List of Solar System objects by size

Parts-per-million chart of the relative mass distribution of the Solar System, each cubelet denoting 2×10²⁴ kg source ↗

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. 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.

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 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 . 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 3.59×10²⁰ 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 more uncertain 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 Center⁶ and JPL Solar System Dynamics,⁵ give somewhat contradictory size and albedo estimates depending on which research paper is being cited.

Graphical overview

Relative diameters of the fifty largest measured bodies in the Solar System, colored by orbital region. Values are diameters in kilometers. Both scales are linear. source ↗

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 km

The following objects have a nominal volumetric 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).⁷ However, Ceres (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 has no known moons, directly determining its mass (estimated to be from 1.7×10²¹ to 6.1×10²¹ kg¹²) is impossible without sending a probe.

Body^{note 1}	Image	Radius^{note 2}		Volume		Mass		Surface area		Density	Gravity^{note 3}		Type	Discovery
Body^{note 1}	Image	(km)	(R_🜨)	(10⁹ km³)	(V_🜨)	(10²¹ kg)	(M_🜨)	(10⁶ km²)	🜨	(g/cm³)	(m/s²)	(🜨)	Type	Discovery
Sun	source ↗	695700 ± ?¹³	109.2¹⁴	1,409,300,000¹⁴	1,301,000¹⁴	1988475000±92000¹⁵	333,000¹⁴	6,078,700¹⁴	11,918¹⁴	1.409¹⁴	274.0¹⁴	27.94¹⁴	G2V-class star	prehistoric
Jupiter	source ↗	69886±0.4¹⁶	10.97	1,431,280	1,321	1898125±88¹⁷	317.83	61,419¹⁸	120.41	1.3262±0.0003¹⁷	24.79¹⁷	2.528	gas giant planet; has rings	prehistoric
Saturn	source ↗	58232±6¹⁷ (136775 for A Ring)	9.140	827,130	764	568317±26¹⁷	95.162	42,612¹⁹	83.54	0.6871±0.0002¹⁷	10.44¹⁷	1.065	gas giant planet; has rings	prehistoric
Uranus	source ↗	25362±7¹⁷	3.981	68,340	63.1	86809.9±4.0¹⁷	14.536	8083.1²⁰	15.85	1.270±0.001¹⁷	8.69¹⁷	0.886	ice giant planet; has rings	1781
Neptune	source ↗	24622±19¹⁷	3.865	62,540	57.7	102409.2±4.8¹⁷	17.147	7618.3²¹	14.94	1.638±0.004¹⁷	11.15¹⁷	1.137	ice giant planet; has rings	1846
Earth	source ↗	6371.0084±0.0001¹⁷	1	1,083.21	1	5972.17±0.28¹⁷	1	510.06447²²	1	5.5134±0.0003¹⁷	9.81¹⁷	1	terrestrial planet	prehistoric
Venus	source ↗	6051.8±1.0¹⁷	0.9499	928.43	0.857	4867.31±0.23¹⁷	0.815	460.2²³	0.903	5.243±0.003¹⁷	8.87¹⁷	0.905	terrestrial planet	prehistoric
Mars	source ↗	3389.5±0.2¹⁷	0.5320	163.18	0.151	641.691±0.030¹⁷	0.107	144.37²⁴	0.283	3.9340±0.0007¹⁷	3.71¹⁷	0.379	terrestrial planet	prehistoric
Ganymede Jupiter III	source ↗	2634.1±0.3²⁵	0.4135	76.30	0.0704	148.19	0.0248	86.999²⁶	0.171	1.936²⁵	1.428	0.146	moon of Jupiter (icy)	1610
Titan Saturn VI	source ↗	2574.73±0.09²⁷	0.4037^a	71.50	0.0658	134.518±0.003²⁸	0.0225	83.3054²⁹	0.163	1.880±0.004³⁰	1.354	0.138	moon of Saturn (icy)	1655
Mercury	source ↗	2439.4±0.1¹⁷	0.3829	60.83	0.0562	330.103±0.021¹⁷	0.0553	74.797³¹	0.147	5.4289±0.0007¹⁷	3.70¹⁷	0.377	terrestrial planet	prehistoric
Callisto Jupiter IV	source ↗	2410.3±1.5³²	0.3783	58.65	0.0541	107.594	0.018	73.005³³	0.143	1.834±0.003³²	1.23603	0.126	moon of Jupiter (icy)	1610
Io Jupiter I	source ↗	1821.6±0.5⁵	0.2859	25.32	0.0234	89.32	0.015	41.698³⁴	0.082	3.528±0.006³⁵	1.797	0.183	moon of Jupiter (terrestrial)	1610
Moon Earth I	source ↗	1737.4±0.1³⁶	0.2727	21.958	0.0203	73.46³⁷	0.0123	37.937³⁸	0.074	3.344±0.005³⁶	1.625	0.166	moon of Earth (terrestrial)	prehistoric
Europa Jupiter II	source ↗	1560.8±0.5⁵	0.2450	15.93	0.0147	48.00	0.008035	30.613³⁹	0.06	3.013±0.005	1.316	0.134	moon of Jupiter (terrestrial)	1610
Triton Neptune I	source ↗	1353.4±0.9^a²⁷	0.2124^a	10.38	0.0096	21.39±0.03	0.003599	23.018⁴⁰	0.045	2.061	0.782	0.0797	moon of Neptune (icy)	1846
Pluto 134340	source ↗	1188.3±0.8⁴¹	0.187	7.057	0.00651	13.03±0.03	0.0022	17.79	0.034	1.853±0.004⁴²	0.620	0.063	dwarf planet; plutino; multiple	1930
Eris 136199	source ↗	1163±6^b⁴³	0.1825^b	6.59	0.0061	16.38±0.2^c	0.0028	17	0.033	2.43±0.05	0.824	0.083	dwarf planet; SDO; binary	2003
Titania Uranus III	source ↗	788.4±0.6⁴⁶	0.1237^d	2.06	0.0019	3.4550±0.0509⁴⁷	0.00059	7.82⁴⁸	0.015	1.683	0.378	0.0385	moon of Uranus	1787
Haumea 136108	source ↗	772+20 −19⁴⁹	0.12	1.98^e	0.0018	3.95244+0.01109 −0.01103⁵¹	0.00066	8.14	0.016	2.050+0.157 −0.152⁴⁹^f	0.401	0.0409	dwarf planet; resonant KBO (7:12); trinary; has rings	2004
Rhea Saturn V	source ↗	763.5±0.5⁵²	0.1199^d	1.87	0.0017	2.307	0.00039	7.34⁵³	0.014	1.2372±0.0029⁵²	0.26	0.027	moon of Saturn	1672
Oberon Uranus IV	source ↗	761.4±2.6^a²⁷	0.1195^a	1.85	0.0017	3.1104±0.0749⁴⁷	0.0005	7.285⁵⁴	0.014	1.682	0.347	0.035	moon of Uranus	1787
Iapetus Saturn VIII	source ↗	734.4±2.8 ⁵⁵⁵²	0.1153	1.66	0.0015	1.806	0.00033	6.8	0.013	1.0887±0.0127⁵²	0.223	0.0227	moon of Saturn	1671
Makemake 136472	source ↗	715±7⁵⁶	0.112	1.53	0.0014	2.69±0.20⁵⁷^g	0.00045	6.4	0.013	1.76±0.17	0.35	0.0357	dwarf planet; cubewano	2005
Gonggong 225088	source ↗	615±25⁵⁸^g	0.0983	1.03	0.0009	1.75±0.07⁵⁸	0.00029	4.753	0.009	1.74±0.16⁵⁸	0.3	0.0306	dwarf planet; resonant SDO (3:10)	2007
Charon Pluto I	source ↗	606.0±0.5⁴¹	0.0951	0.932	0.0009	1.5897±0.0045⁴²	0.00025	4.578⁵⁹	0.009	1.705±0.006⁴²	0.288	0.0294	moon of Pluto	1978
Umbriel Uranus II	source ↗	584.7±2.8²⁷	0.0918	0.837	0.0008	1.2885±0.0225⁴⁷	0.00020	4.3⁶⁰	0.008	1.539	0.234	0.024	moon of Uranus	1851
Ariel Uranus I	source ↗	578.9±0.6²⁷	0.0909	0.813	0.0007	1.2331±0.0180⁴⁷	0.000226	4.211⁶¹	0.008	1.517	0.269	0.027	moon of Uranus	1851
Dione Saturn IV	source ↗	561.4±0.4⁵⁵⁵²	0.0881	0.741	0.0007	1.0954868±0.0000246⁵²	0.000183	3.965⁶²	0.008	1.478±0.003	0.232	0.0237	moon of Saturn	1684
Quaoar 50000	source ↗	548.8±1.1⁶³	0.0879	0.737	0.0007	1.212±0.005⁶³	0.0002	3.83	0.008	1.751±0.013⁶³	0.3	0.0306	dwarf planet; cubewano; binary; has rings	2002
Tethys Saturn III	source ↗	531.1±0.6⁶⁴⁵²	0.0834	0.624	0.0006	0.6174959±0.0000146⁵²	0.000103	3.57⁶⁵	0.007	0.984±0.003⁶⁴	0.145	0.015	moon of Saturn	1684
Ceres 1	source ↗	469.7±0.1⁶⁶	0.0742	0.433	0.0004	0.938392±0.000005⁶⁷	0.000157	2.85⁶⁸	0.006⁶⁸	2.1616±0.0025⁶⁷	0.28	0.029	dwarf planet; belt asteroid	1801
Orcus 90482	source ↗	455+25 −20⁶⁹	0.0719	0.404	0.0004	0.548±0.010⁴⁵	0.000092			1.4±0.2⁴⁵	0.2	0.0204	dwarf planet; plutino; binary	2004
Sedna 90377	source ↗	453+157 −129⁷⁰	0.0785	0.516	0.0005								dwarf planet; sednoid; detached object	2003
Salacia 120347	source ↗	419±22⁷¹	0.0664	0.373	0.0003	0.4861+0.0076 −0.0074⁷²^g	0.000082			1.5±0.1⁷³	0.185	0.0168	cubewano; binary	2004
star giant planet terrestrial planet dwarf planet possible dwarf planet moon of Earth moon of Jupiter moon of Saturn moon of Uranus moon of Neptune moon of Pluto

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.⁷⁴ 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.¹⁰ Many intrinsically bright TNOs like 2018 VG18 and 2017 OF201 do not have directly measured sizes (e.g. via stellar occultation and radiometry of thermal emission), so their sizes are estimated based on an assumed albedo.⁷⁵ In the list below, TNOs with unmeasured sizes are only listed if they have been mentioned in press releases and the scientific literature.

Body^{note 1}	Image	Radius^{note 2} (km)	Mass (10¹⁸ kg)	Density (g/cm³)	Type^{note 4}	Refs^{note 5} r · M
Máni 307261	source ↗	398±12	–	–	cubewano	⁷⁶
Achlys 208996	source ↗	386±6 (area equivalent)	≈ 200^h	0.87±0.01 (assuming HE)⁷⁹	plutino; binary	⁷⁹
Aya 55565	source ↗	384+19.5 −19	–	–	cubewano	⁸⁰
2010 JO₁₇₉ 574372		≈ 375±75ⁱ	–	–	SDO	⁸¹
Chiminigagua 532037	source ↗	371+39 −41.5	–	–	SDO; binary	⁸²
2017 OF201	source ↗	≈ 350ⁱ	–	–	eTNO	⁸³
Ixion 28978	source ↗	348.390+5.375 −4.435(area equivalent)	–	–	plutino	⁸⁴
2021 DR15	source ↗	345±80ⁱ	–	–	SDO	⁸⁵
Goibniu 90568	source ↗	340±17	–	–	cubewano	⁸⁶
Ritona 145452	source ↗	339.5+27.5 −36.5	–	–	cubewano	⁸⁶
2015 RR245 523794	source ↗	≈ 335ⁱ	–	–	resonant KBO (2:9)	⁸⁷
Uni 55637	source ↗	329.5±19	125±3^g	0.82±0.11	cubewano; binary	⁸⁸ · ⁸⁹
Varuna 20000	source ↗	327+77 −51	≈ 160	0.992+0.086 −0.015⁹⁰	cubewano	⁹¹
2003 UZ₄₁₃ 455502	source ↗	325+0.5 −87.5	≈ 300^j	2.64	plutino	⁹²
Varda 174567	source ↗	324	244±6^h	≈1.9⁴⁹	cubewano; binary	⁴⁹ · ⁹⁴
Rumina 145451	source ↗	≈ 322	–	–	SDO	⁹⁵⁹⁶
Gǃkúnǁʼhòmdímà 229762	source ↗	317+5 −4	136.1±3.3	1.007+0.050 −0.049⁴⁹	SDO; binary	⁴⁹ · ⁹⁷
2014 UZ224 (DeeDee)	source ↗	317.5+28.5 −30.5	–	–	SDO	⁹⁸
2008 OG₁₉ 470599		309.5+28 −56.5ⁱ	–	0.609±0.004	SDO	⁹⁹ · ⁹⁹
Dysnomia Eris I	source ↗	307.5+60 −50	82±57	0.7±0.5	moon of Eris	⁴⁵
2007 JJ₄₃ 278361	source ↗	305+85 −70ⁱ	–	–	cubewano	¹⁰⁰
2004 XR₁₉₀ (Buffy) 612911	source ↗	300±85	–	–	SDO	¹⁰¹
2005 QU₁₈₂ 303775		292+77.5 −72	–	–	SDO	⁹²
2014 EZ₅₁ 523692	source ↗	> 288	–	–	SDO	¹⁰²
Xewioso 78799	source ↗	283+36 −37	–	–	cubewano	¹⁰³
2015 BP₅₁₉ (Caju) 768325		275±75ⁱ			eTNO	¹⁰⁴
Vesta 4	source ↗	262.7±0.1	259.0271±0.0058	3.456±0.035¹⁰⁵	belt asteroid type V	¹⁰⁵ · ¹⁰⁶
2003 VS₂ 84922	source ↗	262±4	–	–	plutino	¹⁰⁷
Pallas 2	source ↗	256±2	204±3	2.92±0.08	belt asteroid type B	¹⁰⁸¹⁰⁹
2004 TY₃₆₄ 120348		256+19 −20	–	–	cubewano	¹¹⁰
2005 TB₁₉₀ 145480	source ↗	253.5+63.5 −58	–	–	detached object	¹¹⁰¹¹¹
Enceladus Saturn II	source ↗	252.1±0.2	108.0±0.1	1.609±0.005	moon of Saturn	⁵⁵ · ¹¹²
2002 TC₃₀₂ 84522	source ↗	250±7	–	–	resonant SDO (2:5)	¹¹³
2018 VG18 (Farout)		≈ 250ⁱ	–	–	resonant SDO (2:9)	¹¹⁴
2005 UQ₅₁₃ 202421		249+32 −38	–	–	cubewano	⁸⁰
Miranda Uranus V	source ↗	235.8±0.7	62.93±3.00	1.148	moon of Uranus	¹¹⁵ · ⁴⁷
Dziewanna 471143	source ↗	235+18 −5	–	–	SDO	¹¹⁶
2002 XV₉₃ 612533	source ↗	235+22 −15	–	–	plutino	¹¹⁷
1999 DE₉ 26375		231±23	–	–	resonant SDO (2:5)	¹¹⁸
2003 FY₁₂₈ 120132		230±11	–	–	SDO	¹¹¹
2012 VP113 (Biden)	source ↗	≈ 225ⁱ	–	–	sednoid	¹¹⁹
2002 VR₁₂₈ 84719		224+24 −22	–	–	plutino	¹²⁰
Vanth Orcus I	source ↗	221±5	87±8	1.5+1.0 −0.5	moon of 90482 Orcus	¹²¹ · ⁴⁵
Hygiea 10	source ↗	216±4	87.4±6.9	2.06±0.20	belt asteroid type C	¹²² · ¹⁰⁹
2004 NT₃₃ 444030		212+44 −40	–	–	cubewano	⁸⁰
Proteus Neptune VIII	source ↗	210±7	15.5–31^k	≈ 0.46–0.91¹²⁴	moon of Neptune	⁵ · ⁵
Chaos 19521	source ↗	208+42 −15 equivalent	–	–	cubewano	¹²⁵
2001 QF₂₉₈ 469372	source ↗	204+20 −22	–	–	plutino	¹²⁰
Huya 38628	source ↗	203±8	40.1	1.073±0.066	plutino; binary	¹²⁶ · ¹²⁷
2004 PF₁₁₅ 175113		203+49 −38	–	–	plutino	¹²⁰
Ilmarë Varda I	source ↗	201.5±20	22	–	moon of 174567 Varda	⁷¹
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), being 200 km nicknamed the "potato radius" by astronomers. The largest of these may have a hydrostatic-equilibrium shape, but most are irregular (i.e., potato-shaped). 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).¹²⁸ Many TNOs are omitted from this list as their sizes are poorly known.⁷⁵

Body^{note 1}	Image	Radius^{note 2} (km)	Mass (10¹⁸ kg)	Type	Refs^{note 5} r · M
2004 UX₁₀ 144897		199+16.3 −19.7	≳ 30	plutino	¹²⁰ · ¹²⁹
1993 SC 15789		199+55 −85.5	≈ 47	plutino	¹³⁰
Mimas Saturn I	source ↗	198.2±0.3	37.49±0.03	moon of Saturn	⁵⁵ · ¹¹²²⁷
1998 SN₁₆₅ 35671		196±20		cubewano	⁸⁰
Actaea Salacia I	source ↗	196.5±16.5	20	moon of 120347 Salacia	⁷¹
2002 KX₁₄ 119951	source ↗	194.6±4.4		cubewano	¹³¹
Hiʻiaka Haumea I	source ↗	185±10	16±2	moon of Haumea	¹³² · ¹³²
2001 UR₁₆₃ 42301	source ↗	176±42.5		resonant KBO (4:9)	¹³³
Nereid Neptune II	source ↗	170±25	35.7	moon of Neptune	²⁷
1996 TL₆₆ 15874		170±10		SDO	¹¹¹
2004 XA₁₉₂ 230965		170+60 −47.5		SDO	¹²⁰
Interamnia 704	source ↗	166±3	35.2±5.1	belt asteroid type F	¹³⁴ · ¹⁰⁹
Europa 52	source ↗	160±2	23.9±3.8	belt asteroid type C	¹⁰⁹
1999 CD₁₅₈ 469306		< 155	≈ 48	resonant KBO (4:7)	¹³⁵
2007 OC₁₀ 470316		165+28 −27.5	≈ 30	SDO	¹³⁶
2023 KQ14 (Ammonite)	source ↗	150±40ⁱ		sednoid	¹³⁷
Davida 511	source ↗	149±2	26.6±7.3	belt asteroid type C	¹⁰⁹
2002 TX₃₀₀ 55636	source ↗	143±5	≈ 11	cubewano, Haumea family	¹³⁸ · ¹³⁸
2003 OP₃₂ 120178		137+23.5 −12.5	≈ 45	cubewano, Haumea family	¹³⁵
Sylvia 87	source ↗	137±2	14.3±0.5	outer belt asteroid type X; trinary	¹⁰⁹
Lempo 47171	source ↗	136±9	6.71	plutino; trinary	¹³⁹
Eunomia 15	source ↗	135±2	30.5±1.9	belt asteroid type S	¹⁰⁹
Hyperion Saturn VII	source ↗	135±4	5.62±0.05	moon of Saturn	⁷⁴ · ⁷⁴²⁷
Euphrosyne 31	source ↗	134±2	16.5±2.6	belt asteroid type C; binary	¹⁰⁹
1998 SM₁₆₅ 26308	source ↗	134±14	6.87±1.8	resonant KBO (1:2)	¹⁴⁰ · ¹⁴⁰
Cybele 65	source ↗	131.5±1.5	14.8±1.8	outer belt asteroid type C	¹⁴¹
Juno 3	source ↗	127±1	27.0±2.4	belt asteroid type S	¹⁰⁹
Hiisi Lempo II	source ↗	126±8	5.273	secondary of 47171 Lempo	¹³⁹
Hektor 624	source ↗	125±13	7.9±1.4	Jupiter trojan (L₄) type D; binary	¹⁴² · ¹⁴²
Chariklo 10199	source ↗	124.8+3.0 −2.3	6.4±0.5	centaur; has rings	¹⁴³
Sila 79360	source ↗	124±15	5.89	cubewano; binary	¹⁴⁴¹⁴⁵
2007 RW₁₀ 309239		124±15		quasi-satellite of Neptune	¹¹¹
Altjira 148780	source ↗	123+19 −70	2.388	cubewano; binary	⁸⁰¹⁴⁶
Nunam 79360	source ↗	118±15	4.892	secondary of 79360 Sila	¹⁴⁴¹⁴⁷
Bamberga 324	source ↗	114±2	10.2±0.9	belt asteroid type C	¹⁰⁹
Patientia 451		112.9±2.3	10.9±5.3	belt asteroid type C	¹⁴⁸ · ¹⁴⁹
Psyche 16	source ↗	112±2	26.2±2.9	belt asteroid type M	¹⁰⁹
Ceto 65489	source ↗	112±5	5.4±0.4	extended centaur; binary	¹¹¹ · ¹⁵⁰
Herculina 532	source ↗	111.2±2.4	10	belt asteroid type S	¹⁵¹
Moon of 148780 Altjira	source ↗	110+17 −62	1.695	secondary of 148780 Altjira	⁸⁰¹⁵²
Hesperia 69	source ↗	110±15	5.86±1.18	belt asteroid type M	¹⁵¹ · ¹⁴⁹¹⁵³
Leleākūhonua 541132		110+14 −10		sednoid	¹⁵⁴
Thisbe 88	source ↗	109±2	11.6±2.2	belt asteroid type B	¹⁰⁹
Doris 48	source ↗	108±2	6.9±2.9	belt asteroid type C	¹⁰⁹
Phoebe Saturn IX	source ↗	106.5±0.7	8.29±0.01	moon of Saturn	⁷⁴ · ⁷⁴²⁷
Moon of 38628 Huya	source ↗	106±15	5.1	moon of 38628 Huya	¹²⁶
Fortuna 19	source ↗	105.5±1.0	8.8±1.4	belt asteroid type G	¹⁰⁹
Camilla 107	source ↗	105±4	11.2±0.3	outer belt asteroid type C; trinary	¹⁴⁸ · ¹⁴⁹
Themis 24	source ↗	104±2	6.2±2.9	belt asteroid type C	¹⁰⁹
Amphitrite 29	source ↗	102±1	12.7±2.0	belt asteroid type S	¹⁰⁹
Egeria 13	source ↗	101±2	9.2±2.1	belt asteroid type G	¹⁰⁹
Iris 7	source ↗	100±5	13.5±2.3	belt asteroid type S	¹⁰⁹
Legend: centaur – asteroids orbiting between the outer planets Jupiter trojan – asteroids located in Jupiter's L₄ and L₅ 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.⁷⁵ Asteroid spectral types are mostly Tholen, but some might be SMASS.

Body^{note 1}	Image	Radius^{note 2} (km)	Mass (10¹⁸ kg)	Type	Refs^{note 5} r · M
Elektra 130	source ↗	99.5±1	6.4±0.2	belt asteroid type G; multiple	¹⁰⁹
Bienor 54598		99+3 −3.5	1.119	centaur	¹⁵⁵¹⁵⁶
Chiron 2060 or 95P	source ↗	98±17		centaur; has rings	¹⁵⁷
Hebe 6	source ↗	97.5±1.5	12.4±2.4	belt asteroid type S	¹⁰⁹
Larissa Neptune VII	source ↗	97±3	≈ 4.2	moon of Neptune	¹⁵⁸ · ^l²⁷
Ursula 375	source ↗	96.8±1.3	8.4±5.3	belt asteroid type C	¹⁶⁰ · ¹⁴⁹
Eugenia 45	source ↗	94±1	5.8±0.1	belt asteroid type F; trinary	¹⁰⁹
Hermione 121	source ↗	94±3	5.0±0.3	outer belt asteroid type C; binary	¹⁶¹ · ¹⁴⁹
Daphne 41	source ↗	94±7	6.1±0.9	belt asteroid type C; binary	¹⁰⁹
Aurora 94	source ↗	93.8±3.6	6.2±3.6	belt asteroid type C	¹⁶² · ¹⁴⁹
Bertha 154	source ↗	93.4±0.9	9.2±5.2	belt asteroid type C	¹⁴⁹ · ¹⁴⁹
1995 SM₅₅ 24835		93.4±0.9		cubewano, Haumea family	¹⁶³
Moon of 532037 Chiminigagua		93+12.5 −13		moon of 532037 Chiminigagua	⁸²
Janus Saturn X	source ↗	89.5±1.4	1.898±0.001	moon of Saturn	⁷⁴ · ⁷⁴
Teharonhiawako 88611	source ↗	89+16 −18	2.44±0.03	cubewano; binary	⁸⁰ · ¹⁶⁴
Aegle 96		88.9±0.8	6.4±6.3	belt asteroid type T	¹⁴⁸ · ¹⁴⁹
Galatea Neptune VI	source ↗	88±4	2.12±0.08	moon of Neptune	¹⁵⁸ · ¹⁶⁵²⁷
S/2015 (136472) 1 (MK2)	source ↗	87.5	4.939	moon of Makemake	¹⁶⁶¹⁶⁷
Phorcys Ceto I	source ↗	87+8 −9	≈ 1.67	secondary of 65489 Ceto	¹⁵⁰ · ¹⁵⁰
Palma 372	source ↗	86.8±1.4	5.2±0.6	belt asteroid type B	¹⁶⁸ · ¹⁴⁹
Metis 9	source ↗	86.5±1	8.0±1.9	belt asteroid type S	¹⁴⁸ · ¹⁴⁹
Alauda 702	source ↗	86±28	6.06±0.36	belt asteroid type C; binary	¹⁶⁸ · ¹⁶⁹
Hilda 153	source ↗	85.3±1.6		outer belt asteroid; Hildas	¹⁵¹
Himalia Jupiter VI	source ↗	85	4.2±0.6	moon of Jupiter	⁵ · ¹⁷⁰
Freia 76	source ↗	84.2±1.0	2.0±4.2	outer belt asteroid type P/type X	¹⁶⁰ · ¹⁴⁹
Amalthea Jupiter V	source ↗	83.45±2.4	2.08±0.15	moon of Jupiter	¹⁷¹ · ¹⁷²²⁷
Agamemnon 911	source ↗	83.3±2.0		Jupiter trojan (L₄) type D	¹⁵¹
Elpis 59		82.6±2.3	3±0.5	belt asteroid type CP/type B	¹⁴⁸ · ¹⁴⁹
Eleonora 354	source ↗	82.5±1.5	7.5±2.7	belt asteroid type A	¹⁰⁹
Weywot Quaoar I	source ↗	≈ 82.5	2.4+1.2 −1.1	moon of Quaoar	⁶³
Nemesis 128	source ↗	81.5±2.5	3.4±1.7	belt asteroid type C	¹⁰⁹
Puck Uranus XV	source ↗	81±2	1.91	moon of Uranus	¹⁷³¹⁷⁴
2002 KW₁₄ 307251		80.5+17.5 −20	≈ 30	cubewano	⁸⁰
Sycorax Uranus XVII	source ↗	78.5+11.5 −7.5		moon of Uranus	¹⁷⁵
Io 85	source ↗	77.4±1.9	2.6±1.5	belt asteroid type FC/type B	¹⁵¹ · ¹⁴⁹
Minerva 93	source ↗	77.08±0.65	3.5±0.4	belt asteroid type C; trinary	¹⁴⁸ · ¹⁴⁹
Alexandra 54	source ↗	77.07±0.32	6.2±3.5	belt asteroid type C	¹⁴⁸ · ¹⁴⁹
Laetitia 39		77±2	4.7±1.1	belt asteroid type S	¹⁴⁹ · ¹⁴⁹
Nemausa 51	source ↗	75±1.5	3.9±1.6	belt asteroid type G	¹⁰⁹
Kalliope 22	source ↗	75±2.5	7.7±0.4	belt asteroid type M; binary	¹⁰⁹
Despina Neptune V	source ↗	75±3	0.71	moon of Neptune	²⁷¹⁷⁶
Namaka Haumea II	source ↗	75±25	1.18±0.25	moon of Haumea	¹⁷⁷ · ⁵¹
Manwë 385446	source ↗	≈ 75	≈ 1.41	resonant KBO (4:7); binary	¹⁷⁸ · ¹⁷⁸
Pales 49		≈ 74.9	4.2±2.2	belt asteroid type C	¹⁵¹ · ¹⁴⁹
Parthenope 11	source ↗	74.5±1	5.5±0.4	belt asteroid type S	¹⁰⁹
Arethusa 95	source ↗	74.0±2.4		belt asteroid type C	¹⁶²
Pulcova 762	source ↗	73.7±0.4	1.4±0.1	belt asteroid type F; binary	¹⁴⁸ · ¹⁷⁹
Flora 8	source ↗	73±1	4.0±1.6	belt asteroid type S	¹⁰⁹
Ino 173	source ↗	72.5±1.5	2.2±1.3	belt asteroid type Xc	¹⁰⁹
Adeona 145	source ↗	72±1.5	2.4±0.3	belt asteroid type Xc	¹⁰⁹
Irene 14	source ↗	72±1	2.9±1.9	belt asteroid type S	¹⁶⁰ · ¹⁴⁹
Gǃòʼé ǃHú Gǃkúnǁʼhòmdímà I	source ↗	71±4		secondary of 229762 Gǃkúnǁʼhòmdímà	¹⁸⁰
Aglaja 47		71±4	3.2±1.7	belt asteroid type C	¹⁴⁹ · ¹⁴⁹
Melpomene 18	source ↗	70.5±1	4.5±0.9	belt asteroid type S	¹⁰⁹
Lamberta 187	source ↗	70.5±1	1.9±0.3	belt asteroid type Ch	¹⁰⁹
Patroclus 617	source ↗	70.2±0.4	1.36±0.11	Jupiter trojan (L₅) type P; binary	¹⁴⁸ · ¹⁴⁹
Julia 89	source ↗	70±1.4	4.3±3.2	belt asteroid type S	¹⁰⁹
Typhon 42355	source ↗	69±4.5	0.87±0.03	resonant SDO (7:10); binary	¹⁵⁵ · ¹⁸¹
ǂKá̦gára 469705	source ↗	69±12	1.29±0.07	cold classical KBO; binary	¹⁸²
Massalia 20	source ↗	67.8±1.8	5±1.04	belt asteroid type S	¹⁶⁸ · ¹⁴⁹
Portia Uranus XII	source ↗	67.6±4		moon of Uranus	⁵
Emma 283	source ↗	66.2±0.1	1.38±0.03	belt asteroid type X; binary	¹⁴⁸ · ¹⁴⁹
Paha Lempo I	source ↗	66+4 −4.5	0.746±0.001	moon of 47171 Lempo	¹³⁹ · ¹⁸³
Lucina 146	source ↗	65.9±?		belt asteroid type C	¹⁸⁴
Sawiskera Teharonhiawako I	source ↗	65.5+12 −13		secondary of 88611 Teharonhiawako	⁸⁰
Achilles 588	source ↗	65.0±0.3		Jupiter trojan (L₄) type DU	¹⁴⁸
Panopaea 70		64.0±0.4	4.33±1.09	belt asteroid type C	¹⁴⁸ · ¹⁴⁹
Thule 279		63.3±1.8		outer belt asteroid type D	¹⁵¹
Borasisi 66652	source ↗	63+12.5 −25.5	3.433±0.027	cubewano; binary	⁸⁰ · ¹⁸⁵
Albion 15760		≈ 62.5ⁱ		TNO, first KBO discovered
Hestia 46		62.07±1.7	3.5	belt asteroid type P/type Xc	¹⁵¹ · ¹⁸⁶
Leto 68	source ↗	61.3±1.6	3.28±1.9	belt asteroid type S	¹⁴⁸ · ¹⁴⁹
ǃHãunu ǂKá̦gára I	source ↗	61±9	0.89±0.05	secondary of 469705 ǂKá̦gára	¹⁸⁷
Undina 92		60.46±0.85	4.43±0.25	belt asteroid type X	¹⁶⁰ · ¹⁴⁹
Bellona 28	source ↗	60.45±1.90	2.62±0.15	belt asteroid type S	¹⁸⁸ · ¹⁴⁹
Diana 78		60.30±1.35	1.27±0.13	belt asteroid type C	¹⁸⁹ · ¹⁴⁹
Anchises 1173	source ↗	60.2±1.5		Jupiter trojan (L₅) type P	¹⁶⁰
Bernardinelli-Bernstein C/2014 UN₂₇₁	source ↗	60±7		comet	¹⁹⁰
Galatea 74		59.4±1.4	6.13±5.36	belt asteroid type C	¹⁹¹ · ¹⁴⁹
Deiphobus 1867		59.1±0.8		Jupiter trojan (L₅) type D	¹⁹²
Äneas 1172		59.01±0.40		Jupiter trojan (L₅) type D	¹⁹³
Kleopatra 216	source ↗	59±1	3.0±0.3	belt asteroid type M; trinary	¹⁰⁹
Athamantis 230	source ↗	59±1	2.3±1.1	belt asteroid type S	¹⁰⁹
Diomedes 1437	source ↗	58.89±0.59		Jupiter trojan (L₄) type D	¹⁹⁴
Terpsichore 81		58.9±0.4	6.19±5.31	belt asteroid type C	¹⁹⁵ · ¹⁴⁹
Epimetheus Saturn XI	source ↗	58.1±1.8	0.5266±0.0006	moon of Saturn	⁷⁴ · ⁷⁴
Victoria 12	source ↗	58±1	2.7±1.3	belt asteroid type S	¹⁰⁹
Circe 34	source ↗	57.7±1.0	≈ 3.66±0.03	belt asteroid type C	¹⁴⁸ · ¹⁴⁹
Leda 38	source ↗	57.7±0.7	5.71±5.47	belt asteroid type C	¹⁴⁹ · ¹⁴⁹
Odysseus 1143		57.3±0.3		Jupiter trojan (L₄) type D	¹⁹⁶
Alcathous 2241		56.8±0.9		Jupiter trojan (L₅) type D	¹⁹⁷
Melete 56	source ↗	56.62±0.85	4.61	belt asteroid type P	¹⁵¹ · ¹⁴⁹
Mnemosyne 57		56.3±1.4	≈ 12.6±2.4	belt asteroid type S	¹⁹⁸ · ¹⁴⁹
Nestor 659		56.2±0.9		Jupiter trojan (L₄) type XC	¹⁹⁹
Harmonia 40	source ↗	55.6±0.2		belt asteroid type S	²⁰⁰
Euterpe 27	source ↗	54.9±0.8	1.67±1.01	belt asteroid type S	¹⁶⁰ · ¹⁴⁹
Antilochus 1583		54.4±0.3		Jupiter trojan (L₄) type D	¹⁴⁸
Thorondor Manwë I	source ↗	54	0.5	secondary of 385446 Manwë	¹⁷⁸ · ¹⁷⁸
Thalia 23	source ↗	53.8±1.1	1.96±0.09	belt asteroid type S	²⁰¹ · ¹⁴⁹
Erato 62	source ↗	53.5±0.3		belt asteroid type BU/type Ch	²⁰²
Astraea 5	source ↗	53.3±1.6	2.9	belt asteroid type S	²⁰³ · ¹⁸⁶
Pabu Borasisi I	source ↗	52.5+10 −21		secondary of 66652 Borasisi	⁸⁰
Eos 221		51.76±2.8	≈ 5.87±0.34	belt asteroid type S/type K	¹⁴⁹ · ¹⁴⁹
Aegina 91		51.7±0.2		belt asteroid type C	²⁰⁴
Leukothea 35	source ↗	51.5±0.6		belt asteroid type C	²⁰⁵
Menoetius Patroclus I	source ↗	51.4±0.25		secondary of 617 Patroclus	²⁰⁶
Isis 42	source ↗	51.4±1.4	1.58±0.52	belt asteroid type S	¹⁴⁹ · ¹⁴⁹
Klotho 97	source ↗	50.4±0.3	1.33±0.13	belt asteroid type M	¹⁴⁸ · ¹⁴⁹
Troilus 1208	source ↗	50.3±0.5		Jupiter trojan (L₅) type FCU	²⁰⁷

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.²⁰⁸ 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.¹⁴⁹²⁰⁹

Body^{note 1}	Image	Radius^{note 2} (km)	Mass (10¹⁵ kg)	Type – notes	Refs^{note 5} r · M
Asterope 233		49.8±0.6		belt asteroid type T/type K	²¹⁰
Pholus 5145		49.5+7.5 −7		centaur	¹⁵⁵
Thebe Jupiter XIV	source ↗	49.3±2		moon of Jupiter	¹⁷¹
Lutetia 21	source ↗	49±1	1700±20	belt asteroid type M	¹⁰⁹
Kalypso 53	source ↗	48.631±13.299	≈ 5630±5000	belt asteroid type XC	²¹¹ · ¹⁴⁹
Notburga 626	source ↗	48.42±2.335		belt asteroid type XC	¹⁴⁹
Proserpina 26	source ↗	47.4±0.85	748±895	belt asteroid type S	²¹² · ¹⁴⁹
Juliet Uranus XI	source ↗	46.8±4		moon of Uranus	⁵
Urania 30	source ↗	44±1	1300±900	belt asteroid type S	¹⁰⁹
Ausonia 63	source ↗	46.5±1.5	1200±200	belt asteroid type S	¹⁰⁹
Beatrix 83		44.819±1.326		belt asteroid type X	¹⁴⁸
Concordia 58		44.806±0.419		belt asteroid type C	¹⁴⁸
Echidna Typhon I	source ↗	44.5±3		moon of 42355 Typhon	¹⁸¹
Automedon 2920		44.287±0.898		Jupiter trojan (L₄) type D	²¹³
Antiope 90		43.9±0.5	828±22	belt asteroid type C; binary	²¹⁴ · ²¹⁴
Prometheus Saturn XVI	source ↗	43.1±2.7	159.5±1.5	moon of Saturn	⁷⁴ · ⁷⁴
Danaë 61		42.969±1.076	2890±2780	belt asteroid type S	²¹⁵ · ¹⁴⁹
Thetis 17	source ↗	42.449±1.014	1200	belt asteroid type S	²¹⁶ · ²⁰⁹
Pandora 55	source ↗	42.397±1.251		belt asteroid type M	²¹⁷
Huenna 379		42.394±0.779	383±19	belt asteroid type B/type C; binary	²¹⁸ · ²¹⁹
Virginia 50		42.037±0.121	2310±700	belt asteroid type X/type Ch	²²⁰ · ¹⁴⁹
Feronia 72	source ↗	41.975±2.01	≈ 3320±8490	belt asteroid type TDG	¹⁴⁹ · ¹⁴⁹
S/2000 (90) 1 Antiope I		41.9±0.5		secondary of 90 Antiope	²¹⁴
Poulydamas 4348		41.016±0.313		Jupiter trojan (L₅) type C	²²¹
Logos 58534	source ↗	41±9	458±6.9	cubewano; binary	²²² · ²²²
Pandora Saturn XVII	source ↗	40.7±1.5	137.1±1.9	moon of Saturn	⁷⁴ · ⁷⁴
Thalassa Neptune IV	source ↗	40.7±2.8		moon of Neptune	¹⁵⁸
Niobe 71	source ↗	40.43±0.4		belt asteroid type S	¹⁶⁰
Pomona 32	source ↗	40.38±0.8		belt asteroid type S	²²³
Belinda Uranus XIV	source ↗	40.3±8		moon of Uranus	⁵
Elara Jupiter VII	source ↗	39.95±1.7		moon of Jupiter	²²⁴
Cressida Uranus IX	source ↗	39.8±2		moon of Uranus	⁵
Amycus 55576		38.15±6.25		centaur	¹¹⁸
Hylonome 10370	source ↗	37.545		centaur	²²⁵
Socus 3708		37.831±0.404		Jupiter trojan (L₅) type C	¹⁴⁸
Nysa 44	source ↗	37.83±0.37		belt asteroid type E	¹⁶⁰
Rosalind Uranus XIII	source ↗	36±6		moon of Uranus	⁵
Maja 66	source ↗	35.895±0.46		belt asteroid type C	¹⁶⁰
Ariadne 43	source ↗	35.67±0.627	≈ 1210±220	belt asteroid type S	²²⁶ · ¹⁴⁹
Iphigenia 112		35.535±0.26	≈ 1970±6780	belt asteroid type C	¹⁴⁹ · ¹⁴⁹
Xiangliu Gonggong I		≈ 35±15		moon of 225088 Gonggong
Dike 99	source ↗	33.677±0.208		belt asteroid type C	²²⁷
Echeclus 60558 or 174P		32.3±0.8		centaur	¹⁵⁵
Desdemona Uranus X	source ↗	32±4		moon of Uranus	⁵
Eurybates 3548	source ↗	31.943±0.149		Jupiter trojan (L₄) type CP	¹⁴⁸
Eurynome 79	source ↗	31.739±0.476		belt asteroid type S	²²⁸
Eurydike 75		31.189±0.802		belt asteroid type M	²²⁹
Halimede Neptune IX	source ↗	≈ 31		moon of Neptune	⁵
Phocaea 25	source ↗	30.527±1.232	599±60	belt asteroid type S	¹⁴⁸ · ¹⁴⁹
Naiad Neptune III	source ↗	30.2±3.2		moon of Neptune	¹⁵⁸
Schwassmann– Wachmann 1 29P	source ↗	30.2±3.7		comet	²³⁰
Neso Neptune XIII	source ↗	≈ 30		moon of Neptune	⁵
Angelina 64	source ↗	29.146±0.541		belt asteroid type E	²³¹
Pasiphae Jupiter VIII	source ↗	28.9±0.4		moon of Jupiter	²²⁴
Alkmene 82	source ↗	28.811±0.357		belt asteroid type S	²³²
Nessus 7066	source ↗	28.5±8.5		centaur	¹⁵⁵
Polana 142		27.406±0.139		belt asteroid type F	²³³
Bianca Uranus VIII	source ↗	27±2		moon of Uranus	⁵
Mathilde 253	source ↗	26.4	103.3±4.4	belt asteroid type C	²³⁴ · ²³⁵
Hidalgo 944	source ↗	26.225±1.8		centaur	¹⁶⁰
Orus 21900	source ↗	25.405±0.405		Jupiter trojan (L₄) type C/type D	¹⁴⁸
Amalthea 113		25.069±0.633		belt asteroid type S; binary	¹⁴⁸
Prospero Uranus XVIII	source ↗	≈ 25		moon of Uranus	⁵
Setebos Uranus XIX	source ↗	≈ 24		moon of Uranus	⁵
Carme Jupiter XI	source ↗	23.35±0.45		moon of Jupiter	²²⁴
Klytia 73	source ↗	22.295±0.471		belt asteroid type S	²³⁶
Sao Neptune XI	source ↗	≈ 22		moon of Neptune	⁵
Echo 60	source ↗	21.609±0.286	315±32	belt asteroid type S	²³⁷ · ¹⁴⁹
Metis Jupiter XVI	source ↗	21.5±2	≈ 119.893	moon of Jupiter	¹⁷¹ · ²³⁸
Ophelia Uranus VII	source ↗	21.4±4		moon of Uranus	⁵
Lysithea Jupiter X	source ↗	21.1±0.35		moon of Jupiter	²²⁴
Caliban Uranus XVI	source ↗	21+10 −6		moon of Uranus	¹⁷⁵
Laomedeia Neptune XII	source ↗	≈ 21		moon of Neptune	⁵
Cordelia Uranus VI	source ↗	20.1±3		moon of Uranus	⁵
Psamathe Neptune X	source ↗	≈ 20		moon of Neptune	⁵

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.

Body^{note 1}	Image	Radius^{note 2} (km)	Mass (10¹⁵ kg)	Type – notes	Refs^{note 5} r · M
Urda 167	source ↗	19.968±0.132		belt asteroid type S	²³⁹
Hydra Pluto III	source ↗	19.65	48±42	moon of Pluto	²⁴⁰ · ²⁴¹
Siarnaq Saturn XXIX	source ↗	19.65±2.95		moon of Saturn	²²⁴
Koronis 158	source ↗	19.513±0.231		belt asteroid type S	²⁴²
Nix Pluto II	source ↗	19.017	45±40	moon of Pluto	²⁴⁰ · ²⁴¹
Ganymed 1036	source ↗	18.838±0.199	≈ 167±318	Amor asteroid type S	¹⁴⁸ · ¹⁴⁹
Okyrhoe 52872		18±0.6		centaur	²⁴³
Blarney 2320		18		belt asteroid	²⁴⁴
Helene Saturn XII	source ↗	17.6±0.4		moon of Saturn; Dione trojan (L₄)	⁷⁴
Sinope Jupiter IX	source ↗	17.5±0.3		moon of Jupiter	²²⁴
Hippocamp Neptune XIV	source ↗	17.4±1	≈ 50	moon of Neptune	¹⁵⁸ · ¹⁵⁸
Leucus 11351	source ↗	17.078±0.323		Jupiter trojan (L₄) type D	¹⁴⁸
Stephano Uranus XX	source ↗	≈ 16		moon of Uranus	⁵
Arrokoth 486958	source ↗	15.85±0.25		cubewano; contact binary	²⁴⁵
Ida 243	source ↗	15.7	42±6	belt asteroid type S; binary	²⁴⁶ · ²⁴⁷
Atlas Saturn XV	source ↗	15.1±0.9	6.6	moon of Saturn	⁷⁴ · ⁷⁴
Great comet C/1811 F1	source ↗	15 - 20		comet	²⁴⁸
Ananke Jupiter XII	source ↗	14.55±0.3		moon of Jupiter	²²⁴
Albiorix Saturn XXVI	source ↗	14.3±2.7		moon of Saturn	²²⁴
Linus Kalliope I		14±1	≈ 60	asteroid moon of 22 Kalliope	²⁴⁹ · ²⁵⁰
Dioretsa 20461		14±3		centaur; damocloid	²⁵¹
Pan Saturn XVIII	source ↗	13.7±0.3	4.30±0.22	moon of Saturn	²⁵² · ²⁵²
Perdita Uranus XXV	source ↗	13±1		moon of Uranus	⁵
Telesto Saturn XIII	source ↗	12.4±0.4		moon of Saturn; Tethys trojan (L₄)	⁷⁴
Mab Uranus XXVI	source ↗	12±1		moon of Uranus	⁵
Phobos Mars I	source ↗	11.1±0.15	10.659	moon of Mars	²⁵³ · ²⁵⁴
Paaliaq Saturn XX	source ↗	≈ 11		moon of Saturn	⁵
Francisco Uranus XXII		≈ 11		moon of Uranus	⁵
Leda Jupiter XIII	source ↗	10.75±0.85		moon of Jupiter	²²⁴
Calypso Saturn XIV	source ↗	10.7±0.7		moons of Saturn; Tethys trojan (L₅)	⁷⁴
Polymele 15094	source ↗	10.548±0.068		Jupiter trojan (L₄) type P	¹⁵¹
Margaret Uranus XXIII	source ↗	≈ 10		moon of Uranus	⁵
Ferdinand Uranus XXIV	source ↗	≈ 10		moon of Uranus	⁵
Cupid Uranus XXVII	source ↗	9±1		moon of Uranus	⁵
Ymir Saturn XIX	source ↗	≈ 9		moon of Saturn	⁵
Trinculo Uranus XXI		≈ 9		moon of Uranus	⁵
Eros 433	source ↗	8.42±0.02	6.687±0.003	Amor asteroid type S	²⁵⁵ · ²⁵⁵
Adrastea Jupiter XV	source ↗	8.2±2		moon of Jupiter	⁵
Kiviuq Saturn XXIV	source ↗	≈ 8		moon of Saturn	⁵
Tarvos Saturn XXI	source ↗	≈ 7.5		moon of Saturn	⁵
Kerberos Pluto IV	source ↗	≈ 6.333	16±9	moon of Pluto	²⁵⁶ · ²⁵⁷
Gaspra 951	source ↗	6.266	20–30	belt asteroid type S	²⁵⁸ · ²⁵⁹
Deimos Mars II	source ↗	6.27±0.07	1.51	moon of Mars	²⁶⁰ · ²⁶⁰
Skamandrios Hektor I		6±1.5		asteroid moon of 624 Hektor	¹⁴²
Ijiraq Saturn XXII	source ↗	≈ 6		moon of Saturn	⁵
Tsuchinshan–ATLAS C/2023 A3	source ↗	<5.9±0.2		comet	²⁶¹
Halley's Comet 1P	source ↗	5.75	0.22	comet	²⁶² · ²⁶³
Styx Pluto V	source ↗	≈ 5.5	≈ 7.65	moon of Pluto	²⁵⁶ · ²⁵⁷
Romulus Sylvia I	source ↗	5.4±2.8		asteroid moon of 87 Sylvia	²⁶⁴
Masursky 2685	source ↗	5.372±0.085		belt asteroid type S	²⁶⁵
Erriapus Saturn XXVIII	source ↗	≈ 5		moon of Saturn	⁵
Callirrhoe Jupiter XVII	source ↗	4.8±0.65		moon of Jupiter	²²⁴
Alexhelios Kleopatra I	source ↗	4.45±0.8		asteroid moon of 216 Kleopatra	²⁶⁶
Esclangona 1509		4.085±0.3		inner belt asteroid type S; binary	²⁶⁷
Themisto Jupiter XVIII	source ↗	≈ 4		moon of Jupiter	⁵
Daphnis Saturn XXXV	source ↗	3.8±0.8	0.077±0.015	moon of Saturn	⁷⁴ · ⁷⁴
Petit-Prince Eugenia I		3.5±1		asteroid moon of 45 Eugenia	²⁶⁸
Praxidike Jupiter XXVII	source ↗	3.5±0.35		moon of Jupiter	²²⁴
Bestla Saturn XXXIX	source ↗	≈ 3.5		moon of Saturn	⁵
Remus Sylvia II	source ↗	≈ 3.5		asteroid moon of 87 Sylvia	²⁶⁴
Kalyke Jupiter XXIII	source ↗	3.45±0.65		moon of Jupiter	²²⁴
Cleoselene Kleopatra II	source ↗	3.45±0.8		asteroid moon of 216 Kleopatra	²⁶⁶
Moon of 31 Euphrosyne		3.35±1.2		asteroid moon of 31 Euphrosyne	²⁶⁹
Tempel 1 9P	source ↗	3±0.1		Jupiter-family comet; Deep Impact flyby and impacted	²⁷⁰
Ireland 5029		3		belt asteroid	²⁷¹
Phaethon 3200	source ↗	2.9		Apollo asteroid type F	²⁷²
1999 JM₈ 53319	source ↗	2.7±0.6		Apollo asteroid type X	²⁷³
Borrelly 19P	source ↗	2.66		Jupiter-family comet	²⁷⁴
Šteins 2867	source ↗	2.58±0.084		belt asteroid type E	¹⁴⁸
Atira 163693	source ↗	2.4±0.25		Atira asteroid type S; binary	²⁷⁵
Annefrank 5535	source ↗	2.4		belt asteroid type S	²⁷⁶
Balam 3749	source ↗	2.332±0.107	0.51±0.02	belt asteroid type S; trinary	²⁷⁷ · ²⁷⁸
Pallene Saturn XXXIII	source ↗	2.22±0.07		moon of Saturn	²⁷⁹
Florence 3122	source ↗	2.201±0.015	0.079±0.002	Amor asteroid type S; trinary	¹⁶² · ²⁸⁰
Wild 2 81P	source ↗	2.133		Jupiter family comet	²⁸¹
Litva 2577		2.115		Mars-crosser type EU; trinary	²⁸²
Churyumov–Gerasimenko 67P	source ↗	2	0.00998	Jupiter-family comet	²⁸³ · ²⁸⁴
Donaldjohanson 52246	source ↗	1.948±0.007		belt asteroid type C	²⁸⁵
Camelot 9500		1.9		belt asteroid	²⁸⁶
Cuno 4183	source ↗	1.826±0.051		Apollo asteroid type S/type Q	²⁸⁷
1986 DA 6178		1.575		Amor asteroid type M	²⁸⁸
Pichi üñëm Alauda I		1.55±0.45		asteroid moon of 702 Alauda	²⁸⁹
Toutatis 4179	source ↗	1.516	0.0505	Apollo asteroid type S	²⁹⁰ · ²⁹⁰
Kaʻepaokaʻāwela 514017		1.5		Jupiter trojan	²⁹¹
Methone Saturn XXXII	source ↗	1.45±0.03		moon of Saturn	²⁷⁹
Carpo Jupiter XLVI		1.44		Moon of Jupiter
Gault 6478	source ↗	1.4+0.2 −0.1		Phocaea asteroid type S	²⁹²
1998 QE₂ 285263	source ↗	1.375		Amor asteroid type S; binary	²⁹³
Polydeuces Saturn XXXIV	source ↗	1.3±0.4		moon of Saturn; Dione trojan (L₅)	⁷⁴
2001 SN₂₆₃ 153591	source ↗	1.315±0.2	0.00951±0.00013	Amor asteroid type C; trinary	²⁹⁴ · ²⁹⁵
S/2003 (1509) 1 Moon of 1509 Esclangona		1.285		asteroid moon of 1509 Esclangona	²⁹⁶
APL 132524	source ↗	≈ 1.25		belt asteroid type S	²⁹⁷
Camillo 3752	source ↗	1.153±0.044		Apollo asteroid type S	¹⁶²
Cruithne 3753	source ↗	1.036±0.053		Aten asteroid type Q; quasi-satellite of Earth	²⁹⁸
1996 HW1 8567	source ↗	1.01		Amor asteroid	²⁹⁹

Below 1 km

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,³⁰⁰ 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 1994 WR₁₂ 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.)

Object	Image	Radius^{note 2} (m)	Mass (10⁹ kg)	Type – notes	Refs^{note 5} r · M
Ra-Shalom 2100	source ↗	990±25		Aten asteroid type C	¹⁶⁰
Geographos 1620	source ↗	980±30		Apollo asteroid type S	¹⁴⁸
Midas 1981	source ↗	975±35		Apollo asteroid type S	¹⁶⁰
Mithra 4486	source ↗	924.5±11		Apollo asteroid type S	¹⁶²
2006 VW₁₃₉ 300163	source ↗	900±0.1		Active asteroid	³⁰¹
1998 OH 12538		831.5±164.5		Apollo asteroid type S	¹⁶²
Tantalus 2102	source ↗	824.5±22.5		Apollo asteroid type Q	³⁰²
Braille 9969	source ↗	820		Mars-crosser type Q	³⁰³
2005 GO₂₁ 308242	source ↗	780		Aten asteroid type S	³⁰⁴
Apollo 1862	source ↗	≈ 750		Apollo asteroid type Q	³⁰⁵
1999 JD₆ 85989	source ↗	731±10.5		Aten asteroid type K; contact binary	³⁰⁶
Icarus 1566	source ↗	730		Apollo asteroid type S	³⁰⁷
Dactyl Ida I	source ↗	700		asteroid moon of 243 Ida	³⁰⁸
Castalia 4769		700		Apollo asteroid type S; contact binary	³⁰⁹
2007 PA₈ 214869	source ↗	675±70		Apollo asteroid type Q	³¹⁰
Moshup 66391	source ↗	658.5±20	2490±54	Aten asteroid type S; binary	³¹¹ · ³¹²
1950 DA 29075	source ↗	653	≈ 2000	Apollo asteroid type S	³¹³ · ³¹⁴
2006 HY₅₁ 394130		609±114		Apollo asteroid	³¹⁵
Hartley 2 103P	source ↗	570±80	≈ 300	Jupiter-family comet	³¹⁶ · ³¹⁶
2003 SD₂₂₀ 163899	source ↗	515		Aten asteroid type S	³¹⁷
Nyx 3908	source ↗	500±75		Amor asteroid type V	³¹⁸
Wikipedia 274301		475		Vestian asteroid	³¹⁹ · ³²⁰
Astronautica 100000		470		Hungaria asteroid type E	³¹⁹ · ³²⁰
2001 WN₅ 153814		466±5.5		Apollo asteroid	³²¹
2017 YE5	source ↗	450±25		Apollo asteroid type S; binary	³²²
Ryugu 162173	source ↗	432.5±7.5	≈ 450	Apollo asteroid type Cg	³²³ · ³²⁴
1997 AE₁₂ 162058		423.5±6.5		Amor asteroid type S	³²⁵
2014 JO₂₅ 671294	source ↗	409		Apollo asteroid type S; contact binary	³²⁶
Hermes 69230	source ↗	400±50		Apollo asteroid type Sq	³²⁷
Didymos 65803	source ↗	390±4	527	Apollo asteroid type Xk; binary	³²⁸ · ³²⁹
Dinkinesh 152830	source ↗	369		belt asteroid type Sq	³³⁰
Aten 2062		365±15		Aten asteroid type S	¹⁴⁸
Aegaeon Saturn LIII	source ↗	330±60		moon of Saturn	²⁷⁹
2015 TB145	source ↗	325±15		Apollo asteroid type S	³³¹
2001 WR₁ 172034		315.5±9		Amor asteroid type S	³³²
1994 CC 136617	source ↗	310±30	266±32.9	Apollo asteroid type Sq; trinary	³³³ · ³³⁴
LINEAR 252P	source ↗	300±30		Jupiter-family comet	³³⁵
Golevka 6489	source ↗	265±15		Apollo asteroid type Q	³³⁶
ATLAS 3I	source ↗	260 - 374		Interstellar comet	³³⁷
2000 WO₁₀₇ 153201	source ↗	255±41.5		Aten asteroid type X	³³⁸
Bennu 101955	source ↗	245.03±0.08	78±9	Apollo asteroid type B	³³⁹ · ³⁴⁰
Torifune 98943		232.5±7.5		Apollo asteroid	³⁴¹
2002 CU₁₁ 163132		230±8.5		Apollo asteroid	³⁴²
Squannit Moshup I	source ↗	225.5±13.5		asteroid moon of 66391 Moshup	³¹²
2014 HQ124	source ↗	204.5±84		Aten asteroid type S	¹⁴⁸
2013 YP139	source ↗	201±13		Apollo asteroid	³⁴³
2008 EV₅ 341843	source ↗	200±7		Aten asteroid type X/type C	¹⁶²
2006 DP₁₄ 388188	source ↗	≈ 200		Apollo asteroid type S; contact binary	³⁴⁴
1988 EG 6037		199.5±1.35		Apollo asteroid type S	³⁴⁵
2010 TK₇ 706765	source ↗	189.5±61.5		Aten asteroid; Earth trojan (L₄)	³⁴⁶
2006 SU₄₉ 292220		≈ 188.5	≈ 73	Apollo asteroid	³⁴⁷ · ³⁴⁷
2005 YU₅₅ 308635	source ↗	180±20		Apollo asteroid type C	³⁴⁸
2010 SO₁₆ 419624		178.5±63		Apollo asteroid; co-orbital with Earth	³⁴³
Itokawa 25143	source ↗	173	35.1±1.05	Apollo asteroid type S	³⁴⁹ · ³⁴⁹
Nereus 4660	source ↗	165		Apollo asteroid	³⁵⁰
Apophis 99942	source ↗	162.5±7.5	≈ 61	Aten asteroid type Sq	³⁵¹ · ³⁵²
S/2009 S 1	source ↗	≈ 150		moon of Saturn	³⁵³
2005 WK₄ 277475	source ↗	142		Apollo asteroid type S	³⁵⁴
2004 BL₈₆ 357439	source ↗	131.5±13		Apollo asteroid type V; binary	³⁵⁵
2007 TU24	source ↗	125		Apollo asteroid type S	³⁵⁶
Zoozve 524522		≈ 118		Aten asteroid type X; co-orbital with Venus	³⁵⁷
2011 UW₁₅₈ 436724	source ↗	110±20		Apollo asteroid type S	³⁵⁸
Hathor 2340		105±0.015		Aten asteroid type S	³⁵⁹
Dimorphos Didymos I	source ↗	85±15		asteroid moon of 65803 Didymos	³²⁹
Cardea 164207	source ↗	81.5		Apollo asteroid; quasi-satellite of Earth	³⁶⁰
2017 BQ6	source ↗	78		Apollo asteroid type S	³⁶¹
1994 WR12		65		Aten asteroid	³⁶²
YORP 54509	source ↗	61.8		Apollo asteroid type S	³⁶³
2019 OK		28.5 – 165		Apollo asteroid	³⁶⁴
Duende 367943	source ↗	23.75		Aten asteroid type L	³⁶⁵
Kamoʻoalewa 469219		20.5		Apollo asteroid type S; quasi-satellite of Earth	³⁶⁶
2012 TC4	source ↗	11.5		Apollo asteroid type E/type Xe	³⁶⁷
2014 RC	source ↗	≈ 11		Apollo asteroid type Sq	³⁶⁸
1998 KY26	source ↗	5.5±1		Apollo asteroid type X	³⁶⁹
2010 RF12		≈ 3.5	≈ 0.0005	Apollo asteroid	³⁷⁰
2011 MD	source ↗	3+2 −1		Apollo asteroid/Amor asteroid type S	³⁷¹
2020 VT4		2.5 - 5.5		Aten asteroid	³⁶⁴
2012 KT42		2.1 - 4.7		Apollo asteroid	³⁶⁴
2008 TC3	source ↗	2.05	0.00008	Apollo asteroid type F/type M	³⁷²
2023 BU	source ↗	1.5		Apollo asteroid	³⁷³
2015 TC25	source ↗	1		Apollo asteroid type E	³⁷⁴
2018 LA		0.8 - 2.6		Apollo asteroid	³¹⁹ · ³⁷⁵
2025 TF		0.6 - 1.35		Apollo asteroid	³⁶⁴
2011 CQ1		0.5 - 1.15		Aten asteroid	³⁶⁴
2020 CD3	source ↗	0.45±0.05		Apollo asteroid	³⁷⁶
2020 CW		0.41 - 0.9		Apollo asteroid	³⁶⁴
2008 TS26		0.305 - 0.68		Apollo asteroid	³⁷⁷
2015 FF415		0.25		Apollo asteroid	³¹⁹ · ³⁷⁸
2024 BX1		0.22		Apollo asteroid	³⁷⁹
2025 UC11		0.205 - 0.465		Aten asteroid	³⁶⁴
2022 WJ1		0.2 - 0.3		Apollo asteroid	³⁸⁰
EN131090	source ↗	0.1425 - 0.15	0.000000044	Apollo asteroid	³⁸¹

Gallery

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. source ↗

Largest moons of the Solar System to scale. source ↗

Notes

Radius estimated using equatorial radius and assuming body is spherical
Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft
The mass of Eris by itself is the difference between the mass of the system ((1.6466±0.0085)×10²² kg)⁴⁴ and the mass of Dysnomia by itself ((8.2±5.7)×10¹⁹ kg).⁴⁵
Radius estimated by using three radii and assuming body is spheroid
Calculated in Wolfram Alpha using semi axes of 1050 × 840 × 537⁵⁰(Ellipsoid volume: 1.98395×10^9 km³)
Best fit physical model assuming hydrostatic equilibrium for Haumea.⁵⁰
This value refers to the system mass
Mass calculated by Muñoz-Gutiérrez et al. (2019 & 2021) using Achlys's area-equivalent diameter of 772 km and predicted density of 0.87 g/cm³.⁷⁷^: 2⁷⁸^: 2 Muñoz-Gutiérrez et al. give the mass in terms of Earth masses (M_🜨), which can be converted into kilograms by multiplying by 5.9722×10²⁴ kg/M_🜨. This calculation does not treat Achlys as an ellipsoid (which would have a volume of $V={\frac {4}{3}}\pi abc\approx 1.85\times 10^{17}{\text{ m}}^{3}$ ), though the mass calculated from Achlys's ellipsoid volume and density ( $M=\rho V\approx 1.61\times 10^{20}{\text{ kg}}$ ) is equivalent to Muñoz-Gutiérrez et al.'s mass calculation when rounded to a single digit. Cite error: The named reference "mass" was defined multiple times with different content (see the help page).
Radius estimated from an assumed albedo
very approximate figure, assuming equivalent spherical diameter of ≈600 km and density ≈2.64 g/cm³
A density of 0.4–0.8 g/cm³ was calculated when assuming the volume as a sphere with a radius of 210±7 km.¹²³ The mass was calculated with the provided density and the assumed volume.
The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ×10⁶ km³ obtained from a detailed shape model in Stooke (1994).¹⁵⁹

Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets
Volumetric radius including uncertainties
Given as surface gravity (1 bar for gaseous planets)
Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,⁷⁵ if otherwise not mentioned in the References column
Reference column specifically for radius (r) and mass (M) citations

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Based on a spherical diameter of 250 km and a density of 0.73 g/cm3
Mass calculated using diameter and density
Based on a spherical diameter of 235 km and a density of 0.73 g/cm3
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Mass calculated using diameter and primary’s density
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Mass calculated using dimensions of 254, 110, and 90 km and a density of 0.85
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Mass calculated using a diameter of 175 km and a density of 1.76
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mass calculated using dimensions and density
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"JPL Small-Body Database Browser: 28 Bellona" (2018-10-18 last obs). Retrieved 30 April 2019.
"JPL Small-Body Database Browser: 78 Diana" (2018-10-22 last obs). Retrieved 2 May 2019.
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"JPL Small-Body Database Browser: 74 Galatea" (2018-05-22 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA)" (2018-06-21 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 1172 Aneas (1930 UA)" (2018-07-03 last obs). Retrieved 1 May 2019.
"JPL Small-Body Database Browser: 1437 Diomedes (1937 PB)" (2018-10-22 last obs). Retrieved 30 April 2019.
"JPL Small-Body Database Browser: 81 Terpsichore" (2018-10-22 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 1143 Odysseus (1930 BH)" (2018-10-22 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 2241 Alcathous (1979 WM)" (2018-06-17 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 57 Mnemosyne" (2018-06-25 last obs). Retrieved 30 April 2019.
"JPL Small-Body Database Browser: 659 Nestor (A908 FE)" (2018-10-22 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 40 Harmonia" (2018-09-15 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 23 Thalia" (2018-10-21 last obs). Retrieved 2 May 2019.
"JPL Small-Body Database Browser: 62 Erato" (2018-05-24 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 5 Astraea" (2018-09-16 last obs). Retrieved 30 April 2019.
"JPL Small-Body Database Browser: 91 Aegina" (2018-07-31 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 35 Leukothea" (2018-10-22 last obs). Retrieved 3 May 2019.
"LCDB Data for (617)". Asteroid Lightcurve Database (LCDB). Archived from the original on 19 October 2020. Retrieved 1 May 2019.
"JPL Small-Body Database Browser: 1208 Troilus (1931 YA)" (2018-07-22 last obs). Retrieved 2 May 2019.
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"JPL Small-Body Database Browser: 233 Asterope" (2018-10-24 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 53 Kalypso" (2018-10-18 last obs). Retrieved 30 April 2019.
"JPL Small-Body Database Browser: 26 Prosperina" (2018-10-22 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 2920 Automedon (1981 JR)" (2018-10-15 last obs). Retrieved 2 May 2019.
Johnston, Wm. Robert (21 September 2014). "(90) Antiope and S/2000 (90) 1". Johnston's Archive. Retrieved 14 June 2019.
"JPL Small-Body Database Browser: 61 Danae" (2018-07-13 last obs). Retrieved 4 May 2019.
"JPL Small-Body Database Browser: 17 Thetis" (2018-05-13 last obs). Retrieved 3 May 2019.
"JPL Small-Body Database Browser: 55 Pandora" (2018-10-22 last obs). Retrieved 4 May 2019.
"JPL Small-Body Database Browser: 379 Huenna (A894 AA)" (2018-08-30 last obs). Retrieved 3 May 2019.
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"JPL Small-Body Database Browser: 50 Virginia" (2018-10-19 last obs). Retrieved 3 May 2019.
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External links

[equatorial-31] Radius estimated using equatorial radius and assuming body is spherical

[various-47] Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft

[51] The mass of Eris by itself is the difference between the mass of the system ((1.6466±0.0085)×10²² kg)⁴⁴ and the mass of Dysnomia by itself ((8.2±5.7)×10¹⁹ kg).⁴⁵

[three_radii-53] Radius estimated by using three radii and assuming body is spheroid

[WolframVolume-58] Calculated in Wolfram Alpha using semi axes of 1050 × 840 × 537⁵⁰(Ellipsoid volume: 1.98395×10^9 km³)

[HE-60] Best fit physical model assuming hydrostatic equilibrium for Haumea.⁵⁰

[system_mass-67] This value refers to the system mass

[mass-91] Mass calculated by Muñoz-Gutiérrez et al. (2019 & 2021) using Achlys's area-equivalent diameter of 772 km and predicted density of 0.87 g/cm³.⁷⁷^: 2⁷⁸^: 2 Muñoz-Gutiérrez et al. give the mass in terms of Earth masses (M_🜨), which can be converted into kilograms by multiplying by 5.9722×10²⁴ kg/M_🜨. This calculation does not treat Achlys as an ellipsoid (which would have a volume of $V={\frac {4}{3}}\pi abc\approx 1.85\times 10^{17}{\text{ m}}^{3}$ ), though the mass calculated from Achlys's ellipsoid volume and density ( $M=\rho V\approx 1.61\times 10^{20}{\text{ kg}}$ ) is equivalent to Muñoz-Gutiérrez et al.'s mass calculation when rounded to a single digit. Cite error: The named reference "mass" was defined multiple times with different content (see the help page).

[assumedalbedo-94] Radius estimated from an assumed albedo

[106] very approximate figure, assuming equivalent spherical diameter of ≈600 km and density ≈2.64 g/cm³

[139] A density of 0.4–0.8 g/cm³ was calculated when assuming the volume as a sphere with a radius of 210±7 km.¹²³ The mass was calculated with the provided density and the assumed volume.

[mass_estimate-176] The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ×10⁶ km³ obtained from a detailed shape model in Stooke (1994).¹⁵⁹

[A-13] Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets

[B-14] Volumetric radius including uncertainties

[Gravity-15] Given as surface gravity (1 bar for gaseous planets)

[default-86] Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,⁷⁵ if otherwise not mentioned in the References column

[Refs-87] Reference column specifically for radius (r) and mass (M) citations

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[Elliot2010-154] Elliot, J. L.; Person, M. J.; Zuluaga, C. A.; Bosh, A. S.; Adams, E. R.; Brothers, T. C.; et al. (2010). "Size and albedo of Kuiper belt object 55636 from a stellar occultation" (PDF). Nature. 465 (7300): 897–900. Bibcode:2010Natur.465..897E. doi:10.1038/nature09109. PMID 20559381. S2CID 4431420. Archived from the original (PDF) on February 22, 2014.

[johnston-47171-155] Johnston, Wm. Robert (8 October 2017). "(47171) Lempo, Paha, and Hiisi". Johnston's Archive. Retrieved 10 June 2019.

[johnston-26308-156] Johnston, Wm. Robert (21 September 2014). "(26308) 1998 SM165 and S/2001 (26308) 1". Johnston's Archive. Retrieved 28 April 2019.

[Marsset2022-157] Marsset et al. (2022) The equilibrium shape of (65) Cybele: primordial or relic of a large impact?

[Marchis-2014-158] Marchis, F.; Durech, J.; Castillo-Rogez, J.; Vachier, F.; Cuk, M.; Berthier, J.; et al. (March 2014). "The Puzzling Mutual Orbit of the Binary Trojan Asteroid (624) Hektor". The Astrophysical Journal Letters. 783 (2): 6. arXiv:1402.7336. Bibcode:2014ApJ...783L..37M. doi:10.1088/2041-8205/783/2/L37. S2CID 19868908.

[Morgado2021-159] Morgado, B. E.; Sicardy, B.; Braga-Ribas, F.; Desmars, J.; Gomes-Júnior, A. R.; Bérard, D.; et al. (January 2020). "Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020". Astronomy & Astrophysics. 652: A141. arXiv:2107.07904. Bibcode:2021A&A...652A.141M. doi:10.1051/0004-6361/202141543. S2CID 236034389. A141.

[johnston-79360-160] Johnston, Wm. Robert (20 September 2014). "(79360) Sila-Nunam". Johnston's Archive. Retrieved 28 April 2019.

[161] Based on a spherical diameter of 250 km and a density of 0.73 g/cm3

[162] Mass calculated using diameter and density

[163] Based on a spherical diameter of 235 km and a density of 0.73 g/cm3

[Mainzer-2016-164] Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. 247: EAR–A–COMPIL–5–NEOWISEDIAM–V1.0. Bibcode:2016PDSS..247.....M. Retrieved 31 October 2018.

[Carry2012-165] Carry, B. (December 2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. Bibcode:2012P&SS...73...98C. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.

[Grundy2007-166] Grundy, W.M.; Stansberry, J.A.; Noll K.S.; Stephens, D.C.; et al. (2007). "The orbit, mass, size, albedo, and density of (65489) Ceto/Phorcys: A tidally-evolved binary Centaur". Icarus. 191 (1): 286–297. arXiv:0704.1523. Bibcode:2007Icar..191..286G. doi:10.1016/j.icarus.2007.04.004. S2CID 1532765.

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[168] Mass calculated using diameter and primary’s density

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[170] Buie, Marc W.; Leiva, Rodrigo; Keller, John M.; Desmars, Josselin; Sicardy, Bruno; Kavelaars, J. J.; et al. (April 2020). "A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua". The Astronomical Journal. 159 (5): 230. arXiv:2011.03889. Bibcode:2020AJ....159..230B. doi:10.3847/1538-3881/ab8630. S2CID 219039999. 230.

[TNOsCool11-171] Duffard, R.; Pinilla-Alonso, N.; Santos-Sanz, P.; Vilenius, E.; Ortiz, J. L.; Mueller, T.; et al. (April 2014). ""TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs". Astronomy and Astrophysics. 564: 17. arXiv:1309.0946. Bibcode:2014A&A...564A..92D. doi:10.1051/0004-6361/201322377. S2CID 119177446.

[172] Mass calculated using dimensions of 254, 110, and 90 km and a density of 0.85

[Sickafoose2023-173] Sickafoose, Amanda A.; Levine, Stephen E.; Bosh, Amanda S.; Person, Michael J.; Zuluaga, Carlos A.; Knieling, Bastian; Lewis, Mark C.; Schindler, Karsten (1 November 2023). "Material around the Centaur (2060) Chiron from the 2018 November 28 UT Stellar Occultation". The Planetary Science Journal. 4 (11): 221. arXiv:2310.16205. Bibcode:2023PSJ.....4..221S. doi:10.3847/PSJ/ad0632.

[Showalter2019-174] Showalter, M. R.; de Pater, I.; Lissauer, J. J.; French, R. S. (2019). "The seventh inner moon of Neptune" (PDF). Nature. 566 (7744): 350–353. Bibcode:2019Natur.566..350S. doi:10.1038/s41586-019-0909-9. PMC 6424524. PMID 30787452.

[Stooke1994-175] Stooke, Philip J. (1994). "The surfaces of Larissa and Proteus". Earth, Moon, and Planets. 65 (1): 31–54. Bibcode:1994EM&P...65...31S. doi:10.1007/BF00572198. S2CID 121825800.

[AKARI-177] Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117.

[johnston-121-178] Johnston, Wm. Robert (21 September 2014). "(121) Hermione and S/2002 (121) 1 ("LaFayette")". Johnston's Archive. Retrieved 5 June 2019.

[WISE-179] Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 118700974.

[Ortiz2025-180] Ortiz, Jose L.; Morales, N.; Sicardy, B.; Fernandez-Valenzuela, E.; Braga-Ribas, F.; Kilic, Y.; et al. (18 Sep 2025). "A high geometric albedo and small size for the Haumea cluster member (24835) 1995 SM ₅₅ determined from a stellar occultation and photometric observations". Astronomy & Astrophysics. 703: A147. arXiv:2509.15384. Bibcode:2025A&A...703A.147O. doi:10.1051/0004-6361/202556498.

[johnston-88611-181] Johnston, Wm. Robert (20 September 2014). "(88611) Teharonhiawako and Sawiskera". Johnston's Archive. Retrieved 13 June 2019.

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[183] "In Depth | Makemake - NASA Solar System Exploration". 14 November 2017.

[184] Mass calculated using a diameter of 175 km and a density of 1.76

[Masiero-2012-185] Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (10 October 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): L8. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317.

[Rojo-2011-186] Rojo, P.; Margot, J. L. (February 2011). "Mass and Density of the B-type Asteroid (702) Alauda". The Astrophysical Journal. 727 (2): 5. arXiv:1011.6577. Bibcode:2011ApJ...727...69R. doi:10.1088/0004-637X/727/2/69. S2CID 59449907.

[Emelyanov2005-187] Emelyanov, N.V.; Archinal, B. A.; A'hearn, M. F.; et al. (2005). "The mass of Himalia from the perturbations on other satellites" (PDF). Astronomy and Astrophysics. 438 (3): L33–L36. Bibcode:2005A&A...438L..33E. doi:10.1051/0004-6361:200500143.

[ThomasBurns1998-188] Thomas, P. C.; Burns, J. A.; Rossier, L.; Simonelli, D.; Veverka, J.; Chapman, C. R.; Klaasen, K.; Johnson, T. V.; Belton, M. J. S.; Galileo Solid State Imaging Team (September 1998). "The Small Inner Satellites of Jupiter". Icarus. 135 (1): 360–371. Bibcode:1998Icar..135..360T. doi:10.1006/icar.1998.5976.

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[FarkasTakacs2017-192] Farkas-Takács, A.; Kiss, Cs.; Pál, A.; Molnár, L.; Szabó, Gy. M.; Hanyecz, O.; et al. (September 2017). "Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations". The Astronomical Journal. 154 (3): 13. arXiv:1706.06837. Bibcode:2017AJ....154..119F. doi:10.3847/1538-3881/aa8365. S2CID 118869078. 119.

[193] ss calculated using dimensions and density

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[Rabinowitz2019-195] Rabinowitz, David L.; Benecchi, Susan D.; Grundy, William M.; Verbiscer, Anne J.; Thirouin, Audrey (November 2019). "The Complex Rotational Light Curve of (385446) Manwë-Thorondor, a Multi-Component Eclipsing System in the Kuiper Belt". arXiv:1911.08546 [astro-ph.EP].

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[johnston-229762-197] Johnston, Wm. Robert (9 October 2021). "(229762) Gǃkúnǁʼhòmdímà and GǃòʼéǃHú". Johnston's Archive. Retrieved 2025-09-07.

[johnston-42355-198] Johnston, Wm. Robert (31 January 2015). "(42355) Typhon and Echidna". Johnston's Archive. Retrieved 14 June 2019.

[johnston-469705-199] Johnston, Wm. Robert (9 October 2021). "(469705) |Kagara [sic] and !Haunu". Johnston's Archive. Retrieved 2025-09-07.

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[Grundy2011-202] Grundy, W. M.; Noll, K. S.; Nimmo, F.; Roe, H. G.; Buie, M. W.; Porter, S. B.; Benecchi, S. D.; Stephens, D. C.; Levison, H. F.; Stansberry, J. A. (2011). "Five new and three improved mutual orbits of transneptunian binaries" (PDF). Icarus. 213 (2): 678. arXiv:1103.2751. Bibcode:2011Icar..213..678G. doi:10.1016/j.icarus.2011.03.012. S2CID 9571163.

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[204] Johnston, Wm. Robert (9 October 2021). "(469705) |Kagara and !Haunu". Johnston's Archive. Retrieved 2025-09-07.

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[jplssd-78-206] "JPL Small-Body Database Browser: 78 Diana" (2018-10-22 last obs). Retrieved 2 May 2019.

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[jplssd-74-208] "JPL Small-Body Database Browser: 74 Galatea" (2018-05-22 last obs). Retrieved 2 May 2019.

[jplssd-1867-209] "JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA)" (2018-06-21 last obs). Retrieved 2 May 2019.

[jplssd-1172-210] "JPL Small-Body Database Browser: 1172 Aneas (1930 UA)" (2018-07-03 last obs). Retrieved 1 May 2019.

[jplssd-1437-211] "JPL Small-Body Database Browser: 1437 Diomedes (1937 PB)" (2018-10-22 last obs). Retrieved 30 April 2019.

[jplssd-81-212] "JPL Small-Body Database Browser: 81 Terpsichore" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-1143-213] "JPL Small-Body Database Browser: 1143 Odysseus (1930 BH)" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-2241-214] "JPL Small-Body Database Browser: 2241 Alcathous (1979 WM)" (2018-06-17 last obs). Retrieved 2 May 2019.

[jplssd-57-215] "JPL Small-Body Database Browser: 57 Mnemosyne" (2018-06-25 last obs). Retrieved 30 April 2019.

[jplssd-659-216] "JPL Small-Body Database Browser: 659 Nestor (A908 FE)" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-40-217] "JPL Small-Body Database Browser: 40 Harmonia" (2018-09-15 last obs). Retrieved 3 May 2019.

[jplssd-23-218] "JPL Small-Body Database Browser: 23 Thalia" (2018-10-21 last obs). Retrieved 2 May 2019.

[jplssd-62-219] "JPL Small-Body Database Browser: 62 Erato" (2018-05-24 last obs). Retrieved 3 May 2019.

[jplssd-5-220] "JPL Small-Body Database Browser: 5 Astraea" (2018-09-16 last obs). Retrieved 30 April 2019.

[jplssd-91-221] "JPL Small-Body Database Browser: 91 Aegina" (2018-07-31 last obs). Retrieved 3 May 2019.

[jplssd-35-222] "JPL Small-Body Database Browser: 35 Leukothea" (2018-10-22 last obs). Retrieved 3 May 2019.

[lcdb-617-223] "LCDB Data for (617)". Asteroid Lightcurve Database (LCDB). Archived from the original on 19 October 2020. Retrieved 1 May 2019.

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[jplssd-53-228] "JPL Small-Body Database Browser: 53 Kalypso" (2018-10-18 last obs). Retrieved 30 April 2019.

[jplssd-26-229] "JPL Small-Body Database Browser: 26 Prosperina" (2018-10-22 last obs). Retrieved 3 May 2019.

[jplssd-2920-230] "JPL Small-Body Database Browser: 2920 Automedon (1981 JR)" (2018-10-15 last obs). Retrieved 2 May 2019.

[johnston-90-231] Johnston, Wm. Robert (21 September 2014). "(90) Antiope and S/2000 (90) 1". Johnston's Archive. Retrieved 14 June 2019.

[jplssd-61-232] "JPL Small-Body Database Browser: 61 Danae" (2018-07-13 last obs). Retrieved 4 May 2019.

[jplssd-17-233] "JPL Small-Body Database Browser: 17 Thetis" (2018-05-13 last obs). Retrieved 3 May 2019.

[jplssd-55-234] "JPL Small-Body Database Browser: 55 Pandora" (2018-10-22 last obs). Retrieved 4 May 2019.

[jplssd-379-235] "JPL Small-Body Database Browser: 379 Huenna (A894 AA)" (2018-08-30 last obs). Retrieved 3 May 2019.

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[jplssd-50-237] "JPL Small-Body Database Browser: 50 Virginia" (2018-10-19 last obs). Retrieved 3 May 2019.

[jplssd-4348-238] "JPL Small-Body Database Browser: 4348 Poulydamas (1988 RU)" (2018-07-13 last obs). Retrieved 4 May 2019.

[johnston-58534-239] Johnston, Wm. Robert (20 September 2014). "(58534) Logos and Zoe". Johnston's Archive. Retrieved 4 May 2019.

[jplssd-32-240] "JPL Small-Body Database Browser: 32 Pomona" (2018-06-12 last obs). Retrieved 4 May 2019.

[Grav2015-241] Grav, T.; Bauer, J. M.; Mainzer, A. K.; Masiero, J. R.; Nugent, C. R.; Cutri, R. M.; et al. (August 2015). "NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn". The Astrophysical Journal. 809 (1): 9. arXiv:1505.07820. Bibcode:2015ApJ...809....3G. doi:10.1088/0004-637X/809/1/3. S2CID 5834661. 3.

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[jplssd-43-243] "JPL Small-Body Database Browser: 43 Ariadne" (2018-10-20 last obs). Retrieved 4 May 2019.

[jplssd-99-244] "JPL Small-Body Database Browser: 99 Dike" (2018-10-24 last obs). Retrieved 4 May 2019.

[jplssd-79-245] "JPL Small-Body Database Browser: 79 Eurynome" (2018-08-18 last obs). Retrieved 4 May 2019.

[jplssd-75-246] "JPL Small-Body Database Browser: 75 Eurydike" (2019-05-08 last obs). Retrieved 3 June 2019.

[jplssd-29P-247] "JPL Small-Body Database Browser: 29P/Schwassmann-Wachmann 1" (2018-10-16 last obs). Retrieved 4 May 2019.

[jplssd-64-248] "JPL Small-Body Database Browser: 64 Angelina" (2019-05-09 last obs). Retrieved 3 June 2019.

[jplssd-82-249] "JPL Small-Body Database Browser: 82 Alkmene" (2019-05-09 last obs). Retrieved 3 June 2019.

[jplssd-142-250] "JPL Small-Body Database Browser: 142 Polana" (2019-05-08 last obs). Retrieved 4 May 2019.

[jplssd-253-251] "JPL Small-Body Database Browser: 253 Mathilde" (2018-10-22 last obs). Retrieved 4 May 2019.

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[jplssd-73-253] "JPL Small-Body Database Browser: 73 Klytia" (2019-05-11 last obs). Retrieved 5 June 2019.

[jplssd-60-254] "JPL Small-Body Database Browser: 60 Echo" (2019-05-11 last obs). Retrieved 3 June 2019.

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[jplssd-167-256] "JPL Small-Body Database Browser: 167 Urda" (2018-05-11 last obs). Retrieved 5 June 2019.

[phasecurves-257] Verbiscer, A. J.; Porter, S. B.; Buratti, B. J.; Weaver, H. A.; Spencer, J. R.; Showalter, M. R.; Buie, M. W.; Hofgartner, J. D.; Hicks, M. D.; Ennico-Smith, K.; Olkin, C. B.; Stern, S. A.; Young, L. A.; Cheng, A. (2018). "Phase Curves of Nix and Hydra from the New Horizons Imaging Cameras". The Astrophysical Journal. 852 (2): L35. Bibcode:2018ApJ...852L..35V. doi:10.3847/2041-8213/aaa486.

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[jplssd-158-259] "JPL Small-Body Database Browser: 158 Koronis" (2018-05-08 last obs). Retrieved 12 June 2019.

[jplssd-52872-260] "JPL Small-Body Database Browser: 52872 Okyrhoe (1998 SG35)" (2018-08-18 last obs). Retrieved 4 May 2019.

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[262] Stern, S.A.; et al. (9 January 2019). "Overview of initial results from the reconnaissance flyby of a Kuiper Belt planetesimal: 2014 MU69". arXiv:1901.02578 [astro-ph.EP].

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[Descamps2008-266] Descamps, P.; Marchis, F.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses". Icarus. 196 (2): 578–600. arXiv:0710.1471. Bibcode:2008Icar..196..578D. doi:10.1016/j.icarus.2008.03.014. S2CID 118437111.

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