File:Hot eyeball planet.jpg
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| Description |
English: An eyeball planet is a hypothetical type of tidally locked planet, for which tidal locking induces spatial features (for example in the geography or composition of the planet) resembling an eyeball. They are terrestrial planets where liquids may be present, in which tidal locking will induce a spatially dependent temperature gradient (the planet will be hotter on the side facing the star and colder on the other side). This temperature gradient may therefore limit the places in which liquid may exist on the surface of the planet to ring-or disk-shaped areas.
A "hot" eyeball planet is usually close to its host star, and the centre of the "eye", facing the star (day side), is made of rock while liquid is present on the opposite side (night side). |
| Date | |
| Source | Own work |
| Author | Pablo Carlos Budassi |
Planet concept illustrated especially for Wikimedia Commons by Pablo Carlos Budassi. Source: https://www.pablocarlosbudassi.com/2021/02/planet-types.html Background image by ESO/Serge Brunier: https://commons.wikimedia.org/wiki/File:ESO_-_Milky_Way.jpg Suggestions for improving this image are welcome: pablocarlosbudassi@gmail.com
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 15:20, 15 August 2023 | | 1,080 × 1,080 (386 KB) | Celestialobjects (talk | contribs) | Uploaded own work with UploadWizard |
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