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It is important to know at any age!
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 here is another
Dr. Lieber and his colleagues did a study to test the theory of full-moon "lunacy". They studied data on murders in Dade County of Florida which covered 15 years and a total of 1,887 deaths by homicide. When they compared the deaths with the phases of the moon, they found that the two rose and fell together for the entire 15 years! With the approach of a full or new moon, there was a sharp spike in the murder rate, and then a decline during the first and last quarters of the moon.
There are currently over a thousand known KBOs, and more than 100,000 KBOs over 62 miles in diameter are believed to exist. Pluto is compositionally similar to many other objects inhabiting the Kuiper Belt, and its orbital period is characteristic of a class of KBOs termed plutinos, that share the same 2:3 resonance with Neptune.
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Galileo Galilei first spotted the planet Neptune with his primitive "spyglass" on December 28, 1612. He observed it again on January 27, 1613. Unfortunately, on both occasions, Galileo thought that the giant, remote planet was a fixed star, appearing near the planet Jupiter in the dark night sky. Because of this mistake, Galileo is not credited with the discovery of Neptune.
NASA's Galileo spacecraft imaged Europa during a flyby on September 7, 1996. In fact, so far there have only been flyby missions to this fascinating object. Galileo viewed Europa's surface much more closely than the Pioneers and Voyagers, and it revealed to astronomers a bizarre surface that looked like broken glass, repaired by an icy glue oozing up from below.
The vanished, ill-fated, large moon could have been a few hundred kilometers in diameter. The large moon would also have allowed a handful of other smaller moons to form--including the duo of small, shapeless ones that survive today. However, this large inner moon would have been born close to or within the Roche limit. This is why it is likely that it crashed into Mars as a result of tidal forces within several million years--and the collection of other small moons followed their leader. Only Phobos and Deimos kept their distance.