2013/12/31

Expedition 38 Sends New Year’s Greetings on Off-Duty Day


On the last day of 2013, the six station residents had off-duty time on orbit while still conducting some science, maintenance work and exercise. The Expedition 38 crew also sent down messages in their native languages to bring in the New Year. The international crew of six will also have New Year's Day off.
Commander Oleg Kotov and his fellow cosmonauts Sergey Ryazanskiy and Mikhail Tyurin gathered in the Japanese Kibo laboratory to downlink a New Year’s greeting to their Russian colleagues. The event was conducted live with Russian space organizations including the Gagarin Cosmonaut Training Center, Institute of Bio-Medical Problems and RSC (Rocket and Space Corporation) Energia.
While astronauts Rick Mastracchio, Mike Hopkins and Koichi Wakata enjoyed an off-duty day New Year’s Eve, microgravity research continued to benefit life on Earth and in space. The station’s systems are continuing to operate normally following spacewalk repairs to its external cooling system, and Mission Control teams around the world will ring in the New Year monitoring their performance. Wakata also radioed a new year’s greeting to his colleagues at the Japan Aerospace Exploration Agency.

Wakata assisted Mastracchio during a periodic fitness evaluation as part of the human research program on the International Space Station. Wakata monitored Mastracchio’s blood pressure as he was working out on an exercise cycle, also known as the Cycle Ergometer with Vibration Isolation and Stabilization System, or CEVIS.

Hopkins worked maintenance on combustion research hardware in the Destiny lab during the afternoon. He replaced a multi-drop combustion apparatus fuel reservoir inside the Combustion Integrated Rack (CIR). Afterward, he also replaced a manifold bottle inside the CIR.

Tyurin conducted photography for the Uragan (Hurricane) experiment that observes natural and man-made changes to the Earth’s geography. Ryazanskiy ran laptop computer anti-virus scans and Kotov updated the station’s inventory management system.

2013/12/30

Antares Launch Scheduled Jan. 7

The NASA Wallops Flight Facility and Virginia’s Mid-Atlantic Regional Spaceport are set to support the launch of Orbital Sciences’ Corp. Antares rocket at 1:55 p.m. EST, Jan. 7.
The Antares rocket will carry Orbital’s Cygnus cargo spacecraft to the International Space Station.
The cargo craft will be filled with 2,780 pounds of supplies for the station, including vital science experiments to expand the research capability of the Expedition 38 crew members aboard the orbiting laboratory, crew provisions, spare parts and experiment hardware. Also aboard the flight are 23 student experiments that will involve more than 10,000 students on the ground. These experiments will involve life sciences topics ranging from amoeba reproduction to calcium in the bones to salamanders.
The launch may be visible, weather permitting, to residents throughout the mid-Atlantic region from New York City to North Carolina.
Public viewing of the launch will be available at the NASA Visitor Center at Wallops and at the Chincoteague National Wildlife Refuge/Assateague National Seashore. Visitors are reminded that alcohol and pets are not allowed on the Visitor Center grounds.

2013/12/24

Space Station Research: Top Ten Results (Part 1) + (Part 2)

NASA has been observing the 15th Anniversary of the launch of the first few modules of the International Space Station back in November of 1998. In this coming February, we'll mark the 13th Anniversary of the arrival of the U.S. Laboratory Destiny to the International Space Station on a space shuttle mission during Expedition One. Science research has been going on on board the space station throughout the assembly process, but now that the assembly is essentially complete the science activity both inside and outside the space station is taking the primary focus of the activity on orbit. A few months ago, the International Astronautical Federation asked International Space Station Chief Scientist, Julie Robinson, to share the top 10 research results from the station at the International Astronautical Congress in Beijing, and she joins Pat Ryan of NASA Public Affairs to talk about some of those.

Space Station Research: Top Ten Results (Part 1)


Space Station Research: Top Ten Results (Part 2) 

 

Spacewalkers Complete Installation of Ammonia Pump Module

Spacewalkers Rick Mastracchio and Mike Hopkins completed a second spacewalk to install a spare ammonia pump module. The U.S. Quest airlock began repressurization at 2:23 p.m. EDT Tuesday signaling the official end of their spacewalk.
Tuesday’s main tasks included the removal and installation of a spare pump module. The first task was to remove the spare pump module from the space station’s External Stowage Platform-3. After that was completed, the module was bolted to the S1 truss and connected to Loop A of the station’s external Active Thermal Control System.
Hopkins attached himself to the Canadarm2 and took a ride to the worksite. Mastracchio tethered himself to the station and translated to the S1 truss to assist his partner. Japanese astronaut Koichi Wakata operated the Canadarm2 from inside the Destiny laboratory.
While doing the connection work, the duo demated ammonia fluid lines from a jumper box that enabled ammonia flow during the repair spacewalks. After experiencing some difficulty disconnecting a fluid line the spacewalkers reported seeing ammonia flakes escaping a valve. As a precaution, mission controllers asked the spacewalkers to inspect their spacesuits for possible ammonia contamination. Once they were back in the Quest airlock the duo conducted more ammonia decontamination procedures on their spacesuits. All four fluid lines were successfully reconnected to the newly installed pump module restoring ammonia flow.
Afterward, Hopkins and Mastracchio completed electrical connections to the pump module. Power was successfully restored to the ammonia pump module. However, flight controllers will perform more tests before restarting the pump and returning it to full functionality.
The duo was originally scheduled to finish the installation work on Monday before mission controllers detected a spacesuit configuration issue at the end of Saturday’s spacewalk, in which the spacewalkers removed a faulty pump that experienced a problem with its internal flow control valve Dec. 11.
The suspect pump was removed from the starboard truss and parked in a temporary location on the station’s Mobile Base System rail car where it can stay until at least next June. Managers decided an extra day of preparation was necessary to get a backup spacesuit ready for Mastracchio.

The Christmas Eve spacewalk lasted seven hours and 30 minutes. This was the 176th spacewalk in support of space station assembly and maintenance. Mastracchio holds 51 hours and 28 minutes spacewalking time over eight spacewalks. Hopkins holds 12 hours and 58 minutes over two spacewalks.

NASA's Deep Space Network Celebrates 50 Years

The Deep Space Network first existed as just a few small antennas as part of the Deep Space Instrumentation Facility. That facility, originally operated by the U.S. Army in the 1950s, morphed into the Deep Space Network on Dec. 24, 1963, and quickly became the de facto network for missions into deep space.
During its first year of operation, the network communicated with three spacecraft - Mariner 2, IMP-A and Atlas Centaur 2. Today, it communicates with 33 via three antenna complexes in Goldstone, Calif.; near Madrid, Spain; and near Canberra, Australia, maintaining round-the-clock coverage of the solar system.
During the past 50 years, antennas of the Deep Space Network have communicated with most of the missions that have gone to the moon and far into deep space. The highlights include relaying the moment when astronaut Neil Armstrong stepped onto the surface of the moon in a "giant leap for mankind"; transmitting data from numerous encounters with the outer planets of our solar system; communicating images taken by rovers exploring Mars; and relaying the data confirming that NASA's Voyager 1 spacecraft had entered interstellar space.
Space agencies in Europe, Japan and Russia have also relied on the Deep Space Network when planning and communicating with their own missions over the decades. The Deep Space Network has been used recently by India's first interplanetary probe, the Mars Orbiter Mission.
JPL, a division of the California Institute of Technology in Pasadena, manages the Deep Space Network for NASA.

2013/12/23

Space Station Live: Doug Wheelock Talks About Repair Spacewalks

Public Affairs Officer Dan Huot talks to astronaut Doug Wheelock talks about the spacewalks by Expedition 38 crew members Rick Mastracchio and Mike Hopkins to repair a faulty pump module.

During Expedition 24, Wheelock and fellow astronaut Tracy Caldwell-Dyson, worked during a set of spacewalks to remove and replace an ammonia pump module.

Enormous Aquifer Discovered Under Greenland Ice Sheet


Buried underneath compacted snow and ice in Greenland lies a large liquid water reservoir that has now been mapped by researchers using data from NASA's Operation IceBridge airborne campaign.
A team of glaciologists serendipitously found the aquifer while drilling in southeast Greenland in 2011 to study snow accumulation. Two of their ice cores were dripping water when the scientists lifted them to the surface, despite air temperatures of minus 4 F (minus 20 C). The researchers later used NASA's Operation Icebridge radar data to confine the limits of the water reservoir, which spreads over 27,000 square miles (69,930 square km) – an area larger than the state of West Virginia. The water in the aquifer has the potential to raise global sea level by 0.016 inches (0.4 mm).
"When I heard about the aquifer, I had almost the same reaction as when we discovered Lake Vostok [in Antarctica]: it blew my mind that something like that is possible," said Michael Studinger, project scientist for Operation IceBridge, a NASA airborne campaign studying changes in ice at the poles. "It turned my view of the Greenland ice sheet upside down – I don't think anyone had expected that this layer of liquid water could survive the cold winter temperatures without being refrozen."
Southeast Greenland is a region of high snow accumulation. Researchers now believe that the thick snow cover insulates the aquifer from cold winter surface temperatures, allowing it to remain liquid throughout the year. The aquifer is fed by meltwater that percolates from the surface during the summer.
The new research is being presented in two papers: one led by University of Utah's Rick Forster that was published on Dec. 22 in the journal Nature Geoscience and one led by NASA's Lora Koenig that has been accepted for publication in the journal Geophysical Research Letters. The findings will significantly advance the understanding of how melt water flows through the ice sheet and contributes to sea level rise.
When a team led by Forster accidentally drilled into water in 2011, they weren't able to continue studying the aquifer because their tools were not suited to work in an aquatic environment. Afterward, Forster's team determined the extent of the aquifer by studying radar data from Operation IceBridge together with ground-based radar data. The top of the water layer clearly showed in the radar data as a return signal brighter than the ice layers.
Koenig, a glaciologist with NASA's Goddard Space Flight Center in Greenbelt, Md., co-led another expedition to southeast Greenland with Forster in April 2013 specifically designed to study the physical characteristics of the newly discovered water reservoir. Koenig's team extracted two cores of firn (aged snow) that were saturated with water. They used a water-resistant thermoelectric drill to study the density of the ice and lowered strings packed with temperature sensors down the holes, and found that the temperature of the aquifer hovers around 32 F (zero C), warmer than they had expected it to be.
Koenig and her team measured the top of the aquifer at around 39 feet (12 meters) under the surface. This was the depth at which the boreholes filled with water after extracting the ice cores. They then determined the amount of water in the water-saturated firn cores by comparing them to dry cores extracted nearby. The researchers determined the depth at which the pores in the firn close, trapping the water inside the bubbles – at this point, there is a change in the density of the ice that the scientists can measure. This depth is about 121 feet (37 meters) and corresponds to the bottom of the aquifer. Once Koenig’s team had the density, depth and spatial extent of the aquifer, they were able to come up with an estimated water volume of about 154 billion tons (140 metric gigatons). If this water was to suddenly discharge to the ocean, this would correspond to 0.016 inches (0.4 mm) of sea level rise.
Researchers think that the perennial aquifer is a heat reservoir for the ice sheet in two ways: melt water carries heat when it percolates from the surface down the ice to reach the aquifer. And if the trapped water were to refreeze, it would release latent heat. Altogether, this makes the ice in the vicinity of the aquifer warmer, and warmer ice flows faster toward the sea.
"Our next big task is to understand how this aquifer is filling and how it's discharging," said Koenig. "The aquifer could offset some sea level rise if it's storing water for long periods of time. For example after the 2012 extreme surface melt across Greenland, it appears that the aquifer filled a little bit. The question now is how does that water leave the aquifer on its way to the ocean and whether it will leave this year or a hundred years from now."

2013/12/21

NASA Releases New Earthrise Simulation Video

NASA has issued a new visualization of the events leading to one of the iconic photographs of the 20th Century – Earth rising over the moon captured by the crew of the Apollo 8 mission.
The photo known as Earthrise is the first color photograph of Earth taken by a person in lunar orbit. Earthrise is the cover photo of TIME's Great Images of the 20th Century, and is the central photo on the cover of LIFE's 100 Photographs That Changed the World.
"Earthrise had a profound impact on our attitudes toward our home planet, quickly becoming an icon of the environmental movement," says Ernie Wright, project lead with the Scientific Visualization Studio at NASA's Goddard Space Flight Center in Greenbelt, Md.
The visualization clearly shows how Apollo 8 Commander Frank Borman and crew members William A. Anders and James A. Lovell worked together to photograph the stunning scene as their spacecraft orbited the moon on December 24, 1968. The video allows anyone to virtually ride with the astronauts and experience the awe they felt at the vista in front of them.

2013/12/17

Station Cooling System Update From Flight Director

Expedition 38 Lead Flight Director Judd Frieling joins NASA Public Affairs Officer Dan Huot for an update on the International Space Station's ammonia pump module and the efforts by the Flight Control Team to resolve the issue with a software upload.

Hubble Watches Super Star Create Holiday Light Show

This festive NASA Hubble Space Telescope image resembles a holiday wreath made of sparkling lights. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our sun and 200 times larger.
RS Puppis rhythmically brightens and dims over a six-week cycle. It is one of the most luminous in the class of so-called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our sun’s luminosity.
The nebula flickers in brightness as pulses of light from the Cepheid propagate outwards. Hubble took a series of photos of light flashes rippling across the nebula in a phenomenon known as a "light echo." Even though light travels through space fast enough to span the gap between Earth and the moon in a little over a second, the nebula is so large that reflected light can actually be photographed traversing the nebula.
By observing the fluctuation of light in RS Puppis itself, as well as recording the faint reflections of light pulses moving across the nebula, astronomers are able to measure these light echoes and pin down a very accurate distance. The distance to RS Puppis has been narrowed down to 6,500 light-years (with a margin of error of only one percent).
The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Md., conducts Hubble science operations. STScI is operated by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.

2013/12/16

Work Continues on Station Cooling Issue

Kenny Todd, ISS Mission Operations Integration Manager, provides an update on the efforts to regulate temperatures in one of two cooling loops on the International Space Station affected by the malfunction last week of a flow control valve in a cooling pump on the station's starboard truss.

Cygnus Launch Preps Continue as Managers Mull Repair Spacewalks

NASA managers are evaluating whether to go for a Dec. 19 launch of Orbital Sciences’ Cygnus commercial resupply craft or move ahead with a series of spacewalks to repair a pump that is part of a cooling loop that shutdown last Wednesday due to low temperatures seen in the line.
Ground controllers have been sending commands to another valve that is part of the station’s cooling system. The hope is that this valve can be positioned in a way to help maintain the proper temperature in the loop, which could allow them to reintegrate part of the station’s internal electronics.
 Momentum continues at Wallops Flight Facility in Virginia for the launch of the Cygnus spacecraft Thursday at 9:19 p.m. EST. The new cargo craft was loaded Saturday with its manifested gear and is targeted for arrival at the International Space Station on Sunday.

Meanwhile, momentum continues at Wallops Flight Facility in Virginia for the launch of the Cygnus spacecraft Thursday at 9:19 p.m. EST. The new cargo craft was loaded Saturday with its manifested gear and is targeted for arrival at the International Space Station next week.
The Antares rocket’s upper stage was outfitted Monday with its fairing that houses the Cygnus vehicle during ascent. The Antares is scheduled to roll out to its launch pad early Tuesday morning pending a review by station program managers.
NASA astronauts Rick Mastracchio and Mike Hopkins began checking their spacewalk tools, trying on their spacesuits and reviewing procedures inside the Quest airlock over the weekend. The NASA astronauts were assisted by Japanese astronaut Koichi Wakata and Expedition 38 Commander Oleg Kotov.
Kotov and Flight Engineer Sergey Ryazanskiy are also preparing for spacewalk. This is a pre-planned spacewalk scheduled for Dec. 27 outside the station’s Russian segment. The duo will install a foot restraint; install medium and high resolution cameras; jettison gear from a pair of external experiments; and install a new experiment as well as a payload boom on the Zvezda service module.
Flight Engineer and fellow cosmonaut Mikhail Tyurin worked maintenance on the Russian side of station. He performed some plumbing work, transferred science data to a laptop computer and updated the station’s inventory management system.

2013/12/13

Space Station Live: Antibiotic Effectiveness in Space

NASA Public Affairs Officer Brandi Dean talks with Dr. David Klaus, principal investigator for Antibiotic Effectiveness in Space from BioServe Space Technologies, University of Colorado. Klaus discusses the NPL Vacccine-21 experiment that is being sent to the International Space Station aboard the Cygnus commercial cargo craft this month.

NASA Selects SpaceX to Begin Negotiations for Use of Historic Launch Pad

NASA has selected Space Exploration Technologies Corporation (SpaceX) of Hawthorne, Calif., to begin negotiations on a lease to use and operate historic Launch Complex (LC) 39A at the agency's Kennedy Space Center in Florida.
Permitting use and operation of this valuable national asset by a private-sector, commercial space partner will ensure its continued viability and allow for its continued use in support of U.S. space activities.
The reuse of LC-39A is part of NASA’s work to transform the Kennedy Space Center into a 21st century launch complex capable of supporting both government and commercial users. Kennedy is having success attracting significant private sector interest in its unique facilities. The center is hard at work assembling NASA’s Orion spacecraft and preparing its infrastructure for the Space Launch System rocket, which will launch from LC-39B and take American astronauts into deep space, including to an asteroid and Mars.
NASA made the selection decision Thursday after the U.S. Government Accountability Office (GAO) denied a protest filed against the Agency by Blue Origin LLC on Sept. 13.  In its protest, Blue Origin raised concerns about the competitive process NASA was using to try to secure a potential commercial partner or partners to lease and use LC-39A.  Blue Origin had argued the language in the Announcement for Proposals (AFP) favored one proposed use of LC-39A over others. The GAO disagreed.
While the GAO protest was underway, NASA was prohibited from selecting a commercial partner for LC-39A from among the proposals submitted in response to the agency's AFP that had been issued on May 23.  However, while the GAO considered the protest, NASA continued evaluating the proposals in order to be prepared to make a selection when permitted to do so.  After the GAO rendered its decision Thursday in NASA’s favor, the agency completed its evaluation and selection process.
NASA notified all proposers on Friday of its selection decision concerning LC-39A.  Further details about NASA’s decision will be provided to each proposer when NASA furnishes the source selection statement to the proposers. In addition, NASA will offer each the opportunity to meet to discuss NASA’s findings related to the proposer’s individual proposal.  NASA will release the source selection statement to the public once each proposer has been consulted to ensure that any proprietary information has been appropriately redacted.
NASA will begin working with SpaceX to negotiate the terms of its lease for LC-39A. During those ongoing negotiations, NASA will not be able to discuss details of the pending lease agreement.
Since the late 1960s, Kennedy's launch pads 39 A and B have served as the starting point for America's most significant human spaceflight endeavors -- Apollo, Skylab, Apollo-Soyuz and all 135 space shuttle missions. LC-39A is the pad where Apollo 11 lifted off from on the first manned moon landing in 1969, as well as launching the first space shuttle mission in 1981 and the last in 2011.

2013/12/12

Station Flight Controller Talks to Pennsylvania High School Students

From NASA's International Space Station Mission Control Center, Joe Pascucci, Trajectory Operations Officer (TOPO), participates in a Digital Learning Network (DLN) event with students from East Stroudsburg High School, East Stroudsburg, Pa.

The DLN connects students and teachers with NASA experts and education specialists using online communication technologies like video/web conferencing and webcasting. Register for free, interactive events listed in the catalog or watch the webcasts.

Train Like an Astronaut: Fit Explorer Series

The next phase of Astronaut Mike Hopkin's mission is well underway and we have some exciting new downlink footage of his training that we will be sharing in the next few weeks...Curious? Check out this sneak peak at what's to come!

Space Station Live: Studying Combustion to Make Space Exploration Safe

NASA Public Affairs officer Brandi Dean interviews Dr. Sandra Olson, Spacecraft Fire Safety Researcher at NASA Glenn Research Center, about BASS-II (Burning and Suppression of Solids) in advance of its launch aboard the Orbital Sciences' Cygnus spacecraft. BASS-II, a combustion science experiment, will study air flow on combustion in space and observe how materials ignite and their flammability.

Results could help designers create safer materials and fabrics and improve fire prevention techniques. The safety of a vehicle and crew is extremely important as NASA plans missions beyond low-Earth orbit. BASS-II is the second version of the BASS experiment that began September 2011. Read more about BASS...

Hubble Space Telescope Sees Evidence of Water Vapor Venting off Jupiter Moon

NASA’s Hubble Space Telescope has observed water vapor above the frigid south polar region of Jupiter's moon Europa, providing the first strong evidence of water plumes erupting off the moon's surface.
Previous scientific findings from other sources already point to the existence of an ocean located under Europa's icy crust. Researchers are not yet fully certain whether the detected water vapor is generated by erupting water plumes on the surface, but they are confident this is the most likely explanation.
Should further observations support the finding, this would make Europa the second moon in the solar system known to have water vapor plumes. The findings are being published in the Dec. 12 online issue of Science Express, and reported at the meeting of the American Geophysical Union in San Francisco.
“By far the simplest explanation for this water vapor is that it erupted from plumes on the surface of Europa,” said lead author Lorenz Roth of Southwest Research Institute in San Antonio. "If those plumes are connected with the subsurface water ocean we are confident exists under Europa's crust, then this means that future investigations can directly investigate the chemical makeup of Europa's potentially habitable environment without drilling through layers of ice. And that is tremendously exciting."
In 2005, NASA’s Cassini orbiter detected jets of water vapor and dust spewing off the surface of Saturn’s moon Enceladus. Although ice and dust particles have subsequently been found in the Enceladus plumes, only water vapor gases have been measured at Europa so far.
Hubble spectroscopic observations provided the evidence for Europa plumes in December 2012. Time sampling of Europa's auroral emissions measured by Hubble's imaging spectrograph enabled the researchers to distinguish between features created by charged particles from Jupiter's magnetic bubble and plumes from Europa's surface, and also to rule out more exotic explanations such as serendipitously observing a rare meteorite impact.
The imaging spectrograph detected faint ultraviolet light from an aurora, powered by Jupiter’s intense magnetic field, near the moon’s south pole. Excited atomic oxygen and hydrogen produce a variable auroral glow and leave a telltale sign that are the products of water molecules being broken apart by electrons along magnetic field lines.
“We pushed Hubble to its limits to see this very faint emission. These could be stealth plumes, because they might be tenuous and difficult to observe in the visible light,” said Joachim Saur of the University of Cologne, Germany. Saur, who is principal investigator of the Hubble observation campaign, co-wrote the paper with Roth.
Roth suggested that long cracks on Europa’s surface, known as lineae, might be venting water vapor into space. Cassini has seen similar fissures that host the Enceladus jets.
Also the Hubble team found that the intensity of the Europa plumes, like those at Enceladus, varies with Europa’s orbital position. Active jets have only been seen when the moon is farthest from Jupiter. The researchers could not detect any sign of venting when Europa is closer to Jupiter.
One explanation for the variability is that these lineae experience more stress as gravitational tidal forces push and pull on the moon and open vents at larger distances from Jupiter.  The vents are narrowed or closed when the moon is closest to the gas-giant planet.
"The apparent plume variability supports a key prediction that Europa should tidally flex by a significant amount if it has a subsurface ocean," said Kurt Retherford, also of Southwest Research Institute.
The Europa and Enceladus plumes have remarkably similar abundances of water vapor. Because Europa has a roughly 12 times stronger gravitational pull than Enceladus, the minus-40-degree-Fahrenheit (minus-40-degree-Celsius) vapor for the most part doesn’t escape into space as it does at Enceladus, but rather falls back onto the surface after reaching an altitude of 125 miles (201 kilometers), according to the Hubble measurements. This could leave bright surface features near the moon’s south polar region, the researchers hypothesize.
“If confirmed, this new observation once again shows the power of the Hubble Space Telescope to explore and opens a new chapter in our search for potentially habitable environments in our solar system,” said John Grunsfeld, an astronaut who participated Hubble servicing missions and now serves as NASA's associate administrator for science in Washington. “The effort and risk we took to upgrade and repair Hubble becomes all the more worthwhile when we learn about exciting discoveries like this one from Europa.”

NASA Testing Modified "Pumpkin Suit" for Asteroid Mission Spacewalks

NASA is taking steps to make spacewalking on an asteroid a reality. In the Neutral Buoyancy Laboratory (NBL) near the agency's Johnson Space Center in Houston, engineers are testing a modified version of the pumpkin-orange Advanced Crew Escape System (ACES) worn by space shuttle astronauts during launch and reentry for use by future crew in the Orion spacecraft.
As the agency plans human deep space missions, including a voyage to a relocated asteroid, care is being taken to efficiently use space inside Orion. The white Extravehicular Mobility Unit spacesuits used by crews to conducts spacewalks on the International Space Station are too bulky to carry in the spacecraft, so NASA is looking at ways to alter the ACES suits for multiple uses both inside and outside the spacecraft.
"The shell of them is very much the same, and to the casual user you may not even notice the difference, but internally we modified them to work with the plumbing inside Orion," said Dustin Gohmert, Crew Survival Systems Manager at Johnson.
Through a series of tests in the NBL, engineers are learning what features need to be included to improve the suit's mobility beyond the needs of the trip from the launch pad to space and its return to Earth, such as enhanced gloves and elbow joints with improved mobility for spacewalks.
The ACES pumpkin suit was worn by space shuttle crews beginning in 1994 and builds on the earliest spacesuit worn by Ed White during the first venture outside a spacecraft in 1965.
"We're stepping back to our heritage to be able to use one suit for multiple tasks," said Gohmert.
NASA is looking at a broad range of ideas and techniques as the agency further refines its mission design for the agency's asteroid initiative, an effort that combines human exploration, space technology and science work being done across the agency to find and redirect and asteroid to a stable orbit near the moon for exploration by astronauts.
The NBL tests are helping with the evaluation of options for spacewalking techniques like how best to get out of Orion and traverse the spacecraft toward the captured asteroid. NASA is making use of previous experience and proving designs to accelerate development, ensure crew safety and increase reliability.

2013/12/11

Clay-Like Minerals Found on Icy Crust of Europa

This image, using data from NASA's Galileo mission, shows the first detection of clay-like minerals on the surface of Jupiter's moon Europa. The clay-like minerals appear in blue in the false-color patch of data from Galileo's Near-Infrared Mapping Spectrometer.
A new analysis of data from NASA's Galileo mission has revealed clay-type minerals at the surface of Jupiter's icy moon Europa that appear to have been delivered by a spectacular collision with an asteroid or comet. This is the first time such minerals have been detected on Europa's surface. The types of space rocks that deliver such minerals typically also often carry organic materials.
"Organic materials, which are important building blocks for life, are often found in comets and primitive asteroids," said Jim Shirley, a research scientist at NASA's Jet Propulsion Laboratory, Pasadena, Calif. Shirley is giving a talk on this topic at the American Geophysical Union meeting in San Francisco on Friday, Dec. 13. "Finding the rocky residues of this comet crash on Europa's surface may open up a new chapter in the story of the search for life on Europa," he said.
Many scientists believe Europa is the best location in our solar system to find existing life. It has a subsurface ocean in contact with rock, an icy surface that mixes with the ocean below, salts on the surface that create an energy gradient, and a source of heat (the flexing that occurs as it gets stretched and squeezed by Jupiter's gravity). Those conditions were likely in place shortly after Europa first coalesced in our solar system.
Scientists have also long thought there must be organic materials at Europa, too, though they have yet to detect them directly. One theory is that organic material could have arrived by comet or asteroid impacts, and this new finding supports that idea.
Shirley and colleagues, funded by a NASA Outer Planets Research grant, were able to see the clay-type minerals called phyllosilicates in near-infrared images from Galileo taken in 1998. Those images are low resolution by today's standards, and Shirley’s group is applying a new technique for pulling a stronger signal for these materials out of the noisy picture. The phyllosilicates appear in a broken ring about 25 miles (40 kilometers) wide, which is about 75 miles (120 kilometers) away from the center of a 20-mile-diameter (30 kilometers) central crater site.
The leading explanation for this pattern is the splash back of material ejected when a comet or asteroid hits the surface at an angle of 45 degrees or more from the vertical direction. A shallow angle would allow some of the space rock's original material to fall back to the surface. A more head-on collision would likely have vaporized it or driven that space rock's materials below the surface. It is hard to see how phyllosilicates from Europa’s interior could make it to the surface, due to Europa’s icy crust, which scientists think may be up to 60 miles (100 kilometers) thick in some areas.
Therefore, the best explanation is that the materials came from an asteroid or comet. If the body was an asteroid, it was likely about 3,600 feet (1,100 meters) in diameter. If the body was a comet, it was likely about 5,600 feet (1,700 meters) in diameter. It would have been nearly the same size as the comet ISON before it passed around the sun a few weeks ago.
“Understanding Europa’s composition is key to deciphering its history and its potential habitability," said Bob Pappalardo of JPL, the pre-project scientist for a proposed mission to Europa. "It will take a future spacecraft mission to Europa to pin down the specifics of its chemistry and the implications for this moon hosting life.

2013/12/10

NASA's Juno Gives Starship-Like View of Earth Flyby

When NASA’s Juno spacecraft flew past Earth on Oct. 9, 2013, it received a boost in speed of more than 8,800 mph (about 7.3 kilometer per second), which set it on course for a July 4, 2016, rendezvous with Jupiter, the largest planet in our solar system. One of Juno's sensors, a special kind of camera optimized to track faint stars, also had a unique view of the Earth-moon system. The result was an intriguing, low-resolution glimpse of what our world would look like to a visitor from afar.
"If Captain Kirk of the USS Enterprise said, ‘Take us home, Scotty,’ this is what the crew would see," said Scott Bolton, Juno principal investigator at the Southwest Research Institute, San Antonio. “In the movie, you ride aboard Juno as it approaches Earth and then soars off into the blackness of space. No previous view of our world has ever captured the heavenly waltz of Earth and moon."
The Juno Earth flyby movie is available at: http://www.youtube.com/watch?v=_CzBlSXgzqI&feature=youtu.be . The music accompaniment is an original score by Vangelis.
The cameras that took the images for the movie are located near the pointed tip of one of the spacecraft's three solar-array arms. They are part of Juno's Magnetic Field Investigation (MAG) and are normally used to determine the orientation of the magnetic sensors. These cameras look away from the sunlit side of the solar array, so as the spacecraft approached, the system's four cameras pointed toward Earth. Earth and the moon came into view when Juno was about 600,000 miles (966,000 kilometers) away -- about three times the Earth-moon separation.
During the flyby, timing was everything. Juno was traveling about twice as fast as a typical satellite, and the spacecraft itself was spinning at 2 rpm. To assemble a movie that wouldn't make viewers dizzy, the star tracker had to capture a frame each time the camera was facing Earth at exactly the right instant. The frames were sent to Earth, where they were processed into video format.
"Everything we humans are and everything we do is represented in that view," said the star tracker's designer, John Jørgensen of the Danish Technical University, near Copenhagen.
Also during the flyby, Juno's Waves instrument, which is tasked with measuring radio and plasma waves in Jupiter's magnetosphere, recorded amateur radio signals. This was part of a public outreach effort involving ham radio operators from around the world. They were invited to say "HI" to Juno by coordinating radio transmissions that carried the same Morse-coded message. Operators from every continent, including Antarctica, participated.
"With the Earth flyby completed, Juno is now on course for arrival at Jupiter on July 4, 2016," said Rick Nybakken, Juno project manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif.
The Juno spacecraft was launched from Kennedy Space Center in Florida on August 5, 2011. Juno’s launch vehicle was capable of giving the spacecraft only enough energy to reach the asteroid belt, at which point the sun’s gravity pulled it back toward the inner solar system. Mission planners designed the swing by Earth as a gravity assist to increase the spacecraft’s speed relative to the sun, so that it could reach Jupiter. (The spacecraft’s speed relative to Earth before and after the flyby is unchanged.)
After Juno arrives and enters into orbit around Jupiter in 2016, the spacecraft will circle the planet 33 times, from pole to pole, and use its collection of science instruments to probe beneath the gas giant's obscuring cloud cover. Scientists will learn about Jupiter's origins, internal structure, atmosphere and magnetosphere.
Juno's name comes from Greek and Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief from his wife, but the goddess Juno used her special powers to peer through the clouds and reveal Jupiter's true nature.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft. JPL is a division of the California Institute of Technology in Pasadena.

NASA Mars Spacecraft Reveals a More Dynamic Red Planet

NASA's Mars Reconnaissance Orbiter has revealed to scientists slender dark markings -- possibly due to salty water – that advance seasonally down slopes surprisingly close to the Martian equator.
"The equatorial surface region of Mars has been regarded as dry, free of liquid or frozen water, but we may need to rethink that," said Alfred McEwen of the University of Arizona in Tucson, principal investigator for the Mars Reconnaissance Orbiter (MRO) High Resolution Imaging Science Experiment (HiRISE) camera.
Tracking how these features recur each year is one example of how the longevity of NASA orbiters observing Mars is providing insight about changes on many time scales. Researchers at the American Geophysical Union meeting Tuesday in San Francisco discussed a range of current Martian activity, from fresh craters offering glimpses of subsurface ice to multi-year patterns in the occurrence of large, regional dust storms.
The seasonally changing surface flows were first reported two years ago on mid-latitude southern slopes. They are finger-like features typically less than 16 feet (5 meters) wide that appear and extend down steep, rocky slopes during spring through summer, then fade in winter and return the next spring. Recently observed slopes stretch as long as 4,000 feet (1,200 meters).
McEwen and co-authors reported the equatorial flows at the conference and in a paper published online Tuesday by Nature Geoscience. Five well-monitored sites with these markings are in Valles Marineris, the largest canyon system in the solar system. At each of these sites, the features appear on both north- and south-facing walls. On the north-facing slopes, they are active during the part of the year when those slopes get the most sunshine. The counterparts on south-facing slopes start flowing when the season shifts and more sunshine hits their side.
"The explanation that fits best is salty water is flowing down the slopes when the temperature rises," McEwen said. "We still don't have any definite identification of water at these sites, but there's nothing that rules it out, either."
Dissolved salts can keep water melted at temperatures when purer water freezes, and they can slow the evaporation rate so brine can flow farther. This analysis used data from the Compact Reconnaissance Imaging Spectrometer for Mars and the Context Camera on the MRO as well as the Thermal Emission Imaging System experiment on NASA's Mars Odyssey orbiter.
Water ice has been identified in another dynamic process researchers are monitoring with MRO. Impacts of small asteroids or bits of comets dig many fresh craters on Mars every year. Twenty fresh craters have exposed bright ice previously hidden beneath the surface. Five were reported in 2009. The 15 newly reported ones are distributed over a wider range of latitudes and longitudes.
"The more we find, the more we can fill in a global map of where ice is buried," said Colin Dundas of the U.S. Geological Survey in Flagstaff, Ariz. "We've now seen icy craters down to 39 degrees north, more than halfway from the pole to the equator. They tell us that either the average climate over several thousand years is wetter than present or that water vapor in the current atmosphere is concentrated near the surface. Ice could have formed under wetter conditions, with remnants from that time persisting today, but slowly disappearing."
Mars' modern climate becomes better known each year because of a growing set of data from a series of orbiters that have been studying Mars continually since 1997. That has been almost nine Martian years because a year on Mars is almost two years long on Earth. Earlier missions and surface landers have added insight about the dynamics of Mars' atmosphere and its interaction with the ground.
"The dust cycle is the main driver of the climate system," said Robert Haberle of NASA's Ames Research Center in Moffett Field, Calif.
One key question researchers want to answer is why dust storms encircle Mars in some years and not in others. These storms affect annual patterns of water vapor and carbon dioxide in the atmosphere, freezing into polar ice caps in winter and replenishing the atmosphere in spring. Identifying significant variations in annual patterns requires many Martian years of observations.
The data emerging from long-term studies will help future human explorers of Mars know where to find resources such as water, how to prepare for hazards such as dust storms, and where to be extra careful about contamination with Earth microbes.
Launched in 2005, Mars Reconnaissance Orbiter and its six instruments have provided more high-resolution data about the Red Planet than all other Mars orbiters combined. Data are made available for scientists worldwide to research, analyze and report their findings.
NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the MRO and Mars Odyssey missions for NASA's Science Mission Directorate in Washington. Lockheed Martin Space Systems in Denver built both orbiters. The University of Arizona Lunar and Planetary Laboratory operates the HiRISE camera, which was built by Ball Aerospace & Technologies Corp. of Boulder, Colo.

Fire vs. Ice: The Science of ISON at Perihelion

After a year of observations, scientists waited with bated breath on Nov. 28, 2013, as Comet ISON made its closest approach to the sun, known as perihelion. Would the comet disintegrate in the fierce heat and gravity of the sun? Or survive intact to appear as a bright comet in the pre-dawn sky?
Some remnant of ISON did indeed make it around the sun, but it quickly dimmed and fizzled as seen with NASA's solar observatories. This does not mean scientists were disappointed, however. A worldwide collaboration ensured that observatories around the globe and in space, as well as keen amateur astronomers, gathered one of the largest sets of comet observations of all time, which will provide fodder for study for years to come.
On Dec. 10, 2013, researchers presented science results from the comet's last days at the 2013 Fall American Geophysical Union meeting in San Francisco, Calif. They described how this unique comet lost mass in advance of reaching perihelion and most likely broke up during its closest approach, as well, as summarized what this means for determining what the comet was made of.
"The comet's story begins with the very formation of the solar system," said Karl Battams, an astrophysicist at the Naval Research Lab in Washington, D.C. "The dirty snowball that we came to call Comet ISON was created at the same time as the planets."
ISON circled the solar system in the Oort cloud, more than 4.5 trillion miles away from the sun. At some point a few million years ago, something occurred – perhaps the passage of a nearby star – to knock ISON out of its orbit and send it hurtling along a path for its first trip into the inner solar system.
The comet was first spotted 585 million miles away in September 2012 by two Russian astronomers: Vitali Nevski and Artyom Novichonok. The comet was named after the project that discovered it, the International Scientific Optical Network, or ISON, and given an official designation of C/2012 S1 (ISON). When comet scientists mapped out Comet ISON's orbit they learned that the comet would swing within 1.1 million miles of the sun's surface, making it what's known as a sungrazing comet, providing opportunities to study this pristine bit of the early solar system as it lost material while approaching the higher temperatures of the sun. With this knowledge, an international campaign to observe the comet was born. The number of space-based, ground-based, and amateur observations was unprecedented, including 12 NASA space-based assets observing Comet ISON over the past year.
Near the beginning of October, 2013, two months before perihelion, NASA's Mars Reconnaissance Observer, or MRO, turned its HiRISE instrument to view the comet during its closest approach to Mars in October 2013.
"The size of ISON's nucleus could be a little over half a mile across --- at the most.  Very likely it could have been as small as several hundred yards," said Alfred McEwen, the principal investigator for the HiRISE instrument at Arizona State University, in Tucson.
In other words, Comet ISON might have been the length of five or six football fields. This small size was near the borderline of how big ISON needed to be to survive its trip around the sun.
During that trip around the sun, Geraint Jones, a comet scientist at University College London's Mullard Space Science Laboratory in the UK studied the comet's dust tails to better understand what happened as it rounded the sun. By fitting models of the dust tail to the actual observations from NASA's Solar Terrestrial Observatory, or STEREO, and the joint European Space Agency/NASA Solar and Heliospheric Observatory, or SOHO, Jones showed that very little dust was produced after perihelion, which may suggest that the comet's nucleus had already broken up by that time.

While the comet was visible in STEREO and SOHO images going into perihelion, it was not visible in the data from NASA's Solar Dynamics Observatory, or SDO, or from ground based solar observatories during its closest approach to the sun. Dean Pesnell, project scientist for SDO at NASA's Goddard Space Flight Center in Greenbelt, Md., explained why Comet ISON wasn't visible in SDO and what could be learned from that: SDO is tuned to see wavelengths of light that would indicate the presence of oxygen, which is very common in comets.
"The fact that ISON did not show oxygen despite how close it came to the sun provides information about how high was the evaporation temperature of ISON's material," said Pesnell. "This limits what it could have been made of."
When Comet ISON was first spotted in September 2012, it was relatively bright for a comet at such a great distance from the sun. Consequently, many people had high hopes it would provide a beautiful light show visible in the night sky throughout December 2013. That potential ended when Comet ISON disrupted during perihelion. However, the legacy of the comet will go on for years as scientists analyze the tremendous data set collected during ISON's journey.

Space Station Live: Fluid Motion Study Using Mini-Satellites

NASA Public Affairs Officer Brandi Dean talks with Dr. Paul Schallhorn, the principal investigator for the SPHERES-Slosh experiment. This study, which takes a look at fluid motion in microgravity, will use the International Space Station's free-flying satellites known as Synchronized Position Hold, Engage, Reorient, Experimental Satellites, or SPHERES.

The hardware for SPHERES-Slosh will be launching to the station Dec. 18 aboard the Cygnus cargo craft during the Orbital 1 commercial resupply mission.

IRIS Provides Unprecedented Images of Sun

The region located between the surface of the sun and its atmosphere has been revealed as a more violent place than previously understood, according to images and data from NASA's newest solar observatory, the Interface Region Imaging Spectrograph, or IRIS.
Solar observatories look at the sun in layers. By capturing light emitted by atoms of different temperatures, they can focus in on different heights above the sun's surface extending well out into the solar atmosphere, the corona. On June 27, 2013, IRIS, was launched, to study what's known as the interface region – a layer between the sun's surface and corona that previously was not well observed.
Over its first six months, IRIS has thrilled scientists with detailed images of the interface region, finding even more turbulence and complexity than expected. IRIS scientists presented the mission's early observations at a press conference at the Fall American Geophysical Union meeting on Dec. 9, 2013.

"The quality of images and spectra we are receiving from IRIS is amazing," said Alan Title, IRIS principal investigator at Lockheed Martin in Palo Alto, Calif. "And we're getting this kind of quality from a smaller, less expensive mission, which took only 44 months to build."
For the first time, IRIS is making it possible to study the explosive phenomena in the interface region in sufficient detail to determine their role in heating the outer solar atmosphere. The mission’s observations also open a new window into the dynamics of the low solar atmosphere that play a pivotal role in accelerating the solar wind and driving solar eruptive events.
Tracking the complex processes in the interface region requires instrument and modeling capabilities that are only now within our technological reach. IRIS captures both images and what's known as spectra, which display how much of any given wavelength of light is present. This, in turn, corresponds to how much material in the solar atmosphere is present at specific velocities, temperatures and densities. IRIS's success is due not only to its high spatial and temporal resolution, but also because of parallel development of advanced computer models. The combined images and spectra have provided new imagery of a region that was always known to be dynamic, but shows it to be even more violent and turbulent than imagined.
"We are seeing rich and unprecedented images of violent events in which gases are accelerated to very high velocities while being rapidly heated to hundreds of thousands of degrees," said Bart De Pontieu, the IRIS science lead at Lockheed Martin. "These types of observations present significant challenges to current theoretical models."
DePontieu has been culling images of two particular types of events on the sun that have long been interesting to scientists. One is known as a prominence, which are cool regions within the interface region that appear as giant loops of solar material rising up above the solar surface. When these prominences erupt they lead to solar storms that can reach Earth. IRIS shows highly dynamic and finely structured flows sweeping throughout the prominence.
The second type of event is called a spicule, which are giant fountains of gas – as wide as a state and as long as Earth – that zoom up from the sun's surface at 150,000 miles per hour. Spicules may play a role in distributing heat and energy up into the sun's atmosphere, the corona. IRIS imaging and spectral data allows us to see at high resolution, for the first time, how the spicules evolve. In both cases, observations are more complex than what existing theoretical models predicted.

"We see discrepancies between these observations and the models and that is great news for advancing knowledge," said Mats Carlsson, an astrophysicist at the University of Oslo in Norway. "By seeing something we don't understand we have a chance of learning something new."
Carlsson helps support the crucial computer model component of IRIS' observations. The computer models require an intense amount of power. Modeling just an hour of events on the sun can take several months of computer time. IRIS relies on supercomputers at NASA's Ames Research Center in Moffett Field, Calif., the Norwegian supercomputer collaboration and the Partnership for Advanced Computing in Europe.
Such computer models had helped design the IRIS instruments by providing a basis for the instrument performance requirements. Currently, they are used for analysis of IRIS data, as they represent the state of knowledge about what scientists understand about the interface region. By comparing models with actual observations, researchers figure out where the models fail, and therefore where the current state of knowledge is not complete.
By filling in these gaps, IRIS observations are helping round out our images of the solar atmosphere. The Japanese Aerospace Exploration Agency/NASA Hinode mission provides detailed imagery of the solar surface. NASA's Solar Dynamics Observatory offers imagery of what's higher up in the corona. Now, IRIS provides unprecedented information about the crucial layer in between, to finally help us understand how energy moves through the lower levels of the solar atmosphere driving the solar wind and heating the corona.

NASA Engineers Crush Giant Fuel Tank To Improve Rocket Designs

Think of it as high-tech can crushing. Only the can is enormous, as big as part of the largest rocket ever made.
During a series of tests from Dec. 9-13 at NASA's Marshall Space Flight Center in Huntsville, Ala., engineers will apply nearly a million pounds of force to the top of an empty but pressurized rocket fuel tank. The test will eventually buckle and destroy the structure of the thin cylindrical tank wall while instruments precisely measure and record everything, millisecond by millisecond.
"What we learn will make it possible for NASA to design safe but still thinner and lighter structures for the Space Launch System and other spacecraft," said Dr. Mark Hilburger, senior research engineer in the Structural Mechanics and Concepts Branch at NASA's Langley Research Center in Hampton, Va.
In rocket science and engineering, every pound counts, and it costs to lift every pound to orbit. Rocket tanks are one of the heaviest parts of the rocket. If engineers can make tanks stronger and lighter, rockets can carry heavier payloads to space. That's the goal of the Shell Buckling and Knockdown Factor Project led by the NASA Engineering and Safety Center (NESC) in collaboration with Marshall and Langley teams.
Langley engineers are conducting their second full-scale tank test, nicknamed Can Crusher II, in Marshall's unique facility designed to test the full-size structures. Marshall engineers conducting the test have a keen interest in the results because the data will enhance the design of the heavy-lift Space Launch System (SLS), which is being developed by Marshall and will be the largest, most powerful rocket ever built.
Launch vehicles are composed of thin-walled cylindrical structures; if they are made lighter, buckling from the forces of launch and flight becomes a major concern. The project is developing a new, extremely accurate set of design standards for NASA and the aerospace industry, which has been using data that dates back to Apollo-era studies.
"In the 1960s when we went to the moon, those engineers did an amazing job with what they had," Hilburger said. "But they had to build conservative margins into their calculations because they didn't have today's materials or design, test and simulation tools. That means they built the launch vehicle heavier than it had to be, which can reduce the payload it can carry."
Since 2007, the Shell Buckling Knockdown Factors Project has been using cutting-edge test and analysis techniques to amass new data for design. The ultimate goal is to develop analyses and models that reflect the real-life test articles with extreme accuracy, so designers can use high-fidelity computer simulations and virtual tests to save time and money. "But we have to make sure that we ground those models in these carefully conducted real-world tests," Hilburger said.
In March 2011, the project team came to Marshall for what they believed to be the first test-to-failure of a full-scale, 27.5-foot-diameter, 20-foot-tall aluminum lithium test cylinder just for research purposes. It was reinforced with an orthogrid stiffener pattern, and the team squeezed it until it buckled, revealing the edges of the design margin.
The cylinder to be tested this time is External Tank-derived Test Article 2, or ETTA 2 Like ETTA 1 in 2011, it was built at Marshall from panels used for external tanks in the space shuttle program. This one is also 27.5 foot in diameter, the same diameter as SLS tanks, and 20 feet tall but will feature a different orthogrid stiffener pattern. Engineers can compare the results of this test to the first one to see if one pattern results in a stronger tank. At the top and bottom of the can are the load or pressure introduction structures made in the 1970s for the shuttle program.
"Using the heritage tank panels and Marshall’s valuable test facilities is saving millions in test dollars and time," Hilburger said.
The team prepared for next week's test to failure by running a series of sub-critical tests over the last few months. They've fitted the cylinder with more than 800 strain gauges, and 80 displacement transducers, and speckled ETTA 2 with markers used by a digital image correlation system. Cameras set up around the tank monitor the position of the dots during testing.
"We can actually track minute changes in the position of those dots and from that calculate displacements and strains on the entire test article," Hilburger said.
This week, there will be additional  exercises, and then the final day will be a test to failure scenario.
"We'll pressurize the structure to simulate an internal fuel pressure," Hilburger said. "And then we'll slowly start applying a combination of compression and bending to simulate a typical rocket flight condition."
Data from the team's work is already being incorporated into designs for the core stage of the SLS.
"When the new core stage flies, our design factors will be flying with it. It's very gratifying, but it's also nerve-wracking. When you're trying to reduce excess margins, you're obviously closer to failure, and want to make sure it's being done safely and with as much knowledge as possible.”
The shell buckling project activity has also given engineers at Marshall a great opportunity to hone skills. A lot of new technicians have received on-the-job training that will translate directly into SLS testing.
"This is my first large-scale structural test," said Matt Cash, lead test engineer for ETTA 2. "It's a fantastic experience, and everything I’m learning helps me prepare for SLS structural testing." Cash earned a degree in civil engineering with an emphasis on structures from the University of Alabama in Tuscaloosa. He's been a NASA employee for three years, and worked on the 2011 full-scale shell buckling test.
Because Marshall is one of the few places in the world where this kind of testing can be done, Cash said he's thrilled to be in the right place at the right time.
"The tests will provide extremely valuable data to SLS. I couldn't be happier to get to be a part of it."

2013/12/06

Science on the Shuttle's Spacelab

NASA Public Affairs Officer Lori Meggs talks about the 30th anniversary of the Spacelab Program with Marshall Space Flight Center Deputy Director Teresa Vanhooser.

Spacelab was a module inside the shuttle's payload bay where numerous science experiments were conducted. Vanhooser discusses how the missions were managed from Marshall and how it has paved the way for science on station today.

Fifteen Years Ago, International Space Station Assembly Begins

On Dec. 6, 1998, the crew of space shuttle mission STS-88 began construction of the International Space Station, attaching the U.S.-built Unity node and the Russian-built Zarya module together in orbit. The crew carried a large-format IMAX® camera, used to take this image of Unity lifted out of Endeavour's payload bay to position it upright for connection to Zarya.
Zarya, launched on Nov. 20, 1998, was the first piece of the International Space Station. Also known as the Functional Cargo Block (FGB), it would provide a nucleus of orientation control, communications and electrical power while the station waited for its other elements. Two weeks later, on Dec. 4, 1998, NASA's space shuttle Endeavour launched Unity, the first U.S. piece of the complex, during the STS-88 mission.

Thinking Inside the Box, Launching into Space

Two tiny, cube-shaped research satellites hitched a ride to Earth orbit to validate new hardware and software technologies for future NASA Earth-observing instruments.
The cube satellites, or “CubeSats,” which typically have a volume of exactly 33.814 ounces (1 liter), were launched on a United Launch Alliance Atlas V rocket at 11:14 p.m. PST last night (Dec. 5) from California's Vandenberg Air Force Base as part of the NROL-39 GEMSat mission. Led by NASA's Jet Propulsion Laboratory, Pasadena, Calif., and developed with university and industry partners, these two CubeSats will help enable near-real-time processing capabilities relevant to future climate science measurements.
One of the CubeSats that launched was developed in collaboration with California Polytechnic State University, San Luis Obispo, and is called the Intelligent Payload Experiment, or IPEX. It enables imagery to be transmitted more rapidly from satellite missions back to Earth. By using new software and algorithms, the spacecraft can sift through the data, looking only for the most important images that the scientists urgently need on the ground. This method is designed to speed delivery time of critical data products from days to minutes.
“IPEX will demonstrate software that will enable future NASA missions to recognize science events such as flooding, volcanism and wildfires, and respond by sending alerts and autonomously acquiring follow-up imagery,” said Steve Chien of JPL, principal investigator for the IPEX mission.
The other CubeSat launched is the Michigan Multipurpose Mini-satellite/CubeSat On-board processing Validation Experiment, or M-Cubed/COVE.
M-Cubed, developed in partnership with the University of Michigan, Ann Arbor, will image Earth. The COVE payload will use these data to validate an instrument image data processing algorithm that will greatly reduce the science data transmission rate required for on-orbit operations.
“The COVE payload will advance processor and algorithm technology designed for use in a future science instrument to characterize properties of aerosols and clouds, which will help our understanding of global climate change,” said Paula Pingree of JPL, principal investigator of the MCubed/COVE-2 mission.
These technology validation missions are sponsored by NASA’s Earth Science Technology Office. They are designed to satisfy their science objectives within six months, but will remain in Earth orbit for many years.
The California Institute of Technology in Pasadena manages JPL for NASA.
The NROL-39 GEMSat mission lifted off from California's Vandenberg Air Force Base on Dec. 5, 2013, aboard a United Launch Alliance Atlas V rocket.

Artist's concept of the Intelligent Payload Experiment (IPEX) and M-Cubed/COVE-2, two NASA Earth-orbiting cube satellites ("CubeSats") that were launched as part of the NROL-39 GEMSat mission from California's Vandenberg Air Force Base on Dec. 5, 2013.

Space to Ground

The "Space to Ground" web series, available every Friday, features a short wrap-up of the week's activities aboard the International Space Station that showcases the diversity of activities taking place aboard the world's only orbiting laboratory.
If you have questions or comments, use #spacetoground to interact with us. You might just see them in one of our episodes!

2013/12/05

Heat Shield for NASA's Orion Spacecraft Arrives at Kennedy Space Center

Orion's heat shield is loaded onto the Super Guppy in Manchester, N.H., for transport to Kennedy Space Center in Florida.
NASA's Orion spacecraft is just about ready to turn up the heat. The spacecraft's heat shield arrived at the agency's Kennedy Space Center in Florida Wednesday night aboard the agency's Super Guppy aircraft.
The heat shield, the largest of its kind ever built, is to be unloaded Thursday and is scheduled for installation on the Orion crew module in March, in preparation for Orion's first flight test in September 2014.
› Video: Textron team readies Orion heat shield for shipment to Kennedy
"The heat shield completion and delivery to Kennedy, where Orion is being prepared, is a major step toward Exploration Flight Test-1 next year," said Dan Dumbacher, NASA's deputy associate administrator for exploration systems development in Washington. "Sending Orion into space for the first time is going to give us crucial data to improve our design decisions and develop Orion to send humans on future missions to an asteroid and Mars."
The heat shield began its journey in January 2012 in Colorado, at Orion prime contractor Lockheed Martin's Waterton Facility near Denver. That was the manufacturing site for a titanium skeleton and carbon fiber skin that give the heat shield its shape and provide structural support during landing. They were shipped in March to Textron Defense Systems near Boston, where they were used in construction of the heat shield itself.
Textron installed a fiberglass-phenolic honeycomb structure on the skin, filled each of the honeycomb's 320,000 cells with the ablative material Avcoat, then X-rayed and sanded each cell to match Orion's design specifications. The Avcoat-treated shell will shield Orion from the extreme heat it will experience as it returns to Earth. The ablative material will wear away as it heats up during Orion's re-entry into the atmosphere, preventing heat from being transferred to the rest of the capsule.
"Many people across the country have poured a tremendous amount of hard work into building this heat shield," said Orion Program Manager Mark Geyer. "Their efforts are a critical part of helping us understand what it takes to bring a human-rated spacecraft back safely from deep space."
Before and during its manufacture, the heat shield material was subjected to arc-jet testing NASA's Ames Research Center in California and NASA's Johnson Space Center in Houston. Arc jets heat and expand gasses to very high temperatures and supersonic and hypersonic speeds, thus simulating the heating conditions that a returning spacecraft will experience.
The heat shield delivered to Kennedy will be used during Exploration Flight Test-1, a two-orbit flight that will take an uncrewed Orion capsule to an altitude of 3,600 miles. The returning capsule is expected to encounter temperatures of almost 4,000 degrees Fahrenheit as it travels through Earth's atmosphere at up to 20,000 mph, faster than any spacecraft in the last 40 years.
Data gathered during the flight will influence decisions about design improvements on the heat shield and other Orion systems, authenticate existing computer models, and innovative new approaches to space systems and development. It also will reduce overall mission risks and costs for future Orion missions, which include exploring an asteroid and Mars.

Laser Instrument on NASA Mars Rover Tops 100,000 Zaps

NASA's Curiosity Mars rover has passed the milestone of 100,000 shots fired by its laser. It uses the laser as one way to check which chemical elements are in rocks and soils.
The 100,000th shot was one of a series of 300 to investigate 10 locations on a rock called "Ithaca" in late October, at a distance of 13 feet, 3 inches (4.04 meters) from the laser and telescope on rover's mast. The Chemistry and Camera instrument (ChemCam) uses the infrared laser to excite material in a pinhead-size spot on the target into a glowing, ionized gas, called plasma. ChemCam observes that spark with the telescope and analyzes the spectrum of light to identify elements in the target.
"Passing 100,000 laser shots is terribly exciting and is providing a remarkable set of chemical data for Mars," said ChemCam co-investigator Horton Newsom of the University of New Mexico, Albuquerque.
As of the start of December, ChemCam has fired its laser on Mars more than 102,000 times, at more than 420 rock or soil targets. Virtually every shot yields a spectrum of data returned to Earth. Most targets get zapped at several points with 30 laser pulses at each point. The instrument has also returned more than 1,600 images taken by its remote micro-imager camera.
An international team of scientists and students is mining information from ChemCam to document the diversity or materials on the surface inside Mars' Gale Crater and the geological processes that formed them. "These materials include dust, wind-blown soil, water-lain sediments derived from the crater rim, veins of sulfates and igneous rocks that may be ejecta from other parts of Mars," Newsom said.
Each pulse delivers more than a million watts of power for about five one-billionths of a second. The technique used by ChemCam, called laser-induced breakdown spectroscopy, has been used to assess composition of targets in other extreme environments, such as inside nuclear reactors and on the sea floor. Experimental applications have included environmental monitoring and cancer detection. NASA's Mars Science Laboratory Project, using the Curiosity rover, is the first mission to use it on another planet.
ChemCam is one of 10 instruments in Curiosity's science payload. The U.S. Department of Energy's Los Alamos National Laboratory, Los Alamos, N.M., developed ChemCam in partnership with scientists and engineers funded by the French national space agency, CNES, the University of Toulouse and research agency, CNRS. The laser was built by Thales, Paris. More information about ChemCam is available at http://www.msl-chemcam.com .
NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project, including Curiosity, for NASA's Science Mission Directorate, Washington. JPL designed and built the rover.
Since landing on Mars in August 2012, NASA's Curiosity Mars rover has fired the laser on its Chemistry and Camera (ChemCam) instrument more than 100,000 times at rock and soil targets up to about 23 feet (7 meters) away.