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It is important to know at any age!

Moons can be found in a rich assortment of various sizes, shapes, and types. Although they are generally solid little worlds, a few of them are known to sport atmospheres. Indeed, the atmosphere of the second largest moon in our Solar System, Titan of Saturn, is so dense that it hides Titan's strange hydrocarbon-slashed surface beneath a thick orange veil.



and here is another

Triton also possesses a thin atmosphere composed mainly of nitrogen, and a smaller quantity of methane. This atmosphere probably is the result of Triton's cryovolcanism, which is enhanced by seasonal heating from the Sun. Although little is currently known of Pluto's atmosphere, it is thought to be primarily composed of nitrogen with some carbon monoxide and methane added to the mix--and it is extremely tenuous. Pluto's very thin atmosphere may exist as a gas only when Pluto is nearest to the Sun (perihelion). For most of Pluto's very long year, the atmospheric gases are frozen in the form of ice on its extremely frigid surface. One year on Triton is almost 248 Earth-years long--or 90,471 Earth-days!



and finally

How am I so sure of this? Simple. Because I've personally been using the moon to my advantage for more than 20 years, and know how effective it is. Have you ever had one of those epic days fishing where it seemed like no matter what you threw in the water, you caught fish? If you have, it was more than likely due to the fact that the moon was in a certain phase, rather than your skills as an angler (I hate to burst anyone's bubble, but it's true).

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In a study released in November 2011, Dr. Blankenship and his colleagues discovered the enormous subsurface lake on Europa by carefully scrutinizing two bumpy, circular features in the old Galileo images, taken about a decade earlier. The "chaos terrains" were shown to be bizarre regions of floating and colliding icebergs and ice flows. This jumbled mess collapsed portions of the little moon's ice shelf.



There is an important distinction between the way giant planet systems form--such as those belonging to Jupiter, Saturn, Uranus, and Neptune--and the way that the rocky planets such as Earth, and the dwarf planet, Pluto, take shape. The gaseous giant planets are surrounded by rings, a myriad of moons, and a vast number of tiny dancing moonlets, whereas the rocky planets have none, or only one moon, and no rings to be seen. Until this new model was developed, two scenarios were generally used to explain how the regular moons of our Solar System were born. These two commonly used explanations suggest that the moons of Earth and Pluto came into being following catastrophic impacts. They further suggest that the moons of the giant, outer planets were born in a nebula floating around the newborn gigantic planet. They fail, however, to explain the distribution and chemical composition of the moons circling the gigantic outer four. Something, therefore, up until now, has been missing.



Until 2004, no spacecraft had visited Saturn in over two decades. Pioneer 11 had snapped the very first close-up images of Saturn when it flew past in 1979, Voyager 1 had its rendezvous about a year later, and in August 1981 Voyager 2 had its brief but highly productive encounter. At last, on July 1, 2004, NASA's Cassini spacecraft went into orbit around Saturn, and started taking breathtaking photographs.