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A little interesting about space life.

When Apollo 11 landed on the Moon in 1969, we were presented with our first human contact with the moon. The mission was able to accomplish the task of not only landing on the Moon, but also to return to the Earth with samples from the Moon. These samples along with subsequent presented us with answers regarding the composition of the Moon, which also gave us some basic facts that any theory about how the moon was created must answer/address. We learned:The Moon does not contain an iron core like our Earth does, due to the fact that the Moon's density is only 3.34 grams per cubic centimeter (compared to the Earth's which is 5.52 grams per cubic centimeter).Samples collected from the surface of the Moon reveal that it underwent extreme heat and baking, much more than what the Earth experienced.



and here is another

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 finally

There probably are many more lakes under Europa's ice, Blankenship continued to note. Furthermore, the prospects of searching for life on Europa could greatly improve. This is because research indicates that a percentage of the icy lids that cover the embedded lakes may be considerably thinner than was previously supposed.

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For a long time, planetary scientists thought that in the aftermath of the Moon-forming collision, hydrogen dissociated from water molecules. According to this scenario, both water and other elements that have low boiling temperatures (volatile elements), escaped from the disk and were lost forever to space. This model would form a volatile-element-depleted and bone-dry Moon. At the time, this scenario seemed to be consistent with earlier analyses of lunar samples.



"I think the best thing about this work is that they explain this link between the mass of the moon and the orbital distance, which was known before but not understood," said planetary scientist, Dr. David Nesvorny, in the November 29, 2012 Scientific American. Dr. Nesvorny, of the Southwest Research Institute in Boulder, Colorado, who did not contribute to the new research, added that "If you had asked me a few years ago, I would think of our Moon's formation and the formation of the satellites of the outer planets differently. This puts things on common ground."



Saturn is probably the most beautiful planet in our Sun's lovely family, with its magnificent system of enchanting rings, gleaming icy moons, and myriads of tumbling moonlets that dance and somersault both within and outside of the rings. One of Saturn's moons is Titan, the second largest moon in our Solar System, after Ganymede of Jupiter. Shrouded in a dense orange mist, Titan is famous for its frozen clouds of methane, and hydrocarbon seas and lakes. Titan's thick, veiling atmosphere is composed of a wonderful icy soup of compounds very much like those thought to have been present in Earth's primordial atmosphere. Titan's thick atmosphere--which is much denser than Earth's atmosphere--contains mostly nitrogen, like that of our own planet. But Titan's atmosphere also contains significantly greater percentages of such so-called "smoggy" chemicals as methane and ethane. The smog on Titan is so extremely dense that it actually rains "gasoline-like" liquids down on the surface of this bizarre world. Indeed, some of the chemicals discovered in Titan's atmosphere might indicate that simple and primitive methane-based life (methanogens), might dwell on this truly weird moon.