns and criticisms of the mission. These claims include that the organization lied about the number of applicants, stating that 200,000 individuals applied versus Roche's claim of 2,761, and that many of the applicants had paid to be put on the list. Furthermore, Roche claimed that Mars One is asking finalists for donations from any money earned from guest appearances (which would amount to a minimal portion of the estimated $6 billion required for the mission). Finally, despite being one of 100 finalists, Roche himself has never spoken to any Mars One employee or representative in person, and instead of psychological or psychometric testing as is normal for astronaut candidates (especially for a lengthy, one-way mission), his interview process consisted of a 10-minute Skype conversation.[88][100]

Robert Zubrin, advocate for manned Martian exploration, said "I don't think the business plan closes it. We're going to go to Mars, we need a billion dollars, and we're going to make up the revenue with advertising and media rights and so on. You might be able to make up some of the money that way, but I don't think that anyone who is interested in making money is going to invest on that basis invest in this really risky proposition, and if you're lucky you'll break even? That doesn't fly."[101] Despite his criticisms, Zubrin became an adviser to Mars One on 10 October 2013.[102]

Canadian former astronaut Julie Payette said during the opening speech for an International Civil Aviation Organization conference that she does not think Mars One "is sending anybody anywhere".[56]

In January 2014, German former astronaut Ulrich Walter strongly criticized the project for ethical reasons. Speaking with Tagesspiegel, he estimated the probability of reaching Mars alive at only 30%, and that of surviving there more than three months at less than 20%. He said, "They make their money with that [TV] show. They don't care what happens to those people in space... If my tax money were used for such a mission, I would organize a protest."[103]

Space tourist Richard Garriott stated in response to Mars One, "Many have interesting viable starting plans. Few raise the money to be able to pull it off."[104]

Former astronaut Buzz Aldrin said in an interview that he wants to see humans on Mars by 2035, but he does not think Mars One will be the first to achieve it.[105]

Wired magazine gave it a plausibility score of 2 out of 10 as part of their 2012 Most Audacious Private Space Exploration Plans.[106]

The Daily Mail enumerated reasons why the project will never happen, calling the project "foolish". The project lacks current funding as well as sources for future funding. The organization has no spacecraft or rocket in development or any contracts in place with companies that could provide a spacecraft or rocket. While plans point to SpaceX for both resources, the company has no contracts with Mars One in an industry that typically plans contracts decades in advance.[24] The organization has not shared any research into the effects of microgravity on crews in flight or reduced gravity on the Mars surface. The organization has yet to provide plans or even study how crews might survive dust storms, supply challenges or the increased radiation on Mars.[107]

Read the original here:
Mars One - Wikipedia

Posted in Mars Colonization | Comments Off on Mars One – Wikipedia

Colonization of the Moon – Wikipedia

Posted: at 7:34 am

"Lunar outpost" redirects here. For NASA's former plan to construct an outpost between 2019 and 2024, see Lunar outpost (NASA).

The colonization of the Moon is the proposed establishment of permanent human communities or robotic industries[1][2] on the Moon.

Recent indication that water might be present in noteworthy quantities at the lunar poles has renewed interest in the Moon. Polar colonies could also avoid the problem of long lunar nights about 354 hours,[3] a little more than two weeks and take advantage of the Sun continuously, at least during the local summer (there is no data for the winter yet).[4]

Permanent human habitation on a planetary body other than the Earth is one of science fiction's most prevalent themes. As technology has advanced, and concerns about the future of humanity on Earth have increased, the argument that space colonization is an achievable and worthwhile goal has gained momentum.[5][6] Because of its proximity to Earth, the Moon has been seen as the most obvious natural expansion after Earth. There are also various projects in near future by space tourism startup companies for tourism on the Moon.

The notion of a lunar colony originated before the Space Age. In 1638 Bishop John Wilkins wrote ADiscourse Concerning a New World and Another Planet, in which he predicted a human colony on the Moon.[7]Konstantin Tsiolkovsky (18571935), among others, also suggested such a step.[8] From the 1950s onwards, a number of concepts and designs have been suggested by scientists, engineers and others.

In 1954, science-fiction writer Arthur C. Clarke proposed a lunar base of inflatable modules covered in lunar dust for insulation.[9] A spaceship, assembled in low Earth orbit, would launch to the Moon, and astronauts would set up the igloo-like modules and an inflatable radio mast. Subsequent steps would include the establishment of a larger, permanent dome; an algae-based air purifier; a nuclear reactor for the provision of power; and electromagnetic cannons to launch cargo and fuel to interplanetary vessels in space.

In 1959, John S. Rinehart suggested that the safest design would be a structure that could "[float] in a stationary ocean of dust", since there were, at the time this concept was outlined, theories that there could be mile-deep dust oceans on the Moon.[10] The proposed design consisted of a half-cylinder with half-domes at both ends, with a micrometeoroid shield placed above the base.

Project Horizon was a 1959 study regarding the United States Army's plan to establish a fort on the Moon by 1967.[11]Heinz-Hermann Koelle, a German rocket engineer of the Army Ballistic Missile Agency (ABMA) led the Project Horizon study. The first landing would be carried out by two "soldier-astronauts" in 1965 and more construction workers would soon follow. Through numerous launches (61Saturn I and 88Saturn II), 245tons of cargo would be transported to the outpost by 1966.

Lunex Project was a US Air Force plan for a manned lunar landing prior to the Apollo Program in 1961. It envisaged a 21-airman underground Air Force base on the Moon by 1968 at a total cost of $7.5 billion.

In 1962, John DeNike and Stanley Zahn published their idea of a sub-surface base located at the Sea of Tranquility.[9] This base would house a crew of21, in modules placed four meters below the surface, which was believed to provide radiation shielding on par with Earth's atmosphere. DeNike and Zahn favored nuclear reactors for energy production, because they were more efficient than solar panels, and would also overcome the problems with the long Lunar nights. For the life support system, an algae-based gas exchanger was proposed.

As of 2006, Japan planned to have a Moon base in 2030.[12] and as of 2007, Russia planned to have a Moon base in 202732.[13]

In 2007 Jim Burke of the International Space University in France said people should plan to preserve humanity's culture in the event of a civilization-stopping asteroid impact with Earth. A Lunar Noah's Ark was proposed.[14] Subsequent planning may be taken up by the International Lunar Exploration Working Group (ILEWG).[15][16][17]

In a January 2012 speech Newt Gingrich, Republican candidate for President of the United States of America, proposed a plan to build a U.S. moon colony by the year 2020.[18][19]

In 2016 Johann-Dietrich Wrner, the new Chief of ESA, proposed the International Moon Village that incorporates 3D printing.[20]

Exploration of the Lunar surface by spacecraft began in 1959 with the Soviet Union's Luna program. Luna1 missed the Moon, but Luna2 made a hard landing (impact) into its surface, and became the first artificial object on an extraterrestrial body. The same year, the Luna3 mission radioed photographs to Earth of the Moon's hitherto unseen far side, marking the beginning of a decade-long series of unmanned Lunar explorations.

Responding to the Soviet program of space exploration, US President JohnF. Kennedy in 1961 told the U.S.Congress on May25: "Ibelieve that this nation should commit itself to achieving the goal, before this decade is out, of landing a man on the Moon and returning him safely to the Earth." The same year the Soviet leadership made some of its first public pronouncements about landing a man on the Moon and establishing a Lunar base.

Manned exploration of the lunar surface began in 1968 when the Apollo8 spacecraft orbited the Moon with three astronauts on board. This was mankind's first direct view of the far side. The following year, the Apollo11 Lunar module landed two astronauts on the Moon, proving the ability of humans to travel to the Moon, perform scientific research work there, and bring back sample materials.

Additional missions to the Moon continued this exploration phase. In 1969 the Apollo12 mission landed next to the Surveyor3 spacecraft, demonstrating precision landing capability. The use of a manned vehicle on the Moon's surface was demonstrated in 1971 with the Lunar Rover during Apollo15. Apollo16 made the first landing within the rugged Lunar highlands. However, interest in further exploration of the Moon was beginning to wane among the American public. In 1972 Apollo17 was the final Apollo Lunar mission, and further planned missions were scrapped at the directive of President Nixon. Instead, focus was turned to the Space Shuttle and manned missions in near Earth orbit.

The Soviet manned lunar programs failed to send a manned mission to the Moon. However, in 1966 Luna9 was the first probe to achieve a soft landing and return close-up shots of the Lunar surface. Luna16 in 1970 returned the first Soviet Lunar soil samples, while in 1970 and 1973 during the Lunokhod program two robotic rovers landed on the Moon. Lunokhod1 explored the Lunar surface for 322 days, and Lunokhod2 operated on the Moon about four months only but covered a third more distance. 1974 saw the end of the Soviet Moonshot, two years after the last American manned landing. Besides the manned landings, an abandoned Soviet moon program included building the moonbase "Zvezda", which was the first detailed project with developed mockups of expedition vehicles[21] and surface modules.[22]

In the decades following, interest in exploring the Moon faded considerably, and only a few dedicated enthusiasts supported a return. However, evidence of Lunar ice at the poles gathered by NASA's Clementine (1994) and Lunar Prospector (1998) missions rekindled some discussion,[23][24] as did the potential growth of a Chinese space program that contemplated its own mission to the Moon.[25] Subsequent research suggested that there was far less ice present (if any) than had originally been thought, but that there may still be some usable deposits of hydrogen in other forms.[26] However, in September 2009, the Chandrayaan probe of India, carrying an ISRO instrument, discovered that the Lunar regolith contains 0.1% water by weight, overturning theories that had stood for 40 years.[27]

In 2004, U.S. President George W. Bush called for a plan to return manned missions to the Moon by 2020 (since cancelled see Constellation program). Propelled by this new initiative, NASA issued a new long-range plan that includes building a base on the Moon as a staging point to Mars. This plan envisions a Lunar outpost at one of the Moon's poles by 2024 which, if well-sited, might be able to continually harness solar power; at the poles, temperature changes over the course of a Lunar day are also less extreme,[28] and reserves of water and useful minerals may be found nearby.[28] In addition, the European Space Agency has a plan for a permanently manned Lunar base by 2025.[29][30] Russia has also announced similar plans to send a man to the Moon by 2025 and establish a permanent base there several years later.[6]

A Chinese space scientist has said that the People's Republic of China could be capable of landing a human on the Moon by 2022 (see Chinese Lunar Exploration Program),[31] and Japan and India also have plans for a Lunar base by 2030.[32] Neither of these plans involves permanent residents on the Moon. Instead they call for sortie missions, in some cases followed by extended expeditions to the Lunar base by rotating crew members, as is currently done for the International Space Station.

NASAs LCROSS/LRO mission had been scheduled to launch in October 2008.[33] The launch was delayed until 18 June 2009,[34] resulting in LCROSS's impact with the Moon at 11:30 UT on 9 October 2009.[35][36] The purpose is preparing for future Lunar exploration.

On September 24, 2009 NASA announced the discovery of water on the Moon. The discovery was made by three instruments on board Chandrayaan-1. These were the ISRO's Moon Impact Probe (MIP), the Moon Mineralogy Mapper (M3) and Mini-Sar, belonging to NASA.[37]

On November 13, 2009 NASA announced that the LCROSS mission had discovered large quantities of water ice on the Moon around the LCROSS impact site at Cabeus. Robert Zubrin, president of the Mars Society, relativized the term 'large': "The 30m crater ejected by the probe contained 10million kilograms of regolith. Within this ejecta, an estimated 100kg of water was detected. That represents a proportion of ten parts per million, which is a lower water concentration than that found in the soil of the driest deserts of the Earth. In contrast, we have found continent sized regions on Mars, which are 600,000 parts per million, or 60% water by weight."[38] Although the Moon is very dry on the whole, the spot where the LCROSS impactor hit was chosen for a high concentration of water ice. Dr. Zubrin's computations are not a sound basis for estimating the percentage of water in the regolith at that site. Researchers with expertise in that area estimated that the regolith at the impact site contained 5.6 2.9% water ice, and also noted the presence of other volatile substances. Hydrocarbons, material containing sulfur, carbon dioxide, carbon monoxide, methane and ammonia were present.[39]

In March 2010, NASA reported that the findings of its mini-SAR radar aboard Chandrayaan-1 were consistent with ice deposits at the Moon's north pole. It is estimated there is at least 600million tons of ice at the north pole in sheets of relatively pure ice at least a couple of meters thick.[40]

In March 2014, researchers who had previously published reports on possible abundance of water on the Moon, reported new findings that refined their predictions substantially lower.[41]

Placing a colony on a natural body would provide an ample source of material for construction and other uses in space, including shielding from cosmic radiation. The energy required to send objects from the Moon to space is much less than from Earth to space. This could allow the Moon to serve as a source of construction materials within cis-lunar space. Rockets launched from the Moon would require less locally produced propellant than rockets launched from Earth. Some proposals include using electric acceleration devices (mass drivers) to propel objects off the Moon without building rockets. Others have proposed momentum exchange tethers (see below). Furthermore, the Moon does have some gravity, which experience to date indicates may be vital for fetal development and long-term human health.[42][43] Whether the Moon's gravity (roughly one sixth of Earth's) is adequate for this purpose, however, is uncertain.

In addition, the Moon is the closest large body in the Solar System to Earth. While some Earth-crosser asteroids occasionally pass closer, the Moon's distance is consistently within a small range close to 384,400km. This proximity has several advantages:

There are several disadvantages to the Moon as a colony site:

Three criteria that a Lunar outpost should meet are:[citation needed]

While a colony might be located anywhere, potential locations for a Lunar colony fall into three broad categories.

There are two reasons why the north pole and south pole of the Moon might be attractive locations for a human colony. First, there is evidence that water may be present in some continuously shaded areas near the poles.[62] Second, the Moon's axis of rotation is sufficiently close to being perpendicular to the ecliptic plane that the radius of the Moon's polar circles is less than 50km. Power collection stations could therefore be plausibly located so that at least one is exposed to sunlight at all times, thus making it possible to power polar colonies almost exclusively with solar energy. Solar power would be unavailable only during a lunar eclipse, but these events are relatively brief and absolutely predictable. Any such colony would therefore require a reserve energy supply that could temporarily sustain a colony during lunar eclipses or in the event of any incident or malfunction affecting solar power collection. Hydrogen fuel cells would be ideal for this purpose, since the hydrogen needed could be sourced locally using the Moon's polar water and surplus solar power. Moreover, due to the Moon's uneven surface some sites have nearly continuous sunlight. For example, Malapert mountain, located near the Shackleton crater at the Lunar south pole, offers several advantages as a site:

NASA chose to use a south-polar site for the Lunar outpost reference design in the Exploration Systems Architecture Study chapter on Lunar Architecture.[64]

At the north pole, the rim of Peary Crater has been proposed as a favorable location for a base.[65] Examination of images from the Clementine mission appear to show that parts of the crater rim are permanently illuminated by sunlight (except during Lunar eclipses).[65] As a result, the temperature conditions are expected to remain very stable at this location, averaging 50C (58F).[65] This is comparable to winter conditions in Earth's Poles of Cold in Siberia and Antarctica. The interior of Peary Crater may also harbor hydrogen deposits.[65]

A 1994[66] bistatic radar experiment performed during the Clementine mission suggested the presence of water ice around the south pole.[23][67] The Lunar Prospector spacecraft reported enhanced hydrogen abundances at the south pole and even more at the north pole, in 2008.[68] On the other hand, results reported using the Arecibo radio telescope have been interpreted by some to indicate that the anomalous Clementine radar signatures are not indicative of ice, but surface roughness.[69] This interpretation, however, is not universally agreed upon.[70]

A potential limitation of the polar regions is that the inflow of solar wind can create an electrical charge on the leeward side of crater rims. The resulting voltage difference can affect electrical equipment, change surface chemistry, erode surfaces and levitate Lunar dust.[71]

The Lunar equatorial regions are likely to have higher concentrations of helium-3 (rare on Earth but much sought after for use in nuclear fusion research) because the solar wind has a higher angle of incidence.[72] They also enjoy an advantage in extra-Lunar traffic: The rotation advantage for launching material is slight due to the Moon's slow rotation, but the corresponding orbit coincides with the ecliptic, nearly coincides with the Lunar orbit around Earth, and nearly coincides with the equatorial plane of Earth.

Several probes have landed in the Oceanus Procellarum area. There are many areas and features that could be subject to long-term study, such as the Reiner Gamma anomaly and the dark-floored Grimaldi crater.

The Lunar far side lacks direct communication with Earth, though a communication satellite at the L2 Lagrangian point, or a network of orbiting satellites, could enable communication between the far side of the Moon and Earth.[73] The far side is also a good location for a large radio telescope because it is well shielded from the Earth.[74] Due to the lack of atmosphere, the location is also suitable for an array of optical telescopes, similar to the Very Large Telescope in Chile.[44] To date, there has been no ground exploration of the far side.

Scientists have estimated that the highest concentrations of helium-3 will be found in the maria on the far side, as well as near side areas containing concentrations of the titanium-based mineral ilmenite. On the near side the Earth and its magnetic field partially shields the surface from the solar wind during each orbit. But the far side is fully exposed, and thus should receive a somewhat greater proportion of the ion stream.[75]

Lunar lava tubes are a potential location for constructing a Lunar base. Any intact lava tube on the Moon could serve as a shelter from the severe environment of the Lunar surface, with its frequent meteorite impacts, high-energy ultra-violet radiation and energetic particles, and extreme diurnal temperature variations. Lava tubes provide ideal positions for shelter because of their access to nearby resources. They also have proven themselves as a reliable structure, having withstood the test of time for billions of years.

An underground colony would escape the extreme of temperature on the Moon's surface. The average temperature on the surface of the Moon is about 5C. The day period (about 354 hours) has an average temperature of about 107C (225F), although it can rise as high as 123C (253F). The night period (also 354 hours) has an average temperature of about 153C (243F).[76] Underground, both periods would be around 23C (9F), and humans could install ordinary heaters.[77]

One such lava tube was discovered in early 2009.[78]

The central peaks of large lunar craters may contain material that rose from as far 19 kilometers beneath the surface when the peaks formed by rebound of the compressed rock under the crater. Material moved from the interior of craters is piled in their rims.[79] These and other processes make possibly novel concentrations of minerals accessible to future prospectors from lunar colonies.

A colony in lunar orbit would avoid the extreme temperature swings of the Moon's surface. Since the orbital period in low-lunar orbit is only about two hours, heat would only radiate away from the colony for a short period of time. At the Lagrangian points one and two, the thermal environment would be even more stable as the Sun would be almost continuously visible. This increased solar duration would allow for an almost constant supply of power. Additionally, the colony could be made to spin as has been examined with designs similar to the O'Neill cylinder so as to provide Earth-like gravity. Various lunar orbits are possible such as a Lissajous orbit or a halo orbit. Due to the Moon's lumpy gravity, there exist only a small number of possible orbital inclinations for low lunar orbits. A satellite in such a frozen orbit could be at an inclination of 27, 50, 76, or 86.

There have been numerous proposals regarding habitat modules. The designs have evolved throughout the years as mankind's knowledge about the Moon has grown, and as the technological possibilities have changed. The proposed habitats range from the actual spacecraft landers or their used fuel tanks, to inflatable modules of various shapes. Some hazards of the Lunar environment such as sharp temperature shifts, lack of atmosphere or magnetic field (which means higher levels of radiation and micrometeoroids) and long nights, were unknown early on. Proposals have shifted as these hazards were recognized and taken into consideration.

Some suggest building the Lunar colony underground, which would give protection from radiation and micrometeoroids. This would also greatly reduce the risk of air leakage, as the colony would be fully sealed from the outside except for a few exits to the surface.

The construction of an underground base would probably be more complex; one of the first machines from Earth might be a remote-controlled excavating machine. Once created, some sort of hardening would be necessary to avoid collapse, possibly a spray-on concrete-like substance made from available materials.[80] A more porous insulating material also made in-situ could then be applied. Rowley & Neudecker have suggested "melt-as-you-go" machines that would leave glassy internal surfaces.[81]Mining methods such as the room and pillar might also be used. Inflatable self-sealing fabric habitats might then be put in place to retain air. Eventually an underground city can be constructed. Farms set up underground would need artificial sunlight. As an alternative to excavating, a lava tube could be covered and insulated, thus solving the problem of radiation exposure.

A possibly easier solution would be to build the Lunar base on the surface, and cover the modules with Lunar soil. The Lunar regolith is composed of a unique blend of silica and iron-containing compounds that may be fused into a glass-like solid using microwave energy.[82] Blacic has studied the mechanical properties of lunar glass and has shown that it is a promising material for making rigid structures, if coated with metal to keep moisture out.[83] This may allow for the use of "Lunar bricks" in structural designs, or the vitrification of loose dirt to form a hard, ceramic crust.

A Lunar base built on the surface would need to be protected by improved radiation and micrometeoroid shielding. Building the Lunar base inside a deep crater would provide at least partial shielding against radiation and micrometeoroids. Artificial magnetic fields have been proposed[84][85] as a means to provide radiation shielding for long range deep space manned missions, and it might be possible to use similar technology on a Lunar colony. Some regions on the Moon possess strong local magnetic fields that might partially mitigate exposure to charged solar and galactic particles.[86]

In a turn from the usual engineer-designed lunar habitats, London-based Foster + Partners architectural firm proposed a building construction 3D-printer technology in January 2013 that would use Lunar regolith raw materials to produce Lunar building structures while using enclosed inflatable habitats for housing the human occupants inside the hard-shell Lunar structures. Overall, these habitats would require only ten percent of the structure mass to be transported from Earth, while using local Lunar materials for the other 90 percent of the structure mass.[87] "Printed" Lunar soil will provide both "radiation and temperature insulation. Inside, a lightweight pressurized inflatable with the same dome shape will be the living environment for the first human Moon settlers."[87] The building technology will include mixing Lunar material with magnesium oxide, which will turn the "moonstuff into a pulp that can be sprayed to form the block" when a binding salt is applied that "converts [this] material into a stone-like solid."[87] Terrestrial versions of this 3D-printing building technology are already printing 2 metres (6ft 7in) of building material per hour with the next-generation printers capable of 3.5 metres (11ft) per hour, sufficient to complete a building in a week.[87]

In 2010, The Moon Capital Competition offered a prize for a design of a Lunar habitat intended to be an underground international commercial center capable of supporting a residential staff of 60 people and their families. The Moon Capital is intended to be self-sufficient with respect to food and other material required for life support. Prize money was provided primarily by the Boston Society of Architects, Google Lunar X Prize and The New England Council of the American Institute of Aeronautics and Astronautics.[88]

On January 31, 2013, the ESA working with an independent architectural firm, tested a 3D-printed structure that could be constructed of lunar regolith for use as a Moon base.[89]

A nuclear fission reactor might fulfill most of a Moon base's power requirements.[90] With the help of fission reactors, one could overcome the difficulty of the 354 hour Lunar night. According to NASA, a nuclear fission power station could generate a steady 40kilowatts, equivalent to the demand of about eight houses on Earth.[90] An artists concept of such a station published by NASA envisages the reactor being buried below the Moon's surface to shield it from its surroundings; out from a tower-like generator part reaching above the surface over the reactor, radiators would extend into space to send away any heat energy that may be left over.[91]

Radioisotope thermoelectric generators could be used as backup and emergency power sources for solar powered colonies.

One specific development program in the 2000s was the Fission Surface Power (FSP) project of NASA and DOE, a fission power system focused on "developing and demonstrating a nominal 40 kWe power system to support human exploration missions. The FSP system concept uses conventional low-temperature stainless steel, liquid metal-cooled reactor technology coupled with Stirling power conversion." As of 2010[update], significant component hardware testing had been successfully completed, and a non-nuclear system demonstration test was being fabricated.[92][needs update]

Solar energy is a possible source of power for a Lunar base. Many of the raw materials needed for solar panel production can be extracted on site. However, the long Lunar night (354 hours) is a drawback for solar power on the Moon's surface. This might be solved by building several power plants, so that at least one of them is always in daylight. Another possibility would be to build such a power plant where there is constant or near-constant sunlight, such as at the Malapert mountain near the Lunar south pole, or on the rim of Peary crater near the north pole. A third possibility would be to leave the panels in orbit, and beam the power down as microwaves.

The solar energy converters need not be silicon solar panels. It may be more advantageous to use the larger temperature difference between Sun and shade to run heat engine generators. Concentrated sunlight could also be relayed via mirrors and used in Stirling engines or solar trough generators, or it could be used directly for lighting, agriculture and process heat. The focused heat might also be employed in materials processing to extract various elements from Lunar surface materials.

In the early days,[clarification needed] a combination of solar panels for "day-time" operation and fuel cells for "night-time" operation could be used.[according to whom?]

Fuel cells on the Space Shuttle have operated reliably for up to 17 Earth days at a time. On the Moon, they would only be needed for 354 hours (14 34 days) the length of the Lunar night. Fuel cells produce water directly as a waste product. Current fuel cell technology is more advanced than the Shuttle's cells PEM (Proton Exchange Membrane) cells produce considerably less heat (though their waste heat would likely be useful during the Lunar night) and are lighter, not to mention the reduced mass of the smaller heat-dissipating radiators. This makes PEMs more economical to launch from Earth than the shuttle's cells. PEMs have not yet been proven in space.

Combining fuel cells with electrolysis would provide a "perpetual" source of electricity solar energy could be used to provide power during the Lunar day, and fuel cells at night. During the Lunar day, solar energy would also be used to electrolyze the water created in the fuel cells although there would be small losses of gases that would have to be replaced.

Even if lunar colonies could provide themselves access to a near-continuous source of solar energy, they would still need to maintain fuel cells or an alternate energy storage system to sustain themselves during lunar eclipses and emergency situations.

Conventional rockets have been used for most Lunar explorations to date. The ESA's SMART-1 mission from 2003 to 2006 used conventional chemical rockets to reach orbit and Hall effect thrusters to arrive at the Moon in 13 months. NASA would have used chemical rockets on its AresV booster and Lunar Surface Access Module, that were being developed for a planned return to the Moon around 2019, but this was cancelled. The construction workers, location finders, and other astronauts vital to building, would have been taken four at a time in NASA's Orion spacecraft.

Proposed concepts of Earth-Moon transportation are Space elevators.[93][94]

Lunar colonists will want the ability to transport cargo and people to and from modules and spacecraft, and to carry out scientific study of a larger area of the Lunar surface for long periods of time. Proposed concepts include a variety of vehicle designs, from small open rovers to large pressurized modules with lab equipment, and also a few flying or hopping vehicles.

Rovers could be useful if the terrain is not too steep or hilly. The only rovers to have operated on the surface of the Moon (as of 2008[update]) are the three Apollo Lunar Roving Vehicles (LRV), developed by Boeing, and the two robotic Soviet Lunokhods. The LRV was an open rover for a crew of two, and a range of 92km during one Lunar day. One NASA study resulted in the Mobile Lunar Laboratory concept, a manned pressurized rover for a crew of two, with a range of 396km. The Soviet Union developed different rover concepts in the Lunokhod series and the L5 for possible use on future manned missions to the Moon or Mars. These rover designs were all pressurized for longer sorties.[95]

If multiple bases were established on the Lunar surface, they could be linked together by permanent railway systems. Both conventional and magnetic levitation (Maglev) systems have been proposed for the transport lines. Mag-Lev systems are particularly attractive as there is no atmosphere on the surface to slow down the train, so the vehicles could achieve velocities comparable to aircraft on the Earth. One significant difference with lunar trains, however, is that the cars would need to be individually sealed and possess their own life support systems.

For difficult areas, a flying vehicle may be more suitable. Bell Aerosystems proposed their design for the Lunar Flying Vehicle as part of a study for NASA. Bell also developed the Manned Flying System, a similar concept.

Experience so far indicates that launching human beings into space is much more expensive than launching cargo.

One way to get materials and products from the Moon to an interplanetary way station might be with a mass driver, a magnetically accelerated projectile launcher. Cargo would be picked up from orbit or an Earth-Moon Lagrangian point by a shuttle craft using ion propulsion, solar sails or other means and delivered to Earth orbit or other destinations such as near-Earth asteroids, Mars or other planets, perhaps using the Interplanetary Transport Network.

A Lunar space elevator could transport people, raw materials and products to and from an orbital station at Lagrangian points L1 or L2. Chemical rockets would take a payload from Earth to the L1 Lunar Lagrange location. From there a tether would slowly lower the payload to a soft landing on the lunar surface.

Other possibilities include a momentum exchange tether system.

A cis-Lunar transport system has been proposed using tethers to achieve momentum exchange.[102] This system requires zero net energy input, and could not only retrieve payloads from the Lunar surface and transport them to Earth, but could also soft land payloads on to the Lunar surface.

For long term sustainability, a space colony should be close to self-sufficient. Mining and refining the Moon's materials on-site for use both on the Moon and elsewhere in the Solar System could provide an advantage over deliveries from Earth, as they can be launched into space at a much lower energy cost than from Earth. It is possible that large amounts of matter will need to be launched into space for interplanetary exploration in the 21st century, and the lower cost of providing goods from the Moon might be attractive.[80]

In the long term, the Moon will likely play an important role in supplying space-based construction facilities with raw materials.[95] Zero gravity in space allows for the processing of materials in ways impossible or difficult on Earth, such as "foaming" metals, where a gas is injected into a molten metal, and then the metal is annealed slowly. On Earth, the gas bubbles rise and burst, but in a zero gravity environment, that does not happen. The annealing process requires large amounts of energy, as a material is kept very hot for an extended period of time. (This allows the molecular structure to realign.)

Exporting material to Earth in trade from the Moon is more problematic due to the cost of transportation, which will vary greatly if the Moon is industrially developed (see "Launch costs" above). One suggested trade commodity, Helium-3 (3He) from the solar wind, is thought to have accumulated on the Moon's surface over billions of years, but occurs only rarely on Earth. Helium might be present in the Lunar regolith in quantities of 0.01 ppm to 0.05 ppm (depending on soil). In 2006 3He had a market price of about $1500 per gram ($1.5M per kilogram), more than 120 times the value per unit weight of gold and over eight times the value of rhodium.

In the future 3He may have a role as a fuel in thermonuclear fusion reactors.[103] If the technology for converting helium-3 to energy is developed, there is the potential that it would produce 10 times more electricity than fossil fuels. It should require about 100 tonnes of helium-3 to produce the electricity that Earth uses in a year and there should be enough on the moon to provide that much for 10,000 years.[104]

To reduce the cost of transport, the Moon could store propellants produced from lunar water at one or several depots between the Earth and the Moon, to resupply rockets or satellites in Earth orbit.[105] The Shackleton Energy Company estimate investment in this infrastructure could cost around $25 billion.[106]

Gerard K. O'Neill, noting the problem of high launch costs in the early 1970s, came up with the idea of building Solar Power Satellites in orbit with materials from the Moon.[107] Launch costs from the Moon will vary greatly if the Moon is industrially developed (see "Launch costs" above). This proposal was based on the contemporary estimates of future launch costs of the space shuttle.

On 30 April 1979 the Final Report "Lunar Resources Utilization for Space Construction" by General Dynamics Convair Division under NASA contract NAS9-15560 concluded that use of Lunar resources would be cheaper than terrestrial materials for a system comprising as few as thirty Solar Power Satellites of 10 GW capacity each.[108]

In 1980, when it became obvious NASA's launch cost estimates for the space shuttle were grossly optimistic, O'Neill et al. published another route to manufacturing using Lunar materials with much lower startup costs.[109] This 1980s SPS concept relied less on human presence in space and more on partially self-replicating systems on the Lunar surface under telepresence control of workers stationed on Earth.

Notes

General references

Excerpt from:
Colonization of the Moon - Wikipedia

Posted in Moon Colonization | Comments Off on Colonization of the Moon – Wikipedia

Colonization of Titan – Wikipedia

Posted: at 7:34 am

Saturns largest moon Titan is one of several candidates for possible future colonization of the outer Solar System.

According to Cassini data from 2008, Titan has hundreds of times more liquid hydrocarbons than all the known oil and natural gas reserves on Earth. These hydrocarbons rain from the sky and collect in vast deposits that form lakes and dunes.[1] "Titan is just covered in carbon-bearing materialit's a giant factory of organic chemicals", said Ralph Lorenz, who leads the study of Titan based on radar data from Cassini. "This vast carbon inventory is an important window into the geology and climate history of Titan." Several hundred lakes and seas have been observed, with several dozen estimated to contain more hydrocarbon liquid than Earth's oil and gas reserves. The dark dunes that run along the equator contain a volume of organics several hundred times larger than Earth's coal reserves.[2]

Radar images obtained on July 21, 2006 appear to show lakes of liquid hydrocarbon (such as methane and ethane) in Titan's northern latitudes. This is the first discovery of currently existing lakes beyond Earth.[3] The lakes range in size from about a kilometer in width to one hundred kilometers across.

On March 13, 2007, Jet Propulsion Laboratory announced that it found strong evidence of seas of methane and ethane in the northern hemisphere. At least one of these is larger than any of the Great Lakes in North America.[4]

The American aerospace engineer and author Robert Zubrin identified Saturn as the most important and valuable of the four gas giants in the Solar System, because of its relative proximity, low radiation, and excellent system of moons. He also named Titan as the most important moon on which to establish a base to develop the resources of the Saturn system.[5]

Dr. Robert Zubrin has pointed out that Titan possesses an abundance of all the elements necessary to support life, saying "In certain ways, Titan is the most hospitable extraterrestrial world within our solar system for human colonization." [6] The atmosphere contains plentiful nitrogen and methane, and strong evidence indicates that liquid methane exists on the surface. Evidence also indicates the presence of liquid water and ammonia under the surface, which are delivered to the surface by volcanic activity. Water can easily be used to generate breathable oxygen and nitrogen is ideal to add buffer gas partial pressure to breathable air (it forms about 78% of Earth's atmosphere).[7] Nitrogen, methane and ammonia can all be used to produce fertilizer for growing food.

Titan has a surface gravity of 0.138 g, slightly less than that of the Moon. Managing long-term effects of low gravity on human health would therefore be a significant issue for long-term occupation of Titan, more so than on Mars. These effects are still an active field of study. They can include symptoms such as loss of bone density, loss of muscle density, and a weakened immune system. Astronauts in Earth orbit have remained in microgravity for up to a year or more at a time. Effective countermeasures for the negative effects of low gravity are well-established, particularly an aggressive regime of daily physical exercise or weighted clothing. The variation in the negative effects of low gravity as a function of different levels of low gravity are not known, since all research in this area is restricted to humans in zero gravity. The same goes for the potential effects of low gravity on fetal and pediatric development. It has been hypothesized that children born and raised in low gravity such as on Titan would not be well adapted for life under the higher gravity of Earth.[8]

The atmospheric pressure on Titan's surface is about one and a half times the pressure of Earth's atmosphere at sea level, making Titan the only celestial body in the Solar System besides Earth with a surface atmospheric pressure tolerable to humans. To put it into perspective, 1.5 atmospheres is approximately equivalent to the pressure experienced by a scuba diver on Earth at a water depth of only five meters, whereas the typical maximum recommended depth for recreational scuba divers is forty meters (equivalent to about five atmospheres of pressure). Matching the pressure of a habitat on Titan's surface to the ambient pressure would greatly reduce certain engineering difficulties. Titan's atmosphere is not toxic to humans, however the methane and hydrogen components are flammable in an oxygen atmosphere and would therefore need to be filtered out of buffer gas made from its atmosphere.

On the other hand, the temperature on Titan is about 94 K (179C, or 290.2F), so insulation and heat generation and management would be significant concerns. However, because of the colder temperature the density of the air is closer to 4.5 times that of Earth sea level. At this density, temperature shifts over time and between one locale and another would be far smaller than comparable types of temperature changes present on Earth. The corresponding narrow range of temperature variation reduces the difficulties in structural engineering.

Relative thickness of the atmosphere combined with extreme cold makes additional troubles for human habitation. Unlike in a vacuum, the high atmospheric density makes thermoinsulation a significant engineering problem.

The engineering considerations for a spacesuit suitable for extravehicular activity on Titan's surface are radically different compared to a spacesuit designed for use in a vacuum. On the one hand, such a spacesuit would not need to be pressurized, but it would need to protect the wearer from the extreme cold, in addition to providing a breathable atmosphere. Compared to a vacuum, heat would rapidly dissipate in Titan's thick atmosphere. The degree of difficulty associated with working in such a spacesuit constructed with current technology would probably be at least equivalent to the difficulty associated with using a pressurized spacesuit in a vacuum.

The very high ratio of atmospheric density to surface gravity also greatly reduces the wingspan needed for an aircraft to maintain lift, so much so that a human would be able to strap on wings and easily fly through Titan's atmosphere while wearing a spacesuit that could be manufactured with current technology.[6] Another theoretically possible means to become airborne on Titan would be to use a hot air balloon-like vehicle filled with an Earth-like atmosphere at Earth-like temperatures (because oxygen is only slightly denser than nitrogen, the atmosphere in a habitat on Titan would be about one third as dense as the surrounding atmosphere), although such a vehicle would need a skin able to keep the extreme cold out in spite of the light weight required. Due to Titan's extremely low temperatures, heating of any flight-bound vehicle becomes a key obstacle.[9]

Read this article:
Colonization of Titan - Wikipedia

Posted in Moon Colonization | Comments Off on Colonization of Titan – Wikipedia

Human – Wikipedia

Posted: at 7:34 am

Human[1] Temporal range: 0.1950Ma Middle Pleistocene Recent An adult human male (left) and female (right) in Northern Thailand. Scientific classification Kingdom: Animalia Phylum: Chordata Clade: Synapsida Class: Mammalia Order: Primates Suborder: Haplorhini Family: Hominidae Genus: Homo Species: H.sapiens Binomial name Homo sapiens Linnaeus, 1758 Subspecies

Homo sapiens idaltu White et al., 2003 Homo sapiens sapiens

Modern humans (Homo sapiens, primarily ssp. Homo sapiens sapiens) are the only extant members of Hominina clade (or human clade), a branch of the taxonomical tribe Hominini belonging to the family of great apes. They are characterized by erect posture and bipedal locomotion; manual dexterity and increased tool use, compared to other animals; and a general trend toward larger, more complex brains and societies.[3][4]

Early homininsparticularly the australopithecines, whose brains and anatomy are in many ways more similar to ancestral non-human apesare less often referred to as "human" than hominins of the genus Homo.[5] Several of these hominins used fire, occupied much of Eurasia, and gave rise to anatomically modern Homo sapiens in Africa about 200,000 years ago.[6][7] They began to exhibit evidence of behavioral modernity around 50,000 years ago. In several waves of migration, anatomically modern humans ventured out of Africa and populated most of the world.[8]

The spread of humans and their large and increasing population has had a profound impact on large areas of the environment and millions of native species worldwide. Advantages that explain this evolutionary success include a relatively larger brain with a particularly well-developed neocortex, prefrontal cortex and temporal lobes, which enable high levels of abstract reasoning, language, problem solving, sociality, and culture through social learning. Humans use tools to a much higher degree than any other animal, are the only extant species known to build fires and cook their food, and are the only extant species to clothe themselves and create and use numerous other technologies and arts.

Humans are uniquely adept at utilizing systems of symbolic communication (such as language and art) for self-expression and the exchange of ideas, and for organizing themselves into purposeful groups. Humans create complex social structures composed of many cooperating and competing groups, from families and kinship networks to political states. Social interactions between humans have established an extremely wide variety of values,[9]social norms, and rituals, which together form the basis of human society. Curiosity and the human desire to understand and influence the environment and to explain and manipulate phenomena (or events) has provided the foundation for developing science, philosophy, mythology, religion, anthropology, and numerous other fields of knowledge.

Though most of human existence has been sustained by hunting and gathering in band societies,[10] increasing numbers of human societies began to practice sedentary agriculture approximately some 10,000 years ago,[11] domesticating plants and animals, thus allowing for the growth of civilization. These human societies subsequently expanded in size, establishing various forms of government, religion, and culture around the world, unifying people within regions to form states and empires. The rapid advancement of scientific and medical understanding in the 19th and 20th centuries led to the development of fuel-driven technologies and increased lifespans, causing the human population to rise exponentially. By February 2016, the global human population had exceeded 7.3 billion.[12]

-10

-9

-8

-7

-6

-5

-4

-3

-2

-1

0

-4500

-4000

-3500

-3000

-2500

-2000

-1500

-1000

-500

0

In common usage, the word "human" generally refers to the only extant species of the genus Homo anatomically and behaviorally modern Homo sapiens.

In scientific terms, the meanings of "hominid" and "hominin" have changed during the recent decades with advances in the discovery and study of the fossil ancestors of modern humans. The previously clear boundary between humans and apes has blurred, resulting in now acknowledging the hominids as encompassing multiple species, and Homo and close relatives since the split from chimpanzees as the only hominins. There is also a distinction between anatomically modern humans and Archaic Homo sapiens, the earliest fossil members of the species.

The English adjective human is a Middle English loanword from Old French humain, ultimately from Latin hmnus, the adjective form of hom "man." The word's use as a noun (with a plural: humans) dates to the 16th century.[13] The native English term man can refer to the species generally (a synonym for humanity), and could formerly refer to specific individuals of either sex, though this latter use is now obsolete.[14]

The species binomial Homo sapiens was coined by Carl Linnaeus in his 18th century work Systema Naturae.[15] The generic name Homo is a learned 18th century derivation from Latin hom "man," ultimately "earthly being" (Old Latin hem a cognate to Old English guma "man," from PIE demon-, meaning "earth" or "ground").[16] The species-name sapiens means "wise" or "sapient." Note that the Latin word homo refers to humans of either gender, and that sapiens is the singular form (while there is no such word as sapien).[17]

The genus Homo evolved and diverged from other hominins in Africa, after the human clade split from the chimpanzee lineage of the hominids (great apes) branch of the primates. Modern humans, defined as the species Homo sapiens or specifically to the single extant subspecies Homo sapiens sapiens, proceeded to colonize all the continents and larger islands, arriving in Eurasia 125,00060,000 years ago,[18][19]Australia around 40,000 years ago, the Americas around 15,000 years ago, and remote islands such as Hawaii, Easter Island, Madagascar, and New Zealand between the years 300 and 1280.[20][21]

The closest living relatives of humans are chimpanzees (genus Pan) and gorillas (genus Gorilla).[22] With the sequencing of both the human and chimpanzee genome, current estimates of similarity between human and chimpanzee DNA sequences range between 95% and 99%.[22][23][24] By using the technique called a molecular clock which estimates the time required for the number of divergent mutations to accumulate between two lineages, the approximate date for the split between lineages can be calculated. The gibbons (Hylobatidae) and orangutans (genus Pongo) were the first groups to split from the line leading to the humans, then gorillas (genus Gorilla) followed by the chimpanzees (genus Pan). The splitting date between human and chimpanzee lineages is placed around 48 million years ago during the late Miocene epoch.[25][26] During this split, chromosome 2 was formed from two other chromosomes, leaving humans with only 23 pairs of chromosomes, compared to 24 for the other apes.[27][28]

There is little fossil evidence for the divergence of the gorilla, chimpanzee and hominin lineages.[29][30] The earliest fossils that have been proposed as members of the hominin lineage are Sahelanthropus tchadensis dating from 7 million years ago, Orrorin tugenensis dating from 5.7 million years ago, and Ardipithecus kadabba dating to 5.6 million years ago. Each of these species has been argued to be a bipedal ancestor of later hominins, but all such claims are contested. It is also possible that any one of the three is an ancestor of another branch of African apes, or is an ancestor shared between hominins and other African Hominoidea (apes). The question of the relation between these early fossil species and the hominin lineage is still to be resolved. From these early species the australopithecines arose around 4 million years ago diverged into robust (also called Paranthropus) and gracile branches, possibly one of which (such as A. garhi, dating to 2.5 million years ago) is a direct ancestor of the genus Homo.[citation needed]

The earliest members of the genus Homo are Homo habilis which evolved around 2.8 million years ago.[31]Homo habilis has been considered the first species for which there is clear evidence of the use of stone tools. More recently, however, in 2015, stone tools, perhaps predating Homo habilis, have been discovered in northwestern Kenya that have been dated to 3.3 million years old.[32] Nonetheless, the brains of Homo habilis were about the same size as that of a chimpanzee, and their main adaptation was bipedalism as an adaptation to terrestrial living. During the next million years a process of encephalization began, and with the arrival of Homo erectus in the fossil record, cranial capacity had doubled. Homo erectus were the first of the hominina to leave Africa, and these species spread through Africa, Asia, and Europe between 1.3to1.8 million years ago. One population of H. erectus, also sometimes classified as a separate species Homo ergaster, stayed in Africa and evolved into Homo sapiens. It is believed that these species were the first to use fire and complex tools. The earliest transitional fossils between H. ergaster/erectus and archaic humans are from Africa such as Homo rhodesiensis, but seemingly transitional forms are also found at Dmanisi, Georgia. These descendants of African H. erectus spread through Eurasia from ca. 500,000 years ago evolving into H. antecessor, H. heidelbergensis and H. neanderthalensis. The earliest fossils of anatomically modern humans are from the Middle Paleolithic, about 200,000 years ago such as the Omo remains of Ethiopia and the fossils of Herto sometimes classified as Homo sapiens idaltu.[33] Later fossils of archaic Homo sapiens from Skhul in Israel and Southern Europe begin around 90,000 years ago.[34]

Human evolution is characterized by a number of morphological, developmental, physiological, and behavioral changes that have taken place since the split between the last common ancestor of humans and chimpanzees. The most significant of these adaptations are 1. bipedalism, 2. increased brain size, 3. lengthened ontogeny (gestation and infancy), 4. decreased sexual dimorphism (neoteny). The relationship between all these changes is the subject of ongoing debate.[35] Other significant morphological changes included the evolution of a power and precision grip, a change first occurring in H. erectus.[36]

Bipedalism is the basic adaption of the hominin line, and it is considered the main cause behind a suite of skeletal changes shared by all bipedal hominins. The earliest bipedal hominin is considered to be either Sahelanthropus[37] or Orrorin, with Ardipithecus, a full bipedal, coming somewhat later.[citation needed] The knuckle walkers, the gorilla and chimpanzee, diverged around the same time, and either Sahelanthropus or Orrorin may be humans' last shared ancestor with those animals.[citation needed] The early bipedals eventually evolved into the australopithecines and later the genus Homo.[citation needed] There are several theories of the adaptational value of bipedalism. It is possible that bipedalism was favored because it freed up the hands for reaching and carrying food, because it saved energy during locomotion, because it enabled long distance running and hunting, or as a strategy for avoiding hyperthermia by reducing the surface exposed to direct sun.[citation needed]

The human species developed a much larger brain than that of other primates typically 1,330 cm3 in modern humans, over twice the size of that of a chimpanzee or gorilla.[38] The pattern of encephalization started with Homo habilis which at approximately 600cm3 had a brain slightly larger than chimpanzees, and continued with Homo erectus (8001100cm3), and reached a maximum in Neanderthals with an average size of 12001900cm3, larger even than Homo sapiens (but less encephalized).[39] The pattern of human postnatal brain growth differs from that of other apes (heterochrony), and allows for extended periods of social learning and language acquisition in juvenile humans. However, the differences between the structure of human brains and those of other apes may be even more significant than differences in size.[40][41][42][43] The increase in volume over time has affected different areas within the brain unequally the temporal lobes, which contain centers for language processing have increased disproportionately, as has the prefrontal cortex which has been related to complex decision making and moderating social behavior.[38] Encephalization has been tied to an increasing emphasis on meat in the diet,[44][45] or with the development of cooking,[46] and it has been proposed [47] that intelligence increased as a response to an increased necessity for solving social problems as human society became more complex.

The reduced degree of sexual dimorphism is primarily visible in the reduction of the male canine tooth relative to other ape species (except gibbons). Another important physiological change related to sexuality in humans was the evolution of hidden estrus. Humans are the only ape in which the female is fertile year round, and in which no special signals of fertility are produced by the body (such as genital swelling during estrus). Nonetheless humans retain a degree of sexual dimorphism in the distribution of body hair and subcutaneous fat, and in the overall size, males being around 25% larger than females. These changes taken together have been interpreted as a result of an increased emphasis on pair bonding as a possible solution to the requirement for increased parental investment due to the prolonged infancy of offspring.[citation needed]

By the beginning of the Upper Paleolithic period (50,000 BP), full behavioral modernity, including language, music and other cultural universals had developed.[48][49] As modern humans spread out from Africa they encountered other hominids such as Homo neanderthalensis and the so-called Denisovans. The nature of interaction between early humans and these sister species has been a long-standing source of controversy, the question being whether humans replaced these earlier species or whether they were in fact similar enough to interbreed, in which case these earlier populations may have contributed genetic material to modern humans.[50] Recent studies of the human and Neanderthal genomes suggest gene flow between archaic Homo sapiens and Neanderthals and Denisovans.[51][52][53] In March 2016, studies were published that suggest that modern humans bred with hominins, including Denisovans and Neanderthals, on multiple occasions.[54]

This dispersal out of Africa is estimated to have begun about 70,000 years BP from Northeast Africa. Current evidence suggests that there was only one such dispersal and that it only involved a few hundred individuals. The vast majority of humans stayed in Africa and adapted to a diverse array of environments.[55] Modern humans subsequently spread globally, replacing earlier hominins (either through competition or hybridization). They inhabited Eurasia and Oceania by 40,000 years BP, and the Americas at least 14,500 years BP.[56][57]

Until about 10,000 years ago, humans lived as hunter-gatherers. They gradually gained domination over much of the natural environment. They generally lived in small nomadic groups known as band societies, often in caves. The advent of agriculture prompted the Neolithic Revolution, when access to food surplus led to the formation of permanent human settlements, the domestication of animals and the use of metal tools for the first time in history. Agriculture encouraged trade and cooperation, and led to complex society.[citation needed]

The early civilizations of Mesopotamia, Egypt, India, China, Maya, Greece and Rome were some of the cradles of civilization.[58][59][60] The Late Middle Ages and the Early Modern Period saw the rise of revolutionary ideas and technologies. Over the next 500 years, exploration and European colonialism brought great parts of the world under European control, leading to later struggles for independence. The concept of the modern world as distinct from an ancient world is based on a rapid change progress in a brief period of time in many areas.[citation needed] Advances in all areas of human activity prompted new theories such as evolution and psychoanalysis, which changed humanity's views of itself.[citation needed] The Scientific Revolution, Technological Revolution and the Industrial Revolution up until the 19th century resulted in independent discoveries such as imaging technology, major innovations in transport, such as the airplane and automobile; energy development, such as coal and electricity.[61] This correlates with population growth (especially in America)[62] and higher life expectancy, the World population rapidly increased numerous times in the 19th and 20th centuries as nearly 10% of the 100 billion people lived in the past century.[63]

With the advent of the Information Age at the end of the 20th century, modern humans live in a world that has become increasingly globalized and interconnected. As of 2010, almost 2billion humans are able to communicate with each other via the Internet,[64] and 3.3 billion by mobile phone subscriptions.[65] Although interconnection between humans has encouraged the growth of science, art, discussion, and technology, it has also led to culture clashes and the development and use of weapons of mass destruction.[citation needed] Human civilization has led to environmental destruction and pollution significantly contributing to the ongoing mass extinction of other forms of life called the Holocene extinction event,[66] which may be further accelerated by global warming in the future.[67]

Early human settlements were dependent on proximity to water and, depending on the lifestyle, other natural resources used for subsistence, such as populations of animal prey for hunting and arable land for growing crops and grazing livestock. But humans have a great capacity for altering their habitats by means of technology, through irrigation, urban planning, construction, transport, manufacturing goods, deforestation and desertification. Deliberate habitat alteration is often done with the goals of increasing material wealth, increasing thermal comfort, improving the amount of food available, improving aesthetics, or improving ease of access to resources or other human settlements. With the advent of large-scale trade and transport infrastructure, proximity to these resources has become unnecessary, and in many places, these factors are no longer a driving force behind the growth and decline of a population. Nonetheless, the manner in which a habitat is altered is often a major determinant in population change.[citation needed]

Technology has allowed humans to colonize all of the continents and adapt to virtually all climates. Within the last century, humans have explored Antarctica, the ocean depths, and outer space, although large-scale colonization of these environments is not yet feasible. With a population of over seven billion, humans are among the most numerous of the large mammals. Most humans (61%) live in Asia. The remainder live in the Americas (14%), Africa (14%), Europe (11%), and Oceania (0.5%).[68]

Human habitation within closed ecological systems in hostile environments, such as Antarctica and outer space, is expensive, typically limited in duration, and restricted to scientific, military, or industrial expeditions. Life in space has been very sporadic, with no more than thirteen humans in space at any given time.[69] Between 1969 and 1972, two humans at a time spent brief intervals on the Moon. As of October 2016, no other celestial body has been visited by humans, although there has been a continuous human presence in space since the launch of the initial crew to inhabit the International Space Station on October 31, 2000.[70] However, other celestial bodies have been visited by human-made objects.[71][72][73]

Since 1800, the human population has increased from one billion[74] to over seven billion,[75] In 2004, some 2.5 billion out of 6.3 billion people (39.7%) lived in urban areas. In February 2008, the U.N. estimated that half the world's population would live in urban areas by the end of the year.[76] Problems for humans living in cities include various forms of pollution and crime,[77] especially in inner city and suburban slums. Both overall population numbers and the proportion residing in cities are expected to increase significantly in the coming decades.[78]

Humans have had a dramatic effect on the environment. Humans are apex predators, being rarely preyed upon by other species.[79] Currently, through land development, combustion of fossil fuels, and pollution, humans are thought to be the main contributor to global climate change.[80] If this continues at its current rate it is predicted that climate change will wipe out half of all plant and animal species over the next century.[81][82]

Most aspects of human physiology are closely homologous to corresponding aspects of animal physiology. The human body consists of the legs, the torso, the arms, the neck, and the head. An adult human body consists of about 100 trillion (1014) cells. The most commonly defined body systems in humans are the nervous, the cardiovascular, the circulatory, the digestive, the endocrine, the immune, the integumentary, the lymphatic, the muscoskeletal, the reproductive, the respiratory, and the urinary system.[83][84]

Humans, like most of the other apes, lack external tails, have several blood type systems, have opposable thumbs, and are sexually dimorphic. The comparatively minor anatomical differences between humans and chimpanzees are a result of human bipedalism. One difference is that humans have a far faster and more accurate throw than other animals. Humans are also among the best long-distance runners in the animal kingdom, but slower over short distances.[85][86] Humans' thinner body hair and more productive sweat glands help avoid heat exhaustion while running for long distances.[87]

As a consequence of bipedalism, human females have narrower birth canals. The construction of the human pelvis differs from other primates, as do the toes. A trade-off for these advantages of the modern human pelvis is that childbirth is more difficult and dangerous than in most mammals, especially given the larger head size of human babies compared to other primates. This means that human babies must turn around as they pass through the birth canal, which other primates do not do, and it makes humans the only species where females require help from their conspecifics[clarification needed] to reduce the risks of birthing. As a partial evolutionary solution, human fetuses are born less developed and more vulnerable. Chimpanzee babies are cognitively more developed than human babies until the age of six months, when the rapid development of human brains surpasses chimpanzees. Another difference between women and chimpanzee females is that women go through the menopause and become unfertile decades before the end of their lives. All species of non-human apes are capable of giving birth until death. Menopause probably developed as it has provided an evolutionary advantage (more caring time) to young relatives.[86]

Apart from bipedalism, humans differ from chimpanzees mostly in smelling, hearing, digesting proteins, brain size, and the ability of language. Humans' brains are about three times bigger than in chimpanzees. More importantly, the brain to body ratio is much higher in humans than in chimpanzees, and humans have a significantly more developed cerebral cortex, with a larger number of neurons. The mental abilities of humans are remarkable compared to other apes. Humans' ability of speech is unique among primates. Humans are able to create new and complex ideas, and to develop technology, which is unprecedented among other organisms on Earth.[86]

It is estimated that the worldwide average height for an adult human male is about 172cm (5ft 712in),[citation needed] while the worldwide average height for adult human females is about 158cm (5ft 2in).[citation needed] Shrinkage of stature may begin in middle age in some individuals, but tends to be typical in the extremely aged.[88] Through history human populations have universally become taller, probably as a consequence of better nutrition, healthcare, and living conditions.[89] The average mass of an adult human is 5464kg (120140lb) for females and 7683kg (168183lb) for males.[90] Like many other conditions, body weight and body type is influenced by both genetic susceptibility and environment and varies greatly among individuals. (see obesity)[91][92]

Although humans appear hairless compared to other primates, with notable hair growth occurring chiefly on the top of the head, underarms and pubic area, the average human has more hair follicles on his or her body than the average chimpanzee. The main distinction is that human hairs are shorter, finer, and less heavily pigmented than the average chimpanzee's, thus making them harder to see.[93] Humans have about 2 million sweat glands spread over their entire bodies, many more than chimpanzees, whose sweat glands are scarce and are mainly located on the palm of the hand and on the soles of the feet.[94]

The dental formula of humans is: 2.1.2.32.1.2.3. Humans have proportionately shorter palates and much smaller teeth than other primates. They are the only primates to have short, relatively flush canine teeth. Humans have characteristically crowded teeth, with gaps from lost teeth usually closing up quickly in young individuals. Humans are gradually losing their wisdom teeth, with some individuals having them congenitally absent.[95]

Like all mammals, humans are a diploid eukaryotic species. Each somatic cell has two sets of 23 chromosomes, each set received from one parent; gametes have only one set of chromosomes, which is a mixture of the two parental sets. Among the 23 pairs of chromosomes there are 22 pairs of autosomes and one pair of sex chromosomes. Like other mammals, humans have an XY sex-determination system, so that females have the sex chromosomes XX and males have XY.[96]

One human genome was sequenced in full in 2003, and currently efforts are being made to achieve a sample of the genetic diversity of the species (see International HapMap Project). By present estimates, humans have approximately 22,000 genes.[97] The variation in human DNA is very small compared to other species, possibly suggesting a population bottleneck during the Late Pleistocene (around 100,000 years ago), in which the human population was reduced to a small number of breeding pairs.[98][99]Nucleotide diversity is based on single mutations called single nucleotide polymorphisms (SNPs). The nucleotide diversity between humans is about 0.1%, i.e. 1 difference per 1,000 base pairs.[100][101] A difference of 1 in 1,000 nucleotides between two humans chosen at random amounts to about 3 million nucleotide differences, since the human genome has about 3 billion nucleotides. Most of these single nucleotide polymorphisms (SNPs) are neutral but some (about 3 to 5%) are functional and influence phenotypic differences between humans through alleles.[citation needed]

By comparing the parts of the genome that are not under natural selection and which therefore accumulate mutations at a fairly steady rate, it is possible to reconstruct a genetic tree incorporating the entire human species since the last shared ancestor. Each time a certain mutation (SNP) appears in an individual and is passed on to his or her descendants, a haplogroup is formed including all of the descendants of the individual who will also carry that mutation. By comparing mitochondrial DNA, which is inherited only from the mother, geneticists have concluded that the last female common ancestor whose genetic marker is found in all modern humans, the so-called mitochondrial Eve, must have lived around 90,000 to 200,000 years ago.[102][103][104]

Human accelerated regions, first described in August 2006,[105][106] are a set of 49 segments of the human genome that are conserved throughout vertebrate evolution but are strikingly different in humans. They are named according to their degree of difference between humans and their nearest animal relative (chimpanzees) (HAR1 showing the largest degree of human-chimpanzee differences). Found by scanning through genomic databases of multiple species, some of these highly mutated areas may contribute to human-specific traits.[citation needed]

The forces of natural selection have continued to operate on human populations, with evidence that certain regions of the genome display directional selection in the past 15,000 years.[107]

As with other mammals, human reproduction takes place as internal fertilization by sexual intercourse. During this process, the male inserts his erect penis into the female's vagina and ejaculates semen, which contains sperm. The sperm travels through the vagina and cervix into the uterus or Fallopian tubes for fertilization of the ovum. Upon fertilization and implantation, gestation then occurs within the female's uterus.

The zygote divides inside the female's uterus to become an embryo, which over a period of 38 weeks (9 months) of gestation becomes a fetus. After this span of time, the fully grown fetus is birthed from the woman's body and breathes independently as an infant for the first time. At this point, most modern cultures recognize the baby as a person entitled to the full protection of the law, though some jurisdictions extend various levels of personhood earlier to human fetuses while they remain in the uterus.

Compared with other species, human childbirth is dangerous. Painful labors lasting 24 hours or more are not uncommon and sometimes lead to the death of the mother, the child or both.[108] This is because of both the relatively large fetal head circumference and the mother's relatively narrow pelvis.[109][110] The chances of a successful labor increased significantly during the 20th century in wealthier countries with the advent of new medical technologies. In contrast, pregnancy and natural childbirth remain hazardous ordeals in developing regions of the world, with maternal death rates approximately 100 times greater than in developed countries.[111]

In developed countries, infants are typically 34kg (69pounds) in weight and 5060cm (2024inches) in height at birth.[112][not in citation given] However, low birth weight is common in developing countries, and contributes to the high levels of infant mortality in these regions.[113] Helpless at birth, humans continue to grow for some years, typically reaching sexual maturity at 12 to 15years of age. Females continue to develop physically until around the age of 18, whereas male development continues until around age 21. The human life span can be split into a number of stages: infancy, childhood, adolescence, young adulthood, adulthood and old age. The lengths of these stages, however, have varied across cultures and time periods. Compared to other primates, humans experience an unusually rapid growth spurt during adolescence, where the body grows 25% in size. Chimpanzees, for example, grow only 14%, with no pronounced spurt.[114] The presence of the growth spurt is probably necessary to keep children physically small until they are psychologically mature. Humans are one of the few species in which females undergo menopause. It has been proposed that menopause increases a woman's overall reproductive success by allowing her to invest more time and resources in her existing offspring, and in turn their children (the grandmother hypothesis), rather than by continuing to bear children into old age.[115][116]

For various reasons, including biological/genetic causes,[117] women live on average about four years longer than menas of 2013 the global average life expectancy at birth of a girl is estimated at 70.2 years compared to 66.1 for a boy.[118] There are significant geographical variations in human life expectancy, mostly correlated with economic developmentfor example life expectancy at birth in Hong Kong is 84.8years for girls and 78.9 for boys, while in Swaziland, primarily because of AIDS, it is 31.3years for both sexes.[119] The developed world is generally aging, with the median age around 40years. In the developing world the median age is between 15 and 20years. While one in five Europeans is 60years of age or older, only one in twenty Africans is 60years of age or older.[120] The number of centenarians (humans of age 100years or older) in the world was estimated by the United Nations at 210,000 in 2002.[121] At least one person, Jeanne Calment, is known to have reached the age of 122years;[122] higher ages have been claimed but they are not well substantiated.

Humans are omnivorous, capable of consuming a wide variety of plant and animal material.[123][124] Varying with available food sources in regions of habitation, and also varying with cultural and religious norms, human groups have adopted a range of diets, from purely vegetarian to primarily carnivorous. In some cases, dietary restrictions in humans can lead to deficiency diseases; however, stable human groups have adapted to many dietary patterns through both genetic specialization and cultural conventions to use nutritionally balanced food sources.[125] The human diet is prominently reflected in human culture, and has led to the development of food science.

Until the development of agriculture approximately 10,000 years ago, Homo sapiens employed a hunter-gatherer method as their sole means of food collection. This involved combining stationary food sources (such as fruits, grains, tubers, and mushrooms, insect larvae and aquatic mollusks) with wild game, which must be hunted and killed in order to be consumed.[126] It has been proposed that humans have used fire to prepare and cook food since the time of Homo erectus.[127] Around ten thousand years ago, humans developed agriculture,[128] which substantially altered their diet. This change in diet may also have altered human biology; with the spread of dairy farming providing a new and rich source of food, leading to the evolution of the ability to digest lactose in some adults.[129][130] Agriculture led to increased populations, the development of cities, and because of increased population density, the wider spread of infectious diseases. The types of food consumed, and the way in which they are prepared, have varied widely by time, location, and culture.

In general, humans can survive for two to eight weeks without food, depending on stored body fat. Survival without water is usually limited to three or four days. About 36 million humans die every year from causes directly or indirectly related to starvation.[131] Childhood malnutrition is also common and contributes to the global burden of disease.[132] However global food distribution is not even, and obesity among some human populations has increased rapidly, leading to health complications and increased mortality in some developed, and a few developing countries. Worldwide over one billion people are obese,[133] while in the United States 35% of people are obese, leading to this being described as an "obesity epidemic."[134] Obesity is caused by consuming more calories than are expended, so excessive weight gain is usually caused by an energy-dense diet.[133]

No two humansnot even monozygotic twinsare genetically identical. Genes and environment influence human biological variation from visible characteristics to physiology to disease susceptibly to mental abilities. The exact influence of genes and environment on certain traits is not well understood.[135][136]

Most current genetic and archaeological evidence supports a recent single origin of modern humans in East Africa,[137] with first migrations placed at 60,000 years ago. Compared to the great apes, human gene sequenceseven among African populationsare remarkably homogeneous.[138] On average, genetic similarity between any two humans is 99.9%.[139][140] There is about 23 times more genetic diversity within the wild chimpanzee population, than in the entire human gene pool.[141][142][143]

The human body's ability to adapt to different environmental stresses is remarkable, allowing humans to acclimatize to a wide variety of temperatures, humidity, and altitudes. As a result, humans are a cosmopolitan species found in almost all regions of the world, including tropical rainforests, arid desert, extremely cold arctic regions, and heavily polluted cities. Most other species are confined to a few geographical areas by their limited adaptability.[144]

There is biological variation in the human specieswith traits such as blood type, cranial features, eye color, hair color and type, height and build, and skin color varying across the globe. Human body types vary substantially. The typical height of an adult human is between 1.4m and 1.9m (4ft 7 in and 6ft 3 in), although this varies significantly depending, among other things, on sex and ethnic origin.[145][146] Body size is partly determined by genes and is also significantly influenced by environmental factors such as diet, exercise, and sleep patterns, especially as an influence in childhood. Adult height for each sex in a particular ethnic group approximately follows a normal distribution. Those aspects of genetic variation that give clues to human evolutionary history, or are relevant to medical research, have received particular attention. For example, the genes that allow adult humans to digest lactose are present in high frequencies in populations that have long histories of cattle domestication, suggesting natural selection having favored that gene in populations that depend on cow milk. Some hereditary diseases such as sickle cell anemia are frequent in populations where malaria has been endemic throughout historyit is believed that the same gene gives increased resistance to malaria among those who are unaffected carriers of the gene. Similarly, populations that have for a long time inhabited specific climates, such as arctic or tropical regions or high altitudes, tend to have developed specific phenotypes that are beneficial for conserving energy in those environmentsshort stature and stocky build in cold regions, tall and lanky in hot regions, and with high lung capacities at high altitudes. Similarly, skin color varies clinally with darker skin around the equatorwhere the added protection from the sun's ultraviolet radiation is thought to give an evolutionary advantageand lighter skin tones closer to the poles.[147][148][149][150]

The hue of human skin and hair is determined by the presence of pigments called melanins. Human skin color can range from darkest brown to lightest peach, or even nearly white or colorless in cases of albinism.[143] Human hair ranges in color from white to red to blond to brown to black, which is most frequent.[151] Hair color depends on the amount of melanin (an effective sun blocking pigment) in the skin and hair, with hair melanin concentrations in hair fading with increased age, leading to grey or even white hair. Most researchers believe that skin darkening is an adaptation that evolved as protection against ultraviolet solar radiation, which also helps balancing folate, which is destroyed by ultraviolet radiation. Light skin pigmentation protects against depletion of vitamin D, which requires sunlight to make.[152] Skin pigmentation of contemporary humans is clinally distributed across the planet, and in general correlates with the level of ultraviolet radiation in a particular geographic area. Human skin also has a capacity to darken (tan) in response to exposure to ultraviolet radiation.[153][154][155]

Within the human species, the greatest degree of genetic variation exists between males and females. While the nucleotide genetic variation of individuals of the same sex across global populations is no greater than 0.1%, the genetic difference between males and females is between 1% and 2%. Although different in nature[clarification needed], this approaches the genetic differentiation between men and male chimpanzees or women and female chimpanzees. The genetic difference between sexes contributes to anatomical, hormonal, neural, and physiological differences between men and women, although the exact degree and nature of social and environmental influences on sexes are not completely understood. Males on average are 15% heavier and 15cm taller than females. There is a difference between body types, body organs and systems, hormonal levels, sensory systems, and muscle mass between sexes. On average, there is a difference of about 4050% in upper body strength and 2030% in lower body strength between men and women. Women generally have a higher body fat percentage than men. Women have lighter skin than men of the same population; this has been explained by a higher need for vitamin D (which is synthesized by sunlight) in females during pregnancy and lactation. As there are chromosomal differences between females and males, some X and Y chromosome related conditions and disorders only affect either men or women. Other conditional differences between males and females are not related to sex chromosomes. Even after allowing for body weight and volume, the male voice is usually an octave deeper than the female voice. Women have a longer life span in almost every population around the world.[157][158][159][160][161][162][163][164][165]

Males typically have larger tracheae and branching bronchi, with about 30% greater lung volume per unit body mass. They have larger hearts, 10% higher red blood cell count, and higher hemoglobin, hence greater oxygen-carrying capacity. They also have higher circulating clotting factors (vitamin K, prothrombin and platelets). These differences lead to faster healing of wounds and higher peripheral pain tolerance.[166] Females typically have more white blood cells (stored and circulating), more granulocytes and B and T lymphocytes. Additionally, they produce more antibodies at a faster rate than males. Hence they develop fewer infectious diseases and these continue for shorter periods.[166]Ethologists argue that females, interacting with other females and multiple offspring in social groups, have experienced such traits as a selective advantage.[167][168][169][170][171] According to Daly and Wilson, "The sexes differ more in human beings than in monogamous mammals, but much less than in extremely polygamous mammals."[172] But given that sexual dimorphism in the closest relatives of humans is much greater than among humans, the human clade must be considered to be characterized by decreasing sexual dimorphism, probably due to less competitive mating patterns. One proposed explanation is that human sexuality has developed more in common with its close relative the bonobo, which exhibits similar sexual dimorphism, is polygynandrous and uses recreational sex to reinforce social bonds and reduce aggression.[173]

Humans of the same sex are 99.9% genetically identical. There is extremely little variation between human geographical populations, and most of the variation that does occur is at the personal level within local areas, and not between populations.[143][174][175] Of the 0.1% of human genetic differentiation, 85% exists within any randomly chosen local population, be they Italians, Koreans, or Kurds. Two randomly chosen Koreans may be genetically as different as a Korean and an Italian. Any ethnic group contains 85% of the human genetic diversity of the world. Genetic data shows that no matter how population groups are defined, two people from the same population group are about as different from each other as two people from any two different population groups.[143][176][177][178]

Current genetic research has demonstrated that humans on the African continent are the most genetically diverse.[179] There is more human genetic diversity in Africa than anywhere else on Earth. The genetic structure of Africans was traced to 14 ancestral population clusters. Human genetic diversity decreases in native populations with migratory distance from Africa and this is thought to be the result of bottlenecks during human migration.[180][181] Humans have lived in Africa for the longest time, which has allowed accumulation of a higher diversity of genetic mutations in these populations. Only part of Africa's population migrated out of the continent, bringing just part of the original African genetic variety with them. African populations harbor genetic alleles that are not found in other places of the world. All the common alleles found in populations outside of Africa are found on the African continent.[143]

Geographical distribution of human variation is complex and constantly shifts through time which reflects complicated human evolutionary history. Most human biological variation is clinally distributed and blends gradually from one area to the next. Groups of people around the world have different frequencies of polymorphic genes. Furthermore, different traits are non-concordant and each have different clinal distribution. Adaptability varies both from person to person and from population to population. The most efficient adaptive responses are found in geographical populations where the environmental stimuli are the strongest (e.g. Tibetans are highly adapted to high altitudes). The clinal geographic genetic variation is further complicated by the migration and mixing between human populations which has been occurring since prehistoric times.[143][182][183][184][185][186]

Here is the original post:
Human - Wikipedia

Posted in Human Genetics | Comments Off on Human – Wikipedia

Supercourse: Epidemiology, the Internet, and Global Health

Posted: at 7:34 am

ABCDEFGHIJKLMNOPQRSTUVWXYZ

Academic research council

Achievements public health

Achievements public health

Acne therapeutic strategies

Acute coronary symptoms

Acute coronary syndromes

Adenoviridae and iridoviridae

Adherence hypertension treatment

Administration management medical organizations

Adolescent health risk behavior

Adolescents reproductive health

Adolescents reproductive health

Adverse drug reactions

Advocacy strategy planning

African sleeping sickness

Aids/ hiv current senario

Airborne contaminants

Air pollution armenia

Air pollution armenia

American heart association

Aminoglycosidearginine conjugates

Analytic epidemiology

Anaplasmosis taxonomic

Anemia family practice

Anger regulation interventions

Antimicrobial resistance

Antimicrobrial peptides

Antiretroviral agents

Assessing disease frequency

Assessment bioterrorism threat

Assessment nutritional

Assistive technology devices

Attack preparedness events

Avian influenza: zoonosis

Bacterial membrane vesicles

Bacterial vaginosis pregnancy

Bases of biostatistics

Behaviour medical sciences

Betaserk treatment stroke

Bias confounding chance

Bimaristans (hospitals) islamic

Binomial distribution

Biochemical system medicine

Biological challenges

Biological epidemiologic studies

Biostatistics

Biostatistics public health

Blood donors non-donors

Blood glucose normaization

Bmj triages manuscripts

Body fluid volume regulation

Bolonya declaration education

Bone marrow transplantation

Breast self examination

Bronchial asthma treatmen

Building vulnerability

Burden infectious diseases

Burnout in physicians

Cncer en mxico

Cancer survivorship research

Canine monocytic ehrlichiosis

Capability development

Capture-recapture techniques

Cardiology practice grenada

Cardiometabolic syndrome

Cardiopulmonary resuscitation

Cardio-respiratory illness

Cardiovascular disease

Cardiovascular disease black

Cardiovascular disease prevention

Cardiovascular diseases

Cardiovascular system

Carpal tunnel syndrome

Caseous lymphadenitis

Cause epidemiological approach

Central nervous system

Cervical cancer screening

Changing interpretations

Chemical weapon bioterrorism

Chemiosmotic paradigm

Chickenpox children pregnancy

Child health kazakhstan

Childhood asthma bedding.

Childhood asthma prevalence

Childhood diabetes mellitus

Childhood hearing impairment

Children september 11th attacks

China

Chinese herbal medicines

Chns hypertension control

Cholera global health

Cholesterol education program

Chronic disease management

Chronic fatigue syndrome

Chronic liver disease

Chronic lung diseases

Chronic noncommunicable diseases

Chronic obstructive pulmonary disease

Chronic pulmonary heart

Continue reading here:
Supercourse: Epidemiology, the Internet, and Global Health

Posted in Human Genetics | Comments Off on Supercourse: Epidemiology, the Internet, and Global Health