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A little interesting about space life.
"Their motion is tied together in a way similar to that of three of Jupiter's large moons. If you were sitting on Nix, you would see Styx go around Pluto twice every time Hydra goes around three times," Dr. Hamilton commented in the June 3, 2015 HST Press Release.
and here is another
"We found that the seabed of Ligea Mare is likely covered by a sludge layer of organic-rich compounds," she noted.
Alas, this is not the case with Phobos and Deimos. Phobos, the larger of the duo of little Martian moons, at 22 kilometers in diameter, is lazily tumbling towards Mars and will approach the Roche limit in about 20 million years. At this tragic point, it will shatter into fragments that will ultimately form a spectacular ring around its planet. Only Deimos will remain--bereft of its companion. Deimos is the smaller moon of the pair, and circles its parent-planet further out. This last remaining little moon will be a lonely object lingering in the Martian sky at this sad point--but it was not always thus. The new 2016 study suggests that Mars once possessed a very complex system of many moons.
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The birthday of Earth's Moon came about 95 million years after the formation of the Solar System itself, according to the new calculations. This means that our planet's nearest neighbor in Space is approximately 60 million years younger than earlier estimates indicated.
Following that last giant impact, Earth put on some weight, but this new weight gain was derived from impacts of much smaller bodies, only about the size of asteroids like Vesta. Dr. Jacobson and his team used the later weight gain in order to determine when the unfortunate Theia struck.
Asphaug and co-author Dr. Andreas Reufer of the University of Bern in Switzerland, devised their new giant impact model using sophisticated computer simulations. They discovered that mergers between moons the size of Jupiter's Galilean satellites--which range in size from 1,940 miles wide (Europa) to 3, 271 miles across (Ganymede)--would tear icy stuff off the outer layers of the colliding moons. This icy material would then form spiral arms, which would ultimately merge together due to gravitational attraction to create Saturn's mid-sized icy moons.