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Curious facts about cosmic life and their inhabitants.
How did Triton acquire so many strange properties, and why is Neptune's system of satellites so different from those predicted for a gaseous giant planet? Two planetary scientists, Dr. Raluca Rufu (Weizmann Institute of Science, Israel) and Dr. Robin Canup (Southwest Research Institute, US) demonstrate how Triton wreaked catastrophic havoc on Neptune's first generation of very unfortunate moons.
and here is another
Of the hundreds of bewitching moons in our Sun's family, Titan is remarkable for being the only one boasting a dense atmosphere and large liquid reservoirs on its surface, rendering it in many ways more like the four rocky, terrestrial planets of the warm and well-lit inner Solar System. Indeed, both Earth and Titan possess atmospheres dominated by nitrogen--more than 95 percent nitrogen in Titan's case. However, unlike our Earth, Titan's atmosphere has very little oxygen; the remainder of its atmosphere is primarily composed of methane and trace quantities of other gases--such as ethane. At the truly frigid temperatures found at the Saturn system's great distance from our Sun, Titan's methane and ethane can exist on the surface in their liquid form.
Moons are natural satellites that orbit another body that, in turn, circles its parent-star. A moon is held in place by both its own gravity and the gravitational grip of its host planet. Some planets have moons; some do not. Several asteroids in our Solar System also are orbited by very small moons--and some dwarf planets, such as Pluto, also have moons. One of Pluto's five moons, Charon, is almost 50% the size of Pluto. For this reason, the two frozen worlds inhabiting our Solar System's remote twilight zone, are sometimes classified as a double-planet.
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Our Moon is Earth's only permanent natural satellite. It is also the largest planetary satellite in our Solar System relative to the size of its parent-planet. After Jupiter's volcanic Galilean moon, Io, Earth's Moon is the densest natural satellite among those whose densities have been determined.
The crust of Earth's Moon is 43 miles thick on the near-side hemisphere, and 93 miles on the far-side. It is composed of silicon, magnesium, oxygen, calcium, aluminum, and iron. There are also trace amounts of titanium, uranium, thorium, hydrogen, and potassium.
Icy moons and tumbling, gleaming moonlets dance around within the lovely and very famous rings of the gas-giant planet Saturn. A study released in November 2012 now suggests that most of the moons inhabiting our own Solar System were born from ancient, primordial Saturn-like ring systems that swirled around newborn planets circling the young Sun. According to this study, most of our Solar System's regular satellites--which are those moons that lovingly embrace their parent planets in approximately equatorial orbits--formed in this way. In contrast, the most popular theory explaining moon-formation, suggests that moons emerged simultaneously with their parent planets, as a direct consequence of planetary formation.