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Category Archives: Transhuman News

Happy Birthday, Canadarm2! Spacecraft-Grabbing Robotic Arm Turns 16 – Space.com

Posted: April 25, 2017 at 4:39 am

Happy birthday, Canadarm2! A Canadian-made robotic arm affixed outside the International Space Station turns 16 years old today (April 24).

Canadarm2, also known as the Space Station Remote Manipulator System (SSRMS), arrived at the orbital outpost with mission STS-100 aboard the space shuttle Endeavour on April 19, 2001. Five days and two spacewalks later, Canadarm2's installation was complete.

Canadarm2, a robotic arm outside the International Space Station, turns 16 years old this week! Its installation was completed on April 24, 2001. In this photo, NASA astronaut Stephen Robinson rides Canadarm2 during the STS-114 mission in 2005

Canadian astronaut Chris Hadfieldand NASA astronaut Scott Parazynskispent nearly 15 hours installing Canadarm2 during STS-100. Since then, the arm has been moving around the outside of the space station, handling heavy payloads and occasionally assisting astronauts with about 100 spacewalks, all in the name of space station assembly and maintenance.

Astronauts at the space station now use Canadarm2 to grab and dock incoming spacecraft like Orbital ATK's cargo-resupply ship SS John Glenn, which arrived at the space station on Saturday (April 22).

Sometimes, flight controllers on the ground in Houston will operate Canadarm2 remotely, like when the arm was used to relocate a docking adapterin between two spacewalks last month.

The 58-foot-long (18 meters) arm is one of three robotic components that now make up the space station's Mobile Servicing System, along with a robotic "hand" known as Dextre and a base platform known as the Mobile Remote Servicer Base System (MBS). The MBS allows Canadarm2 and Dextre to move around the outside of the space station's main truss structure "by sliding along a track system mounted along the entire width of the station," theCanadian Space Agencywrote in a description.

"Sometimes, when looking out the window, the best view is not on Earth but on the International Space Station itself," European Space Agency astronaut Thomas Pesquet wrote when he tweeted this photo. "The robotic arm casts a shadow on the solar array, while the rest of our home space is shrouded in darkness."

Canadarm2 may be orbiting roughly 250 miles (400 km) overhead, but you can get firsthand experience with the teenage robot via the Canadian Space Agency's cool Canadarm2 Simulator, an online gamein which you control the robotic arm during a mock mission at the space station.

Email Hanneke Weitering at hweitering@space.com or follow her @hannekescience. Follow us @Spacedotcom, Facebookand Google+. Original article on Space.com.

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American, Russian cheered as they reach space station – The Boston Globe

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BAIKONUR, Kazakhstan A Soyuz space capsule on Thursday safely delivered an American astronaut making his first space flight and a veteran Russian cosmonaut to the International Space Station.

NASAs Jack Fischer and Russias Fyodor Yurchikhin lifted off from the Russia-leased launch facility in Kazakhstan at Thursday afternoon. They reached orbit about nine minutes later, a moment illustrated when a stuffed white dog toy hanging from a string in the capsule began to float.

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About six hours later, they docked at the orbiting outpost.

NASAs Peggy Whitson, the crews commander, Russias Oleg Novitskiy, and Frances Thomas Pesquet greeted Fischer and Yurchikhin with cheers and hugs. They floated into the station two hours after the docking.

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Yurchikhin, making his fifth space flight, and Fischer, who is there for the first time, talked to family and friends at the Baikonur facility who were watching the launch there.

Fischers wife thanked him for what she said was the most unexpected bouquet of flowers that she received as he was launching into space. Fischer told his wife she had veteran cosmonaut Yurchikhin to thank for that.

The two American astronauts are scheduled to speak with President Trump on Monday.

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On that day, Wilson, who on a previous mission became the first woman to command the International Space Station, will break the US astronaut record for the most cumulative time in space. Jeffrey Williams currently holds the 534-day record.

At 57, Whitson also is the oldest woman to have been in space. She is scheduled to return to Earth in September.

Fischer and Yurchikhin will spend more than four months aboard the orbiting space station before also returning to Earth in September.

Associated Press

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REVIEW: Mars – Comicmix.com

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When some of the smartest people alive today insist we need to begin colonizing other worlds, you tend to believe them. When science fiction fans hear those words, we begin to salivate at the possibilities.

National Geographic cannily appeals to both audiences with their hybrid miniseries Mars, which mixes todays science with tomorrows fiction by positing what the actual colonization of the planet, a mere 140 million miles away, might look like. Yeah, we got a glimpse of that in the adaptation of Andrew Weirs The Martian, but this goes further and shows more of the risks involved.

The miniseries, out now from 20th Century Home Entertainment, is a captivating piece of work if unevenly assembled. You get all the usual suspects weighing in why and how we might get there including Space X guru Elon Musk and the ubiquitous Neil deGrasse Tyson. Accompanied by a Greek chorus of NASA scientists and engineers, we get a frim grounding on where we are today and what it will take (including how much and how long) to reach Mars and stay there.

With the firm guiding hand of Brian Grazer and Ron Howard who took us to the edge of space with the gripping Apollo 13 the fictional sections are visually interesting and feel like they could possibly happen over the next hundred years. The most fictional part of the story may be the notion that countries around the world can put aside their partisan issues in order to partner for such a project. Given the expertise and money required, its unlikely any one country can mount such a mission. Of course, its equally unlikely we can all come together fast enough to actually do it on the timetable envision by the likes of Stephen Hawking. That this story takes place in 2033 may be the most fantastic concept of all.

With a nice nod to Greek myth, the Daedalus is sent to Mars and we follow the crew, led by Ben Sawyer (Ben Cotton). The crew and their personal issues are far less interesting than the real science employed to get them there, which is a shame. After all, one reason America was captivated by the Mercury program was the canny PR done to turn the Mercury Seven into instant heroes, their every move followed by an eager public.

Obviously this was intended to be a utopian or dystopic view of life on other worlds, but the hazards and problems encountered are therefore representative, but also almost predictable, spoiling some of the dramatic satisfaction the fictional sections intended.

The sets and tech look fabulous as one would expect from the channel and production team. Watched as an AVC encoded 1080p transfer in 1.78:1, it looks great on the home screen accompanied by a serviceable DTS-HD Master Audio 5.1 mix.

The miniseries does boast a rather impressive physical (and/or CGI) production, with decently realistic sequences set on board the Daedalus and, later, on Mars itself. The fictional elements look has obviously been highly influenced by The Martian (as can clearly be seen in some of the screenshots accompanying this review), with some individual shots looking like they in fact could have been lifted directly from the film. But again and again its the current day scientists and explorers who provide the most riveting information. As odd as it might sound, this is one miniseries that might have benefitted from a kind of reverse seamless branching, where viewers could choose to skip the fictional parts and stick to the facts and only to the facts.

The three-disc Blu-ray set comes with a handful of extras, starting with Making Mars (47:17) which does a fine job recounting how the mockumentary was made. Theres Before Mars A Prequel (33:00) which offers up some welcome backstory for the dramatic portion. Theres the brief Before Mars Behind the Scenes (2:28); Getting to Mars (13:51); Living on Mars (10:26); More Mars (10:29); Behind the Scenes (14:38); and, Cast and Crew Interviews (25:06). Taken as a whole, the extras greatly expands our understanding of the nearby world, the difficulties in getting there, and how we might extend our stay. Additionally, the behind-the-scenes interviews with the production crew shows the meticulous detail that one expects from National Geographic.

Robert Greenberger is best known to comics fans as the editor of Who's Who In The DC Universe, Suicide Squad, and Doom Patrol. He's written and edited several Star Trek novels and is the author of The Essential Batman Encyclopedia. He's known for his work as an editor for Comics Scene, Starlog, and Weekly World News, as well as holding executive positions at both Marvel Comics and DC Comics.

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Space. The Final Frontier For Now | University Observer – University Observer Online

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Interplanetary travel. Celestial colonies. Life on Mars. Dont worry, this isnt the opening to a science-fiction novel all of this is possible. All of this is happening. Ellen Nugent finds out more.

ON July 21st, 1969, Neil Armstrong was the first human to set foot on the moon. NASAs Mars Exploration Rovers landed on the Red Planet in January, 2004. These are merely two examples of such expeditions, feats of scientific and intrepid brilliance, but they are simply not enough for humankind. Dissatisfied with our brief visits and voyages, the distant idea of colonizing new planets is swiftly becoming a reality.

Currently, there are no known planets within our solar system capable of supporting human life, but that hasnt stopped scientists from planning ahead for when we do find such planets. Mars, Venus and our moon have been investigated as potential hosts for human civilization, but low atmospheric oxygen and lack of facilities to support growth have not endeared these planets to potential homeowners.

Asteroids often contain valuable minerals which would allow the growth of food, and artificial gravity could be established in the colonies

Techniques to extract oxygen from carbon-dioxide-rich environments, such as the atmosphere on Mars, could be used to aid in the development of extraterrestrial colonies, but this carbon dioxide is limited. Scientists have also considered terraforming planets giant mirrors would be used to initiate global warming on the desired planet, eventually creating another planet capable of supporting human life. The cost of these procedures is, however, astronomical. There are also issues with the long-term effects of gravity on human development, and exposure to extraterrestrial radiation en route to these proposed settlements.

Scientists are also investigating planets outside our solar system for future colonization. The dwarf star TRAPPIST-1 is located 39 light years away from Earth. (369,000 trillion miles!). Seven Earth-like planets were recently discovered orbiting the star, three of which are hypothetically habitable by humans. The planets also have their disadvantages, however the nearby proximity of the planets to the dwarf star heavily influences day and year length a year on each of the Trappist System planets lasts several days. The distance from the Trappist System to our solar system also hinders colonization of these planets we would require 39 years to reach the system with our current light-speed technologies.

It has also been suggested that asteroids are inhabitable colonies would be drilled into the surface of the asteroid, and a population of asteroids and interlinking space transports would be capable of supporting large human populations. Asteroids often contain valuable minerals which would allow the growth of food, and artificial gravity could be established in the colonies, due to the constant rotation of the Earth.

How would humans live on these planets? Would we build biospheres, creating micro-atmospheres? Would we spend our lives as nomads, passing from spaceship to spaceship?

There are, of course, questions that remain unanswered. Methods of reaching these planets are still debated with our current space travel technology, humans will only reach these planets in a generation ship (a ship in which descendants of the original crew will reach the planet), or in an induced hibernation state. How would humans live on these planets? Would we build biospheres, creating micro-atmospheres? Would we spend our lives as nomads, passing from spaceship to spaceship? What are the ethical concerns of sending a population that exploited and stripped their own planet in search of new worlds?

At this time, we have no answers for these questions space colonisation is still heavily debated, and we are unlikely to see progress until all issues have been addressed. It is clear, however, that space colonization is becoming steadily more attractive. Earths resources are steadily running dry humans will enter a time of crisis in the near future. Research into extraterrestrial settlements is a priority. The colonisation of other planets would reduce the stresses of overpopulation and human action on Earth, and would also protect the human race in the case of a worldwide disaster.

No matter if an asteroid strike occurred, or if Yellowstone got bored and erupted for a change of pace humankind would be safe, with populations sequestered on their planetary settlements, or making their way to distant stars.

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McCormick professor creates 3D-printing materials using martian, lunar dust simulants – Daily Northwestern

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McCormick Prof. Ramille Shah.

Source: Ramille Shah

Source: Ramille Shah

McCormick Prof. Ramille Shah.

Catherine Kim, Assistant Campus Editor April 23, 2017

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McCormick Prof. Ramille Shah has developed a 3D-printing method using simulants of lunar and martian dust, which could be used for planet colonization.

Shah said she has been working with her Tissue Engineering and Additive Manufacturing Laboratory to develop a 3D-painting process using materials that can easily be found on planets and moons in preparation for planet colonization. For more than five years, the lab has been developing 3D-printing technology that allows it to print a variety of different types of materials with one 3D printer, Shah said. In the past, lab members have printed using biomaterials, graphene and metals, she said. They decided to test using lunar and martian dust simulants based on the senior thesis project of alumna Katie Koube (McCormick 14), Shah said.

In order to colonize or inhabit extraterrestrial places like the moon or Mars, people will need to be able to use the very limited resources that are available, she said. This 3D-printing ink technology and process allows the creation of functional objects from the dust found on the surface of these extraterrestrial bodies.

Products of 3D inks made out of lunar or martian dust simulants are flexible, almost reminiscent of tires, Shah said. She said it is fascinating to see how bouncy the products are, despite their high particle loading.

The flexibility can be adjusted through methods such as heating, which will center the particles together and create more ceramic-like materials, Shah said. McCormick Prof. David Dunand said he is collaborating with Shah to fire the products to give them hard, ceramic-like properties, which can be used for building materials.

The technology developed for heating the products is based on the expected habitat, which is Mars or the moon, where most people would be working indoors. Dunand said he and Shah are currently looking into ways to use minimal energy to heat the products while dust can be easily collected, energy comes at a much higher price in space, he said. They are currently researching ways of heating the products in air and in hydrogen, Dunand said.

You dont want to be wasteful, like we are here on Earth , he said. (In space) every bit matters because ultimately theres a lot of dust, but youre limited in energy. When you fire bricks, it takes a lot of energy do that.

Fourth-year graduate student Shannon Taylor, who works in Shahs lab, said research for planet colonization is necessary because having a plan will be crucial in assuring its success when the time comes.

Were not there yet, but at the point we get there we cant send people without all of this in place, Taylor said. We have to know exactly what were doing because its super expensive and ultimately human lives are at risk.

Shah said the potential of the 3D-printing methods developed by her lab goes beyond creating products for just planet colonization. Her lab has managed to mix different types of inks together to create multi-functional objects that can be used on Earth as well, such as material that can be both electrically conducting and bone-regenerating, she said.

It starts to really expand what we can do as far as materials development and discovering materials that have very new properties, she said.

Allyson Chiu contributed reporting.

Email: [emailprotected] Twitter: @ck_525

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Powering the Future: A Look at the Engines and Fuel that Drives SpaceX Vehicles – Breaking Energy

Posted: at 4:38 am

Space Exploration Technologies Corporation better known as SpaceX was founded just 15 years ago by Elon Musk, the world famous entrepreneur and genius behind other notable ventures such as Tesla Motors, Solar City and others. The aerospace manufacturer and space transport company was started with modest goals such as reducing space transportation cost and enabling the colonization of Mars.

SpaceX has developed the Falcon launch vehicle family and the Dragon spacecraft family. Using these vehicles SpaceX has achieved things which just twenty years ago most people would not have thought possible for a private company. The Falcon launch vehicles are propelled by Merlin rocket engines which is a family of engines developed by SpaceX. The Merlin engine uses RP-1 and liquid oxygen as rocket propellants in a gas-generator cycle.

RP-1 which is also known either as Rocket Propellant-1, or Refined Petroleum-1, is a form of highly refined kerosene which bears a strong similarity to jet fuel. RP-1 has a lower specific impulse than liquid hydrogen but is cheaper to produce, far more stable at room temperature, and far denser which makes it significantly more powerful by volume than liquid hydrogen. RP-1 is most commonly burned using liquid oxygen as an oxidizer.

RP-1 was first formulated by rocket designers in the mid-1950s as a replacement for the alcohol based fuels which were previously the most commonly used liquid rocket fuels. Since its advent by fuel chemists it has been the primary fuel used for rocket propulsion by the United States. The lack of light hydrocarbons in RP-1 give it a very high flash point and make it less of a fire hazard than common gasoline, many forms of diesel fuel, or even some jet fuels. Rocket-grade kerosene gases made by Russia and previously by the Soviet Union are very similar in structure and are commonly designated T-1 and RG-1.

Liquid oxygen was first produced in 1883 and must be kept extremely cold and has a freezing point of -361.82 F and a boiling point of -297.33 F. The extreme temperatures which it must be kept at causes materials it comes in contact with to become extremely brittle. It acts as an extremely powerful oxidizing agent when brought in contact with organic matter and is commonly used as rocket fuel because it creates a very high specific impulse.

The Merlin engine was originally designed by SpaceX for sea recovery and reuse. The injector at the center the Merlin is a pintle type which was first used during the Apollo program. The original version of the Merlin was the Merlin 1A which was used twice in 2006 and 2007 on a Falcon 1 first stage. The Merlin 1B was an upgraded version of the Merlin 1A, but was discarded by SpaceX due to its experience from the Falcon 1.

The Merlin 1C was used from 2008-2012 on the Falcon 1 and the Falcon 9 before being dropped in favor of the Merlin 1D. The Merlin 1D was used on its first flight in 2013 and is the current model in production for SpaceX. It is able to produce more than twice the thrust of the Merlin 1A at sea level. SpaceX indicates that it needs to produce hundreds of engines per year in order to support its current rocket production plans.

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Non-GMO breeding changes the makeup of crops more than genetic engineering – Genetic Literacy Project

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The composition of GM breeding stacks was more similar to the composition of iso-hybrids than was the composition of nonGM hybrids. NonGM breeding more strongly influenced crop composition than did transgenesis or stacking of GM events.

These findings call into question the value of uniquely requiring composition studies for GM crops, especially for breeding stacks composed of GM events previously found to be compositionally normal.

After more than two decades of research, many published reports and hundreds of regulatory submissions, transgenesis has generally been found to have markedly less effect on crop composition compared with traditional breeding. Advances in molecular biology have shown that the types of mutations that are possible during transgene insertion are similar to those associated with the intentional or unintentional random mutagenesis that occurs during traditional breeding, but that GM techniques typically have a smaller impact due to fewer genetic changes.

While the potential for unintended compositional effects is now known to be markedly lower for GM crops compared with those developed using nonGM breeding techniques, government regulation and data requirements for GM crop composition have increased dramatically over the last 20years, with a typical study now costing over one million US dollars

The GLP aggregated and excerpted this blog/article to reflect the diversity of news, opinion, and analysis. Read full, original post:Stacking transgenic event DAS-157-1 alters maize composition less than traditional breeding

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Mechanism of environment-microbe-host interactions revealed … – Baylor College of Medicine News (press release)

Posted: at 4:37 am

Researchers at Baylor College of Medicine have uncovered a new mechanism showing how microbes can alter the physiology of the organisms in which they live. In a paper published in Nature Cell Biology, the researchers reveal how microbes living inside the laboratory worm C. elegans respond to environmental changes and generate signals to the worm that alter the way it stores lipids.

Microbe-host interactions have been known for a long time, but the actual molecular mechanisms that mediate the interactions were largely unknown, said senior author Dr. Meng Wang, associate professor of molecular and human genetics at Baylor and the Huffington Center On Aging. Microbes living inside another organism, the host, can respond to changes in the environment, change the molecules they produce and consequently influence the normal workings of the hosts body, including disease susceptibility.

In this study, Wang and first author Dr. Chih-Chun Lin working in the Wang Lab have dissected for the first time a molecular mechanism by which E. coli bacteria can regulate C. elegans lipid storage.

How E. coli changes lipid storage in C. elegans

C. elegans is a laboratory worm model scientists use to study basic biological mechanisms in health and disease.

This worm naturally consumes and lives with bacteria in its gut and interacts with them in ways that are similar to those between humans and microbes. In the laboratory, we can study basic biological mechanisms by controlling the type of bacteria living inside this worm as well as other variables and then determining the effect on the worms physiology, Wang said.

In this study, Wang and Lin compared two groups of worms. One group received bacteria that had been grown in a nutritionally rich environment. The other group of worms received the same type of bacteria, but it had grown in nutritionally poor conditions. Both groups of worms received the same amount and type of nutrients, the only difference was the type of environment in which the bacteria had grown before they were administered to the worms.

Interestingly, the worms carrying bacteria that came from a nutritionally poor environment had in their bodies twice the amount of fat present in the worms living with the bacteria coming from the nutritionally rich environment.

The researchers then carried out more experiments and determined that it was the lack of the amino acid methionine in the nutritionally poor environment that had triggered the bacteria to adapt by producing different compounds that then initiated a cascade of events in the worm that led to extra fat accumulation. In addition, the researchers observed that the tissues showing extra fat accumulation also had their mitochondria fragmented. The activities of the mitochondria, the balance between their fusion and breaking apart, are known to be tightly coupled with metabolic activities.

A mechanism that reveals unsuspected connections

The researchers found that the bacteria were able to trigger mitochondrial fragmentation and then extra lipid accumulation because the molecular intermediates the bacteria had triggered allowed them to establish communication with the mitochondria.

We have found evidence for the first time that bacteria and mitochondria can talk to each other at the metabolic level, Wang said.

Bacteria and mitochondria are like distant relatives. Evolutionary evidence strongly suggests that mitochondria descend from bacteria that entered other cell types and became incorporated into their structure. Mitochondria play essential roles in many aspects of the cells metabolism, but also maintain genes very similar to those of their bacterial ancestors.

Its interesting that the molecules bacteria generate can chime in the communication between mitochondria and regulate their fusion-fission balance, Wang said. Our findings reveal this kind of common language between bacteria and mitochondria, despite them being evolutionary distant from each other.

Some components of this common language involve proteins such as NR5A, Patched and Sonic Hedgehog. The latter is of particular interest to the researchers because it has not been involved in regulating lipid metabolism and mitochondrial dynamics before.

Microbes in the microbiome can affect many aspects of their hosts functions, and here we present a new molecular mechanism mediating microbe-host communication, Wang said. Having discovered one mechanism encourages us to investigate others that may be related to other physiological aspects, such as the stress response and aging, among others.

This project is supported by the National Institutes of Health grants R01AG045183, R01AT009050, DP1DK113644 and grants from the Howard Hughes Medical Institute. It also is supported in part by a training fellowship from the Burroughs Wellcome Fund and The Houston Laboratory and Population Science Training Program in Gene-Environment Interaction of the University of Texas Health Science Center at Houston (BWF Grant 1008200).

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A Promising Model for a Devastating Genetic Deficiency … – Technology Networks

Posted: at 4:37 am

Researchers from the Global Research Cluster in Japan have developed a potential mouse model for the genetic disorder known as an NGLY1 deficiency. Published in the journal PLOS Genetics, the study describes how a complete knockout of the Ngly1 gene in mice leads to death just before birth, which can be partially rescued by a second knockout of another gene called Engase. When related genes in the mice used for making the knockouts are variable, the doubled-deletion mice survive and have symptoms that are analogous to humans with NGLY1-deficiency, indicating that these mice could be useful for testing potential therapies.

NGLY1-deficiency is a relatively newly discovered genetic disorder, with the first patient identified in 2012. The symptoms are severe, and include delayed development, disordered movement, low muscle tone and strength, and the inability to produce tears. Understanding how lack of NGLY1 leads to these symptoms is critical when considering targets for therapeutic interventions, and creating useful animal models of the disease is therefore equally important.

The RIKEN team has already had some success studying the consequences of Ngly1 deficiency in cultured animal cells. The Ngly1 gene codes for an enzyme that helps remove sugar chains from proteins that are scheduled for degradation. Their research showed that when Ngly1 was absent, sugars normally removed by Ngly1 were improperly removed by another enzyme called ENGase. Knocking out the ENGase gene led to normal protein degradation.

In the current study, the researchers first examined the effects of knocking out Ngly1 in mice. They found that when mice lacked both Ngly1 genesone from each parentthey always died just before birth. However, a double knockout of both Ngly1 and ENGase genes resulted in mice that survived after birth, but not for very long.

This positive result was actually unexpected. We thought that ENGase acted further downstream to Ngly1 in the catabolism of glycoproteins notes team leader Tadashi Suzuki, and were surprised when the double knockout was able to suppress the lethality of Ngly1-KO mice. If ENGase was merely an enzyme downstream of Ngly1, nothing should have happened. This was truly a case of serendipity.

Although the double knockout mice survived, they shared several defects that are similar to the symptoms observed in people with NGLY1-deficiency. As these mice aged, they developed characteristics such as bent spines, trembling, limb-clasping and shaking, and by 45 weeks, the survival rate was reduced to 60%. These mice could therefore be useful model mice for developing treatments for the human genetic disorder.

Another factor affecting survival and symptoms turned out the be the genetic background of the mice, that is, the genotypes of all genes related to Ngly1 and Engase, which likely affect how they function. When mice were crossed with an outbred strain, the single Ngly1 knockout proved less lethal, and the double knockout proved to be even more helpful, with mice only showing hind-limb clasping after 30 weeks.

These findings show that the biological processes involved are quite complicated. Despite this however, it is clear that preventing ENGase from acting can alleviate symptoms of Ngly1 deficiency in mice. Figuring out which aspects of the genetic background help reduce symptoms is perhaps a long-term goal.

Although the condition was only recently discovered, research into NGLY1-deficiency has been facilitated through efforts from the Grace Science Foundation, and the RIKEN team has recently begun a collaboration with Takeda Pharmaceuticals and T-CiRA at Kyoto University.

For now, the next step, says Suzuki, will be to isolate an in vivo inhibitor for ENGase and determine whether it can improve the symptoms related to NGLY1-deficiency. As we do not know much about the pathophysiology of the disorder, this might help us find potential targets for therapy, but also might lead to a better understanding of other diseases. Such chains of unexpected results are the beauty of basic science!

This article has been republished frommaterialsprovided byRIKEN. Note: material may have been edited for length and content. For further information, please contact the cited source.

Reference

Fujihira, H., Masahara-Negishi, Y., Tamura, M., Huang, C., Harada, Y., Wakana, S., . . . Suzuki, T. (2017). Lethality of mice bearing a knockout of the Ngly1-gene is partially rescued by the additional deletion of the Engase gene. PLOS Genetics, 13(4). doi:10.1371/journal.pgen.1006696

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Research presentations at Syracuse autism symposium connect scientists across disciplines – Auburn Citizen

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SYRACUSE A conference held last week at SUNY Upstate Medical University in Syracuse brought together scientists studying autism from different aspects and emphases of the disorder in a way that will benefit one another's research.

That is what Dr. Brian Howell, a Skaneateles resident who researches autism as it relates to brain development at Upstate, observed following the two-day "Autism Symposium 2017: Where We Are, Where We Are Going" that he organized through Upstate's Department of Neuroscience & Physiology.

Calling the symposium a success, Howell said it was the first such event that tried to include the public along with the scientists. The first day which featured "Nightline" correspondent John Donvan speaking about changing attitudes about autism was geared toward the general public.

But, Howell said, some people came back for the second day when scientists from a variety of institutions and backgrounds came together to share their research in a series of presentations.

Those presentations included "a good mix of people that probably don't even necessarily go to the same meetings," Howell said, because of the differences in their disciplines.

"We got people talking across sub-fields in this area, so a lot of scientists said to me that they really appreciated this in terms of not only the science that they heard but also the interpersonal connections that they made," he said.

That goes for him and his department as well, he added. He and his team work with mouse genetics in their research but follow the research in human genetics. There is so much data out there, though, that one needs to be a computer specialist in order to use the data.

"For us, to meet some really good data miners, I think, will help drive our research that we now can set up some collaborations and look more closely at the human data and see how that might inform our work in mice," Howell said. "For me, probably the most benefit I got out of all this work is being able to call up people in different specialties and get their point of view on things."

Along with Donvan, the first day of talks included Dr. Stephan Sanders, from University of California San Francisco, discussing his work sequencing the genomes of thousands of families with autism spectrum disorder to look for gene mutations that might be able to predict autism in children.

Following Sanders, Dr. Arthur Beaudet, from Baylor College of Medicine, talked about a new technology he is developing a blood test for pregnant mothers to isolate fetal cells in the bloodstream, sequence those cells and look for mutations known to be predictors for autism.

On the second day of presentations:

Dr. Steven Hicks, of Penn State College of Medicine, talked about a start-up company, Motion Intelligence, that is developing a noninvasive oral swab to test children's saliva for signs of autism and determine a treatment program when early intervention is most effective.

Dr. Gahan Pandina, of Janssen Research & Development, a branch of Johnson & Johnson, presented on the Autism Anchor app that allows parents to document the behavior of their children with autism in order to provide clinicians with more information during appointments.

Dr. Joseph Dougherty, of Washington University in St. Louis, spoke about computer programs he is using to determine what brain regions and cell types are being impacted by autism and the databases that can put together mutations, cell types and brain regions involved in autism.

Dr. Janine LaSalle, of University of California Davis, highlighted the environmental factors that lead to autism, citing a study that found that prenatal exposure to polychlorinated biphenyls may cause a particular chromosome duplication that leads a child to develop autism.

Weirui Guo, from University of Texas Southwestern, shared his research about a sub-class of autism found in those with fragile X syndrome, a male-specific disorder caused by a defect in the X chromose that results in the overproduction of a certain protein.

Howell gave a presentation about the developmental genes with which he and his team work mice and how mutations in those genes might contribute to autism in both mice and people when autism, unlike mental retardation, does not present obvious brain defects.

As far as where the research in autism goes from here following the symposium both personally and in the wider community, Howell said he and his team hope to take a closer look at human genetics to complement their studies using mice but need partners to be able to do that.

"The human genetic data now, there's so much of it. It's in these massive databases that you basically need a computer degree to be able to access," he said. "We hope to reach out to the computer experts that we've met and mine the genetic data to see if we can develop networks of genes that are involved in autism."

He noted that there is no single mutation that causes autism, but a collection of mutations in an individual adds up to the disorder. Using human genetic data and testing that data in mice, his team might be able to figure out what series of mutations in people lead to autism.

"There are hundreds of genes that might make you at risk for autism, but no one mutation on its own is sufficient," Howell said.

Journal Editor Jonathan Monfiletto can be reached at jonathan.monfiletto@lee.net or (315) 283-1615. Follow him on Twitter @WOC_Monfiletto.

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Research presentations at Syracuse autism symposium connect scientists across disciplines - Auburn Citizen

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