Tidal heating of Io
id:
tidal-heating-of-io-320-1905114
title:
Tidal heating of Io
text:
Tidal heating of Io occurs through the tidal friction processes between Jupiter and its moon. Orbital and rotational energy are dissipated as heat in the crust of the moon. Io has a similar mass and size as the Moon, but Io is the most geologically active body in the Solar System. This is caused by the heating mechanism of Io. The major heating source of Earth and the Moon is radioactive heating, but the heating source on Io is tidal heating. As Jupiter is very massive, the side of Io nearest to
brand slug:
wiki
category slug:
encyclopedia
description:
Dissipation of orbital and rotational friction between Jupiter and Io
original url:
https://en.wikipedia.org/wiki/Tidal_heating_of_Io
date created:
date modified:
2024-03-03T15:15:52Z
main entity:
{"identifier":"Q17033688","url":"https://www.wikidata.org/entity/Q17033688"}
image:
{"content_url":"https://upload.wikimedia.org/wikipedia/commons/5/55/Tidal_heating_on_Io.png","width":2318,"height":2168}
fields total:
13
integrity:
15