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In this fascinating new research, the astronomers announced that they have discovered that a duo of Pluto's moons, dubbed Nix and Hydra, are actually in a chaotic rotation. This basically means that an observer standing on the alien surface of icy, strange Pluto, would not observe the same face of its moons from one night to the next. For those observers visiting the two bizarre moons themselves, things would be even weirder because every day would be a different length from the one that came before it.
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"This is still very much an area of active research, so there is much that scientists including our Department of Terrestrial Magnetism staff scientist Erik Hauri, as well as many other Carnegie colleagues and alumni, are figuring out about how much water exists on the Moon. This is a highly important and challenging question to answer given that we have limited knowledge on the history and distribution of lunar water," explained Dr. Miki Nakajima in a February 26, 2018 Carnegie Institution Press Release. Dr. Nakajima, who is of the Carnegie Institution of Washington (D.C.), along with California Institute of Technology's (Caltech's) Dr. David Stevenson, set out to determine whether prevailing lunar formation models need to be adjusted to explain more recent higher estimates of the quantity of water on Earth's Moon. Caltech is in Pasadena.
The lunar mantle reaches from the top of the partially molten layer to the bottom of the lunar crust. It is thought to be made up of minerals like pyroxine and olivine--both of which are composed of magnesium, iron, silicon and oxygen atoms.
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This new method is based on the fact that elements composing our planet's crust that have a tendency to combine with iron--such as iridium and platinum--arrived at Earth after this last giant collision.
According to the new theory, moon-formation starts at the very edge of a planetary ring, where a fragile baby moon can begin to emerge without the danger of being ripped apart by the fierce gravity of its parent planet. These dancing little moonlets, formed from ring-material, then travel outward. As the ring-system continually produces moonlet after moonlet after moonlet, the small icy worlds coalesce to form increasingly larger moons. The larger moons, in turn, may also merge together, as they dance outward from their parent planet.
"What makes the Saturn system so beautiful and unique could be its youth. While we don't have a preferred time frame for this origin scenario to play out, it could have happened recently if something came along to destabilize the Saturn system, triggering the collisional mergers that formed Titan," Asphaug added.