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A little interesting about space life.

The mass distribution of the moons of Neptune is lopsided. In fact, it is the most lopsided satellite system of any of the giant planets dwelling in our Solar System. Triton accounts for nearly all the mass of the system, with all of the other moons together accounting for only one-third of 1%. This is very similar to the system of moons that circle the ringed-planet Saturn, where the large, smoggy, orange moon Titan--the second-largest moon in our Sun's family (after Ganymede of Jupiter)--accounts for over 95% of the total mass of Saturn's system of moons.



and here is another

The other duo of Pluto's five known moons being studied, Kerberos and Styx, are also currently thought to be in chaotic rotation as well! However, Pluto well may have a few more small moons that have not as yet been spotted--at least, as of this writing.



and finally

The movement of the moons in the Pluto-Charon system provides precious insights into the way planets orbiting in a binary stellar system--or double star system--might behave. "We are learning that chaos may be a common trait of binary systems. It might even have consequences for life on planets orbiting binary stars," Dr. Hamilton explained in the June 3, 2015 HST Press Release.

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The most detailed pictures of Europa show even more intriguing clues that there is slush lurking beneath its brightly shining icy surface. Slightly smaller than Earth's own beloved Moon, Europa's surface temperature could easily freeze an ocean solid over a span of only several million years. However, some astronomers think that warmth from a game of tidal tug-of-war between Europa and Jupiter, as well as other neighboring moons, could be keeping large regions of Europa's subsurface global ocean in a life-friendly liquid state. This process is termed tidal heating, and it refers to a mechanism whereby the gravitational tugs of a nearby object (or objects) flex and bend and contract and expand another object continually. This constant churning causes the victimized object, in this case Europa, to heat up and be considerably more balmy than its great distance from the Sun would otherwise allow it to be.



A fourth, more recent model, is based on the existence of a synestia. A synestia is a doughnut-shaped cloud composed of vaporized molten rock. This recently discovered inhabitant of the Universe is believed to take shape when planet-sized bodies catastrophically blast into one another with both high energy and angular momentum. Soon after the discovery of these puffy celestial "doughnuts" in 2017, planetary scientists came to the realization that they may have a new way to explain Moon-birth. The ancient collisions, that create a synestia, are so violent that the objects that form from these cosmic crash-ups melt and partially vaporize. Ultimately, after having cooled off sufficiently to solidify, they create (almost) spherical planets, such as those inhabiting our own Solar System.



Saturn is the smaller of the two gas-giant planets dwelling in the outer regions of our Solar System, far from the friendly light and warmth of our incandescent golden Star, the Sun. The larger of the two gas-giants is Jupiter, which is also the largest planet in our Solar System. Some scientists think that the two gas giants do not have solid surfaces hidden beneath their immense and heavy gaseous envelopes, although others think that they probably do contain relatively small cores of rocky-icy material. The two other large denizens of the outer limits of our Sun's family are Uranus and Neptune, which are classified as ice-giants, because they have large icy cores buried beneath their heavy atmospheres which, though massive, are not nearly as heavy as the gaseous atmospheres borne by the two gas-giants.