Johns Hopkins Applied Physics Laboratory (APL) planetary scientist Tom Nordhem and his colleagues have researched the Miranda Moon. Researchers have suggested that the small moon of Uranus must have been a deep liquid water ocean below the surface of Miranda, after a study on images taken from the Voyager 2 Spacekraft.
The special thing is that the Voyager 2 Spacecraft passed by Miranda in the year 1986. Then he took pictures of its southern hemisphere. In the pictures, many things came to know about Miranda’s researchers like- there are bumpy slopes and pit areas.
According to a TOI report, Miranda is about 300 miles wide. Its surface is quite interesting. It has deep valleys. There are high peaks and also strange patterns. This provides anticipation that there will be some different decrease in the past. It is also possible that he has a hidden ocean below the snowy surface.
Miranda is located far away our sun and is very cold. Despite this, there may be an ocean between its surface. The reason for this is tidal heating. In this situation, friction is produced in Miranda due to the gravity of Uranus and other close Moon. Heat is formed by that. It can keep an ocean so hot that water is present in liquid form.
However, all this is theory. For strong evidence, space agencies will have to send missions to Miranda.