SPACE: WHERE ARE WE GOING? : SMALL BUSINESS TECHNOLOGY TRANSFER PROGRAM

Sunday, April 29, 2012

NASA SELECTS 10 SMALL BUSINESS TECHNOLOGY TRANSFER PROJECTS

WASHINGTON -- NASA has selected ten proposals from small business and
research institution teams to continue work on innovative
technologies that could advance future missions. The Phase II winners
in the agency's Small Business Technology Transfer (STTR) Program now
can enter negotiations for possible contract awards, with a total for
all projects of approximately $7.49 million.

High-technology firms in seven states submitted proposals in
partnership with research institutions in nine states. The STTR
Program uses a highly competitive, three-phase award system that
provides collaborative opportunities between qualified small
businesses, including women-owned and disadvantaged firms, and
research institutions to address specific technology gaps in NASA's
programs. STTR projects provide a foundation for future technology
developments and are complementary to other NASA research
investments.

Firms and research institutions that participated in Phase I of the
STTR submitted 44 Phase II proposals. Selection criteria included
technical merit and innovation, Phase I results, value to NASA,
commercial potential and company capabilities. Phase I is a
feasibility study to evaluate the scientific and technical merit of
an idea and Phase II will expand on the results of last year's
projects, with up to $750,000 to support research for up to two more
years. Phase III is for the commercialization of the results of Phase
II and requires private sector or non-STTR federal funding.

STTR is part of NASA's Space Technology Program and is managed at the
agency's Ames Research Center at Moffett Field, Calif., with
executive oversight by the Office of the Chief Technologist at NASA
Headquarters in Washington. Individual projects are managed by NASA's
field installations.

STAR FLASH

What caused this outburst of V838 Mon? For reasons unknown, star V838 Mon's outer surface suddenly greatly expanded with the result that it became the brightest star in the entire Milky Way Galaxy in January 2002. Then, just as suddenly, it faded. A stellar flash like this had never been seen before -- supernovas and novas expel matter out into space. Although the V838 Mon flash appears to expel material into space, what is seen in the above image from the Hubble Space Telescope is actually an outwardly moving light echo of the bright flash. In a light echo, light from the flash is reflected by successively more distant rings in the complex array of ambient interstellar dust that already surrounded the star. V838 Mon lies about 20,000 light years away toward the constellation of the unicorn (Monoceros), while the light echo above spans about six light years in diameter. Image Credit: NASA, ESA

THE SPIDERWEB GALAXY

Looking like a spider's web swirled into a spiral, Galaxy IC 342 presents its delicate pattern of dust in this image from NASA's Spitzer Space Telescope. Seen in infrared light, faint starlight gives way to the glowing bright patterns of dust found throughout the galaxy's disk. At a distance of about 10 million light-years, IC 342 is relatively close by galactic standards, however our vantage point places it directly behind the disk of our own Milky Way. The intervening dust makes it difficult to see in visible light, but infrared light penetrates this veil easily. IC 342 belongs to the same group as its even more obscured galactic neighbor, Maffei 2. IC 342 is nearly face-on to our view, giving a clear, top-down view of the structure of its disk. It has a low surface brightness compared to other spirals, indicating a lower density of stars (seen here as a blue haze). Its dust structures show up much more vividly (red). Blue dots are stars closer to us, in our own Milky Way. New stars are forming in the disk at a healthy rate. The very center glows especially brightly in the infrared, highlighting an enormous burst of star formation occurring in this tiny region. To either side of the center, a small bar of dust and gas is helping to fuel this central star formation. Data from Spitzer's infrared array camera are shown in blue (3.6 microns), green (4.5 microns) and red (5.8 and 8.0 microns). Image Credit: NASA/JPL-Caltech

JUMPING TO WARP SPEED

This cockpit view of a hypothetical spacecraft traveling at eight-tenths the speed of light shows the visual distortions that would be experienced at such high speeds. The star field is actually being wrapped toward the front of the craft in addition to being significantly blue-shifted. NASA Glenn leads the Breakthrough Propulsion Physics Project, NASA's primary effort to produce near-term, credible, and measurable progress toward the technology breakthroughs needed to revolutionize space travel and enable interstellar voyages. NASA Lewis (now Glenn) Research Center, Cleveland, Ohio.

OBSERVATION FROM THE SPACE STATION