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Interesting facts about space.
The lakes are the main supporting source sustaining life in the moon. The lakes support an array of living organisms including fish of various varieties and some small sized aquatic mammals also, like on the earth. Only a limited range of water plants grow in the lakes and these are all found in all the lakes in the moon. The most abundant water plant variety resembles seaweeds, but is very much thicker and stronger than the earth's variety. These water plants which grow very rapidly and proliferate in vast quantities are the primary source of food and nutrient for the moon people.
and here is another
Triton was the second moon in our Solar System that was found to have a substantial atmosphere, which is primarily composed of nitrogen--with smaller quantities of carbon monoxide and methane. Discovered by William Lassell in 1846, only seventeen days after the discovery of Neptune, Triton is one of the most frigid worlds in our Solar System, with a surface temperature of only about 38 Kelvin. Triton's frozen surface is coated by nitrogen, carbon dioxide, methane, and water ices, and it has a high geometric albedo of more than 70%. Surface features include a large southern polar cap, ancient cratered planes that are cross-cut by scarps and graben, as well as much younger features thought to have been formed by endogenic processes like cryovolcanism (ice volcanoes).
In a mysterious region beyond the orbit of the beautiful, banded, blue ice-giant planet Neptune--the most distant of the eight major planets from our Sun--there is a dark and frigid domain called the Kuiper Belt. Within this remote region, where our Sun shines with only a weak fire, and appears to be merely a particularly large star suspended in the black sky, a multitude of strange, icy worldlets tumble around our Star. Pluto, a large icy denizen inhabiting the Kuiper Belt, was originally classified as the ninth major planet from our Sun after its discovery in 1930. However, with the realization that this frozen "oddball" is really only one of several large, icy inhabitants of the Kuiper Belt, the International Astronomical Union (IAU) found it necessary to formally define "planet" in 2006--and poor Pluto was unceremoniously ousted from the pantheon of major planets. Pluto, now freshly reclassified as a dwarf planet, nonetheless remains a small world of great interest, debate, and affection. Scientists will soon learn much more about this beloved, distant, ice-ball so far away, when, after a treacherous nine-year journey of three million miles through interplanetary space, NASA's hearty New Horizons spacecraft arrives at Pluto on July 14, 2015.
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Now we know that there are over 100 moons circling the eight major planets of our Sun's family. The majority of our Solar System's moons are icy, small, and frozen worlds that contain only small quantities of rocky material. The distant multitude of sparkling, icy moons in our Solar System are primarily in orbit around the four giant gaseous planets, Here, in this strange, frigid and dimly-lit realm, far from our Star's melting fires and brilliant light, these tiny frozen moons do their fabulous, lovely dance around their quartet of parent-planets. The giant, gaseous worlds that inhabit our Solar System's outer suburbs--Jupiter, Saturn, Uranus, and Neptune--are blanketed by heavy atmospheres of gas, and are accompanied, in their travels around our Star, by their orbiting retinue of many moons and sparkling, icy moonlets.
In addition to shedding new light on the lunar water-mystery, the new research could also have important implications for future exploration of Earth's Moon. The volcanic beads do not harbor a lot of water--only about.05 percent by weight--but the deposits are large, and the water could potentially be extracted.
The research published in the July 4, 2016 issue of Nature Geoscience highlights the main factor differentiating moon-birth around Mars and Earth: the differing rotation speeds of the two planets prompted "completely different tidal actions," Dr. Charnoz explained in the July 4, 2016 CNRS Press Release. Dr. Charnoz proposes that at the time of their respective impacts, "Earth took less than four hours to spin on its axis whereas Mars rotated very slowly over a 24-hour period." The result of this important difference caused Earth to hold on to its single, large Moon, while the Martian collision created a dozen smaller moons alongside a larger moon. As time went by, Martian tidal action--resulting from the planet's slow rotation rate--caused most of the moons, including the largest one, to crash back down to the surface of their parent-planet. As a result, only the two most distant moons, Phobos and Deimos, survived as testimony to the ancient catastrophe.