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Because of the many similarities between Triton and Pluto, it has long been thought that there is some sort of historical connection between them. Indeed, it was once proposed that Pluto is really an escaped moon of Neptune, but this is now thought to be improbable. It is now considered to be much more likely that Triton, like Pluto, orbited our Sun freely, but was unlucky enough to be snared by Neptune--whereas Pluto was left independent and free to wander at will within its distant birthplace.
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The Kuiper Belt, sometimes called the Edgeworth-Kuiper Belt, is a region located in our Solar System's outer limits beyond the realm of the eight major planets. It extends from the orbit of Neptune to approximately 50 AU. Neptune's average distance from our Sun is about 30.1 AU--its perihelion is 29.8 AU, while its aphelion is 30.4 AU.
Of the four terrestrial, rocky planets of the inner Solar System (Mercury, Venus, our Earth, and Mars), both Mercury and Venus are moonless. Earth possesses one lone Moon, but it is a very large one--the fifth largest moon in our entire Solar System, in fact. Mars, on the other hand, has two tiny misshapen moons that resemble rocky potatoes, and are lumpy and dark, as they travel in their nearly circular orbits close to the plane of the Martian equator. The Martian moons, Phobos and Deimos, are probably asteroids that were captured by Mars long ago.
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And now, again, yay plays in more ways than one an important role in and for the lives of the people of Burma who are in their vast majority - some 86% - Buddhists.
"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.
"A major difficulty has been to explain why a giant impact on Mars would have left two moons so different from our own Moon, a huge single mass, that also formed from Earth undergoing such an impact," explained Dr. Sebastien Charnoz in a July 4, 2016 Centre National de la Recherche Scientifique (CNRS) Press Release. Dr. Charnoz is a planetary scientist at the Institut de Physique Du Globe De Paris (IPG) who contributed to the new research.