What is the Benefits of ISS Research - A interview Video

Earth framing the International Space Station

Earth framing the International Space Station in May 2010 following undocking of Atlantis during the STS-132 mission. (NASA)

Almost as soon as the International Space Station was habitable, researchers began using it to study the impact of microgravity and other space effects on several aspects of our daily lives. This unique scientific platform continues to enable researchers from all over the world to put their talents to work on innovative experiments that could not be done anywhere else. 

Although each space station partner has distinct agency goals for station research, each partner shares a unified goal to extend the resulting knowledge for the betterment of humanity. We may not know yet what will be the most important discovery gained from the space station, but we already have some amazing breakthroughs! In the areas of human health, telemedicine, education and observations of Earth from space, there are already demonstrated benefits to human life. Vaccine development research, station-generated images that assist with disaster relief and farming, and education programs that inspire future scientists, engineers and space explorers are just some examples of research benefits. 

The stories featured here summarize the scientific, technological and educational accomplishments of research on the space station that has and will continue to have an impact on life on Earth.

The benefits outlined here serve as examples of the space station's potential as a groundbreaking scientific research facility. Through advancing the state of scientific knowledge of our planet, looking after our health, and providing a space platform that inspires and educates the science and technology leaders of tomorrow, these benefits will drive the legacy of the space station as its research strengthens economies and enhances the quality of life here on Earth for all people.

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Source: Nasa

UCLA and CASIS to collaborate on International Space Station study of possible therapy for bone loss

A study of rodents on the International Space Station will allow astronauts to test the ability of a bone-forming molecule to direct stem cells to induce bone formation. Credit: Nasa

UCLA has received grant funding from the Center for the Advancement of Science in Space to lead a research mission that will send rodents to the International Space Station. The mission will allow astronauts on the space station and scientists on Earth to test a potential new therapy for accelerating bone growth in humans. 

The research will be led by Dr. Chia Soo, a UCLA professor of plastic and reconstructive surgery and orthopaedic surgery who is member of the Eli and Edythe Broad Center of Regenerative Medicine and Stem Cell Research. Soo also is the research director for UCLA Operation Mend, which provides medical care for wounded warriors.

The study will test the ability of a bone-forming molecule called NELL-1 to direct stem cells to induce bone formation and prevent bone degeneration. Their work will build upon previous UCLA studies that were funded by the NIH.

Other members of the UCLA research team are Dr. Kang Ting, a professor of dentistry who discovered NELL-1 and is leading efforts to translate NELL-1 therapy to humans; Dr. Ben Wu, a professor of bioengineering and dentistry who modified the NELL-1 molecule to make it useful for treating osteoporosis; and Dr. Jin Hee Kwak, an assistant professor of dentistry who will manage the study’s daily operations.

Prolonged space flights induce extreme changes in bone and organ systems that cannot be replicated on Earth.

The UCLA–ISS team, which will begin ground operations in early 2015, hopes that the study will provide new insights into the prevention of bone loss or osteoporosis as well as the regeneration of massive bone defects that can occur in wounded military personnel. Osteoporosis is a significant health issue commonly associated with “skeletal disuse” conditions such as immobilization, stroke, cerebral palsy, muscular dystrophy, spinal cord injury and jaw resorption after tooth loss.

“NELL-1 holds tremendous hope not only for preventing bone loss, but one day even restoring healthy bone,” Ting said. “For patients who are bed-bound and suffering from bone loss, it could be life-changing.” 

The UCLA team will oversee the ground operations of the mission in tandem with a flight operation coordinated by CASIS and NASA.  

“A group of 40 rodents will be sent to the International Space Station U.S. National Laboratory onboard the SpaceX Dragon capsule, where they will live for two months in a microgravity environment during the first ever test of NELL-1 in space,” said Dr. Julie Robinson, NASA’s chief scientist for the International Space Station program at the Johnson Space Center.

“CASIS is proud to work alongside UCLA in an effort to promote the station as a viable platform for bone loss inquiry,” said Warren Bates, director of portfolio management for CASIS. “Through investigations like this, we hope to make profound discoveries and enable the development of therapies to counteract bone loss ailments common in humans.”

“Besides testing the limits of NELL-1’s robust bone-producing effects, this mission will provide new insights about bone biology and could uncover important clues for curing diseases such as osteoporosis,” Wu said. 

“NIH has been pleased to work with NASA and CASIS to encourage the use of the International Space Station as a unique microgravity environment that can test innovative hypotheses that will benefit human health on Earth,” said Dr. Joan A. McGowan, director of the division of musculoskeletal diseases at the National Institute of Arthritis and Musculoskeletal and Skin Diseases, part of the NIH.

“This research has enormous translational application for astronauts in space flight and for patients on Earth who have osteoporosis or other bone-loss problems from disease, illness or trauma,” Soo said. “We very much appreciate the dedicated review staff at CASIS and the Center for Scientific Review, the portal for NIH grant applications, who made this effort possible.”

The research is supported by grants from the Center for the Advancement of Science in Space and National Institutes of Health. Additional funding and support are provided by the Eli and Edythe Broad Center of Regenerative Medicine and Stem Cell Research at UCLA, the UCLA School of Dentistry, UCLA department of orthopaedic surgery and the UCLA Orthopaedic Hospital Research Center.

Source: UCLA

DNA survives critical entry into Earth's atmosphere

This image shows the launch of the rocket TEXUS-49 from the Esrange Space Center in Kiruna, North Sweden. Credit: Adrian Mettauer

The genetic material DNA can survive a flight through space and re-entry into Earth's atmosphere -- and still pass on genetic information. A team of scientists from UZH obtained these astonishing results during an experiment on the TEXUS-49 research rocket mission.

Applied to the outer shell of the payload section of a rocket using pipettes, small, double-stranded DNA molecules flew into space from Earth and back again. After the launch, space flight, re-entry into Earth's atmosphere and landing, the so-called plasmid DNA molecules were still found on all the application points on the rocket from the TEXUS-49 mission. And this was not the only surprise: For the most part, the DNA salvaged was even still able to transfer genetic information to bacterial and connective tissue cells. "This study provides experimental evidence that the DNA's genetic information is essentially capable of surviving the extreme conditions of space and the re-entry into Earth's dense atmosphere," says study head Professor Oliver Ullrich from the University of Zurich's Institute of Anatomy.

Spontaneous second mission

The experiment called DARE (DNA atmospheric re-entry experiment) resulted from a spontaneous idea: UZH scientists Dr. Cora Thiel and Professor Ullrich were conducting experiments on the TEXUS-49 mission to study the role of gravity in the regulation of gene expression in human cells using remote-controlled hardware inside the rocket's payload. 

During the mission preparations, they began to wonder whether the outer structure of the rocket might also be suitable for stability tests on so-called biosignatures. "Biosignatures are molecules that can prove the existence of past or present extraterrestrial life," explains Dr. Thiel. And so the two UZH researchers launched a small second mission at the European rocket station Esrange in Kiruna, north of the Arctic Circle.

DNA survives the most extreme conditions

The quickly conceived additional experiment was originally supposed to be a pretest to check the stability of biomarkers during spaceflight and re-entry into the atmosphere. Dr. Thiel did not expect the results it produced: "We were completely surprised to find so much intact and functionally active DNA." The study reveals that genetic information from the DNA can essentially withstand the most extreme conditions.

Various scientists believe that DNA could certainly reach us from outer space as Earth is not insulated: in extraterrestrial material made of dust and meteorites, for instance, around 100 tons of which hits our planet every day.

This extraordinary stability of DNA under space conditions also needs to be factored into the interpretion of results in the search for extraterrestrial life: "The results show that it is by no means unlikely that, despite all the safety precautions, space ships could also carry terrestrial DNA to their landing site. We need to have this under control in the search for extraterrestrial life," points out Ullrich.

Source: University of Zurich

Plants return to Earth after growing in space

Astronaut Reid Wiseman injected a fixative solution onto the seedlings. Credit: NASA

Researchers at Simon Gilroy's lab in the Department of Botany at the University of Wisconsin-Madison this afternoon greeted a truck carrying small containers holding more than 1,000 frozen plants that germinated and grew aboard the International Space Station.

On Tuesday, when Gilroy's team inspected the plants at the Kennedy Space Center in Florida, they saw exactly what they wanted: Petri dishes holding seedlings that sprouted and grew in weightlessness.

After their arrival in Madison, the plants went directly into a deep freeze. After being thawed in a few months, they will donate their RNA to an instrument that will measure the activity of all of their approximately 30,000 genes.

Half of the plants will become subjects in Gilroy's longstanding exploration of the genetic control of the proteins that enable plants to grow in zero gravity. "Gravity is a fantastically pervasive force that affects all biology," says Gilroy. "One astronaut observed that plants get lazy in a weightless environment; they grow long and thin, and don't lay down strong material, just like people lose bone mass in space because it isn't needed for supporting weight."

The other half of the experiment represents a departure for Gilroy, and for NASA, the agency supporting this area of space research. After these plants undergo a similar genetic analysis at UW-Madison's Biotech Center, the data will get an initial check-over from Gilroy's group. And then a treasure trove of digital data on plant genetic activity in microgravity will be made available to any researcher interested in mining it.

"Access to space is very rare," Gilroy says. "Traditionally, a research group will put an experiment in space, get the results and publish. But NASA is trying a new mode, called geneLAB, where the research group will put organisms in space, then, as soon as possible, release the raw data to anyone who wants to analyze it. They hope it will speed up major advances on these tiny samples that we can afford to place in space. I see this as open-source science."

Through the process called transcription, genes produce RNA that becomes the template for proteins, and in both sets of experiments, the RNA data will show which genes become more or less active in microgravity, when compared to an identical set of plants grown on Earth.

While Gilroy plans to focus on structural proteins, the geneLAB experiment compares four variants of Arabidopsis called ecotypes. "This data should provide a broad field of investigation -- far more than one lab can handle," Gilroy says. "We are going to end up with an enormous amount of transcription data. We will do some initial work to check the major genes which go up or down, but there's tremendous potential for further analysis by other labs around the world."

But while the geneLab approach sounds promising, Gilroy concedes that it carries no guarantees. "This may be a path forward in crowd-sourcing science. At the least, as a single lab we could never analyze this data as fully as many labs around the world all working with it."

The "Biological Research in Canister" containers that held these experiments on board the space station were designed, tested and operated according to NASA's rigorous approach, Gilroy says. "Each project represents an enormous investment, and you really want everything to go perfectly. You become one of the most careful scientists in the world. You test everything, make duplicates, and are always considering what may go wrong so you can do another test."

NASA is an unfamiliar world to most botanists, but Gilroy seems to be enjoying every step of the way, and has even learned the organization's peculiar parlance. "At first, talking in acronyms is very strange," he says, "and you can't understand anything when NASA people start going into NASA-speak. But once you get into it, you catch yourself doing the exact same thing."

In the microgravity experiments, Gilroy is exploring the genetic basis of a phenomenon known to gardeners and horticulturalists for many years. Plants that grow up without mechanical stresses -- due to wind, rain or other disturbances -- "are much more susceptible to pests, are not as robust," Gilroy says, "but if you go into a greenhouse and shake the plants, they grow up more compact, strong, and resistant to stress. They are even more resistant to plant diseases."

It turns out that the same signaling system used to detect mechanical stresses like gravity is also used to defend against pathogens. That may explain why plants in space appear more susceptible to disease.

That overlap raises the stakes for understanding the impact of gravity on plants beyond the notion of building stronger crops that can stand up in the field. Understanding the signals could help in the never ending battle against plant disease.

Likewise, NASA has its own practical interest in the research: Plants will supply food and oxygen for long-distance space travel, and keeping them healthy will be a matter of life and death. "If you are growing plants as part of a human life support system," Gilroy says, "you'd rather not have them suddenly die."

Source: University of Wisconsin-Madison

Breezy science, plant studies and more head to space station on SpaceX-4

This Artist's rendering of the ISS-RapidScat instrument (inset), will measure ocean surface wind speed and direction and help improve weather forecasts. It will be installed on the end of the station's Columbus laboratory. Credit: NASA/JPL-Caltech/Johnson Space Center

Imagine a dragon flying through the heavens on mighty, outstretched wings. The majestic beast knows the currents of winds and how to harness their power as it soars above the clouds. SpaceX's real Dragon -- the company's spacecraft that transports supplies and science to the International Space Station (ISS) -- will deliver, and later return, new technology, biology and biotechnology and Earth and space science research to the orbiting outpost.

One of the new Earth science investigations heading into orbit is the ISS-Rapid Scatterometer (ISS-RapidScat). ISS-RapidScat monitors ocean winds from the vantage point of the space station. This space-based scatterometer is a remote sensing instrument that uses radar pulses reflected from the ocean's surface at different angles to calculate surface wind speed and direction. This information will be useful for weather forecasting and hurricane monitoring.

"We'll be able to see how wind speed changes with the time of day," said Ernesto Rodríguez, principal investigator for ISS-RapidScat at NASA's Jet Propulsion Laboratory in Pasadena, California. "ISS-RapidScat will link together all previous and current scatterometer missions, providing us with a more complete picture of how ocean winds change. Combined with data from the European ASCAT scatterometer mission, we'll be able to observe 90 percent of Earth's surface at least once a day, and in many places, several times a day."

In addition to improving weather models, RapidScat enhances measurements from other international scatterometers by cross-checking their data. Due to its unique orbit, RapidScat will observe different parts of the planet at different times of day. This allows the instrument to track the effects of the sun on ocean winds as the day progresses. Because the instrument reuses leftover hardware originally built to test parts of the now inoperable NASA QuikScat scatterometer, this investigation demonstrates a unique way to replace an instrument aboard an aging satellite.

New biomedical hardware launching on SpaceX's fourth commercial resupply mission to the space station will facilitate prolonged biological studies in microgravity. The Rodent Research Hardware and Operations Validation (Rodent Research-1) investigation provides a platform for long-duration rodent experiments in space. These experiments examine how microgravity affects animals, providing information relevant to human spaceflight, discoveries in basic biology and knowledge that may have direct impact toward human health on Earth. Rodent Research-1 tests the operational capabilities of the new hardware system, including the transporter, rodent habitat and access unit.

Because rodents experience developmental stages and aging processes more quickly than humans, they make ideal research model organisms to infer information about disease development and progression in humans. Model organisms are non-human species with characteristics that allow them easily to be maintained, reproduced and studied in a laboratory.

"In the coming years, rodent studies conducted aboard the space station will gather foundational data that will help advance human space exploration and provide new opportunities to improve quality of life on Earth," said Ruth Globus, Ph.D., Rodent Research Project scientist and researcher in the Space Biosciences Division at NASA's Ames Research Center in Moffett Field, California.

Another biological research investigation aboard Dragon includes a new plant study. The Biological Research in Canisters (BRIC) hardware has supported a variety of plant growth experiments aboard the space station. The BRIC-19 investigation, the first to collect data for the geneLAB research platform, will focus on the growth and development of Arabidopsis thaliana seedlings in microgravity. A. thaliana is a small flowering plant related to cabbage, and its genetic makeup is simple and well-understood by the plant biology community. This knowledge offers easy recognition of any changes that occur as a result of microgravity adaptation.

Plant development on Earth is impacted by mechanical forces such as wind or a plant's own weight. Researchers hope to get a better understanding of how the growth responses of plants are altered by the absence of these forces when grown in microgravity.

The BRIC hardware helps to maximize research and minimize space and crew time since it does not use power to operate and the canister is the size of a bread box. This study may add to the collective body of knowledge about basic plant growth phenomena and could help improve farming practices on Earth.

In addition to Earth and biological science studies, several new technology demonstrations are making their way to the space station. One of those, known as the Special Purpose Inexpensive Satellite, or SpinSat, will test how a small satellite moves and positions itself in space using new thruster technology. It will launch into orbit from the space station through the new Cyclops small satellite deployer, also known as the Space Station Integrated Kinetic Launcher for Orbital Payload Systems (SSIKLOPS).

SpinSat is a spherical satellite measuring 22 inches in diameter. It will test advanced thruster technology that uses a new class of non-pyrotechnic materials known as Electrically-Controlled Solid Propellants (ESP). ESPs are ignited only by electric current.

Researchers can use high-resolution atmospheric data captured by SpinSat to determine the density of the thermosphere, one of the uppermost layers of the atmosphere. With better knowledge of the thermosphere, engineers and scientists can refine satellite and telecommunications technology.

Another new technology demonstration catching a ride on the Dragon is the 3-D Printing In Zero-G Technology Demonstration (3-D Printing In Zero-G), which will be the first ever 3-D printer in space. Additive manufacturing could enable parts to be manufactured quickly and cheaply in space, instead of waiting for the next cargo resupply vehicle delivery. The research team also can gain valuable insight into improving 3-D printing technology on Earth by demonstrating it in microgravity.

With so many new investigations that directly impact human life, this Dragon's delivery is helping the space station make discoveries off the Earth, for the Earth.

Source: Nasa

Latest measurements from the AMS experiment unveil new territories in the flux of cosmic rays

The Alpha Magnetic Spectrometer (AMS[1]) collaboration has today presented its latest results. These are based on the analysis of 41 billion particles detected with the space-based AMS detector aboard the International Space Station. Credit: Image courtesy of CERN

The Alpha Magnetic Spectrometer (AMS[1]) collaboration has today presented its latest results. These are based on the analysis of 41 billion particles detected with the space-based AMS detector aboard the International Space Station. The results, presented during a seminar at CERN[2], provide new insights into the nature of the mysterious excess of positrons observed in the flux of cosmic rays. The findings are published today in the journal Physical Review Letters.

Cosmic rays are particles commonly present in the universe. They consist mainly of protons and electrons, but there are also many other kinds of particles, including positrons, travelling through space. Positrons are the antimatter counterparts of electrons, with the same mass but opposite charge. The presence of some positrons in space can be explained from the collisions of cosmic rays, but this phenomenon would only produce a tiny portion of antimatter in the overall cosmic ray spectrum. Since antimatter is extremely rare in the universe, any significant excess of antimatter particles recorded in the flux of energetic cosmic rays indicates the existence of a new source of positrons. Very dense stars, such as pulsars, are potential candidates.

The AMS experiment is able to map the flux of cosmic rays with unprecedented precision and in the results published today, the collaboration presents new data at energies never before recorded. The AMS collaboration has analysed 41 billion primary cosmic ray events among which 10 million have been identified as electrons and positrons. The distribution of these events in the energy range of 0.5 to 500 GeV shows a well-measured increase of positrons from 8 GeV with no preferred incoming direction in space. The energy at which the positron fraction ceases to increase has been measured to be 275±32 GeV.

"This is the first experimental observation of the positron fraction maximum after half a century of cosmic rays experiments," said AMS spokesperson Professor Samuel Ting. 

"Measurements are underway by the AMS team to determine the rate of decrease at which the positron fraction falls beyond the turning point."

This rate of decrease after the "cut-off energy" is very important to physicists as it could be an indicator that the excess of positrons is the signature of dark matter particles annihilating into pairs of electrons and positrons. Although the current measurements could be explained by objects such as pulsars, they are also tantalizingly consistent with dark matter particles with mass of the order of 1 TeV. Different models on the nature of dark matter predict different behaviour of the positron excess above the positron fraction expected from ordinary cosmic ray collisions. Therefore, results at higher energies will be of crucial importance in the near future to evaluate if the signal is from dark matter or from a cosmic source.

"With AMS and with the LHC to restart in the near future at energies never reached before, we are living in very exciting times for particle physics as both instruments are pushing boundaries of physics," said CERN Director-General Rolf Heuer.

AMS also reported a new observation that both the electron flux and the positron flux change their behaviour at about 30 GeV, the fluxes being significantly different from each other both in their magnitude and energy dependence. In particular, between 20 and 200 GeV, the rate of change of the positron flux is surprisingly higher than that for electrons. 

This is important proof that the excess seen in the positron fraction is due to a relative excess of high-energy positrons, and not the loss of high-energy electrons. This new result is very important for a better understanding of the origin of cosmic ray electrons and positrons, and may be the sign of an unknown phenomenon.

In his seminar, Professor Ting also presented some interesting new results to be published in the near future. These show that, at high energies and over a wide energy range, the combined flux of electrons plus positrons can be described by a single constant spectral index, with no existence of structure as suspected by previous measurements of other experiments.

Notes:

[1] The AMS detector is operated by a large international collaboration led by Nobel laureate Samuel Ting. AMS involves about 600 researchers from China, Denmark, Finland, France, Germany, Italy, Korea, Mexico, the Netherlands, Portugal, Spain, Switzerland, Taiwan, and the United-States. The AMS detector was assembled at CERN, tested at ESA's ESTEC centre in the Netherlands and launched on 16 May 2011 onboard NASA's Space Shuttle Endeavour. It is installed on the International Space Station where it tracks incoming charged particles such as protons, electrons and antimatter particles such as positrons, mapping the flux of cosmic rays with unprecedented precision.

[2] CERN, the European Organization for Nuclear Research, is the world's leading laboratory for particle physics. Its headquarters are in Geneva. Its Member States are currently: Austria, Belgium, Bulgaria, the Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Israel, Italy, the Netherlands, Norway, Poland, Portugal, the Slovak Republic, Spain, Sweden, Switzerland and the United Kingdom. Romania is a Candidate for Accession and Serbia is an Associate Member State in the pre-stage to Membership. India, Japan, the Russian Federation, the United States of America, Turkey, the European Commission and UNESCO have Observer status.

Source: CERN

CASIS research set for launch aboard SpaceX mission to space station

The Bone Densitometer developed by Techshot, Inc. will enable X-ray testing for research studies aboard the International Space Station. Credit: CASIS

This fall marks another commercial cargo flight to the International Space Station. In September, SpaceX's Dragon spacecraft is scheduled to blast off to the orbital laboratory carrying supplies and investigations as part of the company's fourth contracted mission to the complex.

Included in the cargo will be the third suite of research investigations sponsored by the Center for the Advancement of Science in Space (CASIS). With the role of managing the U.S. National Laboratory on the space station, CASIS is responsible for brokering and facilitating research investigations on the station with clear Earth applications and benefits.

The latest collection of CASIS-sponsored research, termed Advancing Research Knowledge (ARK)-2, centers heavily on life sciences. Studies include those focused on drug development, disease understanding and validation testing. Each investigation will use the unique conditions aboard the space station to advance researchers' understanding in those areas of study.

Additionally, CASIS and NASA have partnered with Techshot Inc., of Greenville, Indiana, to develop a new hardware device capable of assisting with research that may improve understandings of muscle wasting and diseases like osteoporosis.

The CASIS-sponsored hardware and life science investigations destined for the space station's national laboratory include the Bone Densitometer, which will be the first X-ray machine installed on the space station. A joint project between CASIS, NASA and Techshot, the facility will be instrumental in conducting rodent research on station. The Bone 

Densitometer will allow astronauts to examine bone density of model organisms in space through the use of Dual-Energy X-ray Absorptiometry (DEXA) technology. In short, researchers will be able to assess bone density loss by measuring energy levels absorbed by bones via the device.

The Rodent Research-1 investigation kicks off a series of NASA and CASIS-sponsored investigations focused on rodent research aboard the space station. The study will be the first to use the Bone Densitometer in an effort to help scientists examine the effects of long duration spaceflight. There are numerous applications to these investigations including studying bone loss, muscle atrophy and cardiovascular anomalies. However, the primary focus of this inaugural mission will be to assess the operational capabilities of the new hardware designed for these investigations.

The Drug Metabolism study will assist researchers in the area of drug development and human biology. This investigation is led by a scientist from the U.S. Department of Veteran Affairs, Dr. Timothy Hammond, who is looking to study yeast cells in microgravity. The goal of this investigation is to explore the changes in these cells in space to improve drug development for various diseases, including cancer therapeutics.

The Protein Crystal Optimization study is an investigation aiming to leverage the unique location of the space station to examine the internal structure of three medically important proteins. The space environment should allow researchers to grow the selected protein crystals to an optimal size and quality to allow for closer examination via neutron diffraction. This protein crystal growth in microgravity may reveal new characteristics that are masked by gravity on Earth. By studying these three proteins, medically relevant to salmonella infection, peptic ulcer disease, and biomarkers for heart attack and liver disease, researchers can apply insights towards improved treatments.

A New Era In Commercial Use of the Space Station

The space station's national laboratory affords researchers the ability to conduct experiments in a distinctive environment with factors and variables that are near impossible to replicate on the ground. With access to our nation's only orbiting laboratory, CASIS works with new and non-traditional users to take advantage of this resource. A great example of novel commercial research heading to station is the Cobra Puma Golf investigation.

The Cobra Puma Golf-electroplating investigation, also launching aboard SpaceX, is a materials science investigation sponsored by CASIS in collaboration with COBRA PUMA Golf (CPG). The CPG research and development team will examine the impacts of microgravity on electroplating -- the process of coating a metallic surface using an electric current. The study will test a variety of coating substances on materials used in golf equipment manufacturing. The insight gained from this investigation will aid CPG in identifying improved material development techniques.

CPG's project is another example of a commercial user leveraging the capabilities of the ISS National Lab to advance ground research. Through brokering research investigations with commercial companies, CASIS hopes to demonstrate the space station is not only a test-bed for groundbreaking research and development, but a unique laboratory that can help differentiate investigations initiatives from ground-based studies.

The mission is another milestone for the space community, showcasing how commercial endeavors can work hand-in-hand with research goals. The studies of ARK-2 exemplify the diverse possibilities for the space station and users of the research platform. From commercial launch providers that transport investigations to space, to commercial researchers looking to use the national laboratory, science in space is good for life on Earth.

Source: NASA

Keeping upright: How much gravity is enough?

The experimental setup. (A) Participants lay on a human centrifuge with their feet out so that centripetal force from the centrifuge produced a centripetal force simulating gravity along the long axis of the body. (B) They viewed a screen mounted above their heads which presented a scene tilted at 112° relative to their bodies. The direction signaled by each cue to upright is indicated by arrow: red, vision; green, simulated gravity and blue, the body. (C) Thus, the three vectors involved in determining the perceptual upright (body, gravity and vision) could be dissociated.
 Credit: Harris et al; doi:10.1371/journal.pone.0106207.g001

Keeping upright in a low-gravity environment is not easy, and NASA documents abound with examples of astronauts falling on the lunar surface. Now, a new study by an international team of researchers led by York University professors Laurence Harris and Michael Jenkin, published today in PLOS ONE, suggests that the reason for all these moon mishaps might be because its gravity isn't sufficient to provide astronauts with unambiguous information on which way is "up."

"The perception of the relative orientation of oneself and the world is important not only to balance, but also for many other aspects of perception including recognizing faces and objects and predicting how objects are going to behave when dropped or thrown," says Harris. "Misinterpreting which way is up can lead to perceptual errors and threaten balance if a person uses an incorrect reference point to stabilize themselves."

Using a short-arm centrifuge provided by the European Space Agency, the international team simulated gravitational fields of different strengths, and used a York-invented perceptual test to measure the effectiveness of gravity in determining the perception of up. 

The team found that the threshold level of gravity needed to just influence a person's orientation judgment was about 15 per cent of the level found on Earth -- very close to that on the moon.

The team also found that Martian gravity, at 38 per cent of that on Earth, should be sufficient for astronauts to orient themselves and maintain balance on any future manned missions to Mars.

"If the brain does not sense enough gravity to determine which way is up, astronauts may get disoriented, which can lead to errors like flipping switches the wrong way or moving the wrong way in an emergency," says Jenkin. "Therefore, it's crucial to understand how the direction of up is established and to establish the relative contribution of gravity to this direction before journeying to environments with gravity levels different to that of Earth."

This work builds upon results obtained in long-duration microgravity by Harris and Jenkin and other members of York's Centre for Vision Research on board the International Space Station during the Bodies in the Space Environment project, funded by the Canadian Space Agency.

Source: York University

Where do astronauts go when they need 'to go?'

NASA researchers sought to design a way to contain urine in the inevitable event that future astronauts would need 'to go' while wearing their spacesuits.

Alan Shepard became the first American to fly in space on May 5, 1961. Although NASA engineers had put considerable planning into his mission, dubbed Freedom 7, noticeably missing from this extensive preparation was a way for him to urinate in his spacesuit. 

During a lengthy launch delay, the inevitable happened, and Shepard's urine short-circuited his electronic biosensors. In less than a year, engineers had remedied this seeming oversight for John Glenn's Mercury orbital flight. The system developed for Glenn stood the test of time, remaining in use until the early days of the Space Shuttle program.

In a new article, Hunter Hollins of the National Air and Space Museum reviews the history of urine collection in space and the considerations necessary to accommodate this basic physiological function. That first successful urine collection device, used in 1962, has been on display at the National Air and Space Museum since 1976.

The new article, titled "Forgotten Hardware: How to Urinate in a Spacesuit," appears in the June 2013 edition of Advances in Physiology Education, a journal published by the American Physiological Society

No Need "To Go?"

Hollins writes that though the general public was interested in how astronauts would tackle taking care of this basic need in space (a letter stored in NASA's Historical Reference Collection from a Pennsylvania schoolgirl questioned where the first man in space would use the toilet), NASA's scientists and technicians seemed to ignored the problem before Shepard's mission. Combined with a lack of funding and little crosstalk between the organizations that would end up comprising NASA, scientists in the organization also assumed that the first astronauts would be able to "hold it" during their very short missions.

However, though Shepard's spaceflight was scheduled to last only 15 minutes, he spent eight hours in his spacesuit due to launch delays. During a four-hour stint on the launch pad, he relieved himself in the suit, damaging the electronic medical data sensors attached to his body.

After this understandable event, NASA researchers sought to design a way to contain urine in the inevitable event that future astronauts would need to go while wearing their spacesuits.

New Device a Relief for Astronauts

Working around the spacesuit itself was one barrier to successful urine collection. The pressure suits worn by astronauts help keep their occupants alive during spaceflight by ensuring that pressures inside stay within a healthy physiological range. However, the bulky, uncomfortable suits left little room for devices to capture urine.

The first iteration of urine collection devices proposed for space were in-dwelling catheters, a tube threaded through the penis to collect urine continuously from the bladder. However, such catheters are extremely uncomfortable and greatly increase the risk of infection.

After Gus Grissom's Mercury-Redstone 4 mission followed Shepard's in 1961 -- in which Grissom urinated between two pairs of rubber pants -- NASA researchers set about developing a more suitable urine collection device. They ended up basing theirs on the simple personal urinals already available at the time for people with medical problems, such as impaired bladder control, or those without access to public urinals, such as police officers on a long shift.

In the end, the resulting device resembled a condom made out of more durable materials and open on one end, with a tube connected to a storage container. On Glenn's Mercury-Atlas 6 mission, he voided a full bladder into the new device, confirming its utility.

Tweaks Still Necessary

Astronauts regularly used this type of device with minimal modifications until the early days of the Space Shuttle program, Hollins writes. However, those and modern urine collection devices still aren't perfect. Hollins notes that in a survey done in 2010, the majority of U.S. Air Force pilots flying high altitude spy planes reported problems with the urine collection devices they wore, including poor fit, leaking, and skin damage from extended contact with urine.

"It is the job of the engineer/physiologist to ensure that the man-machine interface promotes the health and safety of the human body," Hollins says.

Source: American Physiological Society (APS)

NASA's Chandra X-ray Observatory celebrates 15th anniversary

To celebrate Chandra's 15th anniversary, four newly processed images of supernova remnants have been released. Credit: NASA/CXC/SAO

Fifteen years ago, NASA's Chandra X-ray Observatory was launched into space aboard the Space Shuttle Columbia. Since its deployment on July 23, 1999, Chandra has helped revolutionize our understanding of the universe through its unrivaled X-ray vision.

Chandra, one of NASA's current "Great Observatories," along with the Hubble Space Telescope and Spitzer Space Telescope, is specially designed to detect X-ray emission from hot and energetic regions of the universe.

With its superb sensitivity and resolution, Chandra has observed objects ranging from the closest planets and comets to the most distant known quasars. It has imaged the remains of exploded stars, or supernova remnants, observed the region around the supermassive black hole at the center of the Milky Way, and discovered black holes across the universe. Chandra also has made a major advance in the study of dark matter by tracing the separation of dark matter from normal matter in collisions between galaxy clusters. It is also contributing to research on the nature of dark energy.

To celebrate Chandra's 15th anniversary, four new images of supernova remnants -- the Crab Nebula, Tycho, G292.0+1.8, and 3C58 -- are being released. These supernova remnants are very hot and energetic and glow brightly in X-ray light, which allows Chandra to capture them in exquisite detail.

"Chandra changed the way we do astronomy. It showed that precision observation of the X-rays from cosmic sources is critical to understanding what is going on," said Paul Hertz, NASA's Astrophysics Division director in Washington. "We're fortunate we've had 15 years -- so far -- to use Chandra to advance our understanding of stars, galaxies, black holes, dark energy, and the origin of the elements necessary for life."

Chandra orbits far above Earth's X-ray absorbing atmosphere at an altitude up to 139,000 km (86,500 mi), allowing for long observations unobscured by Earth's shadow. When it was carried into space in 1999, it was the largest satellite ever launched by the shuttle.

"We are thrilled at how well Chandra continues to perform," said Belinda Wilkes, director of the Chandra X-ray Center (CXC) in Cambridge, Massachusetts. "The science and operations teams work very hard to ensure that Chandra delivers its astounding results, just as it has for the past decade and a half. We are looking forward to more ground-breaking science over the next decade and beyond."

Originally called the Advanced X-ray Astrophysics Facility (AXAF), the telescope was first proposed to NASA in 1976. Prior to its launch aboard the shuttle, the observatory was renamed in honor of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar. Known to the world as Chandra (which means "moon" or "luminous" in Sanskrit), he was widely regarded as one of the foremost astrophysicists of the 20th century.

"Chandra continues to be one of the most successful missions that NASA has ever flown as measured against any metric -- cost, schedule, technical success and, most of all, scientific discoveries," said Martin Weisskopf, Chandra Project Scientist at the Marshall Space Flight Center in Huntsville, Ala. "It has been a privilege to work on developing and maintaining this scientific powerhouse, and we look forward to many years to come."

To help celebrate this anniversary, Chandra scientists -- including former CXC Director, Harvey Tananbaum -- will participate in a Google+ Hangout July 22 beginning at 3 p.m. EDT. For more information on this event, visit: http://go.nasa.gov/1jXcXYT

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Source: NASA

Gecko grippers get a microgravity test flight

Scientists at NASA's Jet Propulsion Laboratory in Pasadena, California, are working on adhesive gripping tools that could grapple objects such as orbital debris or defunct satellites that would otherwise be hard to handle.
Credit: Image courtesy of NASA/Jet Propulsion Laboratory

There are no garbage trucks equipped to leave the atmosphere and pick up debris floating around Earth. But what if we could send a robot to do the job?

Scientists at NASA's Jet Propulsion Laboratory in Pasadena, California, are working on adhesive gripping tools that could grapple objects such as orbital debris or defunct satellites that would otherwise be hard to handle.

The gecko gripper project was selected for a test flight through the Flight Opportunities Program of NASA's Space Technology Mission Directorate. As a test, researchers used the grippers in brief periods of weightlessness aboard NASA's C-9B parabolic flight aircraft in August.

"Orbital debris is a serious risk to spacecraft, including the International Space Station," said Aaron Parness, a JPL robotics researcher who is the principal investigator for the grippers. "This is definitely a problem we're going to have to deal with. Our system might one day contribute to a solution."

The gripping system developed by Parness and colleagues was inspired by geckos, lizards that cling to walls with ease. Geckos' feet have branching arrays of tiny hairs, the smallest of which are hundreds of times thinner than a human hair. This system of hairs can conform to a rough surface without a lot of force. Although researchers cannot make a perfect replica of the gecko foot, they have put "hair" structures on the adhesive pads of the grippers.

The synthetic hairs, also called stalks, are wedge-shaped and have a slanted, mushroom-shaped cap. When the gripping pad lightly touches part of an object, only the very tips of the hairs make contact with that surface.

"The stickiness of the grippers can be turned on and off, by changing the direction in which you pull the hairs," Parness said.

To get the gripper to stick to a surface, force is applied to the adhesive pad material in a manner that makes the hairs bend. This increases the real area of contact between the hairs and the surface, which corresponds to greater adhesion. When the force is relaxed and the hairs go back to being upright, this process turns off the stickiness.

A phenomenon called van der Waals forces, named for Nobel Prize-winning physicist Johannes Diderik van der Waals, explains the non-permanent stickiness of the grippers, as well as gecko feet. These temporary adhesive forces happen because electrons orbiting the nuclei of atoms are not evenly spaced, creating a slight electrical charge. Such forces persist even in extreme temperature, pressure and radiation conditions.

"The reliability of van der Waals forces, even in severe environments, makes them particularly useful for space applications," Parness said.

"The system could grapple objects in space that are spinning or tumbling, and would otherwise be hard to target," he said.

In the recent tests, the grippers were able to grapple a 20-pound cube as it floated. The grippers also were able to grapple a researcher wearing a vest made of spacecraft material panels, representing a 250-pound "object." 

Members of the research team held the device with adhesive pads during the test, but the eventual idea is to integrate the grippers into a robotic arm or leg.

In total, the grippers have been tested on more than 30 spacecraft surfaces at JPL. They also have been tested successfully in a JPL thermal vacuum chamber, with total vacuum conditions and temperatures of minus 76 degrees Fahrenheit (minus 60 degrees Celsius) to simulate the conditions of space. While Parness was in graduate school at Stanford University in Palo Alto, California, the grippers were tested separately in more than 30,000 cycles of "on" and "off," with the adhesive staying strong. Several prototypes have since been designed.

There are more than 21,000 pieces of orbital debris larger than 3.9 inches (10 centimeters) in Earth's orbit. The U.S. Space Surveillance Network routinely tracks these objects. In 2009, an accidental collision occurred between an operational communications satellite and a large piece of debris, destroying the satellite.

Besides grappling orbital debris, the grippers could help inspect spacecraft or assist small satellites in docking to the International Space Station. The grippers are another example of how technology drives exploration.

The California Institute of Technology manages JPL for NASA.

Source: NASA/Jet Propulsion Laboratory

NASA's CATS eyes clouds, smoke and dust from the space station

The interactions between clouds and aerosols are illustrated in this image, taken by retired astronaut Chris Hadfield onboard the International Space Station. It shows contrails produced by aircraft (bright streaks) over the ocean. Credit: NASA/Chris Hadfield

Turn on any local TV weather forecast and you can get a map of where skies are blue or cloudy. But for scientists trying to figure out how clouds affect Earth's environment, what's happening inside that shifting cloud cover is critical and hard to see.

To investigate the layers and composition of clouds and tiny airborne particles like dust, smoke and other atmospheric aerosols, , scientists at NASA's Goddard Space Flight Center in Greenbelt, Maryland have developed an instrument called the Cloud-Aerosol Transport System, or CATS. The instrument, which launches to the International Space Station in December 2014, will explore new technologies that could also be used in future satellite missions.

From space, streaks of white clouds can be seen moving across Earth's surface. Other tiny solid and liquid particles called aerosols are also being transported around the atmosphere, but these are largely invisible to our eyes. Aerosols are both natural and man-made, and include windblown desert dust, sea salt, smoke from fires, sulfurous particles from volcanic eruptions, and particles from fossil fuel combustion.

Currently, scientists get a broad picture of clouds and air quality conditions in the atmosphere and generate air quality forecasts by combining satellite, aircraft, and ground-based data with sophisticated computer models. However, most datasets do not provide information about the layered structure of clouds and aerosols.

CATS will provide data about aerosols at different levels of the atmosphere. The data are expected to improve scientists' ability to track different cloud and aerosol types throughout the atmosphere. These datasets will be used to improve strategic and hazard-warning capabilities of events in near real-time, such as tracking plumes from dust storms, volcanic eruptions, and wildfires. The information could also feed into climate models to help understand the effects of clouds and aerosols on Earth's energy balance.

Clouds and aerosols reflect and absorb energy from the sun in a complex way. For example, when the sun's energy reaches the top of the atmosphere, clouds can reflect incoming sunlight, cooling Earth's surface. However, clouds can also absorb heat emitted from Earth and re-radiate it back down, warming the surface. The amount of warming or cooling is heavily dependent on the height, thickness, and structure of clouds in the atmosphere above.

"Clouds are one of the largest uncertainties in predicting climate change," said Matt McGill, principal investigator and payload developer for CATS at Goddard. "For scientists to create more accurate models of Earth's current and future climate, they'll have to include more accurate representations of clouds."

That's where a new instrument like CATS comes in. CATS is a lidar -- similar to a radar, but instead of sending out sound, lidars use light. CATS will send a laser pulse through the atmosphere towards a distant object like a cloud droplet or aerosol particle. Once the energy reaches the object, some of the energy is reflected back to the lidar receiver. Scientists can calculate the distance between the instrument and the object, based on the time it takes the energy to return to the receiver, thereby determining the altitudes of cloud and aerosol layers. The intensity of this return pulse also allows scientists to infer other properties, such as the composition of clouds, and the abundance and sizes of aerosols,.

In 2006 NASA launched the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations, or CALIPSO, spacecraft -- a joint mission between NASA and France's space agency, the Centre National d'Études Spatiales. CALIPSO carries a lidar that provides vertical distributions and properties of clouds and aerosols along a flight track. However, the CALIPSO lidar has exceeded its three-year prime mission and has been using its backup laser since 2009.

A unique opportunity to continue gathering this type of data presented itself in 2011 when the International Space Station Progam's NASA Research Office offered scientists at Goddard a mounting location aboard the space station for a new lidar instrument -- CATS, and provided the funding for its construction.

Designed to operate for at least six months, CATS has a goal of operating for three years. With beams at three wavelengths (1064, 532, and 355 nanometers), CATS will be used to derive a variety of properties of cloud and aerosol layers. These properties include layer height, layer thickness, and at least coarse information on the type of aerosols and cloud in various atmospheric layers.

CATS will orbit aboard the space station, which flies at an altitude between 230 miles (375 kilometers) and 270 miles (435 kilometers) above Earth's surface at a 51-degree inclination. This unique orbit path will allow the CATS instrument to observe locations at different times of day and allow scientists to study day-to-night changes in cloud and aerosol effects from space.

Studying clouds and aerosols won't just help scientists study the climate, it's also a chance to investigate air quality and how atmospheric particles affect daily life. That can range from volcano ash plumes, to dust storms, to pollution outbreaks, to wildfires, like the California Rim Fire in September 2013 that choked Yosemite National Park during the busy Labor Day weekend. These particles pose health risks to populations, especially to the medically vulnerable, By infusing CATS data directly into aerosol models, data from CATS can make a difference in tracking and responding to impacts of similar events in the future.

Source:  NASA/Goddard Space Flight Center