![List of Solar System objects by size](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly91cGxvYWQud2lraW1lZGlhLm9yZy93aWtpcGVkaWEvY29tbW9ucy90aHVtYi84Lzg1L1NvbGFyX3N5c3RlbV9tYXNzX2Rpc3RyaWJ1dGlvbl9wcG1fY2hhcnQuc3ZnLzE2MDBweC1Tb2xhcl9zeXN0ZW1fbWFzc19kaXN0cmlidXRpb25fcHBtX2NoYXJ0LnN2Zy5wbmc=.png )
This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius. These lists can be sorted according to an object's radius and mass and, for the most massive objects, volume, density, and surface gravity, if these values are available.
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTkwYUhWdFlpODRMemcxTDFOdmJHRnlYM041YzNSbGJWOXRZWE56WDJScGMzUnlhV0oxZEdsdmJsOXdjRzFmWTJoaGNuUXVjM1puTHpJeU1IQjRMVk52YkdGeVgzTjVjM1JsYlY5dFlYTnpYMlJwYzNSeWFXSjFkR2x2Ymw5d2NHMWZZMmhoY25RdWMzWm5MbkJ1Wnc9PS5wbmc=.png)
These lists contain the Sun, the planets, dwarf planets, many of the larger small Solar System bodies (which includes the asteroids), all named natural satellites, and a number of smaller objects of historical or scientific interest, such as comets and near-Earth objects.
Many trans-Neptunian objects (TNOs) have been discovered; in many cases their positions in this list are approximate, as there is frequently a large uncertainty in their estimated diameters due to their distance from Earth.
Solar System objects more massive than 1021kilograms are known or expected to be approximately spherical. Astronomical bodies relax into rounded shapes (spheroids), achieving hydrostatic equilibrium, when their own gravity is sufficient to overcome the structural strength of their material. It was believed that the cutoff for round objects is somewhere between 100 km and 200 km in radius if they have a large amount of ice in their makeup; however, later studies revealed that icy satellites as large as Iapetus (1,470 kilometers in diameter) are not in hydrostatic equilibrium at this time, and a 2019 assessment suggests that many TNOs in the size range of 400–1,000 kilometers may not even be fully solid bodies, much less gravitationally rounded. Objects that are ellipsoids due to their own gravity are here generally referred to as being "round", whether or not they are actually in equilibrium today, while objects that are clearly not ellipsoidal are referred to as being "irregular."
Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation, and can sometimes even have quite different equatorial diameters (scalene ellipsoids such as Haumea). Unlike bodies such as Haumea, the irregular bodies have a significantly non-ellipsoidal profile, often with sharp edges.
There can be difficulty in determining the diameter (within a factor of about 2) for typical objects beyond Saturn. (See 2060 Chiron as an example) For TNOs there is some confidence in the diameters, but for non-binary TNOs there is no real confidence in the masses/densities. Many TNOs are often just assumed to have Pluto's density of 2.0 g/cm3, but it is just as likely that they have a comet-like density of only 0.5 g/cm3.
For example, if a TNO is incorrectly assumed to have a mass of 3.59×1020 kg based on a radius of 350 km with a density of 2 g/cm3 but is later discovered to have a radius of only 175 km with a density of 0.5 g/cm3, its true mass would be only 1.12×1019 kg.
The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters; however, many of the moons with a radius less than ~100 km, such as Jupiter's Himalia, have far less certain masses. Further out from Saturn, the sizes and masses of objects are less clear. There has not yet been an orbiter around Uranus or Neptune for long-term study of their moons. For the small outer irregular moons of Uranus, such as Sycorax, which were not discovered by the Voyager 2 flyby, even different NASA web pages, such as the National Space Science Data Center and JPL Solar System Dynamics, give somewhat contradictory size and albedo estimates depending on which research paper is being cited.
There are uncertainties in the figures for mass and radius, and irregularities in the shape and density, with accuracy often depending on how close the object is to Earth or whether it has been visited by a probe.
Graphical overview
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTkwYUhWdFlpOWlMMkkxTDFOdmJHRnlMWE41YzNSbGJTMTBiM0ExTUMxa2FXRnRaWFJsY2k1emRtY3ZOVFV3Y0hndFUyOXNZWEl0YzNsemRHVnRMWFJ2Y0RVd0xXUnBZVzFsZEdWeUxuTjJaeTV3Ym1jPS5wbmc=.png)
- Relative masses of the bodies of the Solar System. Objects smaller than Saturn are not visible at this scale.
- Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system.
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- Relative masses of the rounded moons of the Solar System. Mimas, Enceladus, and Miranda are too small to be visible at this scale.
Objects with radii over 400 km
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTkwYUhWdFlpOHlMekkzTDAxaGMzTmZZVzVrWDNKaFpHbDFjMTlzWVhKblpWOXpiMnhoY2w5emVYTjBaVzFmYjJKcVpXTjBjeTV3Ym1jdk1qSXdjSGd0VFdGemMxOWhibVJmY21Ga2FYVnpYMnhoY21kbFgzTnZiR0Z5WDNONWMzUmxiVjl2WW1wbFkzUnpMbkJ1Wnc9PS5wbmc=.png)
The following objects have a nominal mean radius of 400 km or greater. It was once expected that any icy body larger than approximately 200 km in radius was likely to be in hydrostatic equilibrium (HE). However, Ceres (r = 470 km) is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium, whereas Iapetus (r = 735 km) is the largest icy body that has been found to not be in hydrostatic equilibrium. The known icy moons in this range are all ellipsoidal (except Proteus), but trans-Neptunian objects up to 450–500 km radius may be quite porous.
For simplicity and comparative purposes, the values are manually calculated assuming that the bodies are all spheres. The size of solid bodies does not include an object's atmosphere. For example, Titan looks bigger than Ganymede, but its solid body is smaller. For the giant planets, the "radius" is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure.
Because Sedna and 2002 MS4 have no known moons, directly determining their mass is impossible without sending a probe (estimated to be from 1.7x1021 to 6.1×1021 kg for Sedna).
Body | Image | Radius | Volume | Mass | Surface area | Density | Gravity | Type | Discovery | |||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(km) | (R🜨) | (109 km3) | (V🜨) | (1021 kg) | (M🜨) | (106km2) | 🜨 | (g/cm3) | (m/s2) | (🜨) | ||||
Sun | ![]() | 695700 ± ? | 109.2 | 1,409,300,000 | 1,301,000 | 1989100000 | 333,000 | 6,078,700 | 11,918 | 1.409 | 274.0 | 27.94 | G2V-class star | prehistoric |
Jupiter | ![]() | 69911±6 | 10.97 | 1,431,280 | 1,321 | 1898187±88 | 317.83 | 61,419 | 120.41 | 1.3262±0.0003 | 24.79 | 2.528 | gas giant planet; has rings | prehistoric |
Saturn | ![]() | 58232±6 (136775 for A Ring) | 9.140 | 827,130 | 764 | 568317±13 | 95.162 | 42,612 | 83.54 | 0.6871±0.0002 | 10.44 | 1.065 | gas giant planet; has rings | prehistoric |
Uranus | ![]() | 25362±7 | 3.981 | 68,340 | 63.1 | 86813±4 | 14.536 | 8083.1 | 15.85 | 1.270±0.001 | 8.69 | 0.886 | ice giant planet; has rings | 1781 |
Neptune | ![]() | 24622±19 | 3.865 | 62,540 | 57.7 | 102413±5 | 17.147 | 7618.3 | 14.94 | 1.638±0.004 | 11.15 | 1.137 | ice giant planet; has rings | 1846 |
Earth | ![]() | 6371.0±0.0001 | 1 | 1,083.21 | 1 | 5972.4±0.3 | 1 | 510.06447 | 1 | 5.5136±0.0003 | 9.81 | 1 | terrestrial planet | prehistoric |
Venus | ![]() | 6051.8±1 | 0.9499 | 928.43 | 0.857 | 4867.5±0.2 | 0.815 | 460.2 | 0.903 | 5.243±0.003 | 8.87 | 0.905 | terrestrial planet | prehistoric |
Mars | ![]() | 3389.5±0.2 | 0.5320 | 163.18 | 0.151 | 641.71±0.03 | 0.107 | 144.37 | 0.283 | 3.9341±0.0007 | 3.71 | 0.379 | terrestrial planet | prehistoric |
Ganymede Jupiter III | ![]() | 2634.1±0.3 | 0.4135 | 76.30 | 0.0704 | 148.2 | 0.0248 | 86.999 | 0.171 | 1.936 | 1.428 | 0.146 | moon of Jupiter (icy) | 1610 |
Titan Saturn VI | ![]() | 2574.73±0.09 | 0.4037 | 71.50 | 0.0658 | 134.5 | 0.0225 | 83.3054 | 0.163 | 1.880±0.004 | 1.354 | 0.138 | moon of Saturn (icy) | 1655 |
Mercury | ![]() | 2439.7±1.0 | 0.3829 | 60.83 | 0.0562 | 330.11±0.02 | 0.0553 | 74.797 | 0.147 | 5.4291±0.007 | 3.70 | 0.377 | terrestrial planet | prehistoric |
Callisto Jupiter IV | ![]() | 2410.3±1.5 | 0.3783 | 58.65 | 0.0541 | 107.6 | 0.018 | 73.005 | 0.143 | 1.834±0.003 | 1.23603 | 0.126 | moon of Jupiter (icy) | 1610 |
Io Jupiter I | ![]() | 1821.6±0.5 | 0.2859 | 25.32 | 0.0234 | 89.32 | 0.015 | 41.698 | 0.082 | 3.528±0.006 | 1.797 | 0.183 | moon of Jupiter (terrestrial) | 1610 |
Moon Earth I | ![]() | 1737.4±0.1 | 0.2727 | 21.958 | 0.0203 | 73.46 | 0.0123 | 37.937 | 0.074 | 3.344±0.005 | 1.625 | 0.166 | moon of Earth (terrestrial) | prehistoric |
Europa Jupiter II | ![]() | 1560.8±0.5 | 0.2450 | 15.93 | 0.0147 | 48.00 | 0.008035 | 30.613 | 0.06 | 3.013±0.005 | 1.316 | 0.134 | moon of Jupiter (terrestrial) | 1610 |
Triton Neptune I | ![]() | 1353.4±0.9 | 0.2124 | 10.38 | 0.0096 | 21.39±0.03 | 0.003599 | 23.018 | 0.045 | 2.061 | 0.782 | 0.0797 | moon of Neptune (icy) | 1846 |
Pluto 134340 | ![]() | 1188.3±0.8 | 0.187 | 7.057 | 0.00651 | 13.03±0.03 | 0.0022 | 17.79 | 0.034 | 1.854±0.006 | 0.620 | 0.063 | dwarf planet; plutino; multiple | 1930 |
Eris 136199 | ![]() | 1163±6 | 0.1825 | 6.59 | 0.0061 | 16.6±0.2 | 0.0028 | 17 | 0.033 | 2.52±0.07 | 0.824 | 0.083 | dwarf planet; SDO; binary | 2003 |
Haumea 136108 | ![]() | 798±6 to 816 | 0.12 | 1.98 | 0.0018 | 4.01±0.04 | 0.00066 | 8.14 | 0.016 | 2.018 | 0.401 | 0.0409 | dwarf planet; resonant KBO (7:12); trinary; has rings | 2004 |
Titania Uranus III | ![]() | 788.9±1.8 | 0.1237 | 2.06 | 0.0019 | 3.40±0.06 | 0.00059 | 7.82 | 0.015 | 1.711±0.005 | 0.378 | 0.0385 | moon of Uranus | 1787 |
Rhea Saturn V | ![]() | 763.8±1.0 | 0.1199 | 1.87 | 0.0017 | 2.307 | 0.00039 | 7.34 | 0.014 | 1.236±0.005 | 0.26 | 0.027 | moon of Saturn | 1672 |
Oberon Uranus IV | ![]() | 761.4±2.6 | 0.1195 | 1.85 | 0.0017 | 3.08±0.09 | 0.0005 | 7.285 | 0.014 | 1.63±0.05 | 0.347 | 0.035 | moon of Uranus | 1787 |
Iapetus Saturn VIII | ![]() | 735.6±1.5 | 0.1153 | 1.66 | 0.0015 | 1.806 | 0.00033 | 6.8 | 0.013 | 1.088±0.013 | 0.223 | 0.0227 | moon of Saturn | 1671 |
Makemake 136472 | ![]() | 715+19 −11 | 0.112 | 1.53 | 0.0014 | ≈ 3.1 | 0.00053 | 6.4 | 0.013 | ≈ 2.1 | 0.57 | 0.0581 | dwarf planet; cubewano | 2005 |
Gonggong 225088 | ![]() | 615±25 | 0.0983 | 1.03 | 0.0009 | 1.75±0.07 | 0.00029 | 4.753 | 0.009 | 1.72±0.16 | 0.3 | 0.0306 | dwarf planet; resonant SDO (3:10) | 2007 |
Charon Pluto I | ![]() | 606.0±0.5 | 0.0951 | 0.932 | 0.0009 | 1.586±0.015 | 0.00025 | 4.578 | 0.009 | 1.70±0.02 | 0.288 | 0.0294 | moon of Pluto | 1978 |
Umbriel Uranus II | ![]() | 584.7±2.8 | 0.0918 | 0.837 | 0.0008 | 1.28±0.03 | 0.00020 | 4.3 | 0.008 | 1.39±0.16 | 0.234 | 0.024 | moon of Uranus | 1851 |
Ariel Uranus I | ![]() | 578.9±0.6 | 0.0909 | 0.813 | 0.0007 | 1.25±0.02 | 0.000226 | 4.211 | 0.008 | 1.66±0.15 | 0.269 | 0.027 | moon of Uranus | 1851 |
Dione Saturn IV | ![]() | 561.7±0.45 | 0.0881 | 0.741 | 0.0007 | 1.095 | 0.000183 | 3.965 | 0.008 | 1.478±0.003 | 0.232 | 0.0237 | moon of Saturn | 1684 |
Quaoar 50000 | ![]() | 543±2 | 0.0879 | 0.737 | 0.0007 | 1.20±0.05 | 0.0002 | 3.83 | 0.008 | 2.0±0.5 | 0.3 | 0.0306 | dwarf planet; cubewano; binary; has rings | 2002 |
Tethys Saturn III | ![]() | 533.0±0.7 | 0.0834 | 0.624 | 0.0006 | 0.617 | 0.000103 | 3.57 | 0.007 | 0.984±0.003 | 0.145 | 0.015 | moon of Saturn | 1684 |
Ceres 1 | ![]() | 469.7±0.1 | 0.0742 | 0.433 | 0.0004 | 0.938 | 0.000157 | 2.85 | 0.006 | 2.17 | 0.28 | 0.029 | dwarf planet; belt asteroid | 1801 |
Orcus 90482 | ![]() | 455+25 −20 | 0.0719 | 0.404 | 0.0004 | 0.548±0.010 | 0.000092 | 1.4±0.2 | 0.2 | 0.0204 | dwarf planet; plutino; binary | 2004 | ||
Sedna 90377 | ![]() | 453+157 −129 | 0.0785 | 0.516 | 0.0005 | dwarf planet; sednoid; detached object | 2003 | |||||||
Salacia 120347 | ![]() | 423±11 | 0.0664 | 0.373 | 0.0003 | 0.492±0.007 | 0.000082 | 1.5±0.1 | 0.165 | 0.0168 | cubewano; binary | 2004 | ||
|
Smaller objects by mean radius
From 200 to 399 km
All imaged icy moons with radii greater than 200 km except Proteus are clearly round, although those under 400 km that have had their shapes carefully measured are not in hydrostatic equilibrium. The known densities of TNOs in this size range are remarkably low (1–1.2 g/cm3), implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies.
Body | Image | Radius (km) | Mass (1018 kg) | Density (g/cm3) | Type | Refs r · M | |||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2002 MS4 307261 | ![]() | 398±12 | – | – | cubewano | ||||||||
2002 AW197 55565 | ![]() | 384±19 | – | – | cubewano | ||||||||
Varda 174567 | ![]() | 373±8 | 245±6 | 1.23±0.04 | cubewano; binary | · | |||||||
2013 FY27 532037 | ![]() | 370±40 | – | – | SDO; binary | ||||||||
2003 AZ84 208996 | ![]() | 362 ~ 386±6 (assuming HE) | 150 ~ 210 (assuming HE) | 0.76 ~ 0.87 (assuming HE) | plutino; binary | ||||||||
2021 DR15 | 356 | 374 | ? | SDO | |||||||||
Ixion 28978 | ![]() | 354.8±0.1 | – | – | plutino | ||||||||
2004 GV9 90568 | ![]() | 340±17 | – | – | cubewano | ||||||||
2005 RN43 145452 | ![]() | 340+28 −37 | – | – | cubewano | ||||||||
Varuna 20000 | ![]() | 327+77 −51 | ≈ 160 | 0.99+0.09 −0.02 | cubewano | ||||||||
2002 UX25 55637 | ![]() | 332±15 | 125±3 | 0.82±0.11 | cubewano; binary | · | |||||||
2005 RM43 145451 | ![]() | 322 | – | – | SDO | ||||||||
Gǃkúnǁʼhòmdímà 229762 | ![]() | 321±14 | 136.1±3.3 | 1.02±0.17 | SDO; binary | · | |||||||
2014 UZ224 | ![]() | 317.5+28.5 −30.5 | – | – | SDO | ||||||||
≈ 317 | – | – | SDO | ||||||||||
2008 OG19 470599 | 309.5+28 −56.5 | – | 0.609±0.004 | SDO | · | ||||||||
2010 JO179 574372 | ≈ 309 | – | – | SDO | |||||||||
2007 JJ43 278361 | 305+85 −70 | – | – | cubewano | |||||||||
Dysnomia Eris I | ![]() | ≈ 300; ≤ 370 | 300–500 < 140 | 1.8–2.4 < 1.2 | moon of Eris | ||||||||
2014 EZ51 523692 | > 288 | – | – | SDO | |||||||||
2010 KZ39 | ≈ 287 | – | – | SDO | |||||||||
2012 VP113 | ≈ 287 | – | – | sednoid | |||||||||
2002 XW93 78799 | 283+36 −37 | – | – | other TNO | |||||||||
2004 XR190 612911 | ![]() | ≈ 278 | – | – | SDO | ||||||||
2002 XV93 612533 | ![]() | 275+11 −12 | – | – | plutino | ||||||||
2015 RR245 523794 | ≈ 270 | – | – | resonant KBO (2:9); binary | |||||||||
2003 UZ413 455502 | ![]() | ≈ 268 | – | – | plutino | ||||||||
2007 JH43 470308 | 264±15 | 95±3 | 38±0.11 | plutino | |||||||||
Vesta 4 | ![]() | 262.7±0.1 | 259 | 3.46 | belt asteroid type V | · | |||||||
2003 VS2 84922 | ![]() | 262±4 | – | – | plutino | ||||||||
2014 FC72 | 257±15 | 275±3 | ? | detached object | |||||||||
Pallas 2 | ![]() | 256±2 | 204±3 | 2.92±0.08 | belt asteroid type B | ||||||||
2004 TY364 120348 | 256+19 −20 | – | – | cubewano | |||||||||
Enceladus Saturn II | ![]() | 252.1±0.2 | 108.0±0.1 | 1.609±0.005 | moon of Saturn | · | |||||||
2002 TC302 84522 | ![]() | 250±7 | – | – | resonant SDO (2:5) | ||||||||
2005 UQ513 202421 | 249+32 −38 | – | – | cubewano | |||||||||
2014 AN55 543354 | ≈ 248 | – | – | SDO | |||||||||
Miranda Uranus V | ![]() | 235.8±0.7 | 65.9±7.5 | 1.2±0.15 | moon of Uranus | · | |||||||
Dziewanna 471143 | ![]() | 235+18 −5 | – | – | SDO | ||||||||
2005 TB190 145480 | ![]() | 232±31 | – | – | detached object | ||||||||
1999 DE9 26375 | 231±23 | – | – | resonant SDO (2:5) | |||||||||
2003 FY128 120132 | 230±11 | – | – | SDO | |||||||||
2002 VR128 84719 | 224+24 −22 | – | – | plutino | |||||||||
Vanth Orcus I | ![]() | 221±5 | 87±8 | 1.5+1.0 −0.5 | moon of 90482 Orcus | · | |||||||
≈ 219 | – | – | SDO | ||||||||||
612581 | ≈ 217 | – | – | plutino | |||||||||
Hygiea 10 | ![]() | 216±4 | 87.4±6.9 | 2.06±0.20 | belt asteroid type C | · | |||||||
2004 NT33 444030 | 212+44 −40 | – | – | cubewano | |||||||||
Proteus Neptune VIII | ![]() | 210±7 | 44 | ≈ 1.3 | moon of Neptune | · | |||||||
2002 GJ32 182934 | ≈ 208 | – | – | cubewano | |||||||||
2005 QU182 303775 | 208±37 | – | – | SDO | |||||||||
Chaos 19521 | ![]() | 208+42 −15 equivalent | – | – | cubewano | ||||||||
2002 KX14 119951 | ![]() | 207.5±0.5 | – | – | cubewano | ||||||||
1996 TO66 19308 | ![]() | 204±5 ~ 90±5 (assuming albedo) | 210 ~ 175 (assuming albedo) | ? | resonant KBO (11:19) | ||||||||
2001 QF298 469372 | ![]() | 204+20 −22 | – | – | plutino | ||||||||
Huya 38628 | ![]() | 203±8 | > 50 | > 1.43 | plutino; binary | · | |||||||
2004 PF115 175113 | 203+49 −38 | – | – | plutino | |||||||||
2003 QW90 307616 | 200±5 | 135 | ? | cubewano | |||||||||
2004 PT107 469615 | 200±5 | 100 | ? | cubewano | |||||||||
Legend:
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From 100 to 199 km
This list contains a selection of objects estimated to be between 100 and 199 km in radius (200 and 399 km in diameter). The largest of these may have a hydrostatic-equilibrium shape, but most are irregular. Most of the trans-Neptunian objects (TNOs) listed with a radius smaller than 200 km have "assumed sizes based on a generic albedo of 0.09" since they are too far away to directly measure their sizes with existing instruments. Mass switches from 1021 kg to 1018 kg (Zg). Main-belt asteroids have orbital elements constrained by (2.0 AU < a < 3.2 AU; q > 1.666 AU) according to JPL Solar System Dynamics (JPLSSD). Many TNOs are omitted from this list as their sizes are poorly known.
Body | Image | Radius (km) | Mass (1018 kg) | Type | Refs r · M | |
---|---|---|---|---|---|---|
2004 UX10 144897 | 199±20 | ≈ 30 | plutino | · | ||
1998 VG44 33340 | 199±20 | ≈ 47 | plutino | |||
1993 SC 15789 | 199±20 | ≈ 47 | plutino | |||
Mimas Saturn I | ![]() | 198.2±0.3 | 37.49±0.03 | moon of Saturn | · | |
1998 SN165 35671 | 196±20 | cubewano | ||||
2001 UR163 42301 | ![]() | ≈ 176 | resonant KBO (4:9) | |||
1995 SM55 24835 | 173 (assuming albedo of 0.7) | ? | ? | cubewano | ||
2001 YH140 126154 | 172±20 | ≈ 85 | resonant KBO (3:5) | |||
2010 ER65 552555 | 170±20 | ≈ 30 | SDO | |||
Nereid Neptune II | ![]() | 170±25 | moon of Neptune | |||
1996 TL66 15874 | 170±10 | SDO | ||||
2004 XA192 230965 | 170+60 −47.5 | SDO | ||||
2010 ET65 471137 | 170±20 | ≈ 30 | SDO | |||
2002 WC19 119979 | ![]() | ≈ 169 | 77±5 | resonant KBO (1:2); binary | · | |
2005 CA79 612931 | 167±20 | ≈ 60 | resonant KBO (1:2) | |||
Interamnia 704 | ![]() | 166±3 | 35.2±5.1 | belt asteroid type F | · | |
Ilmarë Varda I | ![]() | 163±18 | moon of 174567 Varda | |||
Europa 52 | ![]() | 160±2 | 23.9±3.8 | belt asteroid type C | ||
Hiʻiaka Haumea I | ![]() | ≈ 160 | 17.9±1.1 | moon of Haumea | · | |
2002 KW14 307251 | 160±20 | ≈ 30 | cubewano | |||
1999 CD158 469306 | 155±20 | ≈ 48 | resonant KBO (4:7) | |||
2007 OC10 470316 | 155±20 | ≈ 30 | SDO | |||
2005 RR43 145453 | 150±20 | ≈ 60 | cubewano | |||
Davida 511 | ![]() | 149±2 | 26.6±7.3 | belt asteroid type C | ||
2002 TX300 55636 | ![]() | 143±5 | cubewano | |||
Actaea Salacia I | ![]() | 143±12 | moon of 120347 Salacia | |||
Sylvia 87 | ![]() | 137±2 | 14.3±0.5 | outer belt asteroid type X; trinary | ||
2003 OP32 120178 | 137±20 | ≈ 45 | cubewano | |||
Lempo 47171 | ![]() | 136±9 | plutino; trinary | |||
Eunomia 15 | ![]() | 135±2 | 30.5±1.9 | belt asteroid type S | ||
Hyperion Saturn VII | ![]() | 135±4 | 5.62±0.05 | moon of Saturn | · | |
Euphrosyne 31 | ![]() | 134±2 | 16.5±2.6 | belt asteroid type C; binary | ||
1998 SM165 26308 | ![]() | 134±14 | 6.87±1.8 | resonant KBO (1:2) | · | |
Cybele 65 | ![]() | 131.5±1.5 | 14.8±1.8 | outer belt asteroid type C | ||
Chariklo 10199 | ![]() | ≈ 130 | centaur; has rings | |||
Juno 3 | ![]() | 127±1 | 27.0±2.4 | belt asteroid type S | ||
Hiisi Lempo II | ![]() | 126±8 | secondary of 47171 Lempo | |||
Hektor 624 | ![]() | 125±13 | 7.9±1.4 | Jupiter trojan (L4) type D; binary | · | |
Sila 79360 | ![]() | 124±15 | 10.8±0.22 | cubewano; binary | ||
2007 RW10 309239 | 124±15 | quasi-satellite of Neptune | ||||
Altjira 148780 | ![]() | 123+19 −70 | cubewano; binary | |||
Nunam 79360 | ![]() | 118±15 | secondary of 79360 Sila | |||
Bamberga 324 | ![]() | 114±2 | 10.2±0.9 | belt asteroid type C | ||
Patientia 451 | 112.9±2.3 | 10.9±5.3 | belt asteroid type C | · | ||
Psyche 16 | ![]() | 112±2 | 26.2±2.9 | belt asteroid type M | ||
Ceto 65489 | ![]() | 112±5 | 5.4±0.4 | extended centaur; binary | · | |
Herculina 532 | ![]() | 111.2±2.4 | belt asteroid type S | |||
S/2007 (148780) 1 Altjira I | ![]() | 110+17 −62 | secondary of 148780 Altjira | |||
Hesperia 69 | ![]() | 110±15 | 5.86±1.18 | belt asteroid type M | · | |
Thisbe 88 | ![]() | 109±2 | 11.6±2.2 | belt asteroid type B | ||
Doris 48 | ![]() | 108±2 | 6.9±2.9 | belt asteroid type C | ||
Chiron 2060 or 95P | ![]() | 108±5 | centaur; has rings | |||
Phoebe Saturn IX | ![]() | 106.5±0.7 | 8.29±0.01 | moon of Saturn | · | |
Satellite of (38628) Huya Huya I | ![]() | 106±15 | moon of 38628 Huya | |||
Fortuna 19 | ![]() | 105.5±1.0 | 8.8±1.4 | belt asteroid type G | ||
Camilla 107 | ![]() | 105±4 | 11.2±0.3 | outer belt asteroid type C; trinary | · | |
Themis 24 | ![]() | 104±2 | 6.2±2.9 | belt asteroid type C | ||
Amphitrite 29 | ![]() | 102±1 | 12.7±2.0 | belt asteroid type S | ||
Egeria 13 | ![]() | 101±2 | 9.2±2.1 | belt asteroid type G | ||
Iris 7 | ![]() | 100±5 | 13.5±2.3 | belt asteroid type S | ||
Legend:
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From 50 to 99 km
This list contains a selection of objects 50 and 99 km in radius (100 km to 199 km in average diameter). The listed objects currently include most objects in the asteroid belt and moons of the giant planets in this size range, but many newly discovered objects in the outer Solar System are missing, such as those included in the following reference.Asteroid spectral types are mostly Tholen, but some might be SMASS.
Body | Image | Radius (km) | Mass (1018 kg) | Type | Refs r · M |
---|---|---|---|---|---|
Elektra 130 | ![]() | 99.5±1 | 6.4±0.2 | belt asteroid type G; multiple | |
Bienor 54598 | 99+3 −3.5 | centaur | |||
Hebe 6 | ![]() | 97.5±1.5 | 12.4±2.4 | belt asteroid type S | |
Larissa Neptune VII | ![]() | 97±3 | ≈ 4.2 | moon of Neptune | · |
Ursula 375 | ![]() | 96.8±1.3 | 8.4±5.3 | belt asteroid type C | · |
S/2018 (532037) 1 | ≈ 95 | moon of 2013 FY27 | |||
Eugenia 45 | ![]() | 94±1 | 5.8±0.1 | belt asteroid type F; trinary | |
Hermione 121 | ![]() | 94±3 | 5.0±0.3 | outer belt asteroid type C; binary | · |
Daphne 41 | ![]() | 94±7 | 6.1±0.9 | belt asteroid type C; binary | |
Aurora 94 | ![]() | 93.8±3.6[dubious – discuss] | 6.2±3.6 | belt asteroid type C | · |
Bertha 154 | ![]() | 93.4±0.9 | 9.2±5.2[dubious – discuss] | belt asteroid type C | · |
Janus Saturn X | ![]() | 89.5±1.4 | 1.898±0.001 | moon of Saturn | · |
Teharonhiawako 88611 | ![]() | 89+16 −18 | 2.44±0.03[dubious – discuss] | cubewano; binary | · |
Aegle 96 | 88.9±0.8 | 6.4±6.3 | belt asteroid type T | · | |
Galatea Neptune VI | ![]() | 88±4 | 2.12±0.08 | moon of Neptune | · |
Phorcys Ceto I | ![]() | 87+8 −9 | ≈ 1.67 | secondary of 65489 Ceto | · |
Palma 372 | ![]() | 86.8±1.4[dubious – discuss] | 5.2±0.6 | belt asteroid type B | · |
Metis 9 | ![]() | 86.5±1 | 8.0±1.9 | belt asteroid type S | · |
Alauda 702 | ![]() | 86±28 | 6.06±0.36[dubious – discuss] | belt asteroid type C; binary | · |
Hilda 153 | ![]() | 85.3±1.6 | outer belt asteroid; Hildas | ||
Himalia Jupiter VI | ![]() | 85 | 4.2±0.6 | moon of Jupiter | · |
Namaka Haumea II | ![]() | ≈ 85 | 1.8±1.5 | moon of Haumea | · |
Weywot Quaoar I | ![]() | ≈ 85 | < ≈ 5 | moon of 50000 Quaoar | |
Freia 76 | ![]() | 84.2±1.0 | 2.0±4.2[dubious – discuss] | outer belt asteroid type P/type X | · |
Amalthea Jupiter V | ![]() | 83.45±2.4 | 2.08±0.15 | moon of Jupiter | · |
Agamemnon 911 | ![]() | 83.3±2.0 | Jupiter trojan (L4) type D | ||
Elpis 59 | 82.6±2.3 | 3±0.5 | belt asteroid type CP/type B | · | |
Eleonora 354 | ![]() | 82.5±1.5 | 7.5±2.7 | belt asteroid type A | |
Nemesis 128 | ![]() | 81.5±2.5 | 3.4±1.7 | belt asteroid type C | |
Puck Uranus XV | ![]() | 81±2 | moon of Uranus | ||
S/2015 (136472) 1 Makemake I | ![]() | ≈ 80 | moon of Makemake | ||
Sycorax Uranus XVII | ![]() | 78.5+11.5 −7.5 | moon of Uranus | ||
Io 85 | ![]() | 77.4±1.9[dubious – discuss] | 2.6±1.5 | belt asteroid type FC/type B | · |
Minerva 93 | ![]() | 77.08±0.65 | 3.5±0.4 | belt asteroid type C; trinary | · |
Alexandra 54 | ![]() | 77.07±0.32 | 6.2±3.5[dubious – discuss] | belt asteroid type C | · |
Laetitia 39 | 77±2 | 4.7±1.1 | belt asteroid type S | · | |
Nemausa 51 | ![]() | 75±1.5 | 3.9±1.6 | belt asteroid type G | |
Kalliope 22 | ![]() | 75±2.5 | 7.7±0.4 | belt asteroid type M; binary | |
Despina Neptune V | ![]() | 75±3 | moon of Neptune | ||
Manwë 385446 | ![]() | ≈ 75 | ≈ 1.41 | resonant KBO (4:7); binary | · |
Pales 49 | ≈ 74.9 | 4.2±2.2 | belt asteroid type C | · | |
Parthenope 11 | ![]() | 74.5±1 | 5.5±0.4 | belt asteroid type S | |
Arethusa 95 | ![]() | 74.0±2.4 | belt asteroid type C | ||
Pulcova 762 | ![]() | 73.7±0.4 | 1.4±0.1 | belt asteroid type F; binary | · |
Flora 8 | ![]() | 73±1 | 4.0±1.6 | belt asteroid type S | |
Ino 173 | ![]() | 72.5±1.5 | 2.2±1.3 | belt asteroid type Xc | |
Adeona 145 | ![]() | 72±1.5 | 2.4±0.3 | belt asteroid type Xc | |
Irene 14 | ![]() | 72±1 | 2.9±1.9 | belt asteroid type S | · |
Melpomene 18 | ![]() | 70.5±1 | 4.5±0.9 | belt asteroid type S | |
Lamberta 187 | ![]() | 70.5±1 | 1.9±0.3 | belt asteroid type Ch | |
Aglaja 47 | 71±4 | 3.2±1.7 | belt asteroid type C | · | |
Patroclus 617 | ![]() | 70.2±0.4 | 1.36±0.11 | Jupiter trojan (L5) type P; binary | · |
Julia 89 | ![]() | 70±1.4 | 4.3±3.2 | belt asteroid type S | |
Typhon 42355 | ![]() | 69±4.5 | 0.87±0.03 | resonant SDO (7:10); binary | · |
Massalia 20 | ![]() | 67.8±1.8 | 5±1.04 | belt asteroid type S | · |
Portia Uranus XII | ![]() | 67.6±4 | moon of Uranus | ||
Emma 283 | ![]() | 66.2±0.1 | 1.38±0.03 | belt asteroid type X; binary | · |
Paha Lempo I | ![]() | 66+4 −4.5 | 0.746±0.001 | moon of 47171 Lempo | · |
Lucina 146 | ![]() | 65.9±? | belt asteroid type C | ||
Sawiskera Teharonhiawako I | ![]() | 65.5+12 −13 | secondary of 88611 Teharonhiawako | ||
Achilles 588 | ![]() | 65.0±0.3 | Jupiter trojan (L4) type DU | ||
Panopaea 70 | 64.0±0.4 | 4.33±1.09 | belt asteroid type C | · | |
Thule 279 | 63.3±1.8 | outer belt asteroid type D | |||
Borasisi 66652 | ![]() | 63+12.5 −25.5 | 3.433±0.027 | cubewano; binary | · |
Hestia 46 | 62.07±1.7 | 3.5 | belt asteroid type P/type Xc | · | |
Leto 68 | ![]() | 61.3±1.6 | 3.28±1.9 | belt asteroid type S | · |
Undina 92 | 60.46±0.85 | 4.43±0.25 | belt asteroid type X | · | |
Bellona 28 | ![]() | 60.45±1.90 | 2.62±0.15 | belt asteroid type S | · |
Diana 78 | 60.30±1.35 | 1.27±0.13 | belt asteroid type C | · | |
Anchises 1173 | ![]() | 60.2±1.5 | Jupiter trojan (L5) type P | ||
Bernardinelli-Bernstein C/2014 UN271 | ![]() | 60±7 | comet | ||
Galatea 74 | 59.4±1.4 | 6.13±5.36 | belt asteroid type C | · | |
Deiphobus 1867 | 59.1±0.8 | Jupiter trojan (L5) type D | |||
Äneas 1172 | 59.01±0.40 | Jupiter trojan (L5) type D | |||
Kleopatra 216 | ![]() | 59±1 | 3.0±0.3 | belt asteroid type M; trinary | |
Athamantis 230 | ![]() | 59±1 | 2.3±1.1 | belt asteroid type S | |
Diomedes 1437 | ![]() | 58.89±0.59 | Jupiter trojan (L4) type D | ||
Terpsichore 81 | 58.9±0.4 | 6.19±5.31 | belt asteroid type C | · | |
Epimetheus Saturn XI | ![]() | 58.1±1.8 | 0.5266±0.0006 | moon of Saturn | · |
Victoria 12 | ![]() | 58±1 | 2.7±1.3 | belt asteroid type S | |
Circe 34 | ![]() | 57.7±1.0 | ≈ 3.66±0.03 | belt asteroid type C | · |
Leda 38 | ![]() | 57.7±0.7 | 5.71±5.47 | belt asteroid type C | · |
Odysseus 1143 | 57.3±0.3 | Jupiter trojan (L4) type D | |||
Alcathous 2241 | 56.8±0.9 | Jupiter trojan (L5) type D | |||
Melete 56 | ![]() | 56.62±0.85 | 4.61 | belt asteroid type P | · |
Mnemosyne 57 | 56.3±1.4 | ≈ 12.6±2.4 | belt asteroid type S | · | |
Nestor 659 | 56.2±0.9 | Jupiter trojan (L4) type XC | |||
Harmonia 40 | ![]() | 55.6±0.2 | belt asteroid type S | ||
Leleākūhonua 541132 | 55+7 −5 | sednoid | |||
Euterpe 27 | ![]() | 54.9±0.8 | 1.67±1.01 | belt asteroid type S | · |
Antilochus 1583 | 54.4±0.3 | Jupiter trojan (L4) type D | |||
Thorondor Manwë I | ![]() | 54 | 0.5 | secondary of 385446 Manwë | · |
Thalia 23 | ![]() | 53.8±1.1 | 1.96±0.09 | belt asteroid type S | · |
Erato 62 | ![]() | 53.5±0.3 | belt asteroid type BU/type Ch | ||
Astraea 5 | ![]() | 53.3±1.6 | 2.9 | belt asteroid type S | · |
Pabu Borasisi I | ![]() | 52.5+10 −21 | secondary of 66652 Borasisi | ||
Eos 221 | 51.76±2.8 | ≈ 5.87±0.34 | belt asteroid type S/type K | · | |
Aegina 91 | 51.7±0.2 | belt asteroid type C | |||
Leukothea 35 | ![]() | 51.5±0.6 | belt asteroid type C | ||
Menoetius Patroclus I | ![]() | 51.4±0.25 | secondary of 617 Patroclus | ||
Isis 42 | ![]() | 51.4±1.4 | 1.58±0.52 | belt asteroid type S | · |
Klotho 97 | ![]() | 50.4±0.3 | 1.33±0.13 | belt asteroid type M | · |
Troilus 1208 | ![]() | 50.3±0.5 | Jupiter trojan (L5) type FCU |
From 20 to 49 km
This list includes few examples since there are about 589 asteroids in the asteroid belt with a measured radius between 20 and 49 km. Many thousands of objects of this size range have yet to be discovered in the trans-Neptunian region. The number of digits is not an endorsement of significant figures. The table switches from ×1018 kg to ×1015 kg (Eg). Most mass values of asteroids are assumed.
This article includes a list of the most massive known objects of the Solar System and partial lists of smaller objects by observed mean radius These lists can be sorted according to an object s radius and mass and for the most massive objects volume density and surface gravity if these values are available Parts per million chart of the relative mass distribution of the Solar System each cubelet denoting 2 1024 kg These lists contain the Sun the planets dwarf planets many of the larger small Solar System bodies which includes the asteroids all named natural satellites and a number of smaller objects of historical or scientific interest such as comets and near Earth objects Many trans Neptunian objects TNOs have been discovered in many cases their positions in this list are approximate as there is frequently a large uncertainty in their estimated diameters due to their distance from Earth Solar System objects more massive than 1021kilograms are known or expected to be approximately spherical Astronomical bodies relax into rounded shapes spheroids achieving hydrostatic equilibrium when their own gravity is sufficient to overcome the structural strength of their material It was believed that the cutoff for round objects is somewhere between 100 km and 200 km in radius if they have a large amount of ice in their makeup however later studies revealed that icy satellites as large as Iapetus 1 470 kilometers in diameter are not in hydrostatic equilibrium at this time and a 2019 assessment suggests that many TNOs in the size range of 400 1 000 kilometers may not even be fully solid bodies much less gravitationally rounded Objects that are ellipsoids due to their own gravity are here generally referred to as being round whether or not they are actually in equilibrium today while objects that are clearly not ellipsoidal are referred to as being irregular Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation and can sometimes even have quite different equatorial diameters scalene ellipsoids such as Haumea Unlike bodies such as Haumea the irregular bodies have a significantly non ellipsoidal profile often with sharp edges There can be difficulty in determining the diameter within a factor of about 2 for typical objects beyond Saturn See 2060 Chiron as an example For TNOs there is some confidence in the diameters but for non binary TNOs there is no real confidence in the masses densities Many TNOs are often just assumed to have Pluto s density of 2 0 g cm3 but it is just as likely that they have a comet like density of only 0 5 g cm3 For example if a TNO is incorrectly assumed to have a mass of 3 59 1020 kg based on a radius of 350 km with a density of 2 g cm3 but is later discovered to have a radius of only 175 km with a density of 0 5 g cm3 its true mass would be only 1 12 1019 kg The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters however many of the moons with a radius less than 100 km such as Jupiter s Himalia have far less certain masses Further out from Saturn the sizes and masses of objects are less clear There has not yet been an orbiter around Uranus or Neptune for long term study of their moons For the small outer irregular moons of Uranus such as Sycorax which were not discovered by the Voyager 2 flyby even different NASA web pages such as the National Space Science Data Center and JPL Solar System Dynamics give somewhat contradictory size and albedo estimates depending on which research paper is being cited There are uncertainties in the figures for mass and radius and irregularities in the shape and density with accuracy often depending on how close the object is to Earth or whether it has been visited by a probe Graphical overviewRelative diameters of the fifty largest bodies in the Solar System colored by orbital region Values are diameters in kilometers Both scales are linear Relative masses of the bodies of the Solar System Objects smaller than Saturn are not visible at this scale Relative masses of the Solar planets Jupiter at 71 of the total and Saturn at 21 dominate the system Relative masses of the solid bodies of the Solar System Earth at 48 and Venus at 39 dominate Bodies less massive than Pluto are not visible at this scale Relative masses of the rounded moons of the Solar System Mimas Enceladus and Miranda are too small to be visible at this scale Objects with radii over 400 kmPlot of log10 mass versus log10 radius of the 34 largest objects in the solar system including the fitted regression line and a plot of residuals The following objects have a nominal mean radius of 400 km or greater It was once expected that any icy body larger than approximately 200 km in radius was likely to be in hydrostatic equilibrium HE However Ceres r 470 km is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium whereas Iapetus r 735 km is the largest icy body that has been found to not be in hydrostatic equilibrium The known icy moons in this range are all ellipsoidal except Proteus but trans Neptunian objects up to 450 500 km radius may be quite porous For simplicity and comparative purposes the values are manually calculated assuming that the bodies are all spheres The size of solid bodies does not include an object s atmosphere For example Titan looks bigger than Ganymede but its solid body is smaller For the giant planets the radius is defined as the distance from the center at which the atmosphere reaches 1 bar of atmospheric pressure Because Sedna and 2002 MS4 have no known moons directly determining their mass is impossible without sending a probe estimated to be from 1 7x1021 to 6 1 1021 kg for Sedna Body Image Radius Volume Mass Surface area Density Gravity Type Discovery km R 109 km3 V 1021 kg M 106km2 g cm3 m s2 Sun 695700 109 2 1 409 300 000 1 301 000 1989 100 000 333 000 6 078 700 11 918 1 409 274 0 27 94 G2V class star prehistoricJupiter 69911 6 10 97 1 431 280 1 321 1898 187 88 317 83 61 419 120 41 1 3262 0 0003 24 79 2 528 gas giant planet has rings prehistoricSaturn 58232 6 136775 for A Ring 9 140 827 130 764 568317 13 95 162 42 612 83 54 0 6871 0 0002 10 44 1 065 gas giant planet has rings prehistoricUranus 25362 7 3 981 68 340 63 1 86813 4 14 536 8083 1 15 85 1 270 0 001 8 69 0 886 ice giant planet has rings 1781Neptune 24622 19 3 865 62 540 57 7 102413 5 17 147 7618 3 14 94 1 638 0 004 11 15 1 137 ice giant planet has rings 1846Earth 6371 0 0 0001 1 1 083 21 1 5972 4 0 3 1 510 06447 1 5 5136 0 0003 9 81 1 terrestrial planet prehistoricVenus 6051 8 1 0 9499 928 43 0 857 4867 5 0 2 0 815 460 2 0 903 5 243 0 003 8 87 0 905 terrestrial planet prehistoricMars 3389 5 0 2 0 5320 163 18 0 151 641 71 0 03 0 107 144 37 0 283 3 9341 0 0007 3 71 0 379 terrestrial planet prehistoricGanymede Jupiter III 2634 1 0 3 0 4135 76 30 0 0704 148 2 0 0248 86 999 0 171 1 936 1 428 0 146 moon of Jupiter icy 1610Titan Saturn VI 2574 73 0 09 0 4037 71 50 0 0658 134 5 0 0225 83 3054 0 163 1 880 0 004 1 354 0 138 moon of Saturn icy 1655Mercury 2439 7 1 0 0 3829 60 83 0 0562 330 11 0 02 0 0553 74 797 0 147 5 4291 0 007 3 70 0 377 terrestrial planet prehistoricCallisto Jupiter IV 2410 3 1 5 0 3783 58 65 0 0541 107 6 0 018 73 005 0 143 1 834 0 003 1 23603 0 126 moon of Jupiter icy 1610Io Jupiter I 1821 6 0 5 0 2859 25 32 0 0234 89 32 0 015 41 698 0 082 3 528 0 006 1 797 0 183 moon of Jupiter terrestrial 1610Moon Earth I 1737 4 0 1 0 2727 21 958 0 0203 73 46 0 0123 37 937 0 074 3 344 0 005 1 625 0 166 moon of Earth terrestrial prehistoricEuropa Jupiter II 1560 8 0 5 0 2450 15 93 0 0147 48 00 0 008035 30 613 0 06 3 013 0 005 1 316 0 134 moon of Jupiter terrestrial 1610Triton Neptune I 1353 4 0 9 0 2124 10 38 0 0096 21 39 0 03 0 003599 23 018 0 045 2 061 0 782 0 0797 moon of Neptune icy 1846Pluto 134340 1188 3 0 8 0 187 7 057 0 00651 13 03 0 03 0 0022 17 79 0 034 1 854 0 006 0 620 0 063 dwarf planet plutino multiple 1930Eris 136199 1163 6 0 1825 6 59 0 0061 16 6 0 2 0 0028 17 0 033 2 52 0 07 0 824 0 083 dwarf planet SDO binary 2003Haumea 136108 798 6 to 816 0 12 1 98 0 0018 4 01 0 04 0 00066 8 14 0 016 2 018 0 401 0 0409 dwarf planet resonant KBO 7 12 trinary has rings 2004Titania Uranus III 788 9 1 8 0 1237 2 06 0 0019 3 40 0 06 0 00059 7 82 0 015 1 711 0 005 0 378 0 0385 moon of Uranus 1787Rhea Saturn V 763 8 1 0 0 1199 1 87 0 0017 2 307 0 00039 7 34 0 014 1 236 0 005 0 26 0 027 moon of Saturn 1672Oberon Uranus IV 761 4 2 6 0 1195 1 85 0 0017 3 08 0 09 0 0005 7 285 0 014 1 63 0 05 0 347 0 035 moon of Uranus 1787Iapetus Saturn VIII 735 6 1 5 0 1153 1 66 0 0015 1 806 0 00033 6 8 0 013 1 088 0 013 0 223 0 0227 moon of Saturn 1671Makemake 136472 715 19 11 0 112 1 53 0 0014 3 1 0 00053 6 4 0 013 2 1 0 57 0 0581 dwarf planet cubewano 2005Gonggong 225088 615 25 0 0983 1 03 0 0009 1 75 0 07 0 00029 4 753 0 009 1 72 0 16 0 3 0 0306 dwarf planet resonant SDO 3 10 2007Charon Pluto I 606 0 0 5 0 0951 0 932 0 0009 1 586 0 015 0 00025 4 578 0 009 1 70 0 02 0 288 0 0294 moon of Pluto 1978Umbriel Uranus II 584 7 2 8 0 0918 0 837 0 0008 1 28 0 03 0 00020 4 3 0 008 1 39 0 16 0 234 0 024 moon of Uranus 1851Ariel Uranus I 578 9 0 6 0 0909 0 813 0 0007 1 25 0 02 0 000226 4 211 0 008 1 66 0 15 0 269 0 027 moon of Uranus 1851Dione Saturn IV 561 7 0 45 0 0881 0 741 0 0007 1 095 0 000183 3 965 0 008 1 478 0 003 0 232 0 0237 moon of Saturn 1684Quaoar 50000 543 2 0 0879 0 737 0 0007 1 20 0 05 0 0002 3 83 0 008 2 0 0 5 0 3 0 0306 dwarf planet cubewano binary has rings 2002Tethys Saturn III 533 0 0 7 0 0834 0 624 0 0006 0 617 0 000103 3 57 0 007 0 984 0 003 0 145 0 015 moon of Saturn 1684Ceres 1 469 7 0 1 0 0742 0 433 0 0004 0 938 0 000157 2 85 0 006 2 17 0 28 0 029 dwarf planet belt asteroid 1801Orcus 90482 455 25 20 0 0719 0 404 0 0004 0 548 0 010 0 000092 1 4 0 2 0 2 0 0204 dwarf planet plutino binary 2004Sedna 90377 453 157 129 0 0785 0 516 0 0005 dwarf planet sednoid detached object 2003Salacia 120347 423 11 0 0664 0 373 0 0003 0 492 0 007 0 000082 1 5 0 1 0 165 0 0168 cubewano binary 2004 star giant planet terrestrial planet presumed dwarf planet moon of Earth moon of Jupiter moon of Saturn moon of Uranus moon of Neptune moon of PlutoSmaller objects by mean radiusFrom 200 to 399 km All imaged icy moons with radii greater than 200 km except Proteus are clearly round although those under 400 km that have had their shapes carefully measured are not in hydrostatic equilibrium The known densities of TNOs in this size range are remarkably low 1 1 2 g cm3 implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies Body Image Radius km Mass 1018 kg Density g cm3 Type Refs r M2002 MS4 307261 398 12 cubewano2002 AW197 55565 384 19 cubewanoVarda 174567 373 8 245 6 1 23 0 04 cubewano binary 2013 FY27 532037 370 40 SDO binary2003 AZ84 208996 362 386 6 assuming HE 150 210 assuming HE 0 76 0 87 assuming HE plutino binary2021 DR15 356 374 SDOIxion 28978 354 8 0 1 plutino2004 GV9 90568 340 17 cubewano2005 RN43 145452 340 28 37 cubewanoVaruna 20000 327 77 51 160 0 99 0 09 0 02 cubewano2002 UX25 55637 332 15 125 3 0 82 0 11 cubewano binary 2005 RM43 145451 322 SDOGǃkunǁʼhomdima 229762 321 14 136 1 3 3 1 02 0 17 SDO binary 2014 UZ224 317 5 28 5 30 5 SDO 317 SDO2008 OG19 470599 309 5 28 56 5 0 609 0 004 SDO 2010 JO179 574372 309 SDO2007 JJ43 278361 305 85 70 cubewanoDysnomia Eris I 300 370 300 500 lt 140 1 8 2 4 lt 1 2 moon of Eris2014 EZ51 523692 gt 288 SDO2010 KZ39 287 SDO2012 VP113 287 sednoid2002 XW93 78799 283 36 37 other TNO2004 XR190 612911 278 SDO2002 XV93 612533 275 11 12 plutino2015 RR245 523794 270 resonant KBO 2 9 binary2003 UZ413 455502 268 plutino2007 JH43 470308 264 15 95 3 38 0 11 plutinoVesta 4 262 7 0 1 259 3 46 belt asteroid type V 2003 VS2 84922 262 4 plutino2014 FC72 257 15 275 3 detached objectPallas 2 256 2 204 3 2 92 0 08 belt asteroid type B2004 TY364 120348 256 19 20 cubewanoEnceladus Saturn II 252 1 0 2 108 0 0 1 1 609 0 005 moon of Saturn 2002 TC302 84522 250 7 resonant SDO 2 5 2005 UQ513 202421 249 32 38 cubewano2014 AN55 543354 248 SDOMiranda Uranus V 235 8 0 7 65 9 7 5 1 2 0 15 moon of Uranus Dziewanna 471143 235 18 5 SDO2005 TB190 145480 232 31 detached object1999 DE9 26375 231 23 resonant SDO 2 5 2003 FY128 120132 230 11 SDO2002 VR128 84719 224 24 22 plutinoVanth Orcus I 221 5 87 8 1 5 1 0 0 5 moon of 90482 Orcus 219 SDO612581 217 plutinoHygiea 10 216 4 87 4 6 9 2 06 0 20 belt asteroid type C 2004 NT33 444030 212 44 40 cubewanoProteus Neptune VIII 210 7 44 1 3 moon of Neptune 2002 GJ32 182934 208 cubewano2005 QU182 303775 208 37 SDOChaos 19521 208 42 15 equivalent cubewano2002 KX14 119951 207 5 0 5 cubewano1996 TO66 19308 204 5 90 5 assuming albedo 210 175 assuming albedo resonant KBO 11 19 2001 QF298 469372 204 20 22 plutinoHuya 38628 203 8 gt 50 gt 1 43 plutino binary 2004 PF115 175113 203 49 38 plutino2003 QW90 307616 200 5 135 cubewano2004 PT107 469615 200 5 100 cubewanoLegend SDO scattered disc object cubewano classical Kuiper belt object plutino 2 3 orbital resonance with NeptuneFrom 100 to 199 km This list contains a selection of objects estimated to be between 100 and 199 km in radius 200 and 399 km in diameter The largest of these may have a hydrostatic equilibrium shape but most are irregular Most of the trans Neptunian objects TNOs listed with a radius smaller than 200 km have assumed sizes based on a generic albedo of 0 09 since they are too far away to directly measure their sizes with existing instruments Mass switches from 1021 kg to 1018 kg Zg Main belt asteroids have orbital elements constrained by 2 0 AU lt a lt 3 2 AU q gt 1 666 AU according to JPL Solar System Dynamics JPLSSD Many TNOs are omitted from this list as their sizes are poorly known Body Image Radius km Mass 1018 kg Type Refs r M2004 UX10 144897 199 20 30 plutino 1998 VG44 33340 199 20 47 plutino1993 SC 15789 199 20 47 plutinoMimas Saturn I 198 2 0 3 37 49 0 03 moon of Saturn 1998 SN165 35671 196 20 cubewano2001 UR163 42301 176 resonant KBO 4 9 1995 SM55 24835 173 assuming albedo of 0 7 cubewano2001 YH140 126154 172 20 85 resonant KBO 3 5 2010 ER65 552555 170 20 30 SDONereid Neptune II 170 25 moon of Neptune1996 TL66 15874 170 10 SDO2004 XA192 230965 170 60 47 5 SDO2010 ET65 471137 170 20 30 SDO2002 WC19 119979 169 77 5 resonant KBO 1 2 binary 2005 CA79 612931 167 20 60 resonant KBO 1 2 Interamnia 704 166 3 35 2 5 1 belt asteroid type F Ilmare Varda I 163 18 moon of 174567 VardaEuropa 52 160 2 23 9 3 8 belt asteroid type CHiʻiaka Haumea I 160 17 9 1 1 moon of Haumea 2002 KW14 307251 160 20 30 cubewano1999 CD158 469306 155 20 48 resonant KBO 4 7 2007 OC10 470316 155 20 30 SDO2005 RR43 145453 150 20 60 cubewanoDavida 511 149 2 26 6 7 3 belt asteroid type C2002 TX300 55636 143 5 cubewanoActaea Salacia I 143 12 moon of 120347 SalaciaSylvia 87 137 2 14 3 0 5 outer belt asteroid type X trinary2003 OP32 120178 137 20 45 cubewanoLempo 47171 136 9 plutino trinaryEunomia 15 135 2 30 5 1 9 belt asteroid type SHyperion Saturn VII 135 4 5 62 0 05 moon of Saturn Euphrosyne 31 134 2 16 5 2 6 belt asteroid type C binary1998 SM165 26308 134 14 6 87 1 8 resonant KBO 1 2 Cybele 65 131 5 1 5 14 8 1 8 outer belt asteroid type CChariklo 10199 130 centaur has ringsJuno 3 127 1 27 0 2 4 belt asteroid type SHiisi Lempo II 126 8 secondary of 47171 LempoHektor 624 125 13 7 9 1 4 Jupiter trojan L4 type D binary Sila 79360 124 15 10 8 0 22 cubewano binary2007 RW10 309239 124 15 quasi satellite of NeptuneAltjira 148780 123 19 70 cubewano binaryNunam 79360 118 15 secondary of 79360 SilaBamberga 324 114 2 10 2 0 9 belt asteroid type CPatientia 451 112 9 2 3 10 9 5 3 belt asteroid type C Psyche 16 112 2 26 2 2 9 belt asteroid type MCeto 65489 112 5 5 4 0 4 extended centaur binary Herculina 532 111 2 2 4 belt asteroid type SS 2007 148780 1 Altjira I 110 17 62 secondary of 148780 AltjiraHesperia 69 110 15 5 86 1 18 belt asteroid type M Thisbe 88 109 2 11 6 2 2 belt asteroid type BDoris 48 108 2 6 9 2 9 belt asteroid type CChiron 2060 or 95P 108 5 centaur has ringsPhoebe Saturn IX 106 5 0 7 8 29 0 01 moon of Saturn Satellite of 38628 Huya Huya I 106 15 moon of 38628 HuyaFortuna 19 105 5 1 0 8 8 1 4 belt asteroid type GCamilla 107 105 4 11 2 0 3 outer belt asteroid type C trinary Themis 24 104 2 6 2 2 9 belt asteroid type CAmphitrite 29 102 1 12 7 2 0 belt asteroid type SEgeria 13 101 2 9 2 2 1 belt asteroid type GIris 7 100 5 13 5 2 3 belt asteroid type SLegend centaur asteroids orbiting between the outer planets Jupiter trojan asteroids located in Jupiter s L4 and L5 Lagrange pointsFrom 50 to 99 km This list contains a selection of objects 50 and 99 km in radius 100 km to 199 km in average diameter The listed objects currently include most objects in the asteroid belt and moons of the giant planets in this size range but many newly discovered objects in the outer Solar System are missing such as those included in the following reference Asteroid spectral types are mostly Tholen but some might be SMASS Body Image Radius km Mass 1018 kg Type Refs r MElektra 130 99 5 1 6 4 0 2 belt asteroid type G multipleBienor 54598 99 3 3 5 centaurHebe 6 97 5 1 5 12 4 2 4 belt asteroid type SLarissa Neptune VII 97 3 4 2 moon of Neptune Ursula 375 96 8 1 3 8 4 5 3 belt asteroid type C S 2018 532037 1 95 moon of 2013 FY27Eugenia 45 94 1 5 8 0 1 belt asteroid type F trinaryHermione 121 94 3 5 0 0 3 outer belt asteroid type C binary Daphne 41 94 7 6 1 0 9 belt asteroid type C binaryAurora 94 93 8 3 6 dubious discuss 6 2 3 6 belt asteroid type C Bertha 154 93 4 0 9 9 2 5 2 dubious discuss belt asteroid type C Janus Saturn X 89 5 1 4 1 898 0 001 moon of Saturn Teharonhiawako 88611 89 16 18 2 44 0 03 dubious discuss cubewano binary Aegle 96 88 9 0 8 6 4 6 3 belt asteroid type T Galatea Neptune VI 88 4 2 12 0 08 moon of Neptune Phorcys Ceto I 87 8 9 1 67 secondary of 65489 Ceto Palma 372 86 8 1 4 dubious discuss 5 2 0 6 belt asteroid type B Metis 9 86 5 1 8 0 1 9 belt asteroid type S Alauda 702 86 28 6 06 0 36 dubious discuss belt asteroid type C binary Hilda 153 85 3 1 6 outer belt asteroid HildasHimalia Jupiter VI 85 4 2 0 6 moon of Jupiter Namaka Haumea II 85 1 8 1 5 moon of Haumea Weywot Quaoar I 85 lt 5 moon of 50000 QuaoarFreia 76 84 2 1 0 2 0 4 2 dubious discuss outer belt asteroid type P type X Amalthea Jupiter V 83 45 2 4 2 08 0 15 moon of Jupiter Agamemnon 911 83 3 2 0 Jupiter trojan L4 type DElpis 59 82 6 2 3 3 0 5 belt asteroid type CP type B Eleonora 354 82 5 1 5 7 5 2 7 belt asteroid type ANemesis 128 81 5 2 5 3 4 1 7 belt asteroid type CPuck Uranus XV 81 2 moon of UranusS 2015 136472 1 Makemake I 80 moon of MakemakeSycorax Uranus XVII 78 5 11 5 7 5 moon of UranusIo 85 77 4 1 9 dubious discuss 2 6 1 5 belt asteroid type FC type B Minerva 93 77 08 0 65 3 5 0 4 belt asteroid type C trinary Alexandra 54 77 07 0 32 6 2 3 5 dubious discuss belt asteroid type C Laetitia 39 77 2 4 7 1 1 belt asteroid type S Nemausa 51 75 1 5 3 9 1 6 belt asteroid type GKalliope 22 75 2 5 7 7 0 4 belt asteroid type M binaryDespina Neptune V 75 3 moon of NeptuneManwe 385446 75 1 41 resonant KBO 4 7 binary Pales 49 74 9 4 2 2 2 belt asteroid type C Parthenope 11 74 5 1 5 5 0 4 belt asteroid type SArethusa 95 74 0 2 4 belt asteroid type CPulcova 762 73 7 0 4 1 4 0 1 belt asteroid type F binary Flora 8 73 1 4 0 1 6 belt asteroid type SIno 173 72 5 1 5 2 2 1 3 belt asteroid type XcAdeona 145 72 1 5 2 4 0 3 belt asteroid type XcIrene 14 72 1 2 9 1 9 belt asteroid type S Melpomene 18 70 5 1 4 5 0 9 belt asteroid type SLamberta 187 70 5 1 1 9 0 3 belt asteroid type ChAglaja 47 71 4 3 2 1 7 belt asteroid type C Patroclus 617 70 2 0 4 1 36 0 11 Jupiter trojan L5 type P binary Julia 89 70 1 4 4 3 3 2 belt asteroid type STyphon 42355 69 4 5 0 87 0 03 resonant SDO 7 10 binary Massalia 20 67 8 1 8 5 1 04 belt asteroid type S Portia Uranus XII 67 6 4 moon of UranusEmma 283 66 2 0 1 1 38 0 03 belt asteroid type X binary Paha Lempo I 66 4 4 5 0 746 0 001 moon of 47171 Lempo Lucina 146 65 9 belt asteroid type CSawiskera Teharonhiawako I 65 5 12 13 secondary of 88611 TeharonhiawakoAchilles 588 65 0 0 3 Jupiter trojan L4 type DUPanopaea 70 64 0 0 4 4 33 1 09 belt asteroid type C Thule 279 63 3 1 8 outer belt asteroid type DBorasisi 66652 63 12 5 25 5 3 433 0 027 cubewano binary Hestia 46 62 07 1 7 3 5 belt asteroid type P type Xc Leto 68 61 3 1 6 3 28 1 9 belt asteroid type S Undina 92 60 46 0 85 4 43 0 25 belt asteroid type X Bellona 28 60 45 1 90 2 62 0 15 belt asteroid type S Diana 78 60 30 1 35 1 27 0 13 belt asteroid type C Anchises 1173 60 2 1 5 Jupiter trojan L5 type PBernardinelli Bernstein C 2014 UN271 60 7 cometGalatea 74 59 4 1 4 6 13 5 36 belt asteroid type C Deiphobus 1867 59 1 0 8 Jupiter trojan L5 type DAneas 1172 59 01 0 40 Jupiter trojan L5 type DKleopatra 216 59 1 3 0 0 3 belt asteroid type M trinaryAthamantis 230 59 1 2 3 1 1 belt asteroid type SDiomedes 1437 58 89 0 59 Jupiter trojan L4 type DTerpsichore 81 58 9 0 4 6 19 5 31 belt asteroid type C Epimetheus Saturn XI 58 1 1 8 0 5266 0 0006 moon of Saturn Victoria 12 58 1 2 7 1 3 belt asteroid type SCirce 34 57 7 1 0 3 66 0 03 belt asteroid type C Leda 38 57 7 0 7 5 71 5 47 belt asteroid type C Odysseus 1143 57 3 0 3 Jupiter trojan L4 type DAlcathous 2241 56 8 0 9 Jupiter trojan L5 type DMelete 56 56 62 0 85 4 61 belt asteroid type P Mnemosyne 57 56 3 1 4 12 6 2 4 belt asteroid type S Nestor 659 56 2 0 9 Jupiter trojan L4 type XCHarmonia 40 55 6 0 2 belt asteroid type SLeleakuhonua 541132 55 7 5 sednoidEuterpe 27 54 9 0 8 1 67 1 01 belt asteroid type S Antilochus 1583 54 4 0 3 Jupiter trojan L4 type DThorondor Manwe I 54 0 5 secondary of 385446 Manwe Thalia 23 53 8 1 1 1 96 0 09 belt asteroid type S Erato 62 53 5 0 3 belt asteroid type BU type ChAstraea 5 53 3 1 6 2 9 belt asteroid type S Pabu Borasisi I 52 5 10 21 secondary of 66652 BorasisiEos 221 51 76 2 8 5 87 0 34 belt asteroid type S type K Aegina 91 51 7 0 2 belt asteroid type CLeukothea 35 51 5 0 6 belt asteroid type CMenoetius Patroclus I 51 4 0 25 secondary of 617 PatroclusIsis 42 51 4 1 4 1 58 0 52 belt asteroid type S Klotho 97 50 4 0 3 1 33 0 13 belt asteroid type M Troilus 1208 50 3 0 5 Jupiter trojan L5 type FCUFrom 20 to 49 km This list includes few examples since there are about 589 asteroids in the asteroid belt with a measured radius between 20 and 49 km Many thousands of objects of this size range have yet to be discovered in the trans Neptunian region The number of digits is not an endorsement of significant figures The table switches from 1018 kg to 1015 kg Eg Most mass values of asteroids are assumed Body Image Radius km Mass 1015 kg Type notes Refs r MAsterope 233 49 8 0 6 belt asteroid type T type KPholus 5145 49 5 7 5 7 centaurThebe Jupiter XIV 49 3 2 moon of JupiterLutetia 21 49 1 1700 20 belt asteroid type MKalypso 53 48 631 13 299 5630 5000 belt asteroid type XC Notburga 626 48 42 2 335 belt asteroid type XCProserpina 26 47 4 0 85 748 895 belt asteroid type S Juliet Uranus XI 46 8 4 moon of UranusUrania 30 44 1 1300 900 belt asteroid type SAusonia 63 46 5 1 5 1200 200 belt asteroid type SBeatrix 83 44 819 1 326 belt asteroid type XConcordia 58 44 806 0 419 belt asteroid type CEchidna Typhon I 44 5 3 moon of 42355 TyphonAutomedon 2920 44 287 0 898 Jupiter trojan L4 type DAntiope 90 43 9 0 5 828 22 belt asteroid type C binary Prometheus Saturn XVI 43 1 2 7 159 5 1 5 moon of Saturn Danae 61 42 969 1 076 2890 2780 belt asteroid type S Thetis 17 42 449 1 014 1200 belt asteroid type S Pandora 55 42 397 1 251 belt asteroid type MHuenna 379 42 394 0 779 383 19 belt asteroid type B type C binary Virginia 50 42 037 0 121 2310 700 belt asteroid type X type Ch Feronia 72 41 975 2 01 3320 8490 belt asteroid type TDG S 2000 90 1 Antiope I 41 9 0 5 secondary of 90 AntiopePoulydamas 4348 41 016 0 313 Jupiter trojan L5 type CLogos 58534 41 9 458 6 9 cubewano binary Pandora Saturn XVII 40 7 1 5 137 1 1 9 moon of Saturn Thalassa Neptune IV 40 7 2 8 moon of NeptuneNiobe 71 40 43 0 4 belt asteroid type SPomona 32 40 38 0 8 belt asteroid type SBelinda Uranus XIV 40 3 8 moon of UranusElara Jupiter VII 39 95 1 7 moon of JupiterCressida Uranus IX 39 8 2 moon of UranusAmycus 55576 38 15 6 25 centaurHylonome 10370 37 545 centaurSocus 3708 37 831 0 404 Jupiter trojan L5 type CNysa 44 37 83 0 37 belt asteroid type ERosalind Uranus XIII 36 6 moon of UranusMaja 66 35 895 0 46 belt asteroid type CAriadne 43 35 67 0 627 1210 220 belt asteroid type S Iphigenia 112 35 535 0 26 1970 6780 belt asteroid type C Xiangliu Gonggong I 35 15 moon of 225088 GonggongDike 99 33 677 0 208 belt asteroid type CEcheclus 60558 or 174P 32 3 0 8 centaurDesdemona Uranus X 32 4 moon of UranusEurybates 3548 31 943 0 149 Jupiter trojan L4 type CPEurynome 79 31 739 0 476 belt asteroid type SEurydike 75 31 189 0 802 belt asteroid type MHalimede Neptune IX 31 moon of NeptunePhocaea 25 30 527 1 232 599 60 belt asteroid type S Naiad Neptune III 30 2 3 2 moon of NeptuneSchwassmann Wachmann 1 29P 30 2 3 7 cometNeso Neptune XIII 30 moon of NeptuneAngelina 64 29 146 0 541 belt asteroid type EPasiphae Jupiter VIII 28 9 0 4 moon of JupiterAlkmene 82 28 811 0 357 belt asteroid type SNessus 7066 28 5 8 5 centaurPolana 142 27 406 0 139 belt asteroid type FBianca Uranus VIII 27 2 moon of UranusMathilde 253 26 4 103 3 4 4 belt asteroid type C Hidalgo 944 26 225 1 8 centaur