About Dwarf planet past mars
Smaller trans-Neptunian objects have been called dwarf planets if they appear to be solid bodies, which is a prerequisite for hydrostatic equilibrium: planetologists generally include at least Gonggong, Orcus, and Sedna.
The number ofin theis unknown. Estimates have run as high as 200 in theand over 10,000 in the region beyond.However, consideration of the surprisingly low densities of many.
• • • •.
• • , incl. diameters and albedos measured by Herschel and Spitzer to date, Herschel OT KP "TNOs are Cool: A Survey of the Transneptunian Region" .
Beside directly orbiting the Sun, the qualifying feature of a dwarf planet is that it have "sufficient mass for its self-gravity to overcome .
The assessments of the IAU, Tancredi et al., Brown, and Grundy et al. for some of potential dwarf planets are as follows. For the IAU, the acceptance criteria were for naming purposes; Quaoar was called a dwarf planet in a 2022–2023 IAU annual report.An IAU.
Ceres (: 1 Ceres) is ain the middle mainbetween the orbits ofand . It was the first known , discovered on 1 January 1801 byatin , and announced as a new . Ceres was later classified as an asteroid and then a dwarf planet, the only one not beyond 's orbit.
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