List of Solar System objects by size

Short description: Largest objects of the Solar System

Solar System

Objects

* by orbit
* by size
* by discovery date
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Lists

* Gravitationally-rounded
(equilibrium) objects

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

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 Haumea). Unlike bodies such as Haumea, the irregular bodies have a significantly non-ellipsoidal profile, often with sharp edges.

There can be difficulty in determining the diameter (within a factor of about 2) for typical objects beyond Saturn. (See 2060 Chiron as an example) For TNOs there is some confidence in the diameters, but for non-binary TNOs there is no real confidence in the masses/densities. Many TNOs are often just assumed to have Pluto's density of 2.0 g/cm3, but it is just as likely that they have a comet-like density of only 0.5 g/cm3.[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 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.

## Contents

* 1 Graphical overview
* 2 Objects with radius over 400 km
* 3 Smaller objects by mean radius
* 3.1 From 200 to 399 km
* 3.2 From 100 to 199 km
* 3.3 From 50 to 99 km
* 3.4 From 20 to 49 km
* 3.5 From 1 to 19 km
* 3.6 Below 1 km
* 4 Gallery
* 5 See also
* 6 Notes
* 7 References
* 8 Further reading
* 9 External links

## Graphical overview

* Relative diameters of the fifty largest bodies in the Solar System, colored by orbital region. Values are diameters in kilometers. Scale is linear.

* Relative masses of the bodies of the Solar System. Objects smaller than Saturn are not visible at this scale.

* Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system.

* Relative masses of the solid bodies of the Solar System. Earth at 48% and Venus at 39% dominate. Bodies less massive than Pluto are not visible at this scale.

* Relative masses of the rounded moons of the Solar System. Mimas, Enceladus, and Miranda are too small to be visible at this scale.

## Objects with radius 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, 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 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]).

Body[note 1] | Image  | Radius[note 2] | Volume  | Mass  | Surface area  | Density  | Gravity[note 3] | Type  | Discovery

|
|
|
|
|
|
|
|
|

(km)  | (R🜨)  | (109 km3)  | (V🜨)  | (1021 kg)  | (M🜨)  | (106 km2)  | 🜨  | (g/cm3)  | (m/s2)  | (🜨)
Sun |  | 695508 ± ?[13] | 109.2[13] | 1,409,300,000[13] | 1,301,000[13] | 1989100000[13] | 333,000[13] | 6,078,700[13] | 11,918[13] | 1.409[13] | 274.0[13] | 27.94[13] | G2V-class star | 2 prehistoric

Jupiter |  | 69911±6[14] | 10.97  | 1,431,280  | 1,321  | 1898187±88[14] | 317.83  | 61,419[15] | 120.41  | 1.3262±0.0003[14] | 24.79[14] | 2.528  | gas giant planet; has rings | 5 prehistoric

Saturn |  | 58232±6[14]
(136775 for A Ring) | 9.140  | 827,130  | 764  | 568317±13[14] | 95.162  | 42,612[16] | 83.54  | 0.6871±0.0002[14] | 10.44[14] | 1.065  | gas giant planet; has rings | 8 prehistoric

Uranus |  | 25362±7[14] | 3.981  | 68,340  | 63.1  | 86813±4[14] | 14.536  | 8083.1[17] | 15.85  | 1.270±0.001[14] | 8.87[14] | 0.886  | ice giant planet; has rings | 1781
Neptune |  | 24622±19[14] | 3.865  | 62,540  | 57.7  | 102413±5[14] | 17.147  | 7618.3[18] | 14.94  | 1.638±0.004[14] | 11.15[14] | 1.137  | ice giant planet; has rings | 1846
Earth |  | 6371.0±0.0001[14] | 1  | 1,083.21  | 1  | 5972.4±0.3[14] | 1  | 510.06447[19] | 1  | 5.5136±0.0003[14] | 9.81[14] | 1  | terrestrial planet | 1 prehistoric

Venus |  | 6052±1[14] | 0.9499  | 928.43  | 0.857  | 4867.5±0.2[14] | 0.815  | 460.2[20] | 0.903  | 5.243±0.003[14] | 8.87[14] | 0.905  | terrestrial planet | 4 prehistoric

Mars |  | 3389.5±0.2[14] | 0.5320  | 163.18  | 0.151  | 641.71±0.03[14] | 0.107  | 144.37[21] | 0.283  | 3.9341±0.0007[14] | 3.71[14] | 0.379  | terrestrial planet | 6 prehistoric

Ganymede
Jupiter III |  | 2634.1±0.3 | 0.4135  | 76.30  | 0.0704  | 148.2 | 0.0248  | 86.999[22] | 0.171  | 1.936 | 1.428  | 0.146  | moon of Jupiter (icy)  | 1610
Titan
Saturn VI |  | 2574.73±0.09[23] | 0.4037[lower-alpha 1] | 71.50  | 0.0658  | 134.5 | 0.0225  | 83.3054[24] | 0.163  | 1.880±0.004 | 1.354  | 0.138  | moon of Saturn (icy)  | 1655
Mercury |  | 2439.4±0.1[14] | 0.3829  | 60.83  | 0.0562  | 330.11±0.02[14] | 0.0553  | 74.797[25] | 0.147  | 5.4291±0.007[14] | 3.70[14] | 0.377  | terrestrial planet | 7 prehistoric

Callisto
Jupiter IV |  | 2410.3±1.5[23] | 0.3783  | 58.65  | 0.0541  | 107.6 | 0.018  | 73.005[26] | 0.143  | 1.834±0.003 | 1.23603  | 0.126  | moon of Jupiter (icy)  | 1610

Jupiter I |  | 1821.6±0.5[5] | 0.2859  | 25.32  | 0.0234  | 89.32 | 0.015  | 41.698[27] | 0.082  | 3.528±0.006 | 1.797  | 0.183  | moon of Jupiter (terrestrial)  | 1610
Moon
Earth I |  | 1737.5±0.1[28] | 0.2727  | 21.958  | 0.0203  | 73.46[29] | 0.0123  | 37.937[30] | 0.074  | 3.344±0.005[28] | 1.625  | 0.166  | moon of Earth (terrestrial)  | 3 prehistoric

Europa
Jupiter II |  | 1560.8±0.5[5] | 0.2450  | 15.93  | 0.0147  | 48.00 | 0.008035  | 30.613[31] | 0.06  | 3.013±0.005 | 1.316  | 0.134  | moon of Jupiter (terrestrial)  | 1610
Triton
Neptune I |  | 1353.4±0.9[lower-alpha 1][23] | 0.2124[lower-alpha 1] | 10.38  | 0.0096  | 21.39±0.03 | 0.003599  | 23.018[32] | 0.045  | 2.061 | 0.782  | 0.0797  | moon of Neptune (icy)  | 1846
Pluto
134340 |  | 1188.3±0.8 | 0.187  | 7.057  | 0.00651  | 13.03±0.03 | 0.0022  | 17.79  | 0.034  | 1.854±0.006 | 0.620  | 0.063  | dwarf planet; plutino; multiple | 1930
Eris
136199 |  | 1163±6[lower-alpha 2][33] | 0.1825[lower-alpha 2] | 6.59  | 0.0061  | 16.6±0.2[34] | 0.0028  | 17  | 0.033  | 2.52±0.07 | 0.824  | 0.083  | dwarf planet; SDO; binary | 2003
Haumea
136108 |  | 798±6 to 816[35] | 0.12  | 1.98[lower-alpha 3] | 0.0018  | 4.01±0.04[36] | 0.00066  | 8.14  | 0.016  | 2.018[37][lower-alpha 4] | 0.401  | 0.0409  | dwarf planet;
resonant KBO (7:12);
trinary; has rings | 2004
Titania
Uranus III |  | 788.9±1.8[23] | 0.1237[lower-alpha 5] | 2.06  | 0.0019  | 3.40±0.06 | 0.00059  | 7.82[38] | 0.015  | 1.711±0.005 | 0.378  | 0.0385  | moon of Uranus | 1787
Rhea
Saturn V |  | 763.8±1.0[lower-alpha 5] | 0.1199[lower-alpha 5] | 1.87  | 0.0017  | 2.307 | 0.00039  | 7.34[39] | 0.014  | 1.236±0.005 | 0.26  | 0.027  | moon of Saturn | 1672
Oberon
Uranus IV |  | 761.4±2.6[lower-alpha 1][23] | 0.1195[lower-alpha 1] | 1.85  | 0.0017  | 3.08±0.09 | 0.0005  | 7.285[40] | 0.014  | 1.63±0.05 | 0.347  | 0.035  | moon of Uranus | 1787
Iapetus
Saturn VIII |  | 735.6±1.5[5] | 0.1153  | 1.66  | 0.0015  | 1.806 | 0.00033  | 6.8  | 0.013  | 1.088±0.013 | 0.223  | 0.0227  | moon of Saturn | 1671
Makemake
136472 |  | 715+19
−11[41] | 0.112  | 1.53  | 0.0014  | ≈ 3.1 | 0.00053  | 6.4  | 0.013  | ≈ 2.1 | 0.57  | 0.0581  | dwarf planet; cubewano | 2005
Gonggong
225088 |  | 615±25[42] | 0.0983  | 1.03  | 0.0009  | 1.75±0.07 | 0.00029  | 4.753  | 0.009  | 1.72±0.16 | 0.3  | 0.0306  | dwarf planet?; resonant SDO (3:10)  | 2007
Charon
Pluto I |  | 606.0±0.5 | 0.0951  | 0.932  | 0.0009  | 1.586±0.015 | 0.00025  | 4.578[43] | 0.009  | 1.70±0.02 | 0.288  | 0.0294  | moon of Pluto | 1978
Umbriel
Uranus II |  | 584.7±2.8[23] | 0.0918  | 0.837  | 0.0008  | 1.28±0.03 | 0.00020  | 4.3[44] | 0.008  | 1.39±0.16 | 0.234  | 0.024  | moon of Uranus | 1851
Ariel
Uranus I |  | 578.9±0.6[23] | 0.0909  | 0.813  | 0.0007  | 1.25±0.02 | 0.000226  | 4.211[45] | 0.008  | 1.66±0.15 | 0.269  | 0.027  | moon of Uranus | 1851
Dione
Saturn IV |  | 561.7±0.45[23] | 0.0881  | 0.741  | 0.0007  | 1.095 | 0.000183  | 3.965[46] | 0.008  | 1.478±0.003 | 0.232  | 0.0237  | moon of Saturn | 1684
Quaoar
50000 |  | 543±2 | 0.0879  | 0.737  | 0.0007  | 1.20±0.05[47] | 0.0002  | 3.83  | 0.008  | 2.0±0.5[48] | 0.3  | 0.0306  | cubewano; binary  | 2002
Tethys
Saturn III |  | 533.0±0.7[23] | 0.0834  | 0.624  | 0.0006  | 0.617 | 0.000103  | 3.57[49] | 0.007  | 0.984±0.003[50] | 0.145  | 0.015  | moon of Saturn | 1684
Sedna
90377 |  | 498±40 | 0.0785  | 0.516  | 0.0005  |  |  |  |  |  |  |  | sednoid; detached object | 2003
Ceres
1 |  | 469.7±0.1[51] | 0.0742  | 0.433  | 0.0004  | 0.938[52] | 0.000157  | 2.85[53] | 0.006[53] | 2.17 | 0.28  | 0.029  | dwarf planet; belt asteroid | 1801
Orcus
90482 |  | 455+25
−20 | 0.0719  | 0.404  | 0.0004  | 0.548±0.010[54] | 0.000092  |  |  | 1.4±0.2[54] | 0.2  | 0.0204  | plutino; binary | 2004
Salacia
120347 |  | 423±11 | 0.0664  | 0.3729  | 0.0003  | 0.492±0.007[55] | 0.000082  |  |  | 1.5±0.1[55] | 0.165  | 0.0168  | cubewano; binary | 2004
2002 MS4
307261 |  | 400±12[56] | 0.0628  | 0.2681  | 0.0002  |  |  |  |  |  |  |  | cubewano  | 2002

## 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.[57] 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]

Body[note 1] | Image  | Radius[note 2]
(km) | Mass
(1018 kg) | Density
(g/cm3) | Type[note 4] | Refs[note 5]
r * M

|
|
|
|
|
|

2002 AW197
55565 |

| 384±19 | –  | –  | cubewano  | [59]
Varda
174567 |

| 373±8 | 245±6 | 1.23±0.04 | cubewano; binary  | [60] * [60]
2013 FY27
532037 |

| 370±40 | –  | –  | SDO; binary | [61]
2003 AZ84
208996 |

| 362 ~ 386±6 (assuming HE)  | 150 ~ 210 (assuming HE)  | 0.76 ~ 0.87 (assuming HE)  | plutino; binary | [58][62]
Ixion
28978 |

| 354.8±0.1 | –  | –  | plutino | [63]
2004 GV9
90568 |

| 340±17 | –  | –  | cubewano  | [64]
2005 RN43
145452 |

| 340+28
−37 | –  | –  | cubewano  | [64]
Varuna
20000 |

| 334+77
−43 | ≈ 160 | 0.99+0.09
−0.02 | cubewano  | [65] * [66]
2002 UX25
55637 |

| 332±15 | 125±3 | 0.82±0.11 | cubewano; binary | [67] * [68]
2005 RM43
145451 |

| 322 | –  | –  | SDO  | [69][70]
Gǃkúnǁʼhòmdímà
229762 |

| 321±14 | 136.1±3.3 | 1.02±0.17 | SDO; binary  | [71] * [72]
2014 UZ224 |

| 317.5+28.5
−30.5 | –  | –  | SDO  | [73]
2008 OG19
470599 |  | 309.5+28
−56.5 | –  | 0.609±0.004 | SDO  | [74] * [74]
2007 JJ43
278361 |  | 305+85
−70 | –  | –  | cubewano  | [75]
Chaos
19521 |

| 300+70
−65 | –  | –  | cubewano  | [64]
Dysnomia
Eris I |

| ≈ 300; ≤ 370 | 300–500
< 140 | 1.8–2.4
< 1.2 | moon of Eris | [76][54]
2014 EZ51
523692 |  | > 288 | –  | –  | SDO  | [77]
2012 VP113 |  | ≈ 287 | –  | –  | sednoid | [78]
2002 XW93
78799 |  | 283+36
−37 | –  | –  | other TNO  | [79]
2004 XR190
612911 |

| ≈ 278 | –  | –  | SDO  | [7]
2002 XV93
612533 |

| 275+11
−12 | –  | –  | plutino | [80]
2015 RR245
523794 |  | ≈ 270 | –  | –  | resonant KBO (2:9); binary | [78]
2003 UZ413
455502 |

| ≈ 268 | –  | –  | plutino | [7]
Vesta
4 |

| 262.7±0.1 | 259 | 3.46 | belt asteroid type V | [81] * [81]
2003 VS2
84922 |

| 262±4 | –  | –  | plutino | [82]
Pallas
2 |

| 256±2 | 204±3 | 2.92±0.08 | belt asteroid type B | [83][84]
2004 TY364
120348 |  | 256+19
−20 | –  | –  | cubewano  | [85]
Enceladus
Saturn II |

| 252.1±0.2 | 108.0±0.1 | 1.609±0.005 | moon of Saturn  | [86] * [87]
2002 TC302
84522 |

| 250±7 | –  | –  | resonant SDO (2:5) | [88]
2005 UQ513
202421 |  | 249+32
−38 | –  | –  | cubewano  | [59]
Miranda
Uranus V |

| 235.8±0.7 | 65.9±7.5 | 1.2±0.15 | moon of Uranus  | [89] * [90]
Dziewanna
471143 |

| 235+18
−5 | –  | –  | SDO  | [91]
2005 TB190
145480 |

| 232±31 | –  | –  | detached object | [92]
1999 DE9
26375 |  | 231±23 | –  | –  | resonant SDO (2:5) | [93]
2003 FY128
120132 |  | 230±11 | –  | –  | SDO  | [92]
2002 VR128
84719 |  | 224+24
−22 | –  | –  | plutino | [80]
Vanth
Orcus I |

| 221±5 | 87±8 | 1.5+1.0
−0.5 | moon of 90482 Orcus | [94] * [54]
Hygiea
10 |

| 216±4 | 87.4±6.9 | 2.06±0.20 | belt asteroid type C | [95] * [84]
2004 NT33
444030 |  | 212+44
−40 | –  | –  | cubewano  | [59]
Proteus
Neptune VIII |

| 210±7 | 44 | ≈ 1.3 | moon of Neptune  | [5] * [5]
2005 QU182
303775 |  | 208±37 | –  | –  | SDO  | [92]
2002 KX14
119951 |

| 207.5±0.5 | –  | –  | cubewano  | [96]
2001 QF298
469372 |

| 204+20
−22 | –  | –  | plutino | [80]
Huya
38628 |

| 203±8 | > 50 | > 1.43 | plutino; binary  | [67] * [97]
2004 PF115
175113 |  | 203+49
−38 | –  | –  | plutino | [80]

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).[98] Many TNOs are omitted from this list as their sizes are poorly known.[58]

Body[note 1] | Image  | Radius[note 2]
(km) | Mass
(1018 kg) | Type  | Refs[note 5]
r * M

|
|
|
|
|

2004 UX10
144897 |  | 199±20 | ≈ 30 | plutino | [80] * [99]
Mimas
Saturn I |

| 198.2±0.3 | 37.49±0.03 | moon of Saturn | [86] * [87][23]
1998 SN165
35671 |  | 196±20 |  | cubewano  | [59]
2001 UR163
42301 |

| ≈ 176 |  | resonant KBO (4:9) | [58]
Nereid
Neptune II |

| 170±25 |  | moon of Neptune | [23]
1996 TL66
15874 |  | 170±10 |  | SDO | [92]
2004 XA192
230965 |  | 170+60
−47.5 |  | SDO  | [80]
2002 WC19
119979 |

| ≈ 169 | 77±5 | resonant KBO (1:2); binary | [100] * [100]
Interamnia
704 |

| 166±3 | 35.2±5.1 | belt asteroid type F  | [101] * [84]
Ilmarë
Varda I |

| 163±18 |  | moon of 174567 Varda | [102]
Europa
52 |

| 160±2 | 23.9±3.8 | belt asteroid type C | [84]
Hiʻiaka
Haumea I |

| ≈ 160 | 17.9±1.1 | moon of Haumea | [36] * [36]
Davida
511 |

| 149±2 | 26.6±7.3 | belt asteroid type C | [84]
2002 TX300
55636 |

| 143±5 |  | cubewano  | [103]
Actaea
Salacia I |

| 143±12 |  | moon of 120347 Salacia | [104]
Sylvia
87 |

| 137±2 | 14.3±0.5 | outer belt asteroid type X; trinary | [84]
Lempo
47171 |

| 136±9 |  | plutino; trinary | [105]
Eunomia
15 |

| 135±2 | 30.5±1.9 | belt asteroid type S | [84]
Hyperion
Saturn VII |

| 135±4 | 5.62±0.05 | moon of Saturn | [57] * [57][23]
Euphrosyne
31 |

| 134±2 | 16.5±2.6 | belt asteroid type C; binary | [84]
1998 SM165
26308 |

| 134±14 | 6.87±1.8 | resonant KBO (1:2) | [106] * [106]
Cybele
65 |

| 131.5±1.5 | 14.8±1.8 | outer belt asteroid type C | [107]
Chariklo
10199 |

| ≈ 130 |  | centaur; has rings | [108]
Juno
3 |

| 127±1 | 27.0±2.4 | belt asteroid type S | [84]
Hiisi
Lempo II |

| 126±8 |  | secondary of 47171 Lempo | [105]
Hektor
624 |

| 125±13 | 7.9±1.4 | Jupiter trojan (L4) type D; binary | [109] * [109]
Sila
79360 |

| 124±15 | 10.8±0.22 | cubewano; binary | [110]
2007 RW10
309239 |  | 124±15 |  | quasi-satellite of Neptune  | [92]
Altjira
148780 |

| 123+19
−70 |  | cubewano; binary  | [59]
Nunam
79360 |

| 118±15 |  | secondary of 79360 Sila | [110]
Bamberga
324 |

| 114±2 | 10.2±0.9 | belt asteroid type C | [84]
Patientia
451 |  | 112.9±2.3 | 10.9±5.3 | belt asteroid type C | [111] * [112]
Psyche
16 |

| 112±2 | 26.2±2.9 | belt asteroid type M | [84]
Ceto
65489 |

| 112±5 | 5.4±0.4 | extended centaur; binary | [92] * [113]
Herculina
532 |

| 111.2±2.4 |  | belt asteroid type S | [114]
S/2007 (148780) 1
Altjira I |

| 110+17
−62 |  | secondary of 148780 Altjira | [59]
Hesperia
69 |

| 110±15 | 5.86±1.18 | belt asteroid type M
Thisbe
88 |

| 109±2 | 11.6±2.2 | belt asteroid type B | [84]
Doris
48 |

| 108±2 | 6.9±2.9 | belt asteroid type C | [84]
Chiron
2060 or 95P |

| 108±5 |  | centaur; has rings  | [67]
Phoebe
Saturn IX |

| 106.5±0.7 | 8.29±0.01 | moon of Saturn | [57] * [57][23]
S/2012 (38628) 1
Huya I |

| 106±15 |  | moon of 38628 Huya | [67]
Fortuna
19 | File:19 Fortuna VLT (2021), deconvolved.pdf | 105.5±1.0 | 8.8±1.4 | belt asteroid type G  | [84]
Camilla
107 |

| 105±4 | 11.2±0.3 | outer belt asteroid type C; trinary | [111] * [112]
Themis
24 |

| 104±2 | 6.2±2.9 | belt asteroid type C | [84]
Amphitrite
29 |

| 102±1 | 12.7±2.0 | belt asteroid type S | [84]
Egeria
13 |

| 101±2 | 9.2±2.1 | belt asteroid type G  | [84]
Iris
7 |

| 100±5 | 13.5±2.3 | belt asteroid type S | [84]
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.[58] 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 |

| 99.5±1 | 6.4±0.2 | belt asteroid type G; multiple | [84]
Bienor
54598 |  | 99+3
−3.5 |  | centaur | [115]
Hebe
6 |

| 97.5±1.5 | 12.4±2.4 | belt asteroid type S | [84]
Larissa
Neptune VII |

| 97±3 | ≈ 4.2 | moon of Neptune  | [116] * [lower-alpha 6][23]
Ursula
375 |

| 96.8±1.3 | 8.4±5.3 | belt asteroid type C | [118] * [112]
S/2018 (532037) 1  |  | ≈ 95 |  | moon of 2013 FY27 | [61]
Eugenia
45 | 50px|center  | 94±1 | 5.8±0.1 | belt asteroid type F; trinary | [84]
Hermione
121 |

| 94±3 | 5.0±0.3 | outer belt asteroid type C; binary | [119] * [112]
Daphne
41 | 50px|center  | 94±7 | 6.1±0.9 | belt asteroid type C; binary  | [84]
Aurora
94 |

| 6.2±3.6 | belt asteroid type C | [120] * [112]
Bertha
154 | 50px|center  | 93.4±0.9 | belt asteroid type C | [112] * [112]
Janus
Saturn X |

| 89.5±1.4 | 1.898±0.001 | moon of Saturn  | [57] * [57]
Teharonhiawako
88611 |

| 89+16
−18 | cubewano; binary | [59] * [121]
Aegle
96 |  | 88.9±0.8 | 6.4±6.3 | belt asteroid type T | [111] * [112]
Galatea
Neptune VI |

| 88±4 | 2.12±0.08 | moon of Neptune  | [116] * [122][23]
Phorcys
Ceto I |

| 87+8
−9 | ≈ 1.67 | secondary of 65489 Ceto | [113] * [113]
Palma
372 |

| 5.2±0.6 | belt asteroid type B | [123] * [112]
Metis
9 |

| 86.5±1 | 8.0±1.9 | belt asteroid type S | [111] * [112]
Alauda
702 |

| 86±28 | belt asteroid type C; binary | [123] * [124]
Hilda
153 |

| 85.3±1.6 |  | outer belt asteroid; Hildas  | [114]
Himalia
Jupiter VI |

| 85 | 4.2±0.6 | moon of Jupiter  | [5] * [125]
Namaka
Haumea II |

| ≈ 85 | 1.8±1.5 | moon of Haumea  | [36] * [36]
Weywot
Quaoar I |

| ≈ 85 | < ≈ 5 | moon of 50000 Quaoar |
Freia
76 |

| 84.2±1.0 | outer belt asteroid type P/type X  | [118] * [112]
Amalthea
Jupiter V |

| 83.45±2.4 | 2.08±0.15 | moon of Jupiter  | [126] * [127][23]
Agamemnon
911 |

| 83.3±2.0 |  | Jupiter trojan (L4) type D  | [114]
Elpis
59 |  | 82.6±2.3 | 3±0.5 | belt asteroid type CP/type B | [111] * [112]
Eleonora
354 | 50px|center  | 82.5±1.5 | 7.5±2.7 | belt asteroid type A  | [84]
Nemesis
128 | 50px|center  | 81.5±2.5 | 3.4±1.7 | belt asteroid type C | [84]
Puck
Uranus XV |

| 81±2 |  | moon of Uranus
S/2015 (136472) 1
Makemake I |

| ≈ 80 |  | moon of Makemake  | [128]
Sycorax
Uranus XVII |

| 78.5+11.5
−7.5 |  | moon of Uranus  | [129]

85 |

| 2.6±1.5 | belt asteroid type FC/type B | [114] * [112]
Minerva
93 |

| 77.08±0.65 | 3.5±0.4 | belt asteroid type C; trinary | [111] * [112]
Alexandra
54 |

| 77.07±0.32 | belt asteroid type C | [111] * [112]
Laetitia
39 |  | 77±2 | 4.7±1.1 | belt asteroid type S | [112] * [112]
Nemausa
51 |

| 75±1.5 | 3.9±1.6 | belt asteroid type G  | [84]
Kalliope
22 | 50px|center  | 75±2.5 | 7.7±0.4 | belt asteroid type M; binary | [84]
Despina
Neptune V |

| 75±3 |  | moon of Neptune  | [23]
Manwë
385446 |

| ≈ 75 | ≈ 1.41 | resonant KBO (4:7); binary  | [130] * [130]
Pales
49 |  | ≈ 74.9 | 4.2±2.2 | belt asteroid type C | [114] * [112]
Parthenope
11 | 50px|center  | 74.5±1 | 5.5±0.4 | belt asteroid type S | [84]
Arethusa
95 |

| 74.0±2.4 |  | belt asteroid type C | [120]
Pulcova
762 |

| 73.7±0.4 | 1.4±0.1 | belt asteroid type F; binary | [111] * [131]
Flora
8 | 50px|center  | 73±1 | 4.0±1.6 | belt asteroid type S | [84]
Ino
173 | 50px|center  | 72.5±1.5 | 2.2±1.3 | belt asteroid type Xc  | [84]
Adeona
145 | 50px|center  | 72±1.5 | 2.4±0.3 | belt asteroid type Xc  | [84]
Irene
14 |

| 72±1 | 2.9±1.9 | belt asteroid type S | [118] * [112]
Melpomene
18 | 50px|center  | 70.5±1 | 4.5±0.9 | belt asteroid type S | [84]
Lamberta
187 | 50px|center  | 70.5±1 | 1.9±0.3 | belt asteroid type Ch | [84]
Aglaja
47 |  | 71±4 | 3.2±1.7 | belt asteroid type C | [112] * [112]
Patroclus
617 |

| 70.2±0.4 | 1.36±0.11 | Jupiter trojan (L5) type P; binary | [111] * [112]
Julia
89 |

| 70±1.4 | 4.3±3.2 | belt asteroid type S | [84]
Typhon
42355 |

| 69±4.5 | 0.87±0.03 | resonant SDO (7:10); binary | [115] * [132]
Massalia
20 |

| 67.8±1.8 | 5±1.04 | belt asteroid type S | [123] * [112]
Portia
Uranus XII |

| 67.6±4 |  | moon of Uranus  | [5]
Emma
283 |

| 66.2±0.1 | 1.38±0.03 | belt asteroid type X; binary | [111] * [112]
Paha
Lempo I |

| 66+4
−4.5 | 0.746±0.001 | moon of 47171 Lempo | [105] * [133]
Lucina
146 |

| 65.9±?  |  | belt asteroid type C | [134]
Sawiskera
Teharonhiawako I |

| 65.5+12
−13 |  | secondary of 88611 Teharonhiawako | [59]
Achilles
588 |

| 65.0±0.3 |  | Jupiter trojan (L4) type DU  | [111]
Panopaea
70 |  | 64.0±0.4 | 4.33±1.09 | belt asteroid type C | [111] * [112]
Thule
279 |  | 63.3±1.8 |  | outer belt asteroid type D | [114]
Borasisi
66652 |

| 63+12.5
−25.5 | 3.433±0.027 | cubewano; binary | [59] * [135]
Hestia
46 |  | 62.07±1.7 | 3.5 | belt asteroid type P/type Xc  | [114] * [136]
Leto
68 |

| 61.3±1.6 | 3.28±1.9 | belt asteroid type S | [111] * [112]
Undina
92 |  | 60.46±0.85 | 4.43±0.25 | belt asteroid type X  | [118] * [112]
Bellona
28 |

| 60.45±1.90 | 2.62±0.15 | belt asteroid type S | [137] * [112]
Diana
78 |  | 60.30±1.35 | 1.27±0.13 | belt asteroid type C | [138] * [112]
Anchises
1173 |

| 60.2±1.5 |  | Jupiter trojan (L5) type P | [118]
Bernardinelli-Bernstein
C/2014 UN271 |

| 60±7 |  | comet | [139]
Galatea
74 |  | 59.4±1.4 | 6.13±5.36 | belt asteroid type C | [140] * [112]
Deiphobus
1867 |  | 59.1±0.8 |  | Jupiter trojan (L5) type D | [141]
Äneas
1172 |  | 59.01±0.40 |  | Jupiter trojan (L5) type D  | [142]
Kleopatra
216 |

| 59±1 | 3.0±0.3 | belt asteroid type M; trinary | [84]
Athamantis
230 |

| 59±1 | 2.3±1.1 | belt asteroid type S | [84]
Diomedes
1437 |

| 58.89±0.59 |  | Jupiter trojan (L4) type D  | [143]
Terpsichore
81 |  | 58.9±0.4 | 6.19±5.31 | belt asteroid type C | [144] * [112]
Epimetheus
Saturn XI |

| 58.1±1.8 | 0.5266±0.0006 | moon of Saturn  | [57] * [57]
Victoria
12 |

| 58±1 | 2.7±1.3 | belt asteroid type S | [84]
Circe
34 |

| 57.7±1.0 | ≈ 3.66±0.03 | belt asteroid type C | [111] * [112]
Leda
38 |

| 57.7±0.7 | 5.71±5.47 | belt asteroid type C | [112] * [112]
Odysseus
1143 |  | 57.3±0.3 |  | Jupiter trojan (L4) type D | [145]
Alcathous
2241 |  | 56.8±0.9 |  | Jupiter trojan (L5) type D | [146]
Melete
56 |

| 56.62±0.85 | 4.61 | belt asteroid type P | [114] * [112]
Mnemosyne
57 |  | 56.3±1.4 | ≈ 12.6±2.4 | belt asteroid type S | [147] * [112]
Nestor
659 |  | 56.2±0.9 |  | Jupiter trojan (L4) type XC | [148]
Harmonia
40 |

| 55.6±0.2 |  | belt asteroid type S | [149]
Leleākūhonua
541132 |  | 55+7
−5 |  | sednoid | [150]
Euterpe
27 |

| 54.9±0.8 | 1.67±1.01 | belt asteroid type S | [118] * [112]
Antilochus
1583 |  | 54.4±0.3 |  | Jupiter trojan (L4) type D | [111]
Thorondor
Manwë I |

| 54 | 0.5 | secondary of 385446 Manwë | [130] * [130]
Thalia
23 |

| 53.8±1.1 | 1.96±0.09 | belt asteroid type S | [151] * [112]
Erato
62 |

| 53.5±0.3 |  | belt asteroid type BU/type Ch | [152]
Astraea
5 |

| 53.3±1.6 | 2.9 | belt asteroid type S | [153] * [136]
Pabu
Borasisi I |

| 52.5+10
−21 |  | secondary of 66652 Borasisi | [59]
Eos
221 |  | 51.76±2.8 | ≈ 5.87±0.34 | belt asteroid type S/type K | [112] * [112]
Aegina
91 |  | 51.7±0.2 |  | belt asteroid type C | [154]
Leukothea
35 |

| 51.5±0.6 |  | belt asteroid type C | [155]
Menoetius
Patroclus I |

| 51.4±0.25 |  | secondary of 617 Patroclus | [156]
Isis
42 |

| 51.4±1.4 | 1.58±0.52 | belt asteroid type S | [112] * [112]
Klotho
97 |

| 50.4±0.3 | 1.33±0.13 | belt asteroid type M | [111] * [112]
Troilus
1208 |

| 50.3±0.5 |  | Jupiter trojan (L5) type FCU | [157]

### 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.[158] 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.[112][159]

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  | [160]
Pholus
5145 |  | 49.5+7.5
−7 |  | centaur | [115]
Thebe
Jupiter XIV |

| 49.3±2 |  | moon of Jupiter  | [126]
Lutetia
21 |

| 49±1 | 1700±20 | belt asteroid type M | [84]
Kalypso
53 |

| 48.631±13.299 | ≈ 5630±5000 | belt asteroid type XC | [161] * [112]
Notburga
626 |

| 48.42±2.335 |  | belt asteroid type XC | [112]
Proserpina
26 |

| 47.4±0.85 | 748±895 | belt asteroid type S | [162] * [112]
Juliet
Uranus XI |

| 46.8±4 |  | moon of Uranus  | [5]
Urania
30 |

| 44±1 | 1300±900 | belt asteroid type S | [84]
Ausonia
63 |

| 46.5±1.5 | 1200±200 | belt asteroid type S | [84]
Beatrix
83 |  | 44.819±1.326 |  | belt asteroid type X | [111]
Concordia
58 |  | 44.806±0.419 |  | belt asteroid type C | [111]
Echidna
Typhon I |

| 44.5±3 |  | moon of 42355 Typhon | [132]
Automedon
2920 |  | 44.287±0.898 |  | Jupiter trojan (L4) type D  | [163]
Antiope
90 |  | 43.9±0.5 | 828±22 | belt asteroid type C; binary  | [164] * [164]
Prometheus
Saturn XVI |

| 43.1±2.7 | 159.5±1.5 | moon of Saturn  | [57] * [57]
Danaë
61 |  | 42.969±1.076 | 2890±2780 | belt asteroid type S | [165] * [112]
Thetis
17 |

| 42.449±1.014 | 1200 | belt asteroid type S | [166] * [159]
Pandora
55 |

| 42.397±1.251 |  | belt asteroid type M | [167]
Huenna
379 |  | 42.394±0.779 | 383±19 | belt asteroid type B/type C; binary  | [168] * [169]
Virginia
50 |  | 42.037±0.121 | 2310±700 | belt asteroid type X/type Ch | [170] * [112]
Feronia
72 |

| 41.975±2.01 | ≈ 3320±8490 | belt asteroid type TDG | [112] * [112]
S/2000 (90) 1
Antiope I |  | 41.9±0.5 |  | secondary of 90 Antiope | [164]
Poulydamas
4348 |  | 41.016±0.313 |  | Jupiter trojan (L5) type C | [171]
Logos
58534 |

| 41±9 | 458±6.9 | cubewano; binary  | [172] * [172]
Pandora
Saturn XVII |

| 40.7±1.5 | 137.1±1.9 | moon of Saturn  | [57] * [57]
Thalassa
Neptune IV |

| 40.7±2.8 |  | moon of Neptune  | [116]
Niobe
71 |

| 40.43±0.4 |  | belt asteroid type S | [118]
Pomona
32 |

| 40.38±0.8 |  | belt asteroid type S | [173]
Belinda
Uranus XIV |

| 40.3±8 |  | moon of Uranus  | [5]
Elara
Jupiter VII |

| 39.95±1.7 |  | moon of Jupiter  | [174]
Cressida
Uranus IX |

| 39.8±2 |  | moon of Uranus  | [5]
Amycus
55576 |  | 38.15±6.25 |  | centaur | [93]
Hylonome
10370 |

| 37.545 |  | centaur | [175]
Socus
3708 |  | 37.831±0.404 |  | Jupiter trojan (L5) type C | [111]
Nysa
44 |

| 37.83±0.37 |  | belt asteroid type E | [118]
Rosalind
Uranus XIII |

| 36±6 |  | moon of Uranus  | [5]
Maja
66 |

| 35.895±0.46 |  | belt asteroid type C | [118]
Ariadne
43 |

| 35.67±0.627 | ≈ 1210±220 | belt asteroid type S | [176] * [112]
Iphigenia
112 |  | 35.535±0.26 | ≈ 1970±6780 | belt asteroid type C | [112] * [112]
Xiangliu
Gonggong I |  | ≈ 35±15 |  | moon of (225088) Gonggong  |
Dike
99 |

| 33.677±0.208 |  | belt asteroid type C | [177]
Echeclus
60558 or 174P |  | 32.3±0.8 |  | centaur | [115]
Desdemona
Uranus X |

| 32±4 |  | moon of Uranus  | [5]
Eurybates
3548 |

| 31.943±0.149 |  | Jupiter trojan (L4) type CP | [111]
Eurynome
79 |

| 31.739±0.476 |  | belt asteroid type S | [178]
Eurydike
75 |  | 31.189±0.802 |  | belt asteroid type M | [179]
Halimede
Neptune IX |

| ≈ 31 |  | moon of Neptune  | [5]
Phocaea
25 |

| 30.527±1.232 | 599±60 | belt asteroid type S | [111] * [112]
Naiad
Neptune III |

| 30.2±3.2 |  | moon of Neptune  | [116]
Schwassmann–
Wachmann 1
29P |

| 30.2±3.7 |  | comet | [180]
Neso
Neptune XIII |

| ≈ 30 |  | moon of Neptune  | [5]
Angelina
64 |

| 29.146±0.541 |  | belt asteroid type E  | [181]
Pasiphae
Jupiter VIII |

| 28.9±0.4 |  | moon of Jupiter  | [174]
Alkmene
82 |

| 28.811±0.357 |  | belt asteroid type S | [182]
Nessus
7066 |

| 28.5±8.5 |  | centaur | [115]
Polana
142 |  | 27.406±0.139 |  | belt asteroid type F  | [183]
Bianca
Uranus VIII |

| 27±2 |  | moon of Uranus  | [5]
Mathilde
253 |

| 26.4 | 103.3±4.4 | belt asteroid type C | [184] * [185]
Hidalgo
944 |

| 26.225±1.8 |  | centaur | [118]
Orus
21900 |

| 25.405±0.405 |  | Jupiter trojan (L4) type C/type D  | [111]
Amalthea
113 |  | 25.069±0.633 |  | belt asteroid type S; binary  | [111]
Prospero
Uranus XVIII |

| ≈ 25 |  | moon of Uranus  | [5]
Setebos
Uranus XIX |

| ≈ 24 |  | moon of Uranus  | [5]
Carme
Jupiter XI |

| 23.35±0.45 |  | moon of Jupiter  | [174]
Klytia
73 |

| 22.295±0.471 |  | belt asteroid type S | [186]
Sao
Neptune XI |

| ≈ 22 |  | moon of Neptune  | [5]
Echo
60 |

| 21.609±0.286 | 315±32 | belt asteroid type S | [187] * [112]
Metis
Jupiter XVI |

| 21.5±2 | ≈ 119.893 | moon of Jupiter  | [126] * [188]
Ophelia
Uranus VII |

| 21.4±4 |  | moon of Uranus  | [5]
Lysithea
Jupiter X |

| 21.1±0.35 |  | moon of Jupiter  | [174]
Caliban
Uranus XVI |

| 21+10
−6 |  | moon of Uranus  | [129]
Laomedeia
Neptune XII |

| ≈ 21 |  | moon of Neptune  | [5]
Cordelia
Uranus VI |

| 20.1±3 |  | moon of Uranus  | [5]
Psamathe
Neptune X |

| ≈ 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 |

| 19.968±0.132 |  | belt asteroid type S | [189]
Hydra
Pluto III |

| 19.65 | 48±42 | moon of Pluto  | [190] * [191]
Siarnaq
Saturn XXIX |

| 19.65±2.95 |  | moon of Saturn  | [174]
Koronis
158 |

| 19.513±0.231 |  | belt asteroid type S | [192]
Nix
Pluto II |

| 19.017 | 45±40 | moon of Pluto  | [190] * [191]
Ganymed
1036 |

| 18.838±0.199 | ≈ 167±318 | Amor asteroid type S | [111] * [112]
Okyrhoe
52872 |  | 18±0.6 |  | centaur | [193]
Helene
Saturn XII |

| 17.6±0.4 |  | moon of Saturn; Dione trojan (L4)  | [57]
Sinope
Jupiter IX |

| 17.5±0.3 |  | moon of Jupiter  | [174]
Hippocamp
Neptune XIV |

| 17.4±1 | ≈ 50 | moon of Neptune  | [116] * [116]
Leucus
11351 |

| 17.078±0.323 |  | Jupiter trojan (L4) type D | [111]
Stephano
Uranus XX |

| ≈ 16 |  | moon of Uranus  | [5]
Arrokoth
486958 |

| 15.85±0.25 |  | cubewano; contact binary | [194]
Ida
243 |

| 15.7 | 42±6 | belt asteroid type S; binary  | [195] * [196]
Atlas
Saturn XV |

| 15.1±0.9 | 6.6 | moon of Saturn  | [57] * [57]
Ananke
Jupiter XII |

| 14.55±0.3 |  | moon of Jupiter  | [174]
Albiorix
Saturn XXVI |

| 14.3±2.7 |  | moon of Saturn  | [174]
Pan
Saturn XVIII |

| 14.1±1.3 | 4.95 | moon of Saturn  | [57] * [197]
Linus
Kalliope I |  | 14±1 | ≈ 60 | asteroid moon of 22 Kalliope | [198] * [199]
Dioretsa
20461 |  | 14±3 |  | centaur; damocloid  | [200]
Perdita
Uranus XXV |

| 13±1 |  | moon of Uranus  | [5]
Telesto
Saturn XIII |

| 12.4±0.4 |  | moon of Saturn; Tethys trojan (L4)  | [57]
Mab
Uranus XXVI |

| 12±1 |  | moon of Uranus  | [5]
Phobos
Mars I |

| 11.1±0.15 | 10.659 | moon of Mars  | [201] * [202]
Paaliaq
Saturn XX |

| ≈ 11 |  | moon of Saturn  | [5]
Francisco
Uranus XXII |  | ≈ 11 |  | moon of Uranus  | [5]
Leda
Jupiter XIII |

| 10.75±0.85 |  | moon of Jupiter  | [174]
Calypso
Saturn XIV |

| 10.7±0.7 |  | moons of Saturn; Tethys trojan (L5)  | [57]
Polymele
15094 |

| 10.548±0.068 |  | Jupiter trojan (L4) type P | [114]
Margaret
Uranus XXIII |

| ≈ 10 |  | moon of Uranus  | [5]
Ferdinand
Uranus XXIV |

| ≈ 10 |  | moon of Uranus  | [5]
Cupid
Uranus XXVII |

| 9±1 |  | moon of Uranus  | [5]
Ymir
Saturn XIX |

| ≈ 9 |  | moon of Saturn  | [5]
Trinculo
Uranus XXI |  | ≈ 9 |  | moon of Uranus  | [5]
Eros
433 |

| 8.42±0.02 | 6.687±0.003 | Amor asteroid type S | [203] * [203]
Adrastea
Jupiter XV |

| 8.2±2 |  | moon of Jupiter  | [5]
Kiviuq
Saturn XXIV |

| ≈ 8 |  | moon of Saturn  | [5]
Tarvos
Saturn XXI |

| ≈ 7.5 |  | moon of Saturn  | [5]
Kerberos
Pluto IV |

| ≈ 6.333 | 16±9 | moon of Pluto  | [204] * [205]
Gaspra
951 |

| 6.266 | 20–30 | belt asteroid type S
Deimos
Mars II |

| 6.2±0.18 | 1.476 | moon of Mars  | [5] * [206]
Skamandrios
Hektor I |  | 6±1.5 |  | asteroid moon of 624 Hektor | [109]
Ijiraq
Saturn XXII |

| ≈ 6 |  | moon of Saturn  | [5]
Halley's Comet
1P |

| 5.75 | 0.22 | comet | [207] * [208]
Styx
Pluto V |

| ≈ 5.5 | ≈ 7.65 | moon of Pluto  | [204] * [205]
Romulus
Sylvia I |

| 5.4±2.8 |  | asteroid moon of 87 Sylvia | [209]
Masursky
2685 |

| 5.372±0.085 |  | belt asteroid type S | [210]
Erriapus
Saturn XXVIII |

| ≈ 5 |  | moon of Saturn  | [5]
Callirrhoe
Jupiter XVII |

| 4.8±0.65 |  | moon of Jupiter  | [174]
Alexhelios
Kleopatra I |

| 4.45±0.8 |  | asteroid moon of 216 Kleopatra | [211]
Esclangona
1509 |  | 4.085±0.3 |  | inner belt asteroid type S; binary | [212]
Themisto
Jupiter XVIII |

| ≈ 4 |  | moon of Jupiter  | [5]
Daphnis
Saturn XXXV |

| 3.8±0.8 | 0.077±0.015 | moon of Saturn  | [57] * [57]
Petit-Prince
Eugenia I |  | 3.5±1 |  | asteroid moon of 45 Eugenia | [213]
Praxidike
Jupiter XXVII |

| 3.5±0.35 |  | moon of Jupiter  | [174]
Bestla
Saturn XXXIX |

| ≈ 3.5 |  | moon of Saturn  | [5]
Remus
Sylvia II |

| ≈ 3.5 |  | asteroid moon of 87 Sylvia | [209]
Kalyke
Jupiter XXIII |

| 3.45±0.65 |  | moon of Jupiter  | [174]
Cleoselene
Kleopatra II |

| 3.45±0.8 |  | asteroid moon of 216 Kleopatra | [211]
S/2019 (31) 1
Euphrosyne I |  | 3.35±1.2 |  | asteroid moon of 31 Euphrosyne | [214]
Tempel 1
9P |

| 3±0.1 |  | Jupiter-family comet; Deep Impact flyby and impacted | [215]
Phaethon
3200 |

| 2.9 |  | Apollo asteroid type F | [216]
1999 JM8
53319 |

| 2.7±0.6 |  | Apollo asteroid type X | [217]
Borrelly
19P |

| 2.66 |  | Jupiter-family comet  | [218]
Šteins
2867 |

| 2.58±0.084 |  | belt asteroid type E | [111]
Atira
163693 |

| 2.4±0.25 |  | Atira asteroid type S; binary | [219]
Annefrank
5535 |

| 2.4 |  | belt asteroid type S | [220]
Balam
3749 |

| 2.332±0.107 | 0.51±0.02 | belt asteroid type S; trinary | [221] * [222]
Pallene
Saturn XXXIII |

| 2.22±0.07 |  | moon of Saturn  | [223]
Florence
3122 |

| 2.201±0.015 | 0.079±0.002 | Amor asteroid type S; trinary | [120] * [224]
Wild 2
81P |

| 2.133 |  | Jupiter family comet  | [225]
Litva
2577 |  | 2.115 |  | Mars-crosser type EU; trinary | [226]
Churyumov–Gerasimenko
67P |

| 2 | 0.00998 | Jupiter-family comet  | [227] * [228]
Donaldjohanson
52246 |  | 1.948±0.007 |  | belt asteroid type C | [229]
Cuno
4183 |

| 1.826±0.051 |  | Apollo asteroid type S/type Q | [230]
1986 DA
6178 |  | 1.575 |  | Amor asteroid type M | [231]
Pichi üñëm
Alauda I |  | 1.55±0.45 |  | asteroid moon of 702 Alauda | [232]
Toutatis
4179 |

| 1.516 | 0.0505 | Apollo asteroid type S | [233] * [233]
Methone
Saturn XXXII |

| 1.45±0.03 |  | moon of Saturn  | [223]
Carpo (moon)
Jupiter XLVI |  | 1.44 |  | Moon of Jupiter
1998 QE2
285263 |

| 1.375 |  | Amor asteroid type S; binary | [234]
Polydeuces
Saturn XXXIV |

| 1.3±0.4 |  | moon of Saturn; Dione trojan (L5)  | [57]
2001 SN263
153591 |

| 1.315±0.2 | 0.00951±0.00013 | Amor asteroid type C; trinary | [235] * [236]
S/2003 (1509) 1
Esclangona I |  | 1.285 |  | asteroid moon of 1509 Esclangona | [237]
APL
132524 |

| ≈ 1.25 |  | belt asteroid type S | [238]
Camillo
3752 |

| 1.153±0.044 |  | Apollo asteroid type S | [120]
Cruithne
3753 |

| 1.036±0.053 |  | Aten asteroid type Q; quasi-satellite of Earth  | [239]

### 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,[240] 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.)

Body[note 1] | Image  | Radius[note 2]
(m) | Mass
(109 kg)  | Type – notes  | Refs[note 5]
r * M

|
|
|
|
|

Ra-Shalom
2100 |

| 990±25 |  | Aten asteroid type C | [118]
Geographos
1620 |

| 980±30 |  | Apollo asteroid type S | [111]
Midas
1981 |  | 975±35 |  | Apollo asteroid type S | [118]
Mithra
4486 |  | 924.5±11 |  | Apollo asteroid type S | [120]
1998 OH
12538 |  | 831.5±164.5 |  | Apollo asteroid type S | [120]
Tantalus
2102 |

| 824.5±22.5 |  | Apollo asteroid type Q | [241]
Braille
9969 |

| 820 |  | Mars-crosser type Q | [242]
2005 GO21
308242 |

| 780 |  | Aten asteroid type S | [243]
Apollo
1862 |

| ≈ 750 |  | Apollo asteroid type Q | [244]
1999 JD6
85989 |

| 731±10.5 |  | Aten asteroid type K; contact binary | [245]
Icarus
1566 |

| 730 |  | Apollo asteroid type S | [246]
Dactyl
Ida I |

| 700 |  | asteroid moon of 243 Ida | [247]
Castalia
4769 |  | 700 |  | Apollo asteroid type S; contact binary | [248]
2007 PA8
214869 |

| 675±70 |  | Apollo asteroid type Q | [249]
Moshup
66391 |

| 658.5±20 | 2490±54 | Aten asteroid type S; binary  | [250] * [251]
1950 DA
29075 |

| 653 | ≈ 2000 | Apollo asteroid type S | [252] * [253]
2006 HY51
394130 |  | 609±114 |  | Apollo asteroid | [254]
Hartley 2
103P |

| 570±80 | ≈ 300 | Jupiter-family comet  | [255] * [255]
2003 SD220
163899 |

| 515 |  | Aten asteroid type S | [256]
Nyx
3908 |

| 500±75 |  | Amor asteroid type V | [257]
2001 WN5
153814 |  | 466±5.5 |  | Apollo asteroid | [258]
2017 YE5 |

| 450±25 |  | Apollo asteroid type S; binary | [259]
Ryugu
162173 |

| 432.5±7.5 | ≈ 450 | Apollo asteroid type Cg | [260] * [261]
1997 AE12
162058 |

| 423.5±6.5 |  | Amor asteroid type S | [262]
2014 JO25 |

| 409 |  | Apollo asteroid type S; contact binary | [263]
Hermes
69230 |

| 400±50 |  | Apollo asteroid type Sq | [264]
Didymos
65803 |

| 390±4 | 527 | Apollo asteroid type Xk; binary | [265] * [266]
Aten
2062 |  | 365±15 |  | Aten asteroid type S | [111]
Aegaeon
Saturn LIII |

| 330±60 |  | moon of Saturn  | [223]
2015 TB145 |

| 325±15 |  | Apollo asteroid type S | [267]
1994 CC
136617 |

| 310±30 | 266±32.9 | Apollo asteroid type Sq; trinary | [268] * [269]
2001 WR1
172034 |  | 315.5±9 |  | Amor asteroid type S | [270]
Golevka
6489 |

| 265±15 |  | Apollo asteroid type Q | [271]
Bennu
101955 |

| 262.5±37.5 | 78±9 | Apollo asteroid type B | [272] * [273]
2000 WO107
153201 |

| 255±41.5 |  | Aten asteroid type X | [274]
2002 CU11
163132 |  | 230±8.5 |  | Apollo asteroid | [275]
Squannit
Moshup I |

| 225.5±13.5 |  | asteroid moon of 66391 Moshup | [251]
2014 HQ124 |

| 204.5±84 |  | Aten asteroid type S | [111]
2013 YP139 |

| 201±13 |  | Apollo asteroid | [276]
2008 EV5
341843 |

| 200±7 |  | Aten asteroid type X/type C | [120]
2006 DP14
388188 |

| ≈ 200 |  | Apollo asteroid type S; contact binary | [277]
1988 EG
6037 |  | 199.5±1.35 |  | Apollo asteroid type S | [278]
2010 TK7 |

| 189.5±61.5 |  | Aten asteroid; Earth trojan (L4)  | [279]
2006 SU49
292220 |  | ≈ 188.5 | ≈ 73 | Apollo asteroid  | [280] * [280]
2005 YU55
308635 |

| 180±20 |  | Apollo asteroid type C | [281]
2010 SO16 |  | 178.5±63 |  | Apollo asteroid; co-orbital with Earth  | [276]
Itokawa
25143 |

| 173 | 35.1±1.05 | Apollo asteroid type S | [282] * [282]
Apophis
99942 |

| 162.5±7.5 | ≈ 61 | Aten asteroid type Sq | [283] * [284]
S/2009 S 1  |

| ≈ 150 |  | moon of Saturn  | [285]
2005 WK4 |

| 142 |  | Apollo asteroid type S | [286]
2004 BL86
357439 |

| 131.5±13 |  | Apollo asteroid type V; binary | [287]
2007 TU24 |

| 125 |  | Apollo asteroid type S | [288]
2002 VE68 |  | ≈ 118 |  | Aten asteroid type X; co-orbital with Venus  | [289]
2011 UW158
436724 |

| 110±20 |  | Apollo asteroid type S | [290]
Dimorphos
Didymos I |  | 85±15 |  | asteroid moon of 65803 Didymos | [266]
2017 BQ6 |

| 78 |  | Apollo asteroid type S | [291]
YORP
54509 |

| 61.8 |  | Apollo asteroid type S | [292]
Kamoʻoalewa
469219 |  | 41 |  | Apollo asteroid type S; quasi-satellite of Earth  | [293]
Duende
367943 |

| 23.75 |  | Aten asteroid type L | [294]
1998 KY26 |

| ≈ 15 |  | Apollo asteroid type X | [295]
2012 TC4 |

| 11.5 |  | Apollo asteroid type E/type Xe | [296]
2014 RC |

| ≈ 11 |  | Apollo asteroid type Sq | [297]
2010 RF12 |  | ≈ 3.5 | ≈ 0.0005 | Apollo asteroid  | [298]
2011 MD |

| 3+2
−1 |  | Apollo asteroid/Amor asteroid type S | [299]
2008 TC3 |

| 2.05 | 0.00008 | Apollo asteroid type F/type M | [300] * [300]
2023 BU |  | 1.5 |  | Apollo asteroid | [301]
2008 TS26 |  | ≈ 0.49 |  | Apollo asteroid | [302]

## 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.

Largest moons of the Solar System to scale.

## See also

* List of gravitationally rounded objects of the Solar System
* List of dwarf planets
* List of minor planets
* List of natural satellites
* List of near-Earth asteroids by distance from Sun
* List of Solar System objects most distant from the Sun
* List of space telescopes
* Lists of astronomical objects

## Notes

1. ↑ 1.0 1.1 1.2 1.3 1.4 Radius estimated using equatorial radius and assuming body is spherical
2. ↑ 2.0 2.1 Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft
3. ↑ Calculated in Wolfram Alpha using semi axes of 1050 × 840 × 537 (Ellipsoid volume: 1.98395×10^9 km3)
4. ↑ Best fit, assuming Haumea is in hydrostatic equilibrium
5. ↑ 5.0 5.1 5.2 Radius estimated by using three radii and assuming body is spheroid
6. ↑ 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).[117]

1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets
2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Mean radius including uncertainties
3. ↑ Given as surface gravity (1 bar for gaseous planets)
4. ↑ Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,[58] if otherwise not mentioned in the References column
5. ↑ 5.0 5.1 5.2 5.3 5.4 5.5 Reference column specifically for radius (r) and mass (M) citations

## References

1. ↑ Brown, M.. "The Dwarf Planets". Caltech. http://www.gps.caltech.edu/~mbrown/dwarfplanets/.
2. ↑ "Iapetus' peerless equatorial ridge". The Planetary Society. https://www.planetary.org/blogs/emily-lakdawalla/2012/3389.html.
3. ↑ "Gǃkúnǁ'hòmdímà and Gǃò'é ǃhú". .lowell.edu. http://www2.lowell.edu/~grundy/abstracts/2019.G-G.html.
4. ↑ Britt, D. T.; Consolmagno, G. J.; Merline, W. J. (2006). "Small Body Density and Porosity: New Data, New Insights". Lunar and Planetary Science XXXVII. http://www.lpi.usra.edu/meetings/lpsc2006/pdf/2214.pdf.
5. ↑ 5.00 5.01 5.02 5.03 5.04 5.05 5.06 5.07 5.08 5.09 5.10 5.11 5.12 5.13 5.14 5.15 5.16 5.17 5.18 5.19 5.20 5.21 5.22 5.23 5.24 5.25 5.26 5.27 5.28 5.29 5.30 5.31 5.32 5.33 5.34 5.35 5.36 5.37 5.38 5.39 5.40 5.41 "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 2008-10-24. http://ssd.jpl.nasa.gov/?sat_phys_par.
6. ↑ Williams, D. R. (2007-11-23). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html.
7. ↑ 7.0 7.1 7.2 Brown, Michael E.. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. http://web.gps.caltech.edu/~mbrown/dps.html.
8. ↑ Park, R. S.; Konopliv, A. S.; Bills, B. G.; Rambaux, N.; Castillo-Rogez, J. C.; Raymond, C. A.; Vaughan, A. T.; Ermakov, A. I. et al. (2016). "A partially differentiated interior for (1) Ceres deduced from its gravity field and shape". Nature 537 (7621): 515–517. doi:10.1038/nature18955. PMID 27487219. Bibcode: 2016Natur.537..515P.
9. ↑ "Iapetus' peerless equatorial ridge". http://www.planetary.org/blogs/emily-lakdawalla/2012/3389.html.
10. ↑ 10.0 10.1 Grundy, W.M.; Noll, K.S.; Buie, M.W.; Benecchi, S.D.; Ragozzine, D.; Roe, H.G. (December 2019). "The mutual orbit, mass, and density of transneptunian binary Gǃkúnǁʼhòmdímà ((229762) 2007 UK126)". Icarus 334: 30–38. doi:10.1016/j.icarus.2018.12.037. http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf.(229762)+2007+UK126)&rft.jtitle=Icarus&rft.aulast=Grundy&rft.aufirst=W.M.&rft.au=Grundy, W.M.&rft.au=Noll, K.S.&rft.au=Buie, M.W.&rft.au=Benecchi, S.D.&rft.au=Ragozzine, D.&rft.au=Roe, H.G.&rft.date=December+2019&rft.volume=334&rft.pages=30–38&rft_id=info:doi/10.1016/j.icarus.2018.12.037&rft_id=http://www2.lowell.edu/~grundy/abstracts/preprints/2019.G-G.pdf&rfr_id=info:sid/en.wikibooks.org:Astronomy:List_of_Solar_System_objects_by_size">
11. ↑ "Uranus Fact Sheet". http://nssdc.gsfc.nasa.gov/planetary/factsheet/uranusfact.html.
12. ↑ "90377 Sedna". 12 September 2022. https://www.universeguide.com/kuiperbeltobject/316/sedna.
13. ↑ 13.00 13.01 13.02 13.03 13.04 13.05 13.06 13.07 13.08 13.09 13.10 NASA/JPL, Our Sun, by the numbers Accessed 2020 Oct 22
14. ↑ 14.00 14.01 14.02 14.03 14.04 14.05 14.06 14.07 14.08 14.09 14.10 14.11 14.12 14.13 14.14 14.15 14.16 14.17 14.18 14.19 14.20 14.21 14.22 14.23 14.24 14.25 14.26 14.27 14.28 14.29 14.30 14.31 NASA/JPL Planets and Pluto: Physical Characteristics Last updated 2020-May-29
15. ↑ "By The Numbers | Jupiter - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/jupiter/by-the-numbers/.
16. ↑ "By The Numbers | Saturn - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/saturn/by-the-numbers/.
17. ↑ "By The Numbers | Uranus - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/uranus/by-the-numbers/.
18. ↑ "By the Numbers | Neptune - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/neptune/by-the-numbers/.
19. ↑ "By The Numbers | Earth - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/earth/by-the-numbers/.
20. ↑ "By the Numbers | Venus - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/venus/by-the-numbers/.
21. ↑ "By The Numbers | Mars - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/mars/by-the-numbers/.
22. ↑ "By The Numbers | Ganymede - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/jupiter-moons/ganymede/by-the-numbers/.
23. ↑ 23.00 23.01 23.02 23.03 23.04 23.05 23.06 23.07 23.08 23.09 23.10 23.11 23.12 23.13 23.14 23.15 23.16 "Planetary Satellite Physical Parameters". https://ssd.jpl.nasa.gov/?sat_phys_par.
24. ↑ "By the Numbers | Titan - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/saturn-moons/titan/by-the-numbers/.
25. ↑ "By The Numbers | Mercury - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/mercury/by-the-numbers/.
26. ↑ "By The Numbers | Callisto - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/jupiter-moons/callisto/by-the-numbers/.
27. ↑ "By The Numbers | Io - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/jupiter-moons/io/by-the-numbers/.
28. ↑ 28.0 28.1 Planetary Satellite Physical Parameters
29. ↑ Moon Fact Sheet
30. ↑ "By The Numbers | Earth's Moon - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/earths-moon/by-the-numbers/.
31. ↑ "By The Numbers | Europa - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/jupiter-moons/europa/by-the-numbers/.
32. ↑ "By The Numbers | Triton - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/neptune-moons/triton/by-the-numbers/.
33. ↑ Sicardy, B. (2011). "Size, density, albedo and atmosphere limit of dwarf planet Eris from a stellar occultation". European Planetary Science Congress Abstracts 6: 137. Bibcode: 2011epsc.conf..137S. http://meetingorganizer.copernicus.org/EPSC-DPS2011/EPSC-DPS2011-137-8.pdf. Retrieved 2011-09-14.
34. ↑ Brown, Michael E.; Schaller, Emily L. (15 June 2007). "The Mass of Dwarf Planet Eris". Science 316 (5831): 1585. doi:10.1126/science.1139415. PMID 17569855. Bibcode: 2007Sci...316.1585B.
35. ↑ "The size, shape, density and ring of the dwarf planet Haumea". http://www.astrosurf.com/sogorb/occultations/nature24051.pdf.
36. ↑ 36.0 36.1 36.2 36.3 36.4 Ragozzine, D.; Brown, M. E. (2009). "Orbits and Masses of the Satellites of the Dwarf Planet Haumea (2003 EL61)". The Astronomical Journal 137 (6): 4766–4776. doi:10.1088/0004-6256/137/6/4766. Bibcode: 2009AJ....137.4766R.
37. ↑ Dunham, E. T.; Desch, S. J.; Probst, L. (April 2019). "Haumea's Shape, Composition, and Internal Structure". The Astrophysical Journal 877 (1): 11. doi:10.3847/1538-4357/ab13b3. Bibcode: 2019ApJ...877...41D.
38. ↑ "By The Numbers | Titania - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/uranus-moons/titania/by-the-numbers/.
39. ↑ "By The Numbers | Rhea - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/saturn-moons/rhea/by-the-numbers/.
40. ↑ "By The Numbers | Oberon - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/uranus-moons/oberon/by-the-numbers/.
41. ↑ M.E. Brown (2013). "On the size, shape, and density of dwarf planet Makemake". The Astrophysical Journal Letters 767 (1): L7(5pp). doi:10.1088/2041-8205/767/1/L7. Bibcode: 2013ApJ...767L...7B.
42. ↑ Kiss, Csaba; Marton, Gabor; Parker, Alex H.; Grundy, Will; Farkas-Takacs, Aniko; Stansberry, John; Pal, Andras; Muller, Thomas et al. (2019). "The mass and density of the dwarf planet (225088) 2007 OR10". Icarus 334: 3–10. doi:10.1016/j.icarus.2019.03.013. Bibcode: 2018DPS....5031102K.
Initial publication at the American Astronomical Society DPS meeting #50, with the publication ID 311.02
43. ↑ "By The Numbers | Charon -NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/pluto-moons/charon/by-the-numbers/.
44. ↑ "By The Numbers | Umbriel - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/uranus-moons/umbriel/by-the-numbers/.
45. ↑ "By The Numbers | Ariel - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/uranus-moons/ariel/by-the-numbers/.
46. ↑ "By The Numbers | Dione - NASA Solar System Exploration". https://solarsystem.nasa.gov/moons/saturn-moons/dione/by-the-numbers/.
47. ↑ , Wikidata Q116754015
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56. ↑ Rommel, Flavia L.; Braga-Ribas, Felipe; Vara-Lubiano, Mónica; Ortiz, Jose L.; Desmars, Josselin; Morgado, Bruno E.; Benedetti-Rossi, Gustavo; Sicardy, Bruno et al. (28 June 2021). "Evidence of topographic features on (307261) 2002 MS4 surface". European Planetary Science Congress. doi:10.5194/epsc2021-440. Bibcode: 2021EPSC...15..440R. https://meetingorganizer.copernicus.org/EPSC2021/EPSC2021-440.html.
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119. ↑ Johnston, Wm. Robert (21 September 2014). "(121) Hermione and S/2002 (121) 1 ("LaFayette")". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-00121.html.
120. ↑ 120.0 120.1 120.2 120.3 120.4 120.5 120.6 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M.
121. ↑ Johnston, Wm. Robert (20 September 2014). "(88611) Teharonhiawako and Sawiskera". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-88611.html.
122. ↑ Porco, C.C. (1991). "An Explanation for Neptune's Ring Arcs". Science 253 (5023): 995–1001. doi:10.1126/science.253.5023.995. PMID 17775342. Bibcode: 1991Sci...253..995P.
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124. ↑ Rojo, P.; Margot, J. L. (February 2011). "Mass and Density of the B-type Asteroid (702) Alauda". The Astrophysical Journal 727 (2): 5. doi:10.1088/0004-637X/727/2/69. Bibcode: 2011ApJ...727...69R.
125. ↑ Emelyanov, N.V. et al. (2005). "The mass of Himalia from the perturbations on other satellites". Astronomy and Astrophysics 438 (3): L33–L36. doi:10.1051/0004-6361:200500143. Bibcode: 2005A&A...438L..33E. https://www.aanda.org/articles/aa/pdf/2005/30/aahe201.pdf.
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127. ↑ Anderson, J. D.; Johnson, T. V.; Schubert, G.; Asmar, S.; Jacobson, R. A.; Johnston, D.; Lau, E. L.; Lewis, G. et al. (27 May 2005). "Amalthea's Density is Less Than That of Water". Science 308 (5726): 1291–1293. doi:10.1126/science.1110422. PMID 15919987. Bibcode: 2005Sci...308.1291A.
128. ↑ "In Depth | Makemake - NASA Solar System Exploration". https://solarsystem.nasa.gov/planets/dwarf-planets/makemake/in-depth/.
129. ↑ 129.0 129.1 Farkas-Takács, A.Expression error: Unrecognized word "etal". (September 2017). "Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations". The Astronomical Journal 154 (3): 13. doi:10.3847/1538-3881/aa8365. 119. Bibcode: 2017AJ....154..119F.
130. ↑ 130.0 130.1 130.2 130.3 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].
131. ↑ Johnston, Wm. Robert (21 September 2014). "(762) Pulcova". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-00762.html.
132. ↑ 132.0 132.1 Johnston, Wm. Robert (31 January 2015). "(42355) Typhon and Echidna". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-42355.html.
133. ↑ Benecchi, S.D; Noll, K. S.; Grundy, W. M.; Levison, H. F. (2010). "(47171) 1999 TC36, A Transneptunian Triple". Icarus 207 (2): 978–991. doi:10.1016/j.icarus.2009.12.017. Bibcode: 2010Icar..207..978B.
134. ↑ Pravec, P.; Harris, A. W.; Kusnirak, P.; Galad, A.; Hornoch, K. (2012). "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations". Icarus 221 (1): 365–387. doi:10.1016/j.icarus.2012.07.026. Bibcode: 2012LPICo1667.6089P.
135. ↑ Grundy, W. M.; Noll, K. S.; Nimmo, F.; Roe, H. G.; Buie, M. W.; Porter, S. B.; Benecchi, S. D.; Stephens, D. C. et al. (2011). "Five new and three improved mutual orbits of transneptunian binaries". Icarus 213 (2): 678. doi:10.1016/j.icarus.2011.03.012. Bibcode: 2011Icar..213..678G. http://es.ucsc.edu/~fnimmo/website/Grundy_KBO.pdf.
136. ↑ 136.0 136.1 Michalak, G. (2001). "Determination of asteroid masses". Astronomy & Astrophysics 374 (2): 703–711. doi:10.1051/0004-6361:20010731. Bibcode: 2001A&A...374..703M.
137. ↑ "JPL Small-Body Database Browser: 28 Bellona". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=28.
138. ↑ "JPL Small-Body Database Browser: 78 Diana". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=78.
139. ↑ Hui, Man-To; Jewitt, David; Yu, Liang-Liang; Mutchler, Max J. (12 Apr 2022). "Hubble Space Telescope Detection of the Nucleus of Comet C/2014 UN271 (Bernardinelli–Bernstein)". The Astrophysical Journal Letters 929 (L12): L12. doi:10.3847/2041-8213/ac626a. Bibcode: 2022ApJ...929L..12H.
140. ↑ "JPL Small-Body Database Browser: 74 Galatea". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=74.
141. ↑ "JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1867.
142. ↑ "JPL Small-Body Database Browser: 1172 Aneas (1930 UA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1172.
143. ↑ "JPL Small-Body Database Browser: 1437 Diomedes (1937 PB)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1437.
144. ↑ "JPL Small-Body Database Browser: 81 Terpsichore". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=81.
145. ↑ "JPL Small-Body Database Browser: 1143 Odysseus (1930 BH)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1143.
146. ↑ "JPL Small-Body Database Browser: 2241 Alcathous (1979 WM)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2241.
147. ↑ "JPL Small-Body Database Browser: 57 Mnemosyne". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=57.
148. ↑ "JPL Small-Body Database Browser: 659 Nestor (A908 FE)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=659.
149. ↑ "JPL Small-Body Database Browser: 40 Harmonia". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=40.
150. ↑ Buie, Marc W.Expression error: Unrecognized word "etal". (April 2020). "A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua". The Astronomical Journal 159 (5): 230. doi:10.3847/1538-3881/ab8630. 230. Bibcode: 2020AJ....159..230B.
151. ↑ "JPL Small-Body Database Browser: 23 Thalia". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=23.
152. ↑ "JPL Small-Body Database Browser: 62 Erato". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=62.
153. ↑ "JPL Small-Body Database Browser: 5 Astraea". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=5.
154. ↑ "JPL Small-Body Database Browser: 91 Aegina". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=91.
155. ↑ "JPL Small-Body Database Browser: 35 Leukothea". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=35.
156. ↑ "LCDB Data for (617)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=617|.
157. ↑ "JPL Small-Body Database Browser: 1208 Troilus (1931 YA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1208.
158. ↑ Chamberlin, Alan. "JPL Small-Body Database Search Engine". http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=all;obj_numbered=all;ast_orbit_class=IMB;ast_orbit_class=MBA;ast_orbit_class=OMB;OBJ_field=0;ORB_field=0;combine_mode=AND;c1_group=OBJ;c1_item=Ap;c1_op=<=;c1_value=100;c2_group=OBJ;c2_item=Ap;c2_op=>=;c2_value=40;table_format=HTML;max_rows=50;format_option=comp;c_fields=AcBhBgBjBiBnBsAiAp;.cgifields=format_option;.cgifields=ast_orbit_class;.cgifields=combine_mode;.cgifields=table_format;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=com_orbit_class&query=1&c_sort=ApD.
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160. ↑ "JPL Small-Body Database Browser: 233 Asterope". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=233.
161. ↑ "JPL Small-Body Database Browser: 53 Kalypso". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=53.
162. ↑ "JPL Small-Body Database Browser: 26 Prosperina". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=26.
163. ↑ "JPL Small-Body Database Browser: 2920 Automedon (1981 JR)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2920.
164. ↑ 164.0 164.1 164.2 Johnston, Wm. Robert (21 September 2014). "(90) Antiope and S/2000 (90) 1". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-42355.html.
165. ↑ "JPL Small-Body Database Browser: 61 Danae". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=61.
166. ↑ "JPL Small-Body Database Browser: 17 Thetis". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=17.
167. ↑ "JPL Small-Body Database Browser: 55 Pandora". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=55.
168. ↑ "JPL Small-Body Database Browser: 379 Huenna (A894 AA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=379.
169. ↑ Marchis, Franck; P. Descamps; J. Berthier; D. hestroffer; F. vachier; M. Baek et al. (2008). "Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits". Icarus 195 (1): 295–316. doi:10.1016/j.icarus.2007.12.010. Bibcode: 2008Icar..195..295M.
170. ↑ "JPL Small-Body Database Browser: 50 Virginia". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=50.
171. ↑ "JPL Small-Body Database Browser: 4348 Poulydamas (1988 RU)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4348.
172. ↑ 172.0 172.1 Johnston, Wm. Robert (20 September 2014). "(58534) Logos and Zoe". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-58534.html.
173. ↑ "JPL Small-Body Database Browser: 32 Pomona". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=32.
174. ↑ 174.00 174.01 174.02 174.03 174.04 174.05 174.06 174.07 174.08 174.09 174.10 174.11 Grav, T.Expression error: Unrecognized word "etal". (August 2015). "NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn". The Astrophysical Journal 809 (1): 9. doi:10.1088/0004-637X/809/1/3. 3. Bibcode: 2015ApJ...809....3G.
175. ↑ "LCDB Data for (10370)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=10370|.
176. ↑ "JPL Small-Body Database Browser: 43 Ariadne". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=43.
177. ↑ "JPL Small-Body Database Browser: 99 Dike". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=99.
178. ↑ "JPL Small-Body Database Browser: 79 Eurynome". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=79.
179. ↑ "JPL Small-Body Database Browser: 75 Eurydike". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=75.
180. ↑ "JPL Small-Body Database Browser: 29P/Schwassmann-Wachmann 1". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1000079.
181. ↑ "JPL Small-Body Database Browser: 64 Angelina". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=64.
182. ↑ "JPL Small-Body Database Browser: 82 Alkmene". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=82.
183. ↑ "JPL Small-Body Database Browser: 142 Polana". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=142.
184. ↑ "JPL Small-Body Database Browser: 253 Mathilde". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=253.
185. ↑ D. K. Yeomans (1997). "Estimating the mass of asteroid 253 Mathilde from tracking data during the NEAR flyby". Science 278 (5346): 2106–9. doi:10.1126/science.278.5346.2106. PMID 9405343. Bibcode: 1997Sci...278.2106Y.
186. ↑ "JPL Small-Body Database Browser: 73 Klytia". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=73.
187. ↑ "JPL Small-Body Database Browser: 60 Echo". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=60.
188. ↑ "Metis By the Numbers". NASA Solar System Exploration. 25 April 2019. https://solarsystem.nasa.gov/moons/jupiter-moons/metis/by-the-numbers/.
189. ↑ "JPL Small-Body Database Browser: 167 Urda". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=167.
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192. ↑ "JPL Small-Body Database Browser: 158 Koronis". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=158.
193. ↑ "JPL Small-Body Database Browser: 52872 Okyrhoe (1998 SG35)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=52872.
194. ↑ Stern, S.A. (9 January 2019). "Overview of initial results from the reconnaissance flyby of a Kuiper Belt planetesimal: 2014 MU69". arXiv:1901.02578 [astro-ph.EP]. Invalid `|display-authors=0.` (help)
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199. ↑ F. Marchis (2003). "A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope". Icarus 165 (1): 112–120. doi:10.1016/S0019-1035(03)00195-7. Bibcode: 2003Icar..165..112M.
200. ↑ Harris, Alan W.; Delbó, Marco; Binzel, Richard P.; Davies, John K.; Roberts, Julie; Tholen, David J.; Whiteley, Robert J. (1 October 2001). "Visible to Thermal-Infrared Spectrophotometry of a Possible Inactive Cometary Nucleus". Icarus 153 (2): 332–337. doi:10.1006/icar.2001.6687. Bibcode: 2001Icar..153..332H.
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206. ↑ "Deimos By the Numbers". NASA Solar System Exploration. 25 April 2019. https://solarsystem.nasa.gov/moons/mars-moons/deimos/by-the-numbers/.
207. ↑ "What Have We Learned About Halley's Comet?". Astronomical Society of the Pacific (No. 6 – Fall 1986). 1986. http://www.astrosociety.org/education/publications/tnl/06/06.html.
208. ↑ G. Cevolani; G. Bortolotti; A. Hajduk (1987). "Halley, comet's mass loss and age". Il Nuovo Cimento C (Italian Physical Society) 10 (5): 587–591. doi:10.1007/BF02507255. Bibcode: 1987NCimC..10..587C.
209. ↑ 209.0 209.1 Fang, Julia; Margot, Jean-Luc; Rojo, Patricio (16 July 2012). "Orbits, Masses, and Evolution of Main Belt Triple (87) Sylvia". The Astronomical Journal 144 (2): 70. doi:10.1088/0004-6256/144/2/70. Bibcode: 2012AJ....144...70F.
210. ↑ "JPL Small-Body Database Browser: 2685 Masursky (1981 JN)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2685.
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212. ↑ "JPL Small-Body Database Browser: 1509 Esclangona (1938 YG)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1509.
213. ↑ Wm. Robert Johnston (21 September 2014). "(45) Eugenia, Petit-Prince, and S/2004 (45) 1". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-00045.html.
214. ↑ Johnston, Wm. Robert (27 May 2019). "(31) Euphrosyne". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-00031.html.
215. ↑ "JPL Small-Body Database Browser: 9P/Tempel 1". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=9P.
216. ↑ Agle, D. C.; Brown, Dwayne; Farukhi, Suraiya (22 December 2017). "Arecibo Radar Returns with Asteroid Phaethon Images". NASA. https://www.jpl.nasa.gov/news/news.php?feature=7030.
217. ↑ Reddy, Vishnu; Gaffey, Michael J.; Abell, Paul A.; Hardersen, Paul S. (May 2012). "Constraining albedo, diameter and composition of near-Earth asteroids via near-infrared spectroscopy". Icarus 219 (1): 382–392. doi:10.1016/j.icarus.2012.03.005. Bibcode: 2012Icar..219..382R.
218. ↑ Weaver, H. A.; Stern, S.A.; Parker, J. Wm. (2003). "Hubble Space Telescope STIS Observations of Comet 19P/BORRELLY during the Deep Space 1 Encounter". The Astronomical Journal (The American Astronomical Society) 126 (1): 444–451. doi:10.1086/375752. Bibcode: 2003AJ....126..444W.
219. ↑ Johnston, Wm. Robert (19 February 2017). "(163693) Atira". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-163693.html.
220. ↑ "JPL Small-Body Database Browser: 5535 Annefrank (1942 EM)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=5535.
221. ↑ "JPL Small-Body Database Browser: 3749 Balam (1982 BG1)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3749.
222. ↑ Wm. Robert Johnston (2009-01-13). "(3749) Balam, S/2002 (3749) 1, and third component". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-03749.html.
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224. ↑ Johnston, Wm. Robert (27 May 2019). "(3122) Florence". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-03122.html.
225. ↑ "Comet 81P/Wild 2". The Planetary Society. http://www.planetary.org/explore/topics/asteroids_and_comets/wild2.html.
226. ↑ "LCDB Data for (2577)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=2577|.
227. ↑ "JPL Small-Body Database Browser: 67P/Churyumov-Gerasimenko". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=67P.
228. ↑ Pätzold, M. et al. (4 February 2016). "A homogeneous nucleus for comet 67P/Churyumov–Gerasimenko from its gravity field". Nature 530 (7588): 63–65. doi:10.1038/nature16535. PMID 26842054. Bibcode: 2016Natur.530...63P.
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230. ↑ "JPL Small-Body Database Browser: 4183 Cuno (1959 LM)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4183.
231. ↑ Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus 221 (1): 365–387. doi:10.1016/j.icarus.2012.07.026. Bibcode: 2012Icar..221..365P.
232. ↑ Johnston, Wm. Robert (21 September 2014). "(702) Alauda and Pichi unem". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-00702.html.
233. ↑ 233.0 233.1 Huang, Jiangchuan; Ji, Jianghui; Ye, Peijian; Wang, Xiaolei; Yan, Jun; Meng, Linzhi (2013). "The Ginger-shaped Asteroid 4179 Toutatis: New Observations from a Successful Flyby of Chang'e-2". Scientific Reports (Nature Research) 3 (3411): 3411. doi:10.1038/srep03411. PMID 24336501. Bibcode: 2013NatSR...3E3411H.
234. ↑ Dr. Lance A. M. Benner (28 May 2013). "(285263) 1998 QE2 Goldstone Radar Observations Planning". NASA/JPL Asteroid Radar Research. http://echo.jpl.nasa.gov/asteroids/1998QE2/1998QE2_planning.html.
235. ↑ Fang, Julia; Margot, Jean-Luc; Brozovic, Marina; Nolan, Michael C.; Benner, Lance A. M.; Taylor, Patrick A. (May 2011). "Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution". The Astronomical Journal 141 (5): 15. doi:10.1088/0004-6256/141/5/154. Bibcode: 2011AJ....141..154F.
236. ↑ Johnston, Wm. Robert (21 September 2014). "(153591) 2001 SN263, "Beta", and "Gamma"". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-153591.html.
237. ↑ Johnston, Wm. Robert (21 September 2014). "(1509) Esclangona and S/2003 (1509) 1". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-01509.html.
238. ↑ "New Horizons Mission to Pluto". Technology Org. 18 July 2015. https://www.technology.org/2015/07/18/new-horizons-mission-to-pluto/.
239. ↑ "JPL Small-Body Database Browser: 3753 Cruithne (1986 TO)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3753.
240. ↑ Tedesco, Edward; Metcalfe, Leo (4 April 2002). "New study reveals twice as many asteroids as previously believed" (Press release). European Space Agency. Archived from the original on 6 March 2023. Retrieved 20 October 2012.
241. ↑ "JPL Small-Body Database Browser: 2102 Tantalus (1975 YA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2102.
242. ↑ "LCDB Data for (9969) Braille". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=9969|Braille.
243. ↑ "LCDB Data for (308242)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=308242|.
244. ↑ "JPL Small-Body Database Browser: 1862 Apollo (1932 HA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1862.
245. ↑ "JPL Small-Body Database Browser: 85989 (1999 JD6)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=85989.
246. ↑ Greenberg, Adam H.; Margot, Jean-Luc; Verma, Ashok K.; Taylor, Patrick A.; Naidu, Shantanu P.; Brozovic, Marina. et al. (March 2017). "Asteroid 1566 Icarus's Size, Shape, Orbit, and Yarkovsky Drift from Radar Observations". The Astronomical Journal 153 (3): 16. doi:10.3847/1538-3881/153/3/108. Bibcode: 2017AJ....153..108G.
247. ↑ Chapman, Clark R. (October 1996). "S-Type Asteroids, Ordinary Chondrites, and Space Weathering: The Evidence from Galileo's Fly-bys of Gaspra and Ida". Meteoritics 31 (6): 699–725. doi:10.1111/j.1945-5100.1996.tb02107.x. Bibcode: 1996M&PS...31..699C.
248. ↑ "JPL Small-Body Database Browser: 4769 Castalia (1989 PB)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=4769.
249. ↑ Brozovic, Marina; Benner, Lance A. M.; Magri, Christopher; Scheeres, Daniel J.; Busch, Michael W.; Giorgini, Jon D. (April 2017). "Goldstone radar evidence for short-axis mode non-principal-axis rotation of near-Earth asteroid (214869) 2007 PA8". Icarus 286: 314–329. doi:10.1016/j.icarus.2016.10.016. Bibcode: 2017Icar..286..314B.
250. ↑ "JPL Small-Body Database Browser: 66391 Moshup (1999 KW4)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=66391.
251. ↑ 251.0 251.1 Johnston, Wm. Robert (20 September 2014). "(66391) Moshup and Squannit". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-66391.html.
252. ↑ Busch, Michael W.; Giorgini, Jon D.; Ostro, Steven J.; Benner, Lance A. M.; Jurgens, Raymond F.; Rose, Randy (October 2007). "Physical modeling of near-Earth Asteroid (29075) 1950 DA". Icarus 190 (2): 608–621. doi:10.1016/j.icarus.2007.03.032. Bibcode: 2007Icar..190..608B. https://echo.jpl.nasa.gov/asteroids/29075_1950DA/busch.etal.2007.1950da.pdf.
253. ↑ "Earth Impact Risk Summary: 29075". NASA/JPL Near-Earth Object Program Office. https://cneos.jpl.nasa.gov/sentry/details.html#?des=29075.
254. ↑ "JPL Small-Body Database Browser: 394130 (2006 HY51)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=394130.
255. ↑ 255.0 255.1 Lisse, C. M. et al. (2009). "Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2". Publications of the Astronomical Society of the Pacific 121 (883): 968–975. doi:10.1086/605546. Bibcode: 2009PASP..121..968L.
256. ↑ "LCDB Data for (163899)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=163899|.
257. ↑ "JPL Small-Body Database Browser: 3908 Nyx (1980 PA)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3908.
258. ↑ "JPL Small-Body Database Browser: 153814 (2001 WN5)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=153814.
259. ↑ "LCDB Data for 2017 YE5". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0|2017+YE5.
260. ↑ Müller, T. G.; Durech, J.; Ishiguro, M.; Mueller, M.; Krühler, T.; Yang, H. (March 2017). "Hayabusa-2 mission target asteroid 162173 Ryugu (1999 JU3): Searching for the object's spin-axis orientation". Astronomy and Astrophysics 599: 25. doi:10.1051/0004-6361/201629134. Bibcode: 2017A&A...599A.103M.
261. ↑ Clark, Stephen (6 September 2018). "Hayabusa 2 team sets dates for asteroid landings – Spaceflight Now". https://spaceflightnow.com/2018/09/06/hayabusa-2-team-sets-dates-for-asteroid-landings.
262. ↑ Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T. et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal 152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N.
263. ↑ "LCDB Data for 2014 JO25". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0|2014+JO25.
264. ↑ Marchis, F.Expression error: Unrecognized word "etal". (November 2012). "Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations". Icarus 221 (2): 1130–1161. doi:10.1016/j.icarus.2012.09.013. Bibcode: 2012Icar..221.1130M.
265. ↑ "JPL Small-Body Database Browser: 65803 Didymos (1996 GT)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=65803.
266. ↑ 266.0 266.1 Johnston, Wm. Robert (20 September 2014). "(65803) Didymos". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-65803.html.
267. ↑ Müller, T. G.; Marciniak, A.; Butkiewicz-Bąk, M.; Duffard, R.; Oszkiewicz, D.; Käufl, H. U.; Szakáts, R.; Santana-Ros, T. et al. (February 2017). "Large Halloween asteroid at lunar distance". Astronomy & Astrophysics 598: A63. doi:10.1051/0004-6361/201629584. Bibcode: 2017A&A...598A..63M. https://www.aanda.org/articles/aa/pdf/2017/02/aa29584-16.pdf. Retrieved 9 June 2019.
268. ↑ Brozovic, Marina; Benner, Lance A. M.; Taylor, Patrick A.; Nolan, Michael C. (November 2011). "Radar and optical observations and physical modeling of triple near-Earth Asteroid (136617) 1994 CC". Icarus 216 (1): 241–256. doi:10.1016/j.icarus.2011.09.002. Bibcode: 2011Icar..216..241B.
269. ↑ Johnston, Wm. Robert (21 September 2014). "(136617) 1994 CC, "Beta", and "Gamma"". Johnston's Archive. http://www.johnstonsarchive.net/astro/astmoons/am-136617.html.
270. ↑ "JPL Small-Body Database Browser: 172034 (2001 WR1)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=172034.
271. ↑ "JPL Small-Body Database Browser: 6489 Golevka (1991 JX)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=6489.
272. ↑ Nolan, M. C.; Magri, C. (2013). "Shape model and surface properties of the OSIRIS-REx target Asteroid (101955) Bennu from radar and lightcurve observations". Icarus 226 (1): 629–640. doi:10.1016/j.icarus.2013.05.028. ISSN 0019-1035. Bibcode: 2013Icar..226..629N. http://www.escholarship.org/uc/item/6mh8b2t5.
273. ↑ . Bibcode: 2014Icar..235....5C.
274. ↑ "JPL Small-Body Database Browser: 153201 (2000 WO107)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=153201.
275. ↑ "JPL Small-Body Database Browser: 163132 (2002 CU11)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=163132.
276. ↑ 276.0 276.1 Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T. et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal 814 (2): 13. doi:10.1088/0004-637X/814/2/117. Bibcode: 2015ApJ...814..117N.
277. ↑ "Radar Images of near-Earth Asteroid 2006 DP14". Jet Propulsion Laboratory. 25 February 2014. https://www.jpl.nasa.gov/news/news.php?release=2014-060.
278. ↑ Trilling, D. E.; Mueller, M.; Hora, J. L.; Fazio, G.; Spahr, T.; Stansberry, J. A. et al. (August 2008). "Diameters and Albedos of Three Subkilometer Near-Earth Objects Derived from Spitzer Observations". The Astrophysical Journal Letters 683 (2): L199–L202. doi:10.1086/591668. Bibcode: 2008ApJ...683L.199T.
279. ↑ "JPL Small-Body Database Browser: (2010 TK7)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3548081.
280. ↑ 280.0 280.1 "2006 SU49 Impact Risk". NASA/JPL Near-Earth Object Program Office. http://neo.jpl.nasa.gov/risk/2006su49.html.
281. ↑ M.W. Busch (31 March 2012). "Shape and Spin of Near-Earth Asteroid 308635 (2005 YU55) From Radar Images and Speckle Tracking". Lunar and Planetary Institute. http://www.lpi.usra.edu/meetings/acm2012/pdf/6179.pdf.
282. ↑ 282.0 282.1 Fujiwara, A.; Kawaguchi, J.; Yeomans, D. K.; Abe, M.; Mukai, T.; Okada, T. (June 2006). "The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa". Science 312 (5778): 1330–1334. doi:10.1126/science.1125841. PMID 16741107. Bibcode: 2006Sci...312.1330F. https://www.researchgate.net/publication/7042075. Retrieved 8 June 2019.
283. ↑ "JPL Small-Body Database Browser: 99942 Apophis (2004 MN4)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=99942.
284. ↑ "Earth Impact Risk Summary: 99942". NASA/JPL Near-Earth Object Program Office. https://cneos.jpl.nasa.gov/sentry/details.html#?des=99942.
285. ↑ "A Small Find Near Equinox". Cassini Solstice Mission. Jet Propulsion Laboratory. 7 August 2009. http://saturn.jpl.nasa.gov/photos/imagedetails/index.cfm?imageId=3617.
286. ↑ "LCDB Data for (277475)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=277475|.
287. ↑ Reddy, Vishnu; Gary, Bruce L.; Sanchez, Juan A.; Takir, Driss; Thomas, Cristina A.; Hardersen, Paul S. (September 2015). "The Physical Characterization of the Potentially Hazardous Asteroid 2004 BL86: A Fragment of a Differentiated Asteroid". The Astrophysical Journal 811 (1): 10. doi:10.1088/0004-637X/811/1/65. Bibcode: 2015ApJ...811...65R.
288. ↑ "NASA Scientists Get First Images of Earth Flyby Asteroid". Jet Propulsion Laboratory. 25 January 2008. http://www.jpl.nasa.gov/news/news.cfm?release=2008-014.
289. ↑ "LCDB Data for 2002 VE68". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0|2002+VE68.
290. ↑ Bruce L., Gary (January 2016). "Unusual Properties for the NEA (436724) 2011 UW158". The Minor Planet Bulletin 43 (1): 33–38. ISSN 1052-8091. Bibcode: 2016MPBu...43...33G.
291. ↑ "LCDB Data for 2017 BQ6". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=0|2017+BQ6.
292. ↑ Taylor, Patrick A. (13 April 2007). "Spin Rate of Asteroid (54509) 2000 PH5 Increasing Due to the YORP Effect". Science 316 (5822): 274–277. doi:10.1126/science.1139038. PMID 17347415. Bibcode: 2007Sci...316..274T. http://www.astro.cornell.edu/~jlm/publications/Taylor07.science316.yorp.pdf.
293. ↑ "LCDB Data for (469219)". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=469219|.
294. ↑ Dr. Lance A. M. Benner (13 January 2013). "2012 DA14 Goldstone Radar Observations Planning". NASA/JPL Asteroid Radar Research. http://echo.jpl.nasa.gov/asteroids/2012DA14/2012DA14_planning.html.2012+DA14+Goldstone+Radar+Observations+Planning&rft.atitle=&rft.aulast=Dr.+Lance+A.+M.+Benner&rft.au=Dr.+Lance+A.+M.+Benner&rft.date=13+January+2013&rft.pub=NASA/JPL+Asteroid+Radar+Research&rft_id=http://echo.jpl.nasa.gov/asteroids/2012DA14/2012DA14_planning.html&rfr_id=info:sid/en.wikibooks.org:Astronomy:List_of_Solar_System_objects_by_size">
295. ↑ Ostro, Steven J.; Pravec, Petr; Benner, Lance A. M.; Hudson, R. Scott; Sarounová, Lenka; Hicks, Michael D. (June 1999). "Radar and Optical Observations of Asteroid 1998 KY26". Science 285 (5427): 557–559 (SciHomepage). doi:10.1126/science.285.5427.557. PMID 10417379. Bibcode: 1999Sci...285..557O.
296. ↑ "The 2012 TC4 Observing Campaign – Radar observations UPDATE October 12, 2017". University of Maryland. http://2012tc4.astro.umd.edu/References/TC4RadarUpdate.txt.
297. ↑ "Reports of Meteorite Strike in Nicaragua and Update on Asteroid 2014 RC". NASA/JPL Near-Earth Object Program Office. http://neo.jpl.nasa.gov/news/news185.html.
298. ↑ "Earth Impact Risk Summary: 2010 RF12". NASA/JPL Near-Earth Object Program Office. https://cneos.jpl.nasa.gov/sentry/details.html#?des=2010 RF12.
299. ↑ Mommert, M. (19 June 2014). "Physical properties of near-earth asteroid 2011 MD". The Astrophysical Journal Letters 789 (1): L22. doi:10.1088/2041-8205/789/1/L22. Bibcode: 2014ApJ...789L..22M.
300. ↑ 300.0 300.1 Jenniskens, P. (2009). "The impact and recovery of asteroid 2008 TC3". Nature 458 (7237): 485–488. doi:10.1038/nature07920. PMID 19325630. Bibcode: 2009Natur.458..485J.
301. ↑ "archive.ph". https://cneos.jpl.nasa.gov/ca/.
302. ↑ "Asteroid 2008 TS26". Asteroids Near Earth. https://www.asteroidsnear.com/asteroid-2008-ts26-1490.

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