SPACE: WHERE ARE WE GOING? : STATEMENT FROM NASA ON MEETINGS IN EUROPE

Monday, May 27, 2013

STATEMENT FROM NASA ON MEETINGS IN EUROPE

FROM: NASA
NASA Statement on Space Technology Meetings in Europe

WASHINGTON -- The following is a statement from NASA's associate administrator for space technology, Michael Gazarik, about his meetings this week in Europe to discuss potential cooperation on development of space technologies that will enable NASA's future missions. These include the asteroid initiative announced in the president's fiscal year 2014 budget proposal.

"During my meetings this week with the German Space Agency, DLR; the European Space Program, ESA; and the French Space Program, CNES, I had an opportunity to view and learn about our partner's areas of technology focus and expertise and begin the process of identifying areas of potential cooperation in space technology. Our working-level discussions proved to be informative and productive. Our meetings also allowed me to share NASA's plans for our new asteroid initiative. NASA recognizes cooperation and collaboration are critical to meet increasingly global challenges. I look forward to working with our partners as we create the new knowledge and capabilities needed to enable the space missions of the future."

Gazarik is head of NASA's Space Technology Mission Directorate, which is innovating, developing, testing and flying hardware for use in NASA's future missions

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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

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OBSERVATION FROM THE SPACE STATION