List of Solar System objects by size explained

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.

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 1021 kilograms 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;[1] however, later studies revealed that icy satellites as large as Iapetus (1,470 kilometers in diameter) are not in hydrostatic equilibrium at this time,[2] 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.[3] 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). 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.[4]

For example, if a TNO is incorrectly assumed to have a mass of 3.59 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 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.[5] 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[6] and JPL Solar System Dynamics,[5] 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.

Objects with radii over 400 km

The following objects have a mean radius of at least 400 km. It was once expected that any icy body larger than approximately 200 km in radius was likely to be in hydrostatic equilibrium (HE).[7] However, (r = 470 km) is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium,[8] whereas Iapetus (r = 735 km) is the largest icy body that has been found to not be in hydrostatic equilibrium.[9] 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.[10]

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.[11]

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[12]).

BodyImageRadiusVolumeMassSurface areadata-sort-type="number" DensityGravityTypeDiscovery
data-sort-type="number" (km)data-sort-type="number" (R)data-sort-type="number" (109 km3)data-sort-type="number" data-sort-type="number" (1021 kg)data-sort-type="number" (M)(106 km2)data-sort-type="number" (g/cm3)data-sort-type="number" (m/s2)data-sort-type="number" ()
bgcolor=black[13] [14] 333,0006,078,70011,918274.027.94G2V-class star
Jupiterbgcolor=black[15] 10.971,431,2801,321317.8361,419[16] 120.4124.792.528gas giant planet
has rings
Saturnbgcolor=black
9.140827,13076495.16242,612[17] 83.5410.441.065gas giant planet
has rings
Uranusbgcolor=black3.98168,34063.114.5368083.1[18] 15.858.870.886ice giant planet
has rings
1781
Neptunebgcolor=black3.86562,54057.717.1477618.3[19] 14.9411.151.137ice giant planet
has rings
1846
bgcolor=black11,083.2111510.06447[20] 19.811terrestrial planet
Venusbgcolor=black0.9499928.430.8570.815460.2[21] 0.9038.870.905terrestrial planet
Marsbgcolor=black0.5320163.180.1510.107144.37[22] 0.2833.710.379terrestrial planet
Ganymede
bgcolor=black0.413576.300.07040.024886.999[23] 0.1711.4280.146moon of Jupiter (icy)1610
Titan
bgcolor=black0.403771.500.06580.022583.3054[24] 0.1631.3540.138moon of Saturn (icy)1655
Mercurybgcolor=black0.382960.830.05620.055374.797[25] 0.1473.700.377terrestrial planet
Callisto
bgcolor=black0.378358.650.05410.01873.005[26] 0.1431.236030.126moon of Jupiter (icy)1610
Io
bgcolor=black0.285925.320.02340.01541.698[27] 0.0821.7970.183moon of Jupiter (terrestrial)1610
Moon
bgcolor=black[28] 0.272721.9580.0203[29] 0.012337.937[30] 0.0741.6250.166moon of Earth (terrestrial)
Europa
bgcolor=black0.245015.930.01470.00803530.613[31] 0.061.3160.134moon of Jupiter (terrestrial)1610
Triton
bgcolor=black0.212410.380.00960.00359923.018[32] 0.0450.7820.0797moon of Neptune (icy)1846
Pluto
bgcolor=black0.1877.0570.006510.002217.790.0340.6200.063dwarf planet
plutino; multiple
1930
Eris
[33] 0.18256.590.0061[34] 0.0028170.0330.083dwarf planet
SDO; binary
2003

bgcolor=black to 816[35] 0.121.980.00180.000668.140.016[36] 0.4010.0409dwarf planet

resonant KBO (7:12);
trinary; has rings
2004
Titania
bgcolor=black0.12372.060.00190.000597.82[37] 0.0150.3780.0385moon of Uranus1787
Rhea
bgcolor=black0.11991.870.00170.000397.34[38] 0.0140.260.027moon of Saturn1672
Oberon
bgcolor=black0.11951.850.00170.00057.285[39] 0.0140.3470.035moon of Uranus1787
Iapetus
bgcolor=black0.11531.660.00150.000336.80.0130.2230.0227moon of Saturn1671

bgcolor=black[40] 0.1121.530.00140.000536.40.0130.570.0581dwarf planet
cubewano
2005
Gonggong
bgcolor=black[41] 0.09831.030.00090.000294.7530.0090.30.0306dwarf planet
resonant SDO (3:10)
2007
Charon
bgcolor=black0.09510.9320.00090.000254.578[42] 0.0090.2880.0294moon of Pluto1978
Umbriel
bgcolor=black0.09180.8370.00080.000204.3[43] 0.0080.2340.024moon of Uranus1851
Ariel
bgcolor=black0.09090.8130.00070.0002264.211[44] 0.0080.2690.027moon of Uranus1851
Dione
bgcolor=black0.08810.7410.00070.0001833.965[45] 0.0080.2320.0237moon of Saturn1684
Quaoar
bgcolor=black0.08790.7370.0007[46] 0.00023.830.008[47] 0.30.0306dwarf planet
cubewano; binary; has rings
2002
Tethys
bgcolor=black0.08340.6240.00060.0001033.57[48] 0.007[49] 0.1450.015moon of Saturn1684
Ceres
bgcolor=black[50] 0.07420.4330.0004[51] 0.0001572.85[52] 0.0060.280.029dwarf planet
belt asteroid
1801
Orcus
bgcolor=black0.07190.4040.00040.0000920.20.0204dwarf planet
plutino; binary
2004
Sedna
bgcolor=black0.07850.5160.0005dwarf planet
sednoid; detached object
2003
Salacia
bgcolor=black0.06640.37290.00030.000082[53] 0.0168cubewano
binary
2004

bgcolor=black[54] 0.06280.26810.0002cubewano2002

                  

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, implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies.[10]

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
data-sort-type="number" vkwidth=75 Mass
data-sort- type="number" style="width:65px;"Density
TypeRefs

align=center align=center –align=center –cubewanoalign=center [55]
Varda
align=center align=center align=center cubewano
binary
align=center [56]

bgcolor=blackalign=center align=center –align=center –SDO
binary
align=center [57]

align=center ~ (assuming HE)align=center 150 ~ 210 (assuming HE)align=center ~ (assuming HE)plutino
binary
align=center [58]
Ixion
align=center align=center –align=center –plutinoalign=center [59]

align=center align=center –align=center –cubewanoalign=center [60]

align=center align=center –align=center –cubewanoalign=center
Varuna
align=center align=center align=center cubewanoalign=center [61] [62]

align=center align=center align=center cubewano; binaryalign=center [63]

align=center align=center –align=center –SDOalign=center [64] [65]
Gǃkúnǁʼhòmdímà
bgcolor=blackalign=center align=center align=center SDO; binaryalign=center [66] [67]
––SDO[68]

bgcolor=blackalign=center align=center –align=center SDOalign=center [69]

bgcolor=blackalign=center align=center –align=center –cubewanoalign=center [70]
Chaos
align=center align=center –align=center –cubewanoalign=center
Dysnomia
align=center align=center
align=center
moon of Erisalign=center [71] [72]

bgcolor=blackalign=center align=center –align=center –SDOalign=center [73]
bgcolor=blackalign=center align=center –align=center –sednoidalign=center [74]

bgcolor=blackalign=center align=center –align=center –other TNOalign=center [75]

align=center align=center –align=center –SDOalign=center

bgcolor=blackalign=center align=center –align=center –plutinoalign=center [76]

bgcolor=blackalign=center align=center –align=center –resonant KBO ; binaryalign=center

align=center align=center –align=center –plutinoalign=center
Vesta
bgcolor=blackalign=center align=center align=center belt asteroid type Valign=center [77]

align=center align=center –align=center –plutinoalign=center [78]
Pallas
bgcolor=blackalign=center align=center align=center belt asteroid type Balign=center [79] [80]

bgcolor=blackalign=center align=center –align=center –cubewanoalign=center [81]
Enceladus
bgcolor=blackalign=center align=center align=center moon of Saturnalign=center [82] [83]

align=center align=center –align=center –resonant SDO align=center [84]

bgcolor=blackalign=center align=center –align=center –cubewanoalign=center
Miranda
bgcolor=blackalign=center align=center align=center moon of Uranusalign=center [85] [86]
Dziewanna
align=center align=center –align=center –SDOalign=center [87]

align=center align=center –align=center –detached objectalign=center [88]

bgcolor=blackalign=center align=center –align=center –resonant SDO align=center [89]

bgcolor=blackalign=center align=center –align=center –SDOalign=center

bgcolor=blackalign=center align=center –align=center –plutinoalign=center
Vanth
align=center align=center align=center moon of 90482 Orcusalign=center [90]
Hygiea
bgcolor=blackalign=center align=center align=center belt asteroid type Calign=center [91]

bgcolor=blackalign=center align=center –align=center –cubewanoalign=center
Proteus
bgcolor=blackalign=center align=center align=center moon of Neptunealign=center

bgcolor=blackalign=center align=center –align=center –SDOalign=center

align=center align=center –align=center –cubewanoalign=center [92]

align=center align=center –align=center –plutinoalign=center
Huya
bgcolor=blackalign=center align=center align=center plutino
binary
align=center [93] [94]

bgcolor=blackalign=center align=center –align=center –plutinoalign=center
Legend:

SDO – scattered disc object

cubewano – classical Kuiper belt object

plutino – 2:3 orbital resonance with Neptune

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).[95] Many TNOs are omitted from this list as their sizes are poorly known.

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
data-sort- type="number" style="width:75px;"Mass
TypeRefs

bgcolor=blackalign=center align=center plutinoalign=center [96]
Mimas
bgcolor=blackalign=center align=center moon of Saturnalign=center

bgcolor=blackalign=center align=center cubewanoalign=center

align=center align=center resonant KBO align=center
Nereid
moon of Neptune

bgcolor=blackalign=center align=center SDOalign=center

bgcolor=blackalign=center align=center SDOalign=center

align=center align=center resonant KBO ; binaryalign=center [97]
Interamnia
bgcolor=blackalign=center align=center belt asteroid type Falign=center [98]
Ilmarë
align=center align=center moon of 174567 Vardaalign=center [99]
Europa
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Hiʻiaka
align=center align=center moon of Haumeaalign=center [100]
Davida
bgcolor=blackalign=center align=center belt asteroid type Calign=center

align=center align=center cubewanoalign=center [101]
Actaea
bgcolor=blackalign=center align=center moon of 120347 Salaciaalign=center [102]
Sylvia
bgcolor=blackalign=center align=center outer belt asteroid type X; trinaryalign=center
Lempo
align=center align=center plutino
trinary
align=center [103]
Eunomia
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Hyperion
moon of Saturn[104] [105]
Euphrosyne
bgcolor=blackalign=center align=center belt asteroid type C; binaryalign=center

align=center align=center resonant KBO align=center [106]
Cybele
bgcolor=blackalign=center align=center outer belt asteroid type Calign=center [107]
Chariklo
bgcolor=blackalign=center align=center centaur
has rings
align=center [108]
Juno
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Hiisi
align=center align=center secondary of 47171 Lempoalign=center
Hektor
bgcolor=blackalign=center align=center Jupiter trojan type D; binaryalign=center [109]
Sila
align=center align=center cubewano
binary
align=center [110]

bgcolor=blackalign=center align=center quasi-satellite of Neptunealign=center
Altjira
align=center align=center cubewano
binary
align=center
Nunam
align=center align=center secondary of 79360 Silaalign=center
Bamberga
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Patientia
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Psyche
bgcolor=blackalign=center align=center belt asteroid type Malign=center
Ceto
align=center align=center extended centaur; binaryalign=center
Herculina
bgcolor=blackalign=center align=center belt asteroid type Salign=center
S/2007 (148780) 1
align=center align=center secondary of 148780 Altjiraalign=center
Hesperia
bgcolor=blackalign=center align=center belt asteroid type Malign=center [111]
Thisbe
bgcolor=blackalign=center align=center belt asteroid type Balign=center
Doris
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Chiron
align=center align=center centaur
has rings
align=center
Phoebe
bgcolor=blackalign=center align=center moon of Saturnalign=center
S/2012 (38628) 1
bgcolor=blackalign=center align=center moon of 38628 Huyaalign=center
Fortuna
bgcolor=blackalign=center align=center belt asteroid type Galign=center
Camilla
bgcolor=blackalign=center align=center outer belt asteroid type C; trinaryalign=center [112]
Themis
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Amphitrite
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Egeria
bgcolor=blackalign=center align=center belt asteroid type Galign=center
Iris
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Legend:

centaur – asteroids orbiting between the outer planets

Jupiter trojan – asteroids located in Jupiter's and Lagrange points

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.

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
data-sort- type="number" style="width:75px;"Mass
TypeRefs
Elektra
bgcolor=blackalign=center align=center belt asteroid type G; multiplealign=center
Bienor
bgcolor=blackalign=center align=center centauralign=center
Hebe
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Larissa
bgcolor=blackalign=center align=center moon of Neptunealign=center
Ursula
align=center align=center belt asteroid type Calign=center [113]
S/2018 (532037) 1bgcolor=blackalign=center align=center moon of 2013 FY27align=center
Eugenia
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type F; trinaryalign=center
Hermione
bgcolor=blackalign=center align=center outer belt asteroid type C; binaryalign=center [114]
Daphne
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type C; binaryalign=center
Aurora
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Bertha
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Calign=center
Janus
bgcolor=blackalign=center align=center moon of Saturnalign=center
Teharonhiawako
align=center align=center cubewano
binary
align=center [115]
Aegle
bgcolor=blackalign=center align=center belt asteroid type Talign=center
Galatea
moon of Neptune[116]
Phorcys
align=center align=center secondary of 65489 Cetoalign=center [117]
Palma
bgcolor=blackalign=center align=center belt asteroid type Balign=center [118]
Metis
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Alauda
align=center align=center belt asteroid type C; binaryalign=center [119]
Hilda
outer belt asteroid; Hildas
Himalia
moon of Jupiter[120]
Namaka
bgcolor=#181818 moon of Haumea
Weywot
moon of 50000 Quaoar
Freia
outer belt asteroid type P/type X
Amalthea
moon of Jupiter[121] [122]
Agamemnon
Jupiter trojan type D
Elpis
belt asteroid type CP/type B
Eleonora
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Aalign=center
Nemesis
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Calign=center
Puck
moon of Uranus[123]
S/2015 (136472) 1
bgcolor=blackmoon of Makemake[124]
Sycorax
bgcolor=blackalign=center align=center moon of Uranusalign=center [125]
Io
bgcolor=blackalign=center align=center belt asteroid type FC/type Balign=center
Minerva
bgcolor=blackalign=center align=center belt asteroid type C; trinaryalign=center
Alexandra
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Laetitia
bgcolor=blackalign=center align=center belt asteroid type Salign=center [126]
Nemausa
bgcolor=blackalign=center align=center belt asteroid type Galign=center
Kalliope
frameless|center|upright=0.2belt asteroid type M; binary
Despina
moon of Neptune
Manwë
align=center align=center resonant KBO ; binaryalign=center [127]
Pales
bgcolor=blackalign=center align=center belt asteroid type Calign=center [128]
Parthenope
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Salign=center
Arethusa
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Pulcova
align=center align=center belt asteroid type F; binaryalign=center [129]
Flora
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Salign=center
Ino
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Xcalign=center
Adeona
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Xcalign=center
Irene
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Melpomene
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Salign=center
Lamberta
bgcolor=blackframeless|center|upright=0.2align=center align=center belt asteroid type Chalign=center
Aglaja
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Patroclus
align=center align=center Jupiter trojan type P; binaryalign=center
Julia
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Typhon
align=center align=center resonant SDO (7:10); binaryalign=center [130]
Massalia
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Portia
align=center align=center moon of Uranusalign=center
Emma
bgcolor=blackalign=center align=center belt asteroid type X; binaryalign=center
Paha
align=center align=center moon of 47171 Lempoalign=center [131]
Lucina
bgcolor=blackalign=center ±?align=center belt asteroid type Calign=center [132]
Sawiskera
align=center align=center secondary of 88611 Teharonhiawakoalign=center
Achilles
bgcolor=blackalign=center align=center Jupiter trojan type DUalign=center
Panopaea
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Thule
bgcolor=blackalign=center align=center outer belt asteroid type Dalign=center
Borasisi
align=center align=center cubewano
binary
align=center [133]
Hestia
bgcolor=blackalign=center align=center belt asteroid type P/type Xcalign=center [134]
Leto
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Undina
bgcolor=blackalign=center align=center belt asteroid type Xalign=center
Bellona
align=center align=center belt asteroid type Salign=center [135]
Diana
bgcolor=blackalign=center align=center belt asteroid type Calign=center [136]
Anchises
bgcolor=blackalign=center align=center Jupiter trojan type Palign=center
Bernardinelli-Bernstein
bgcolor=blackalign=center align=center cometalign=center [137]
Galatea
bgcolor=blackalign=center align=center belt asteroid type Calign=center [138]
Deiphobus
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [139]
Äneas
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [140]
Kleopatra
bgcolor=blackalign=center align=center belt asteroid type M; trinaryalign=center
Athamantis
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Diomedes
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [141]
Terpsichore
bgcolor=blackalign=center align=center belt asteroid type Calign=center [142]
Epimetheus
bgcolor=blackalign=center align=center moon of Saturnalign=center
Victoria
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Circe
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Leda
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Odysseus
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [143]
Alcathous
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [144]
Melete
bgcolor=blackalign=center align=center belt asteroid type Palign=center
Mnemosyne
bgcolor=blackalign=center align=center belt asteroid type Salign=center [145]
Nestor
bgcolor=blackalign=center align=center Jupiter trojan type XCalign=center [146]
Harmonia
bgcolor=blackalign=center align=center belt asteroid type Salign=center [147]
Leleākūhonua
bgcolor=blackalign=center align=center sednoidalign=center [148]
Euterpe
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Antilochus
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center
Thorondor
align=center align=center secondary of 385446 Manwëalign=center
Thalia
bgcolor=blackalign=center align=center belt asteroid type Salign=center [149]
Erato
bgcolor=blackalign=center align=center belt asteroid type BU/type Chalign=center [150]
Astraea
bgcolor=blackalign=center align=center belt asteroid type Salign=center [151]
Pabu
align=center align=center secondary of 66652 Borasisialign=center
Eos
bgcolor=blackalign=center align=center belt asteroid type S/type Kalign=center
Aegina
bgcolor=blackalign=center align=center belt asteroid type Calign=center [152]
Leukothea
bgcolor=blackalign=center align=center belt asteroid type Calign=center [153]
Menoetius
align=center align=center secondary of 617 Patroclusalign=center [154]
Isis
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Klotho
bgcolor=blackalign=center align=center belt asteroid type Malign=center
Troilus
align=center align=center Jupiter trojan type FCUalign=center [155]

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.[156] 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  kg to  kg (Eg). Most mass values of asteroids are assumed.[126] [157]

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
data-sort- type="number" style="width:75px;"Mass
Type – notesRefs
Asterope
bgcolor=blackalign=center align=center belt asteroid type T/type Kalign=center [158]
Pholus
bgcolor=blackalign=center align=center centauralign=center
Thebe
bgcolor=blackalign=center align=center moon of Jupiteralign=center
Lutetia
bgcolor=blackalign=center align=center belt asteroid type Malign=center
Kalypso
bgcolor=blackalign=center align=center belt asteroid type XCalign=center [159]
Notburga
bgcolor=blackalign=center belt asteroid type XCalign=center
Proserpina
bgcolor=blackalign=center align=center belt asteroid type Salign=center [160]
Juliet
bgcolor=blackalign=center align=center moon of Uranusalign=center
Urania
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Ausonia
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Beatrix
bgcolor=blackalign=center align=center belt asteroid type Xalign=center
Concordia
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Echidna
align=center align=center moon of 42355 Typhonalign=center
Automedon
bgcolor=blackalign=center align=center Jupiter trojan type Dalign=center [161]
Antiope
bgcolor=blackalign=center align=center belt asteroid type C; binaryalign=center [162]
Prometheus
bgcolor=blackalign=center align=center moon of Saturnalign=center
Danaë
bgcolor=blackalign=center align=center belt asteroid type Salign=center [163]
Thetis
bgcolor=blackalign=center align=center belt asteroid type Salign=center [164]
Pandora
bgcolor=blackalign=center align=center belt asteroid type Malign=center [165]
Huenna
bgcolor=blackalign=center align=center belt asteroid type B/type C; binaryalign=center [166] [167]
Virginia
bgcolor=blackalign=center align=center belt asteroid type X/type Chalign=center [168]
Feronia
bgcolor=blackalign=center align=center belt asteroid type TDGalign=center
S/2000 (90) 1
bgcolor=blackalign=center align=center secondary of 90 Antiopealign=center
Poulydamas
bgcolor=blackalign=center align=center Jupiter trojan type Calign=center [169]
Logos
align=center align=center cubewano
binary
align=center [170]
Pandora
bgcolor=blackalign=center align=center moon of Saturnalign=center
Thalassa
align=center align=center moon of Neptunealign=center
Niobe
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Pomona
bgcolor=blackalign=center align=center belt asteroid type Salign=center [171]
Belinda
bgcolor=blackalign=center align=center moon of Uranusalign=center
Elara
bgcolor=blackalign=center align=center moon of Jupiteralign=center [172]
Cressida
bgcolor=blackalign=center align=center moon of Uranusalign=center
Amycus
bgcolor=blackalign=center align=center centauralign=center
Hylonome
align=center align=center centauralign=center [173]
Socus
bgcolor=blackalign=center align=center Jupiter trojan type Calign=center
Nysa
bgcolor=blackalign=center align=center belt asteroid type Ealign=center
Rosalind
bgcolor=blackalign=center align=center moon of Uranusalign=center
Maja
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Ariadne
bgcolor=blackalign=center align=center belt asteroid type Salign=center [174]
Iphigenia
bgcolor=blackalign=center align=center belt asteroid type Calign=center
Xiangliu
bgcolor=blackalign=center align=center moon of (225088) Gonggongalign=center
Dike
bgcolor=blackalign=center align=center belt asteroid type Calign=center [175]
Echeclus
bgcolor=blackalign=center align=center centauralign=center
Desdemona
bgcolor=blackalign=center align=center moon of Uranusalign=center
Eurybates
align=center align=center Jupiter trojan type CPalign=center
Eurynome
bgcolor=blackalign=center align=center belt asteroid type Salign=center [176]
Eurydike
bgcolor=blackalign=center align=center belt asteroid type Malign=center [177]
Halimede
align=center align=center moon of Neptunealign=center
Phocaea
bgcolor=blackalign=center align=center belt asteroid type Salign=center
Naiad
bgcolor=blackalign=center align=center moon of Neptunealign=center
Schwassmann–
Wachmann 1
bgcolor=blackalign=center align=center cometalign=center [178]
Neso
align=center align=center moon of Neptunealign=center
Angelina
bgcolor=blackalign=center align=center belt asteroid type Ealign=center [179]
Pasiphae
align=center align=center moon of Jupiteralign=center
Alkmene
bgcolor=blackalign=center align=center belt asteroid type Salign=center [180]
Nessus
align=center align=center centauralign=center [181]
Polana
bgcolor=blackalign=center align=center belt asteroid type Falign=center [182]
Bianca
bgcolor=blackalign=center align=center moon of Uranusalign=center
Mathilde
bgcolor=blackalign=center align=center belt asteroid type Calign=center [183] [184]
Hidalgo
bgcolor=blackalign=center align=center centauralign=center
Orus
align=center align=center Jupiter trojan type C/type Dalign=center
Amalthea
bgcolor=blackalign=center align=center belt asteroid type S; binaryalign=center
Prospero
align=center align=center moon of Uranusalign=center
Setebos
align=center align=center moon of Uranusalign=center
Carme
align=center align=center moon of Jupiteralign=center
Klytia
bgcolor=blackalign=center align=center belt asteroid type Salign=center [185]
Sao
bgcolor=blackalign=center align=center moon of Neptunealign=center
Echo
bgcolor=blackalign=center align=center belt asteroid type Salign=center [186]
Metis
bgcolor=blackalign=center align=center moon of Jupiteralign=center [187]
Ophelia
bgcolor=blackalign=center align=center moon of Uranusalign=center
Lysithea
bgcolor=blackalign=center align=center moon of Jupiteralign=center
Caliban
align=center align=center moon of Uranusalign=center
Laomedeia
align=center align=center moon of Neptunealign=center
Cordelia
bgcolor=blackalign=center align=center moon of Uranusalign=center
Psamathe
align=center align=center moon of Neptunealign=center

From 1 to 19 km

This list contains some examples of Solar System objects between 1 and 19 km in radius. This is a common size for asteroids, comets and irregular moons.

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
data-sort- type="number" style="width:75px;"Mass
Type – notesRefs
Urda
bgcolor=blackalign=center align=center belt asteroid type Salign=center [188]
Hydra
bgcolor=blackalign=center align=center moon of Plutoalign=center [189] [190]
Siarnaq
align=center align=center moon of Saturnalign=center
Koronis
bgcolor=blackalign=center align=center belt asteroid type Salign=center [191]
Nix
bgcolor=blackalign=center align=center moon of Plutoalign=center
Ganymed
bgcolor=blackalign=center align=center Amor asteroid type Salign=center
Okyrhoe
bgcolor=blackalign=center align=center centauralign=center [192]
Helene
align=center align=center moon of Saturn; Dione trojan align=center
Sinope
align=center align=center moon of Jupiteralign=center
Hippocamp
bgcolor=blackalign=center align=center moon of Neptunealign=center [193]
Leucus
align=center align=center Jupiter trojan type Dalign=center
Stephano
align=center align=center moon of Uranusalign=center
Arrokoth
bgcolor=blackalign=center align=center cubewano
contact binary
align=center [194]
Ida
bgcolor=blackalign=center align=center belt asteroid type S; binaryalign=center [195]
Atlas
bgcolor=blackalign=center align=center moon of Saturnalign=center
Ananke
align=center align=center moon of Jupiteralign=center
Albiorix
bgcolor=blackalign=center align=center moon of Saturnalign=center
Pan
bgcolor=blackalign=center align=center moon of Saturnalign=center [196]
Linus
bgcolor=blackalign=center align=center asteroid moon of 22 Kalliopealign=center [197] [198]
Dioretsa
bgcolor=blackalign=center align=center centaur
damocloid
align=center [199]
Perdita
bgcolor=blackalign=center align=center moon of Uranusalign=center
Telesto
bgcolor=blackalign=center align=center moon of Saturn; Tethys trojan align=center
Mab
bgcolor=blackalign=center align=center moon of Uranusalign=center
Phobos
bgcolor=blackalign=center align=center moon of Marsalign=center [200] [201]
Paaliaq
bgcolor=blackalign=center align=center moon of Saturnalign=center
Francisco
bgcolor=blackalign=center align=center moon of Uranusalign=center
Leda
align=center align=center moon of Jupiteralign=center
Calypso
align=center align=center moons of Saturn; Tethys trojan align=center
Polymele
align=center align=center Jupiter trojan type Palign=center
Margaret
align=center align=center moon of Uranusalign=center
Ferdinand
align=center align=center moon of Uranusalign=center
Cupid
bgcolor=blackalign=center align=center moon of Uranusalign=center
Ymir
align=center align=center moon of Saturnalign=center
Trinculo
bgcolor=blackalign=center align=center moon of Uranusalign=center
Eros
bgcolor=blackalign=center align=center Amor asteroid type Salign=center [202]
Adrastea
bgcolor=blackalign=center align=center moon of Jupiteralign=center
Kiviuq
align=center align=center moon of Saturnalign=center
Tarvos
align=center align=center moon of Saturnalign=center
Kerberos
bgcolor=blackalign=center align=center moon of Plutoalign=center [203] [204]
Gaspra
bgcolor=blackalign=center align=center belt asteroid type Salign=center [205] [206]
Deimos
bgcolor=blackalign=center align=center moon of Marsalign=center [207]
Skamandrios
bgcolor=blackalign=center align=center asteroid moon of 624 Hektoralign=center
Ijiraq
align=center align=center moon of Saturnalign=center
Halley's Comet
align=center align=center cometalign=center [208] [209]
Styx
bgcolor=blackalign=center align=center moon of Plutoalign=center
Romulus
bgcolor=blackalign=center align=center asteroid moon of 87 Sylviaalign=center [210]
Masursky
bgcolor=blackalign=center align=center belt asteroid type Salign=center [211]
Erriapus
align=center align=center moon of Saturnalign=center
Callirrhoe
bgcolor=blackalign=center align=center moon of Jupiteralign=center
Alexhelios
bgcolor=blackalign=center align=center asteroid moon of 216 Kleopatraalign=center [212]
Esclangona
bgcolor=blackalign=center align=center inner belt asteroid type S; binaryalign=center [213]
Themisto
align=center align=center moon of Jupiteralign=center
Daphnis
bgcolor=blackalign=center align=center moon of Saturnalign=center
Petit-Prince
bgcolor=blackalign=center align=center asteroid moon of 45 Eugeniaalign=center [214]
Praxidike
bgcolor=blackalign=center align=center moon of Jupiteralign=center
Bestla
align=center align=center moon of Saturnalign=center
Remus
bgcolor=blackalign=center align=center asteroid moon of 87 Sylviaalign=center
Kalyke
align=center align=center moon of Jupiteralign=center
Cleoselene
bgcolor=blackalign=center align=center asteroid moon of 216 Kleopatraalign=center
S/2019 (31) 1
bgcolor=blackalign=center align=center asteroid moon of 31 Euphrosynealign=center [215]
Tempel 1
bgcolor=blackalign=center align=center Jupiter-family cometalign=center [216]
Phaethon
align=center align=center Apollo asteroid type Falign=center [217]

align=center align=center Apollo asteroid type Xalign=center [218]
Borrelly
bgcolor=blackalign=center align=center Jupiter-family cometalign=center [219]
Šteins
bgcolor=blackalign=center align=center belt asteroid type Ealign=center
Atira
align=center align=center Atira asteroid type S; binaryalign=center [220]
Annefrank
bgcolor=blackalign=center align=center belt asteroid type Salign=center [221]
Balam
bgcolor=blackalign=center align=center belt asteroid type S; trinaryalign=center [222] [223]
Pallene
align=center align=center moon of Saturnalign=center [224]
Florence
align=center align=center Amor asteroid type S; trinaryalign=center [225] [226]
Wild 2
bgcolor=blackalign=center align=center Jupiter family cometalign=center [227]
Litva
bgcolor=blackalign=center align=center Mars-crosser type EU; trinaryalign=center [228]
Churyumov–Gerasimenko
bgcolor=blackalign=center align=center Jupiter-family cometalign=center [229] [230]
Donaldjohanson
bgcolor=blackalign=center align=center belt asteroid type Calign=center [231]
Cuno
align=center align=center Apollo asteroid type S/type Qalign=center [232]

bgcolor=blackalign=center align=center Amor asteroid type Malign=center [233]
Pichi üñëm
bgcolor=blackalign=center align=center asteroid moon of 702 Alaudaalign=center [234]
Toutatis
align=center align=center Apollo asteroid type Salign=center [235]
Methone
bgcolor=blackalign=center align=center moon of Saturnalign=center
Carpo (moon)
align=center align=center Moon of Jupiter

bgcolor=blackalign=center align=center Amor asteroid type S; binaryalign=center [236]
Polydeuces
bgcolor=blackalign=center align=center moon of Saturn; Dione trojan align=center

bgcolor=blackalign=center align=center Amor asteroid type C; trinaryalign=center [237] [238]
S/2003 (1509) 1
bgcolor=blackalign=center align=center asteroid moon of 1509 Esclangonaalign=center [239]
APL
bgcolor=blackalign=center align=center belt asteroid type Salign=center [240]
Camillo
align=center align=center Apollo asteroid type Salign=center
Cruithne
align=center align=center Aten asteroid type Q; quasi-satellite of Earthalign=center [241]

Below 1 km

See also: Satellite and Space debris. This list contains examples of objects below 1 km in radius. That means that irregular bodies can have a longer chord in some directions, hence the mean radius averages out.In the asteroid belt alone there are estimated to be between 1.1 and 1.9 million objects with a radius above 0.5 km,[242] many of which are in the range 0.5–1.0 km. Countless more have a radius below 0.5 km.Very few objects in this size range have been explored or even imaged. The exceptions are objects that have been visited by a probe, or have passed close enough to Earth to be imaged. Radius is by mean geometric radius. Number of digits not an endorsement of significant figures. Mass scale shifts from × 1015 to 109 kg, which is equivalent to one billion kg or 1012 grams (Teragram – Tg).Currently most of the objects of mass between 109 kg to 1012 kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids (NEAs). The Aten asteroid has less mass than the Great Pyramid of Giza, 5.9 × 109 kg.For more about very small objects in the Solar System, see meteoroid, micrometeoroid, cosmic dust, and interplanetary dust cloud. (See also Visited/imaged bodies.)

BodyImagedata-sort- type="number" style="width:85px; font-weight:normal;"Radius
(m)		data-sort- type="number" style="width:75px;"Mass
(109 kg)		Type – notesRefs
Ra-Shalom
bgcolor=blackalign=center align=center Aten asteroid type Calign=center
Geographos
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center
Midas
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center
Mithra
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center

bgcolor=blackalign=center align=center Apollo asteroid type Salign=center
Tantalus
bgcolor=blackalign=center align=center Apollo asteroid type Qalign=center [243]
Braille
bgcolor=blackalign=center align=center Mars-crosser type Qalign=center [244]

align=center align=center Aten asteroid type Salign=center [245]
Apollo
bgcolor=blackalign=center align=center Apollo asteroid type Qalign=center [246]

align=center align=center Aten asteroid type K; contact binaryalign=center [247]
Icarus
align=center align=center Apollo asteroid type Salign=center [248]
Dactyl
bgcolor=blackalign=center align=center asteroid moon of 243 Idaalign=center [249]
Castalia
bgcolor=blackalign=center align=center Apollo asteroid type S; contact binaryalign=center [250]

align=center align=center Apollo asteroid type Qalign=center [251]
Moshup
bgcolor=blackalign=center align=center Aten asteroid type S; binaryalign=center [252] [253]

bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [254] [255]

bgcolor=blackalign=center align=center Apollo asteroidalign=center [256]
Hartley 2
bgcolor=blackalign=center align=center Jupiter-family cometalign=center [257]

align=center align=center Aten asteroid type Salign=center [258]
Nyx
bgcolor=blackalign=center align=center Amor asteroid type Valign=center [259]

bgcolor=blackalign=center align=center Apollo asteroidalign=center [260]
align=center align=center Apollo asteroid type S; binaryalign=center [261]
Ryugu
bgcolor=blackalign=center align=center Apollo asteroid type Cgalign=center [262] [263]

bgcolor=blackalign=center align=center Amor asteroid type Salign=center [264]
align=center align=center Apollo asteroid type S; contact binaryalign=center [265]
Hermes
align=center align=center Apollo asteroid type Sqalign=center [266]
Didymos
bgcolor=blackalign=center align=center Apollo asteroid type Xk; binaryalign=center [267] [268]
Aten
bgcolor=blackalign=center align=center Aten asteroid type Salign=center
Aegaeon
bgcolor=blackalign=center align=center moon of Saturnalign=center
align=center align=center Apollo asteroid type Salign=center [269]

bgcolor=blackalign=center align=center Apollo asteroid type Sq; trinaryalign=center [270] [271]

bgcolor=blackalign=center align=center Amor asteroid type Salign=center [272]
Golevka
bgcolor=blackalign=center align=center Apollo asteroid type Qalign=center [273]
Bennu
bgcolor=blackalign=center align=center Apollo asteroid type Balign=center [274] [275]

bgcolor=blackalign=center align=center Aten asteroid type Xalign=center [276]

bgcolor=blackalign=center align=center Apollo asteroidalign=center [277]
Squannit
bgcolor=blackalign=center align=center align=center
align=center align=center Aten asteroid type Salign=center
bgcolor=blackalign=center align=center Apollo asteroidalign=center

bgcolor=blackalign=center align=center Aten asteroid type X/type Calign=center

align=center align=center Apollo asteroid type S; contact binaryalign=center [278]

bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [279]
bgcolor=blackalign=center align=center Aten asteroid
Earth trojan
align=center [280]

bgcolor=blackalign=center align=center Apollo asteroidalign=center [281]

bgcolor=blackalign=center align=center Apollo asteroid type Calign=center [282]
bgcolor=blackalign=center align=center Apollo asteroid; co-orbital with Earthalign=center [283]
Itokawa
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [284]
Apophis
bgcolor=blackalign=center align=center Aten asteroid type Sqalign=center [285] [286]
S/2009 S 1align=center align=center moon of Saturnalign=center [287]
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [288]

bgcolor=blackalign=center align=center Apollo asteroid type V; binaryalign=center [289]
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [290]
Zoozve
bgcolor=blackalign=center align=center Aten asteroid type X; co-orbital with Venusalign=center [291]

align=center align=center Apollo asteroid type Salign=center [292]
Dimorphos
bgcolor=blackalign=center align=center asteroid moon of 65803 Didymosalign=center
align=center align=center Apollo asteroid type Salign=center [293]
YORP
bgcolor=blackalign=center align=center Apollo asteroid type Salign=center [294]
Kamoʻoalewa
bgcolor=blackalign=center align=center Apollo asteroid type S; quasi-satellite of Earthalign=center [295]
Duende
bgcolor=blackalign=center align=center Aten asteroid type Lalign=center [296]
bgcolor=blackalign=center align=center Apollo asteroid type Xalign=center [297]
bgcolor=blackalign=center align=center Apollo asteroid type E/type Xealign=center [298]
2014 RCbgcolor=blackalign=center align=center Apollo asteroid type Sqalign=center [299]
bgcolor=blackalign=center align=center Apollo asteroidalign=center [300]
2011 MDalign=center align=center Apollo asteroid/Amor asteroid type Salign=center [301]
bgcolor=blackalign=center align=center Apollo asteroid type F/type Malign=center [302]
2023 BUbgcolor=blackalign=center Apollo asteroid[303]
bgcolor=blackalign=center align=center Apollo asteroidalign=center [304]

Gallery

thumb|upright=3|center|Solar system planets, major moons, and 3 stars of different sizes are shown comparatively in three levels of zoom: one for the rocky planets, one for the gas giants, and one for the stars.

See also

Further reading

External links

Notes and References

  1. Web site: The Dwarf Planets . Brown . M. . Caltech . 2008-09-25 . https://web.archive.org/web/20110116181239/http://www.gps.caltech.edu/~mbrown/dwarfplanets/ . 2011-01-16 . live .
  2. Web site: Iapetus' peerless equatorial ridge . The Planetary Society . 2020-01-04.
  3. Web site: Gǃkúnǁ'hòmdímà and Gǃò'é ǃhú . .lowell.edu . 2020-01-04 . 2019-04-07 . https://web.archive.org/web/20190407045339/http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf .
  4. Web site: 2006 . Small Body Density and Porosity: New Data, New Insights . Lunar and Planetary Science XXXVII . D. T. . Britt . G. J. . Consolmagno . W. J. . Merline . 2008-12-16 . https://web.archive.org/web/20081217064607/http://www.lpi.usra.edu/meetings/lpsc2006/pdf/2214.pdf . 2008-12-17 .
  5. Web site: Planetary Satellite Physical Parameters . JPL (Solar System Dynamics) . 2008-10-24 . 2008-12-16.
  6. Web site: Uranian Satellite Fact Sheet . NASA (National Space Science Data Center) . Williams . D. R. . 2007-11-23 . 2008-12-12 . https://web.archive.org/web/20100105183741/http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html . 2010-01-05 . live .
  7. Web site: How many dwarf planets are there in the outer solar system? . . Brown . Michael E. . 28 April 2019.
  8. 10.1038/nature18955. 27487219. 2016Natur.537..515P. A partially differentiated interior for (1) Ceres deduced from its gravity field and shape. 2016. Park. R. S.. Konopliv. A. S.. Bills. B. G.. Rambaux. N.. Castillo-Rogez. J. C.. Raymond. C. A.. Vaughan. A. T.. Ermakov. A. I.. Zuber. M. T.. Fu. R. R.. Toplis. M. J.. Russell. C. T.. Nathues. A.. Preusker. F.. Nature. 537. 7621. 515–517. 4459985.
  9. Web site: Iapetus' peerless equatorial ridge.
  10. Grundy . W.M. . Noll . K.S. . Buie . M.W. . Benecchi . S.D. . Ragozzine . D. . Roe . H.G. . The mutual orbit, mass, and density of transneptunian binary Gǃkúnǁʼhòmdímà . Icarus . December 2019 . 334 . 30–38 . 10.1016/j.icarus.2018.12.037 . 126574999 . https://web.archive.org/web/20190407045339/http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf . 2019-04-07 .
  11. Web site: Uranus Fact Sheet.
  12. Web site: 90377 Sedna . 12 September 2022 . 2023-08-06.
  13. Meftah . M. . Corbard . T. . Hauchecorne . A. . Morand . F. . Ikhlef . R. . Chauvineau . B. . Renaud . C. . Sarkissian . A. . Damé . L. . 2018-08-01 . Solar radius determined from PICARD/SODISM observations and extremely weak wavelength dependence in the visible and the near-infrared . Astronomy & Astrophysics . en . 616 . A64 . 10.1051/0004-6361/201732159 . 2018A&A...616A..64M . 0004-6361.
  14. NASA/JPL, Our Sun, by the numbers Accessed 2020 Oct 22
  15. NASA/JPL Planets and Pluto: Physical Characteristics Last updated 2020-May-29
  16. Web site: By The Numbers Jupiter - NASA Solar System Exploration. NASA.
  17. Web site: By The Numbers Saturn - NASA Solar System Exploration. NASA.
  18. Web site: By The Numbers Uranus - NASA Solar System Exploration. NASA.
  19. Web site: By the Numbers Neptune - NASA Solar System Exploration. NASA.
  20. Web site: By The Numbers Earth - NASA Solar System Exploration. NASA.
  21. Web site: By the Numbers Venus - NASA Solar System Exploration. NASA.
  22. Web site: By The Numbers Mars - NASA Solar System Exploration. NASA.
  23. Web site: By The Numbers Ganymede - NASA Solar System Exploration. NASA.
  24. Web site: By the Numbers Titan - NASA Solar System Exploration. NASA.
  25. Web site: By The Numbers Mercury - NASA Solar System Exploration. NASA.
  26. Web site: By The Numbers Callisto - NASA Solar System Exploration. NASA.
  27. Web site: By The Numbers Io - NASA Solar System Exploration. NASA.
  28. https://ssd.jpl.nasa.gov/?sat_phys_par Planetary Satellite Physical Parameters
  29. https://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html Moon Fact Sheet
  30. Web site: By The Numbers Earth's Moon - NASA Solar System Exploration. NASA.
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