SPACE: WHERE ARE WE GOING?

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.

SPACE: WHERE ARE WE GOING?

Monday, September 28, 2015

This Week @ NASA, September 25, 2015

Friday, September 25, 2015

Galileo satellites handed over to operator

Thursday, September 24, 2015

Moons In Hiding

Wednesday, September 23, 2015

One-Year Follow-up Response of the United States of America to Priority Recommendations of the Committee on the Elimination of Racial Discrimination in its Concluding Observations on the Combined Seventh to Ninth Periodic Reports of the U.S.

Rosetta reveals comet’s water-ice cycle

Views of Pluto Through the Years

New Pluto Images from NASA’s New Horizons: It’s Complicated

Tuesday, September 22, 2015

New Norcia 3D

Monday, September 21, 2015

More student CubeSats getting ready for space!

Friday, September 18, 2015

ExoMars 2016 targets March launch window

Thursday, September 17, 2015

Destined for Mercury

Tuesday, September 15, 2015

This Week @ NASA, September 11, 2015

ESA Moon challenge

Thursday, September 10, 2015

Sweeping over the south pole of Mars

Watch Galileo launch