Washington, U.S.A. —  NASA was named the best place to work in the federal government among large agencies in a survey released today by the Partnership for Public Service, a nonprofit, non-partisan organization. This ranking, which reflects NASA’s highest results since this index was developed, makes clear that the agency’s work force is focused on carrying out the nation’s new and ambitious space program.

“The best workforce in the nation has made NASA the best place to work in federal government,” said NASA Deputy Administrator Lori Garver, who is accepting the award at a ceremony this morning in Washington, D.C. ”Our employees are carrying out the nation’s new strategic missions in space with heart-stopping landings on Mars, cutting-edge science and ground-breaking partnerships with American companies to resupplying the space station. They are truly leading in the innovation economy.”

The rankings are based on responses from nearly 700,000 federal workers. The Best Places to Work rankings are based on data from the Office of Personnel Management’s annual Federal Employee Viewpoint Survey conducted from April through June 2012 and additional survey data from nine agencies plus the Intelligence Community. This is the seventh edition of the Best Places to Work rankings since the first in 2003.

NASA’s Stennis Space Center was ranked second in the sub-agency component category.

During the past year, NASA’s employees continued to implement America’s ambitious space exploration program, landing the most sophisticated rover on the surface of Mars, carrying out the first-ever commercial mission to the International Space Station and advancing the systems needed to send humans deeper into space.

Just last week, NASA announced the next Mars rover mission and recently announced the first year-long crew stay on the International Space Station. As the agency continues developing the capabilities to explore the solar system and beyond, as well as understand our home planet and make life better here, workers with a wide range of skills and interests will be critical.

For more about NASA, visit: http://www.nasa.gov.

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Washington, U.S.A. – NASA is seeking proposals from accredited U.S. universities focused on innovative, early-stage space technologies that will improve shielding from space radiation, spacecraft thermal management and optical systems.

Each of these technology areas requires dramatic improvements over existing capabilities for future science and human exploration missions. Early stage, or low technology readiness level (TRL) concepts, could mature into tools that solve the hard challenges facing future NASA missions. Researchers should propose unique, disruptive or transformational space technologies that address the specific topics described in this new solicitation.

“Both science and human deep space missions pose serious challenges that require new, innovative technological solutions,” said Space Technology Program Director Michael Gazarik at NASA Headquarters in Washington. “Radiation, thermal management and optical systems were all identified in the National Research Council’s report on NASA Space Technology Roadmaps as priority research areas. This call seeks new ideas in these areas.”

Space radiation poses a known danger to the health of astronauts. NASA is seeking proposals in the area of active radiation shielding (such as “shields” of electromagnetic force fields surrounding a spacecraft to block incoming radiation) or new, multifunction materials that are superior to those that exist today are sought. NASA also is interested in new technologies for active monitoring and read-out of radiation levels astronauts receive during long space trips.

Current space technology for thermal management of fuels in space is limited. NASA is seeking early-stage technologies to improve ways spacecraft fuel tanks and in-space filling stations store cryogenic (very low temperature) propellants, such as hydrogen, over long periods of time and distances. NASA also is seeking novel, low-TRL heat rejection technologies which operate reliably and efficiently over a wide range of thermal conditions.

The next generation of lightweight mirrors and telescopes requires advanced optical systems. NASA is seeking advancement of early-stage active wavefront sensing and control system technologies that enable deployable, large aperture space-based observatories; technologies which enable cost-effective development of grazing-incidence optical systems; and novel techniques to focus and detect X-ray photons and other high-energy particles.

NASA expects to make approximately 10 awards this fall, based on the merit of proposals received. The awards will be made for one year, with an additional year of research possible. The typical annual award value is expected to be approximately $250,000.

Image Courtesy of  NASA

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Earlier this month, NASA (National Aeronautics and Space Administration) once again found groundbreaking evidence that water once existed on Mars. The rover, Opportunity, has discovered a long, thin vein of gypsum deposit, found on the edge of the crater, Endeavor.

In January 2004, NASA sent the twin rovers, Opportunity and Spirit, to Mars as a part of the Mars Exploration Rover Mission to find clues that water once existed. Opportunity and Spirit discovered gypsum to be as much of a common mineral on Mars as it is on Earth. Gypsum, which is used as drywall and as an ingredient for plaster, is found evaporated in sedimentary environments, particularly in saline water beds (or seawater) containing high amounts of dissolved calcium sulfate (CaSO₄).

Since their landing on Mars, the rovers found, in the northern sand dunes, numerous pieces of gypsum, which were blown by winds and, hence, mixed with other minerals and materials. These dunes are similar to the White Sands National Monument located in New Mexico, where the sands are comprised of gypsum crystals. This discovery is one of the few that proves that water existed on Mars, but from where the gypsum originates baffles scientists.

Sometime in early 2010, Spirit had discontinued its mission due to being stuck and its eventual inability to communicate. Opportunity, on the other hand, has remained alive and active, and eventually found the gypsum deposit, slightly jutting out from the bedrock. The vein is approximately 2 cm wide and 50 cm long.

Although this discovery may seem redundant with the ones made in the past, it turns out that this strand of gypsum is more significant than the pieces found in dunes. Not only does it appear to have formed in place, but the deposit tells us that water once flowed through a crevice long ago.

“That can’t be said for other gypsum seen on Mars or for other water-related minerals Opportunity has found,” remarks Steve Squyres, a planetary scientist at Cornell University. “It’s not uncommon on Earth, but on Mars, it’s the kind of thing that makes geologists jump out of their chairs.”

Opportunity and Spirit have analyzed most Martian areas to be acidic – and definitely not suitable for life. However, the spot in which the gypsum deposit was found does contain the substances that cause acidity. Thus, the water may have been more neutral. Not only is the vein a sure sign that Mars once did have water, it also proves that the red and dusty planet may have been more habitable than we thought.

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Earlier this week, the spacecraft, Kepler, discovered two exoplanets around the size of the earth – the first of their kind – orbiting a sun-like star. Named Kepler-20e and Kepler-20f, these exoplanets are a part of the star system, Kepler-20, which lies 950 light years away from Earth near the constellation, Lyra.

“This discovery demonstrates for the first time that Earth-size planets exist around other stars and that we are able to detect them,” says Dr. Francois Fressin, an astronomer at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts.

Launched in 2009, Kepler is a space telescope built and sent by NASA to detect Earth-like exoplanets (also known as extrasolar planets, which are planets that exist outside our solar system) orbiting stars in habitable zones. Its most recent, significant discovery occurred in early December, when it detected the Neptune-sized Kepler-22b, the first of its kind that has been seen orbiting in the “Goldilocks zone” and that might possibly have water and life.

Kepler took a step closer in accomplishing its mission when it detected Kepler-20, Kepler-20e, and Kepler-20f. Kepler-20 is similar to the sun, in that it is a G-type star. It is yellowish, though a bit smaller and cooler. The star contains five planets in total, all of which orbit it closer than Mercury orbits the sun. The three other planets are gas giants, which are about the size of Neptune, and each planet orbits alternating in size.

These newly discovered exoplanets are only Earth-like in their sizes and rocky composition. Kepler-20e orbits its star every 6.1 days, and its temperature is 1400° F. Its diameter, 6900 miles, is 0.87 times the diameter of the Earth’s. Kepler-20f has an orbit of 19.6 days. It has the temperature of 800° F, and it is 1.03 times Earth’s diameter, being 8,200 miles.

Because of their close orbits and high temperatures, these two exoplanets are not able to sustain water, let alone life. For them to have water and life, they have to lie in the “Goldilocks zone,” or the habitable zone, in which a planet cannot be too close or too far (hence, too hot or too cold) from the star it orbits.

Ever since its launch in 2009, Kepler has been detecting hundreds of exoplanets, many of which are not Earth-like, being hostile and sometimes lonely, not orbiting any stars. With its most recent detection of Kepler-22b and of Kepler-20′s two Earth-like planets, Kepler has reached a new landmark, not just in its journey, but in our knowledge of the various kinds of planets that exist in the observable universe.

“This could be an important milestone,” Dr. Fressin states. “I think 10 years, or maybe even 100 years, from now people will look back and ask when was the first Earth-sized planet found. It is very exciting.”

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