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A little interesting about space life.
Over the years, several theories have been proposed to explain the mechanism involved in Triton's capture by Neptune. One theory suggests that Triton was snared in a three-body encounter. According to this scenario, Triton is the lone survivor of a binary Kuiper Belt Object (KBO) that had been fatally jostled during a destructive close encounter with Neptune.
and here is another
"Prior to the Hubble observations, nobody appreciated the intricate dynamics of the Pluto system," Dr. Mark Showalter explained in a June 3, 2015 HST Press Release. Dr. Showalter is of the Search for Extraterrestrial Intelligence (SETI) Institute in Mountain View, California. He is lead author of the Nature paper.
The outer Solar System is more richly endowed with moons than the inner regions. The two enormous gas giant planets, Jupiter and Saturn, and the ice giant planets, Uranus and Neptune, have numerous moons of various sizes, shapes, and origins. As these enormous planets grew, during the early days of our Solar System, they were able to ensnare wandering objects with their mighty gravitational grips.
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Earth's Moon completes one orbit around our planet every 27 days, and it rotates (spins) at the same rate. Because Earth is also moving--rotating on its axis as it circles our Star--from our perspective our lunar companion appears to orbit us every 29 days.
The scientists modeled different temperatures and water abundances that may have been present in the Moon-birthing disk. At higher temperatures, their disk was primarily composed of silicate vapor, which formed as a result of evaporation of the mantles of both the proto-Earth and the doomed Theia. The disk at these higher temperatures also contained a relatively small quantity of hydrogen dissociated from water. In contrast, at lower temperatures, their disk was primarily composed of water, from which hydrogen did not dissociate under this cooler temperature range--thus making its escape mechanism very inefficient.
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.