Category Astronomy/Space

The Curious Case of the Warped Kuiper Belt

1. A yet to be discovered, unseen "planetary mass object" makes its existence known by ruffling the orbital plane of distant Kuiper Belt objects, according to research by Kat Volk and Renu Malhotra of the UA's Lunar and Planetary Laboratory. The object is pictured on a wide orbit far beyond Pluto in this artist's illustration. (Image: Heather Roper/LPL) 2. A planetary mass object the size of Mars would be sufficient to produce the observed perturbations in the distant Kuiper Belt. Credit: Heather Roper/LPL

1. A yet to be discovered, unseen “planetary mass object” makes its existence known by ruffling the orbital plane of distant Kuiper Belt objects, according to research by Kat Volk and Renu Malhotra of the UA’s Lunar and Planetary Laboratory. The object is pictured on a wide orbit far beyond Pluto in this artist’s illustration. (Image: Heather Roper/LPL)
2. A planetary mass object the size of Mars would be sufficient to produce the observed perturbations in the distant Kuiper Belt.
Credit: Heather Roper/LPL

An unknown, unseen “planetary mass object” may lurk in the outer reaches of our solar system, according to new research on the orbits of minor planets. This object would be different from – and much closer than – the so-called Planet Nine, a planet whose existence yet awaits confirmation...

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Origins of Sun’s swirling Spicules discovered

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

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

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...

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Massive Dead Disk Galaxy Challenges Theories of Galaxy Evolution

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)

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)

By combining the power of a “natural lens” in space with the capability of Hubble Space Telescope, astronomers made a surprising discovery – the first example of a compact yet massive, fast-spinning, disk-shaped galaxy that stopped making stars only a few billion years after the big bang...

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The Astronaut’s Extra Nose

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

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

How do we prevent astronauts in space from inhaling hazardous gases? A German-Norwegian hi-tech optical gas sensor provides a solution. “Astronauts must receive early warnings if harmful or unpleasant gases get mixed in with their breathing air,” says Senior Scientist Atle Honne at SINTEF. “Because in space you can’t just open a window to ventilate the room,” he says.

As a child he read everything he could l...

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