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Tritonball is the largest moon of Neptune-icon Neptuneball.

Due to his retrograde orbit and composition, he likely is a captured dwarf planet that once had a binary companion billions of years ago.

He also is one of the few known geologically active moons, with cyrogeysers and cyrovolcanic terrein. Thus, like Earthball, he has relatively few craters, as most of them are covered by water-ammonia "lava" within a relatively short timespan. He also is known to hold a thin, teneous nitrogen atmosphere.

Composition

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Surface Features

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Cyrovolcanism

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Cantaloupe Terrein

On Tritonball's western hemisphere, there are a strange series of fissures that is known as cantaloupe terrein, due to it's resembelance to the skin of a cantaloupe. Although it has relatively few impact craters, it seems to be some of the oldest terrein on his surface.

The terrein, composed of dirty water ice, is found only on Tritonball's surface. There are depressions in the terrein about 30-40 km in diameter, and it is unlikely that they are impact craters, as they are roughly equal in size and have smoothe edges. It is mainly thought this unique feature formed from diapirism.

Orbit - Rotation

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300px-Triton moon mosaic Voyager 2 (large)

A real life photo of Triton for reference

Gallery