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The chaotic motions of the bewitching, bewildering dance of the distant moons, is not necessarily an indication that the Pluto system is trembling on the brink of falling apart. Additional observations are necessary in order to determine the future and ultimate fate of the Pluto system.
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Like Earth's own large Moon, Triton is locked in synchronous rotation with its planet--one side always faces Neptune. However, because of Neptune's odd orbital inclination, both of the moon's polar regions take turns facing the Sun. Spacecraft images of Triton reveal mounds and round pits formed from icy lava flows (cryovolanism), as well as smooth volcanic plains. The surface of the moon is only sparsely cratered, indicating that its surface is new--that is, it is constantly being resurfaced, probably by the "lava" flow from icy volcanoes. Triton is very bright--its fresh, sparkling, new ice-coating is believed to cover a heart of metal and rock. Triton's high density suggests that it contains more rock in its interior than the icy moons of Saturn and Uranus.
NASA's Galileo spacecraft imaged Europa during a flyby on September 7, 1996. In fact, so far there have only been flyby missions to this fascinating object. Galileo viewed Europa's surface much more closely than the Pioneers and Voyagers, and it revealed to astronomers a bizarre surface that looked like broken glass, repaired by an icy glue oozing up from below.
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The new study, which Dr. Milliken co-authored with Dr. Shuai Li, a postdoctoral researcher at the University of Hawaii and a Brown University graduate, is published in the July 24, 2017 issue of the journal Nature Geoscience. The research was part of Dr. Li's doctoral thesis.
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.
JAXA has announced a space mission scheduled to begin in 2022, with an expected return to Earth in 2026. "Its objective is to carry out close-up remote sensing and in-situ observations of both Phobos and Deimos, and to bring back samples from Phobos," commented Dr. Ryuki Hyodo in the July 4, 2016 CNRS Press Release. Dr. Hyodo is a planetary scientist, originally from Kobe University in Japan, and he is also currently collaborating with the IPG. "High-resolution impact simulations are still needed to understand more about the disk structure," he continued to explain to the press.