Artwork of Eris and Dysnomia
Numéro d’image : 12446710
| The dwarf planet Eris and its Moon Dysnomia orbit far beyond the orbit of Pluto. Eris, formerly known as 2003 UB313 or Xena, is the second largest dwarf planet, after Pluto. A dwarf planet is defined as an object large enough to be spherical due to its gravity, and with an independent orbit around the Sun (so not a satellite of a planet). A true planet has to dominate its orbit around the Sun. Eris fails because it is one of many Kuiper Belt objects in the outer solar system. Eris is 2326 km across, while its substantial moon has a diameter of 684 km. | |
| Licence : | Droits gérés |
| Crédit: | Science Photo Library / Garlick, Mark |
| Taille de l’image : | 3375 px × 6000 px |
| Model Release : | Non requis |
| Property Release : | Non requis |
| Restrictions : | - |
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