The number of dwarf planets in the Solar System is unknown. Estimates have run as high as 200 in the Kuiper belt[1] and over 10,000 in the region beyond.[2]
However, consideration of the surprisingly low densities of many large trans-Neptunian objects, as well as spectroscopic analysis of their surfaces, suggests that the number of dwarf planets may be much lower, perhaps only eight among bodies known so far.[3][4] The International Astronomical Union (IAU) defines dwarf planets as being in hydrostatic equilibrium, and notes five bodies in particular: Ceres in the inner Solar System and four in the trans-Neptunian region: Pluto, Eris, Haumea, and Makemake. Only Pluto and Ceres have been confirmed to be in hydrostatic equilibrium, due to the results of the New Horizons and Dawn missions.[5] Eris is generally assumed to be a dwarf planet because it is similar in size to Pluto and even more massive. Haumea and Makemake were accepted as dwarf planets by the IAU for naming purposes and will keep their names if it turns out they are not dwarf planets. 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, Quaoar, and Sedna. (In practice the requirement for hydrostatic equilibrium is always loosened anyway, even by the IAU, as otherwise even Mercury would not be a planet.)
^Mike Brown. "The Dwarf Planets". Retrieved 20 January 2008.
^Stern, Alan (24 August 2012). "The Kuiper Belt at 20: Paradigm Changes in Our Knowledge of the Solar System". Applied Physics Laboratory. Today we know of more than a dozen dwarf planets in the solar system [and] it is estimated that the ultimate number of dwarf planets we will discover in the Kuiper Belt and beyond may well exceed 10,000.
^Grundy, W.M.; Noll, K.S.; Buie, M.W.; Benecchi, S.D.; Ragozzine, D.; Roe, H.G. (December 2019). "The mutual orbit, mass, and density of transneptunian binary Gǃkúnǁʼhòmdímà ((229762) 2007 UK126)" (PDF). Icarus. 334: 30–38. doi:10.1016/j.icarus.2018.12.037. S2CID 126574999. Archived (PDF) from the original on 7 April 2019.
^Cite error: The named reference JWST was invoked but never defined (see the help page).
^"What's Inside Ceres? New Findings from Gravity Data". 2 August 2016.
and 28 Related for: List of possible dwarf planets information
The number ofdwarfplanets in the Solar System is unknown. Estimates have run as high as 200 in the Kuiper belt and over 10,000 in the region beyond....
Eight likeliest dwarfplanets and dates of discovery A dwarfplanet is a small planetary-mass object that is in direct orbit around the Sun, massive enough...
This is a listof the lists of small Solar System bodies and dwarfplanets. Lists of comets Listof minor planetsListof named minor planets (alphabetical)...
objects and dwarfplanets. The catalog consists of hundreds of pages, each containing 1,000 minor planets. Every year, the Minor Planet Center, which...
metals. Within the Solar System, the terrestrial planets accepted by the IAU are the inner planets closest to the Sun: Mercury, Venus, Earth and Mars...
Brown dwarfs are substellar objects that have more mass than the biggest gas giant planets, but less than the least massive main-sequence stars. Their...
like dwarfplanets and some moons to the planets and the Sun. This list does not include small Solar System bodies, but it does include a sample of possible...
rounded objects of the Solar System Listof Solar System objects most distant from the Sun Listofpossibledwarfplanets Discovery was announced two years...
This list covers all known stars, brown dwarfs, and sub-brown dwarfs within 20 light-years (6.13 parsecs) of the Sun. So far, 131 such objects have been...
Only a handful of giant planets and a handful of minor planets are known around white dwarfs. It is a growing list with discoveries of around 6 exoplanets...
This is a listof brown dwarfs. These are objects that have masses between heavy gas giants and low-mass stars. The first isolated brown dwarf discovered...
planetary mass which is not gravitationally bound to any star or brown dwarf. Rogue planets may originate from planetary systems in which they are formed and...
2011). "The stars that host planets". Sky & Telescope. pp. 22–27. "Billions of rocky planets in habitable zones around red dwarfs". European Southern Observatory...
to 1:12. ListofpossibledwarfplanetsListof trans-Neptunian objects Listof Solar System objects by size using the most precise value of Vanth's estimated...
minor planets other than those that are dwarfplanets. Thus SSSBs are: the comets; the classical asteroids, with the exception of the dwarfplanet Ceres;...
respectively. ListofpossibledwarfplanetsListof Solar System objects most distant from the Sun 2017 FP161 "2017 FO161". Minor Planet Center. Retrieved...
This is a listof extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit...
moons of the giant planets have features similar to those on the terrestrial planets and dwarfplanets, and some have been studied as possible abodes of life...
to the IAU, "planets and dwarfplanets are two distinct classes of objects" – in other words, "dwarfplanets" are not planets. A non-satellite body fulfilling...
Asteroid belt ListofpossibledwarfplanetsListof trans-Neptunian objects Planet Nine The literature is inconsistent in the usage of the terms scattered...
is a large trans-Neptunian object and a possibledwarfplanet. It is located in the Kuiper belt, a region of icy objects orbiting beyond Neptune in the...
to remember the planets and dwarfplanetsof the Solar System, with the order of words corresponding to increasing sidereal periods of the bodies. One...