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Only after Triton's orbit became circular, around its adopted parent-planet, could some of the rubble re-accrete to form the moons of Neptune that astronomers observe today. Triton's highly disruptive invasion of the Neptune system may be the reason why the moons of Neptune do not conform to the 10,000:1 ratio of mass between parent-planet and moon-offspring that literally all of the moons observed in the satellite systems of the other giant planets in our Solar System conform to.
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Multiple Light Sources. On the moon, there is only one light source sufficiently strong to form shadows; the Sun. So it is solid to suggest that all shadows on the Moon should run parallel to each other. However, this was apparently not the case during the moon landing.
There are several potential explanations that could account for the sea's composition of pure methane, Dr. Le Gall added. "Either Ligeia Mare is replenished by fresh methane rainfall, or something is removing ethane from it. It is possible that the ethane ends up in the undersea crust, or that it somehow flows into the adjacent sea, Kraken Mare, but that will require further investigation," she noted.
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Our Moon's temperature reaches about 260 degrees Fahrenheit when under a full Sun. However, in darkness, the temperature dives down to approximately -280 degrees Fahrenheit.
Astronomers have for years contemplated two competing hypotheses explaining the origin of the Martian moons. The first proposes that Phobos and Deimos are, indeed, escapees from the Main Asteroid Belt. Alas, this viewpoint begs the question of why they should have been so cruelly captured by their adopted parent-planet in the first place. An alternative theory points to the possibility that the moons were born from the debris left by a violent collision between Mars and a primordial protoplanet--a baby planet still under construction. However, this theory also suffers from uncertainty because it does not explain precisely how this particular tragic mechanism gave rise to Phobos and Deimos.
In 2010 and 2011, the French astrophysicists devised their model to explain how the moons of Saturn were born. They based their findings on data derived from the Cassini probe--that is investigating the Saturn-system--and on numerical simulations. The team found that Saturn's bewitching rings, which are slender disks composed of tiny chunks of gleaming ice surrounding the giant planet, gave rise to the icy moons. This happened because the rings spread as time went by--and when the rings attained a critical distance from the planet (termed the Roche limit), their ends melded together and created small worldlets that broke off and floated away. In this way the rings created the icy moons orbiting Saturn.