Spacewalkers Move Crane, Install Experiment

International Space Station Expedition 30 Flight Engineers Oleg Kononenko and Anton Shkaplerov wrapped up a six-hour, 15-minute spacewalk at 3:46 p.m. EST Thursday.

The two spacewalkers moved the Strela-1 crane from the Pirs docking compartment to begin preparing the Pirs for its replacement next year with a new laboratory and docking module. Kononenko and Shkaplerov used another boom, the Strela-2, to move the hand-operated crane to the Poisk module for future assembly and maintenance work. Both telescoping booms extend like fishing rods and are used to move massive components outside the station. This task was originally scheduled during an Expedition 28 spacewalk on Aug. 3, 2011, but was called off due to time constraints.

While Kononenko and Shkaplerov were on the exterior of Poisk, they also installed the Vinoslivost Materials Sample Experiment, which will investigate the influence of space on the mechanical properties of the materials.

Shuttle Fleet Left Mark in Space, Hearts

The space shuttle left its 30 years of achievements written in the sky above and in the hearts of the astronauts, American and international, who flew in them.

"Personally, looking back on it, I think the shuttle has been one of the most marvelous vehicles that has ever gone into space or done anything," said Bob Crippen, the iconic pilot on the first space shuttle mission in 1981, and commander of three more after that.

The shuttle broke boundaries of all sorts during its career, from technological successes to reflecting the evolution of American and global society. International cooperation that was commonplace as the shuttle neared the end of its work was unforeseen when the shuttle program began.

The thousands of space workers who physically readied the fleet to fly and those who worked meticulous mental problems to calculate orbits and rendezvous along with thrust and innumerable other considerations, also shared in the successes of the spacecraft that served as NASA's flagship for three decades.

"It was not like any airplane that you've ever been on or seen or been around," said Wayne Bingham of the United Space Alliance. "It was just like a big glider that you had played with as a kid, but much more impressive. You just kind of stood in awe of what the orbiter was capable of doing."

Source : http://www.nasa.gov/mission_pages/shuttle/flyout/shuttleachievements.html

NuSTAR Spacecraft Arrives in California

NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, mission arrived at Vandenberg Air Force Base in California this morning after a cross-country trip by truck from the Orbital Sciences Corporation's manufacturing plant in Dulles, Va. The mission is scheduled to launch from Kwajalein Atoll in the Pacific Ocean on March 14.

Once the observatory is offloaded at Vandenberg, it will be moved into a processing hangar, joining the Pegasus XL rocket that is set to carry it to space. Over the weekend, technicians will remove its shipping container so that checkout and other processing activities can begin next week. Once the observatory is integrated with the rocket in mid-February, technicians will encapsulate it in the vehicle fairing, which is also scheduled to arrive at Vandenberg today.

After processing is completed, the rocket and spacecraft will be flown on Orbital's L-1011 carrier aircraft to the Ronald Reagan Ballistic Missile Defense Test Site at Kwajalein Atoll for launch in March.

Read more, visit: http://www.nasa.gov/mission_pages/nustar/news/nustar20120127.html

'We are the Champions' on the International Space Station

In high school, there are champions of football and basketball and even music, but not many students can say they are champs on the International Space Station - but Alliance Rocket students from the United States and virtual participants Alliance CyberAvo, representing schools in Germany and Italy, have now earned that distinction.

Both teams were named the winners in the third annual NASA-sponsored Zero Robotics SPHERES Challenge competition for high school students from the United States and abroad.

NASA, the Defense Advanced Research Projects Agency and the Massachusetts Institute of Technology in Cambridge sponsored the competition, which challenged students to write software code for small satellite robots on the station.

"This competition helps to build critical engineering skills for students, such as problem solving and teamwork, and helps us to find future scientists and engineers to work in space," said Leland Melvin, NASA associate administrator for education at NASA Headquarters in Washington. "The teams this year did not disappoint. The students were exceptional with their designs and flight programs."

Read More : http://www.nasa.gov/mission_pages/station/research/news/Zero_Robotics.html

The 'Un-Flyable' Space Shuttle

The first time NASA engineer George Ware saw a model for the space shuttle, four decades ago, it had a straight wing and tail like a fighter airplane. It had elevators, a rudder and an engine.

It was un-flyable.

"It was their idea that it was going to enter the atmosphere at a 60-degree angle," said Ware, who had just joined the Vehicle Analysis Branch at NASA's Langley Research Center in Hampton, Va., which was tasked with testing shuttle configurations offered by the Johnson Space Center and contractors.

"At some lower speed, closer to transonic, it would pitch over and start flying like an airplane," said Ware, now retired. "It would be on a reusable booster as well."

It was supposed to fly up to 50 times a year at $10 million per trip. But that return to Earth was throwing everybody, because air flow onto the straight wing as it came into the atmosphere caused the plane to crash, at least on paper. Models of all four candidate configurations had problems, and the two boosters attached to them and tested in various combinations didn't help.

Ware still has lab books that look as though they have red-inked brushfires ignited by failed tunnel tests of shuttle and booster. Langley wind tunnels logged 59,200 hours from 1970-82, with the work spread over a dozen facilities. That included time spent with what was the eventual shuttle: a double-delta shaped craft.

For more info, visit : http://www.nasa.gov/mission_pages/shuttle/flyout/unflyable.html

NASA Moves Shuttle Engines From Kennedy To Stennis

The relocation of the RS-25D space shuttle main engine inventory from Kennedy Space Center's Engine Shop in Cape Canaveral, Fla., is underway. The RS-25D flight engines, repurposed for NASA's Space Launch System, are being moved to NASA's Stennis Space Center in south Mississippi.

The Space Launch System (SLS) is a new heavy-lift launch vehicle that will expand human presence beyond low-Earth orbit and enable new missions of exploration across the solar system. The Marshall Space Flight Center in Huntsville, Ala., is leading the design and development of the SLS for NASA, including the engine testing program. SLS will carry the Orion spacecraft, its crew, cargo, equipment and science experiments to destinations in deep space.

"The relocation of RS-25D engine assets represents a significant cost savings to the SLS Program by consolidating SLS engine assembly and test operations at a single facility," said William Gerstenmaier, NASA’s Associate Administrator for Human Exploration and Operations Mission Directorate.

The RS-25Ds - to be used for the SLS core stage - be stored at Stennis until testing begins at a future date. Testing is already under way on the J-2X engine, which is planned for use in the SLS upper stage. Using the same fuel system - hydrogen and liquid oxygen - for both core and upper stages reduces costs by leveraging the existing knowledge base, skills, infrastructure and personnel.

For more info, visit: http://www.nasa.gov/exploration/systems/sls/rs25d.html

Cassini Testing Part of Its Radio System

Engineers with NASA's Cassini mission are conducting diagnostic testing on a part of the spacecraft's radio system after its signal was not detected on Earth during a tracking pass in late December. The spacecraft has been communicating with Earth using a backup part.

The issue occurred with the ultra-stable oscillator, which is used for one type of radio science experiment and also as a means of sending data back to Earth. The spacecraft is currently using an auxiliary oscillator, whose frequency stability is adequate for transmitting data from the spacecraft to Earth. Tests later this month will help mission managers decide whether it will be possible to bring the ultra-stable oscillator back into service.

Some of the data collected for the radio science experiment using the auxiliary oscillator will be of lesser quality than that from the ultra-stable oscillator. Signals used for occultation experiments – where scientists analyze how radio signals are affected as they travel through Saturn's rings or the atmospheres of Saturn and its moons back to Earth – will be of lesser quality. A second kind of radio science investigation using gravity measurements to probe the internal structure of Saturn or its moons will not be affected. Cassini carries 12 science experiments.

The cause is still under investigation, but age may be a factor. The spacecraft launched in 1997 and has orbited Saturn since 2004. Cassini completed its prime mission in 2008 and has had two additional mission extensions. This is the first time its ultra-stable oscillator has had an issue.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory in Pasadena manages the mission for the agency's Science Mission Directorate in Washington.

NASA Propulsion Experiment Provides Data for More Efficient Jet Engines

Aeronautics researchers at NASA's Dryden Flight Research Center recently completed flight tests of a unique experimental jet engine inlet design in the Channeled Center-body Inlet Experiment, or CCIE.

The experimental inlet was checked out on NASA Dryden's F-15B aeronautics research test bed aircraft, which continues to be an innovative and cost-effective tool for flight test of advanced propulsion concepts.

The CCIE project's primary research objective was to define the airflow through the experimental jet engine inlet, then compare it to the airflow through a standard inlet. Inside, airflow around two interchangeable center bodies installed in an air inlet tube was measured. The structures are designed to direct and compress airflow internally through the engine.

One center body is channeled; the other has a conventional, smooth shape. The slots cut along the length of the channeled center body simulate a simple device that in an actual inlet would allow optimization of the amount of air flowing into the engine, resulting in improved airflow efficiency at a wide variety of speeds. This would improve fuel efficiency as well.

Six flights were flown, three with each center body installed. Flight tests were made incrementally at speeds up to Mach 1.74, or about 1.7 times the speed of sound. Flight data from the smooth center body were used to benchmark performance data for the channeled center body. Data points that NASA Dryden engineers collected during the experiment included inlet mass airflow information, internal surface pressure distribution numbers, and airflow distortion, or turbulence, data at the exit end of the device.

For more info, visit : http://www.nasa.gov/centers/dryden/Features/ccie.html

Shuttle Model Move Shows Way for Atlantis

Moving the high fidelity model of the space shuttle Dec. 10 called for an array of planning, about 100 people and a specialized trailer. It also called for the temporary removal of 18 light poles, four traffic signals and some signs.

It took the team about five hours to make the six-mile trip from the Kennedy Space Center Visitor Complex to the Turn Basin across the street from the Vehicle Assembly Building. The group started rolling at 7:30 a.m. so they wouldn't have to worry about the dark.

"It went very well," said Gerald "Jay" Green, project manager for the move. "I felt a great sense of accomplishment when we got it done."

A similar move will be made next year when space shuttle Atlantis is taken the opposite direction to its display location at the Visitor Complex.

The model's convoy never traveled more than about 6 mph. It came to a stop many times along the way so the trailer's built-in jacks could raise or lower the wings to get past obstacles such as guard shacks and traffic lights.

"There were four or five really hard spots," Green said.

But then, moving space shuttles and full-scale model shuttles has always required extra consideration. For instance, crews moving a space shuttle through the mountains in California had to cut slots in the rock to make room for the wings.

Moving the model didn't require such an extreme action, but it took a month of planning and considerable study of potential routes. Even 3-D modeling was incorporated to find problem zones. All this was before Green and his group found out they would have to move it with the wings attached.

For more info, visit :

http://www.nasa.gov/centers/kennedy/news/explorermove.html

NASA Launches Mission to Study Moon From Crust to Core

NASA's twin lunar Gravity Recovery and Interior Laboratory (GRAIL) spacecraft lifted off from Cape Canaveral Air Force Station in Florida at 9:08 a.m. EDT (6:08 a.m. PDT) Saturday, Sept. 10, to study the moon in unprecedented detail.

GRAIL-A is scheduled to reach the moon on New Year's Eve 2011, while GRAIL-B will arrive New Year's Day 2012. The two solar-powered spacecraft will fly in tandem orbits around the moon to measure its gravity field. GRAIL will answer longstanding questions about the moon and give scientists a better understanding of how Earth and other rocky planets in the solar system formed.

"If there was ever any doubt that Florida's Space Coast would continue to be open for business, that thought was drowned out by the roar of today's GRAIL launch," said NASA Administrator Charles Bolden. "GRAIL and many other exciting upcoming missions make clear that NASA is taking its next big leap into deep space exploration, and the space industry continues to provide the jobs and workers needed to support this critical effort."

The spacecraft were launched aboard a United Launch Alliance Delta II rocket. GRAIL mission controllers acquired a signal from GRAIL-A at 10:29 a.m. EDT (7:29 a.m. PDT). GRAIL-B's signal was received eight minutes later. The telemetry downlinked from both spacecraft indicates they have deployed their solar panels and are operating as expected.

NASA Selects Seven Firms to Provide Near-Space Flight Services

NASA has selected seven companies to integrate and fly technology payloads on commercial suborbital reusable platforms that carry payloads near the boundary of space.

As part of NASA's Flight Opportunities Program, each successful vendor will receive an indefinite-delivery, indefinite-quantity contract. These two-year contracts, worth a combined total of $10 million, will allow NASA to draw from a pool of commercial space companies to deliver payload integration and flight services. The flights will carry a variety of payloads to help meet the agency's research and technology needs.

"Through this catalog approach, NASA is moving toward the goal of making frequent, low-cost access to near-space available to a wide range of engineers, scientists and technologists," said NASA Chief Technologist Bobby Braun at NASA Headquarters in Washington. "The government's ability to open the suborbital research frontier to a broad community of innovators will enable maturation of the new technologies and capabilities needed for NASA's future missions in space."

For more info, visit:
http://www.nasa.gov/centers/dryden/news/NewsReleases/2011/11-258.html

NASA scientists have successfully completed flight tests in preparation for deployment of a multi-year airborne science campaign to study the humidity and chemical composition of air entering the tropical tropopause layer of the atmosphere. NASA's Airborne Tropical TRopopause EXperiment (ATTREX) will conduct the science campaign over the Pacific Ocean from three locations in 2013 and 2014.

Studies have shown that even small changes in stratospheric humidity may have climate impacts that are significant compared to those of decadal increases in greenhouse gases. Predictions of stratospheric humidity changes are uncertain, due to gaps in the understanding of the physical processes occurring in the tropical tropopause layer, which ranges from about eight to 11 miles above the ground.

"These were test flights, although we did get science-quality data, including samples from tropical thin cirrus clouds at about 55,000 feet altitude," said Leonhard Pfister, ATTREX deputy principal investigator at NASA’s Ames Research Center in Moffett Field, Calif. "These clouds regulate water vapor in the lower tropical stratosphere, which is important for Earth's radiation balance."

Pfister will discuss the ATTREX mission goals, objectives and planned research flights at the Monday, Dec. 5, afternoon poster session at the American Geophysical Union Fall meeting held at the Moscone Center, San Francisco, Calif.

Led by principal investigator Eric Jensen and project manager Dave Jordan of NASA Ames, scientists integrated instruments onto one of NASA's Global Hawk unmanned aircraft and verified their operation during four checkout flights from NASA's Dryden Flight Research Center at Edwards, Calif.

For more info, visit:
http://www.nasa.gov/centers/dryden/news/NewsReleases/2011/11-37.html

Growing Knowledge in Space

Plants are critical in supporting life on Earth, and with help from an experiment that flew onboard space shuttle Discovery's STS-131 mission, they also could transform living in space.

NASA's Kennedy Space Center partnered with the University of Florida, Miami University in Ohio and Samuel Roberts Noble Foundation to perform three different experiments in microgravity.

The studies concentrated on the effects microgravity has on plant cell walls, root growth patterns and gene regulation within the plant Arabidopsis thaliana. Each of the studies has future applications on Earth and in space exploration.

"Any research in plant biology helps NASA for future long-range space travel in that plants will be part of bioregenerative life support systems," said John Kiss, one of the researchers who participated in the BRIC-16 experiment onboard Discovery's STS-131 flight in April 2010 and a distinguished professor and chair of the Department of Botany at Miami University in Ohio.

The use of plants to provide a reliable oxygen, food and water source could save the time and money it takes to resupply the International Space Station (ISS), and provide sustainable sources necessary to make long-duration missions a reality. However, before plants can be effectively utilized for space exploration missions, a better understanding of their biology under microgravity is essential.

We are in Antarctica

Our military C-17 flight landed on 2.3-meter thick sea ice in McMurdo Sound. McMurdo has three airfields that are used at different times during the austral summer. The sea-ice runway is located a few miles from McMurdo, and it usually operates from October to December, until the sea ice begins to break.

For a large number of us, this is our first time on the southernmost continent on Earth and, as you can imagine, landing on McMurdo Sound’s sea ice felt very special. The first minutes off the plane everyone was looking around and smiling a lot.

Weather conditions on landing were nice, despite a low cloud that turned everything extremely bright and made it difficult to tell the sky from the snow-covered ice.

Shortly after stepping into the snow, we had to jump into one of the two charismatic vehicles that were ready to transport us to McMurdo Station. We could choose between the famous Ivan the Terra Bus (red as our parka, a.k.a. the Big Red) or an orange delta truck from the early 80s (that vehicle was already carrying people from the runway to McMurdo station before I was born!). Both vehicles have incredibly big tires.

Spacecraft Design

MESSENGER's dual-mode, liquid chemical propulsion system is integrated into the spacecraft's structure to make economical use of mass. The structure is primarily composed of a graphite epoxy material. This composite structure provides the strength necessary to survive launch while offering lower mass. Two large solar panels, supplemented with a nickel-hydrogen battery, provide MESSENGER's power.

The "brains" of the spacecraft are redundant integrated electronics modules (IEMs) that house two processors each -- a 25-megahertz (MHz) main processor and a 10-MHz fault-protection processor.

Mercury Dual Imaging System (MDIS): This instrument consists of wide-angle and narrow-angle imagers that will map landforms, track variations in surface spectra and gather topographic information. A pivot platform will help point it in whatever direction the scientists choose. The two instruments will enable MESSENGER to "see" much like our two eyes do.

Gamma-Ray and Neutron Spectrometer (GRNS): This instrument will detect gamma rays and neutrons that are emitted by radioactive elements on Mercury's surface or by surface elements that have been stimulated by cosmic rays. It will be used to map the relative abundances of different elements and will help to determine if there is ice at Mercury's poles, which are never exposed to direct sunlight.

Gamma rays and high-energy X-rays from the Sun, striking Mercury's surface, can cause the surface elements to emit low-energy X-rays. XRS will detect these emitted X-rays to measure the abundances of various elements in the materials of Mercury's crust.

Magnetometer (MAG): This instrument is at the end of a 3.6 meter (nearly 12-foot) boom, and will map Mercury's magnetic field and will search for regions of magnetized rocks in the crust.

Mercury Laser Altimeter (MLA): This instrument contains a laser that will send light to the planet's surface and a sensor that will gather the light after it has been reflected from the surface. Together they will measure the amount of time for light to make a round-trip to the surface and back. Recording variations in this distance will produce highly accurate descriptions of Mercury's topography.

Mercury Atmospheric and Surface Composition Spectrometer (MASCS): This spectrometer is sensitive to light from the infrared to the ultraviolet and will measure the abundances of atmospheric gases, as well as detect minerals on the surface.

Energetic Particle and Plasma Spectrometer (EPPS): EPPS measures the composition, distribution, and energy of charged particles (electrons and various ions) in Mercury's magnetosphere.

Radio Science (RS): RS will use the Doppler effect to measure very slight changes in the spacecraft's velocity as it orbits Mercury. This will allow scientists to study Mercury's mass distribution, including variations in the thickness of its crust.

The Suzaku Spacecrafts and Instruments

The Spacecraft

The Suzaku spacecraft weighs about 1,600 kg (3500 pounds) and it will be 7.1 meters (23 feet) long after the Extensible Optical Bench is extended in orbit. The five X-ray Telescopes (XRTs) and all the instruments (the X-Ray Spectrometer, the 4 X-ray Imaging Spectrometers, and the Hard X-ray Detector) will point in the same direction. This allows scientists to simultaneously study cosmic X-ray sources using the different capabilities of the various onboard instruments.

X-Ray Spectrometer (XRS)

The detectors in the X-Ray Spectrometer (XRS) are X-ray microcalorimeters. They work by monitoring the temperature of a tiny piece of silicon, and measuring the temperature rise that results when it absorbs an X-ray photon. As you might imagine, measuring the temperature increase from a single photon is fairly difficult. The detectors need to be kept extremely cold, almost to absolute zero (60 milliKelvin or 0.06 Kelvin, about -273 C, or about -460 F), requiring a complex cryogenic system which includes liquid helium and solid neon.

The XRS has a limited life of about 2.5 years before the neon and/or helium runs out. The XRS is special because, for the first time, it will provide both high spectral resolution (measuring small differences in the energies of X-ray photons) and high throughput (measuring lots of X rays) in one instrument.

X-ray Imaging Spectrometer (XIS)

There are 4 X-ray Imaging Spectrometers (XIS), each with a 1024x1024-pixel X-ray-sensitive Charge Coupled Device (a CCD, similar to what's in your digital camera, but sensitive to much more energetic light). The use of CCDs for astronomical X-ray spectroscopy was pioneered by the ASCA mission starting in 1993. The XIS has been developed by a collaboration of the Massachusetts Institute of Technology, ISAS, the University of Kyoto, and the University of Osaka. It was fabricated by MIT's Lincoln Laboratory.

For more info, visit: http://www.nasa.gov/mission_pages/astro-e2/spacecraft/index.html

Mars Rover Well-Equipped for Studies

The Mars Science Laboratory is taking a toolbox to Mars that any researcher would be proud of. A drill, metallic brush and even a laser are part of the gear set the Mars Science Laboratory called Curiosity is taking to the red planet in the most ambitious effort yet to discern exactly what is on the surface.

The spacecraft is to launch Nov. 26 atop a United Launch Alliance Atlas V rocket. Liftoff is slated for 10:02 a.m. It will take more than eight months for Curiosity to fly the 354 million miles on its path to Mars. Landing is expected in early August 2012.

Although calling the spacecraft a laboratory might suggest it will stay in one place, Curiosity actually is a rover that will travel some 12 miles inside Gale Crater during its 23-month mission. The size of a car or small SUV, the rover weighs nearly a ton and its scientific payload is 10 times more massive than the instrument sets taken to Mars by previous rovers.

"This is a vehicle on Mars, cruising around, drilling into rocks, chipping away at stuff to see what that planet's made out of," said Omar Baez, the launch director of the MSL mission. "And even if it didn't do that, if it just cruised around Mars and took pictures, the value in that is tremendous."

Curiosity will be the fourth NASA rover to touch down on Mars since July 1997, when the Pathfinder probe and its skateboard-sized Sojourner rover bounced onto the surface and began several months of analysis that suggested early Mars was a lot like Earth, with water at the surface and a thicker atmosphere.

Mars Science Laboratory Launch Milestones

NASA's Mars Science Laboratory is tucked inside its Atlas V rocket, ready for launch on Saturday, Nov. 26, 2011 from Cape Canaveral Air Force Station in Florida. The Nov. 26 launch window extends from 7:02 a.m. to 8:45 a.m. PST (10:02 a.m. to 11:45 a.m. EST). The launch period for the mission extends through Dec. 18.

The spacecraft, which will arrive at Mars in August 2012, is equipped with the most advanced rover ever to land on another planet. Named Curiosity, the rover will investigate whether the landing region has had environmental conditions favorable for supporting microbial life, and favorable for preserving clues about whether life existed.

On Nov. 26, NASA Television coverage of the launch will begin at 4:30 a.m. PST (7:30 a.m. EST). Live launch coverage will be carried on all NASA Television channels. For NASA Television downlink information, schedule information and streaming video, visit: http://www.nasa.gov/ntv .
 The launch coverage will also be streamed live on Ustream at http://www.ustream.tv/nasajpl .