Category Astronomy/Space

At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly. Credit: NASA’s Goddard Space Flight Center

This artist’s concept shows what the young, dead, disk galaxy MACS2129-1, right, would look like when compared with the Milky Way galaxy, left. Although three times as massive as the Milky Way, it is only half the size. MACS2129-1 is also spinning more than twice as fast as the Milky Way. Note that regions of Milky Way are blue from bursts of star formation, while the young, dead galaxy is yellow, signifying an older star population and no new star birth. Credit: NASA, ESA, and Z. Levy (STScI)

400 kilometres above the ground, in the ISS space station, you can’t just stick your head out the window and breathe fresh air, if harmful gases should leak into the indoor environment of NASA astronaut Peggy Whitson and her colleagues. Now, Norwegian and German technologists are developing new and fast working technology for monitoring the indoor air in the space station. Credit: NASA

The different layers of Earth’s airglow can be seen from the International Space Station as it orbits Earth. The very thin green layer above the bottom of the window occurs 95 kilometers (59 miles) above Earth’s surface; the red region above is a different type of airglow. The rectangle represents the portion of the airglow measured in a single WINDII image. Credit: American Geophysical Union