List of Solar System objects by size
| Objects in the Solar System |
|---|
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| Categories |
This is a list of Solar System objects by size, arranged in descending order of mean volumetric radius. The list can also be partially sorted according to an object's mass and, for the largest objects, volume, density and surface gravity. This list contains 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.
The ordering may be different depending on whether one chooses radius or mass, because some objects are denser than others. For instance Uranus is bigger than Neptune but less massive, and although Ganymede and Titan are larger than Mercury, they have less than half its mass. This means some objects in the lower tables, despite their smaller radii, may be more massive than objects in the upper tables because they have a higher density.
Many trans-Neptunian objects (TNOs) have been discovered, and their approximate locations in this list are shown, even though there can be a large uncertainty in their measurement.
Solar System objects more massive than 1021 kilograms (one yottagram [Yg]) are known or expected to be approximately spherical. Astronomical bodies relax into rounded shapes (ellipsoids), achieving hydrostatic equilibrium, when the gravity of their mass is sufficient to overcome the structural strength of their material. These are dubbed "regular". Objects made of ice become regular more easily than those made of rock, and many icy objects are spheroidal at far lower sizes. The cutoff boundary for regularity is somewhere between 100 km and 200 km in radius.[1]
The larger objects in the mass range between 1018 kg to 1021 kg (1 to 1000 zettagrams [Zg]), such as Tethys, Ceres, and Mimas, have relaxed to an oblate-spheroid equilibrium due to their gravity, while the less massive rubble piles (e.g. Amalthea and Janus) are roughly rounded, but not spherical, dubbed "irregular".
Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation, but a characteristic feature of the "irregular"-shaped bodies is that there is a significant difference in the length of their two equatorial diameters.
There can be difficulty in figuring out 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 "unreferenced wiki-assumed" masses/densities. Many TNOs are just assumed to have a density of 2.0 g/cm3, though it is just as likely that they have a comet-like density of only 0.5 g/cm3.[2] Thus most provisional TNOs are not given an MEarth value to prevent from cluttering the list with too many assumptions that could be off by an order of magnitude. For example, if a TNO is poorly assumed to have a mass of 3.59×1020 kg based on a radius of 350 km with a density of 2 g/cm3 and is later discovered to only have a radius of 175 km with a density of 1 g/cm3, the mass estimate would be only 2.24×1019 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. But many of the moons with a radius less than ~100 km, such as Jupiter's Himalia, still have unknown masses with assumed densities.[3] Again, as we get further from the Sun than Saturn, things get less clear. There has not yet been an orbiter around Uranus or Neptune for long-term study of the 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[4] and JPL Solar System Dynamics,[3] have somewhat contradictory size and albedo estimates depending on which research paper is being cited.
Data for objects has varying reliability including uncertainties in the figures for mass and radius, and irregularities in the shape and density, with accuracy often depending on how close it is to Earth or if it has been visited by a probe.
-
The relative masses of the bodies of the Solar System. Objects smaller than Saturn are not visible at this scale.
List [edit]
Objects above ≈400 km in radius [edit]
Anything above this size is probably in hydrostatic equilibrium. Some bodies listed near the end might not be if their predicted or measured size is "grossly in error" or their composition primarily rocky.[5] A lot of the values are manually calculated assuming sphericity. Size may or may not include an object's atmosphere. The diameter of Saturn's rings is around 364,900 km, much wider than Jupiter, but its gaseous sphere is smaller.
| Body | Image | Mean radius (km) |
Mean radius (R⊕) |
Volume (109 km3) |
Volume (V⊕) |
Mass ×1021 kg (Yg) |
Mass (M⊕) |
Density [note 1] g/cm3 |
Surface gravity (m/s2) |
Surface gravity (⊕) |
Type of object | Shape |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Sun | 696,000 | 109.25 | 1,412,000,000 | 1,303,781 | 1,989,100,000 | 332,837 | 1.409 | 274.0 | 28.02 | Star | regular | |
| Jupiter | 69,911 | 10.97 | 1,431,280 | 1,321 | 1,898,600 | 317.83 | 1.33 | 24.79 | 2.535 | Planet (gas giant) | regular | |
| Saturn | 58,232 (w/o rings) |
9.14 | 827,130 | 764 | 568,460 | 95.159 | 0.70 | 10.445 | 1.06 | Planet (gas giant) | regular | |
| Uranus | 25,362 | 3.98 | 68,340 | 63.1 | 86,832 | 14.536 | 1.30 | 8.87 | 0.90 | Planet (gas giant) | regular | |
| Neptune | 24,622 | 3.86 | 62,540 | 57.7 | 102,430 | 17.147 | 1.76 | 11.15 | 1.140 | Planet (gas giant) | regular | |
| Earth | 6,371.0 | 1 | 1,083.21 | 1 | 5,973.6 | 1 | 5.515 | 9.78033 | 0.99732 | Planet (terrestrial) | regular | |
| Venus | 6,051.8 (w/o gas) |
0.950 | 928.43 | 0.857 | 4,868.5 | 0.815 | 5.24 | 8.872 | 0.905 | Planet (terrestrial) | regular | |
| Mars | 3,390.0 | 0.532 | 163.18 | 0.151 | 641.85 | 0.107 | 3.94 | 3.7 | 0.38 | Planet (terrestrial) | regular | |
| Ganymede† Jupiter III |
2,631.2 | 0.413 | 76.30 | 0.0704 | 148.2 | 0.0248 | 1.936 | 1.428 | 0.15 | Satellite of Jupiter | regular | |
| Titan† Saturn VI |
2,576[6] (w/o gas) |
0.404 | 71.52 | 0.0660 | 134.5 | 0.0225 | 1.88 | 1.354 | 0.14 | Satellite of Saturn | regular | |
| Mercury | 2,439.7 | 0.383 | 60.83 | 0.0562 | 330.2 | 0.0553 | 5.43 | 3.7 | 0.38 | Planet (terrestrial) | regular | |
| Callisto† Jupiter IV |
2,410.3 | 0.378 | 58.65 | 0.0541 | 107.6 | 0.018 | 1.83 | 1.23603 | 0.126 | Satellite of Jupiter | regular | |
| Io† Jupiter I |
1,821.5 | 0.286 | 25.32 | 0.0234 | 89.3 | 0.015 | 3.528 | 1.797 | 0.183 | Satellite of Jupiter | regular | |
| Moon Earth I |
1,737.1 | 0.273 | 21.958 | 0.0203 | 73.5 | 0.0123 | 3.3464 | 1.625 | 0.166 | Satellite of Earth | regular | |
| Europa† Jupiter II |
1,561 | 0.245 | 15.93 | 0.0147 | 48 | 0.00803 | 3.01 | 1.316 | 0.134 | Satellite of Jupiter | regular | |
| Triton† Neptune I |
1,353.4 | 0.212 | 10.38 | 0.0096 | 21.5 | 0.00359 | 2.061 | 0.782 | 0.0797 | Satellite of Neptune | regular | |
| ErisR 136199 |
1,163±6[7] | 0.182 | 7 | 0.007 | 16.7[8] | 0.0027 | 2.5 | 0.662 | 0.0677 | Dwarf planet—SDO—binary | regular | |
| PlutoR 134340 |
1,161[9] (w/o gas) |
0.181 | 7 | 0.0066 | 13.105 | 0.0022 | 2.0 | 0.61 | 0.062 | Dwarf planet— KBO |
regular | |
| Titania‡ Uranus III |
788.9 | 0.124 | 2.06 | 0.0019 | 3.526 | 0.00059 | 1.72 | 0.378 | 0.0385 | Satellite of Uranus | regular | |
| Rhea‡ Saturn V |
764.1[10] | 0.12 | 1.87 | 0.0017 | 2.3166 | 0.00039 | 1.23 | 0.26 | 0.027 | Satellite of Saturn | regular | |
| Oberon† Uranus IV |
761.4 | 0.12 | 1.85 | 0.0017 | 3.014 | 0.0005 | 1.63 | 0.347 | 0.035 | Satellite of Uranus | regular | |
| MakemakeRA 136472 |
740±20[11] | 1.7 | 3 | 0.00067 | 1.7[11] | 0.4 | Dwarf planet— KBO |
regular | ||||
| Iapetus† Saturn VIII |
735.6[12] | 0.113 | 1.55 | 0.0014 | 1.9739 | 0.00033 | 1.08 | 0.223 | 0.0227 | Satellite of Saturn | regular | |
| 2007 OR10 225088 "Snow White" |
640±100[13] | 0.1 | 1.0981 | 0.00101 | SDO | unknown | ||||||
| HaumeaR 136108 |
620±30 | 0.117 | 1.3–1.6 | 0.001 | 4.006 | 0.00069 | 2.55[14] | 0.44 | 0.045 | Dwarf planet— KBO—trinary |
regular (scalene ellipsoid) | |
| Charon† Pluto I |
603.5[15] | 0.095 | 0.87 | 0.0008 | 1.52 | 0.00025 | 1.65 | 0.279 | 0.028 | Satellite of Pluto | regular | |
| Umbriel† Uranus II |
584.7 | 0.092 | 0.84 | 0.0008 | 1.2 | 0.00020 | 1.4 | 0.234 | 0.024 | Satellite of Uranus | regular | |
| Ariel ‡ Uranus I |
578.9 | 0.091 | 0.81 | 0.0008 | 1.35 | 0.00022 | 1.67 | 0.269 | 0.027 | Satellite of Uranus | regular | |
| Dione† Saturn IV |
561.6 | 0.088 | 0.73 | 0.0007 | 1.096 | 0.000183 | 1.48 | 0.232 | 0.0236 | Satellite of Saturn | regular | |
| Quaoar 50000 |
540±20 | 0.07 | 0.37 | 0.0003 | 1.6[16] | 0.0003 | 4.2[16] | 0.125 | 0.013 | KBO—Cubewano—binary | unknown | |
| Tethys‡ Saturn III |
533 | 0.083 | 0.624 | 0.0006 | 0.6173 | 0.000103 | 1.15 | 0.145 | 0.015 | Satellite of Saturn | regular | |
| SednaRA 90377 |
500±40[17] | 0.08 | TNO—Detached object[18] | unknown | ||||||||
| Ceres‡ 1 |
471 | 0.076 | 0.437 | 0.0004 | 0.95 | 0.000159 | 2.08 | 0.27 | 0.0275 | Dwarf planet—Asteroid | regular | |
| 2002 MS4 307261 |
470±25[19] | 0.07 | KBO[18] | unknown | ||||||||
| OrcusRA 90482 |
460±10 | 0.06 | 0.23 | 0.0002 | 2.47[20] | KBO—Plutino—binary | unknown | |||||
| 2005 UQ5139 202421 |
460 | 0.06 | 0.22 | 0.0002 | 0.886P | 0.0001 | 2.0 | 0.278 | 0.0284 | KBO—Cubewano | unknown | |
| Salacia 120347 |
430±20 | 0.07 | 0.45 | 1.16[21] | 0.147 | KBO—binary | unknown | |||||
| 2003 MW129 174567 |
410 | 0.06 | 0.22 | 0.0002 | 0.616P | 0.0001 | 2.0 | 0.228 | 0.02 | KBO | unknown |
Objects between ≈400 and ≈200 km in radius [edit]
Most objects in this size range are expected to be round. All the satellites except Proteus are round. The asteroid 10 Hygiea is not, and 2 Pallas and 4 Vesta are borderline. Like the satellites, TNOs in this size range are expected to be round (assuming the estimated size is correct).
| Body | Image | Mean radius (km) |
Mean radius (R⊕) |
Volume (109 km3) |
Volume (V⊕) |
Mass ×1021 kg (Yg) |
Mass (M⊕) |
Density [note 1] g/cm3 |
Surface gravity (m/s2) |
Surface gravity (⊕) |
Type of object | Shape |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 2006 QH1819 | 380 | 0.06 | 0.233 | 0.000215 | 0.467P | 0.00008 | 2.0 | 0.214 | 0.022 | SDO | unknown | |
| 2002 AW197R 55565 |
367[5] | 0.06 | 0.207 | 0.00019 | 0.414P | 0.000069 | 2.0 | 0.206 | 0.0211 | KBO[18] | unknown | |
| 2003 AZ84R 208996 |
363.5[22] | 0.06 | KBO—Plutino—binary | unknown | ||||||||
| Dysnomia Eris I |
342.5[13] | Satellite of Eris | unknown | |||||||||
| 2002 UX25R 55637 |
340.5[5] | 0.0535 | 0.166 | 0.000153 | 0.331P | 0.0000554 | 2.0 | 0.191 | 0.01952 | KBO—binary | unknown | |
| 2007 JJ43 278361 |
338.5[5] | TNO[18] | unknown | |||||||||
| 2004 GV9R 90568 |
338.5[5] | 0.0531 | 0.162 | 0.00015 | 0.325P | 0.0000534 | 2.0 | 0.19 | 0.0194 | KBO | unknown | |
| 2005 RN439 145452 |
330.5[5] | 0.0573 | 0.2036 | 0.00019 | 0.407P | 0.000068 | 2.0 | 0.205 | 0.02096 | KBO[18] | unknown | |
| 2010 KZ39 | 330.5[5] | TNO—Detached object[23] or Cubewano[24] | unknown | |||||||||
| IxionRA 28978 |
325[5] | 0.051 | 0.144 | 0.000133 | 0.3 | 5.0E-5 | 2.086 | 0.19 | 0.021 | KBO—Plutino | unknown | |
| 2004 XA192 230965 |
322[5] | 0.055 | 0.177 | 0.00016 | 0.354P | 0.000059 | 2.0 | 0.195 | 0.02 | TNO[18] | unknown | |
| 2001 UR1639 42301 |
306.5[5] | 0.05 | 0.134 | 0.00012 | 0.269P | 0.000045 | 2.0P | 0.178 | 0.018 | SDO[18] | unknown | |
| 2010 RF43 | 306.5[5] | SDO | unknown | |||||||||
| 2003 UZ4139 | 306.5[5] | 0.048 | 0.116 | 0.00012 | 0.33P | 0.000055 | 2.0P | 0.241 | 0.0246 | KBO—Plutino | unknown | |
| 2004 PF115 175113 |
306.5[5] | KBO—Plutino | unknown | |||||||||
| Chaos 19521 |
300[19] | 0.0585 | 0.216 | 0.0002 | 0.4328P | 0.00007 | 2.0P | 0.209 | 0.021 | KBO—Cubewano | unknown | |
| 2007 UK1269 229762 |
300[13] | SDO | unknown | |||||||||
| 2008 ST291 | 299[5] | SDO | unknown | |||||||||
| 2010 RE64 | 299[5] | KBO | unknown | |||||||||
| 2010 FX86 | 299[5] | KBO—Cubewano | unknown | |||||||||
| 2002 TC302 84522 |
292[25] | 2:5 resonance | unknown | |||||||||
| (119951) 2002 KX149 | 292[5] | KBO | unknown | |||||||||
| 2005 RM439 145451 |
292[18] | 0.0455 | 0.102 | 0.00009 | 0.2P | 0.000034 | 2.0P | 0.159 | 0.016 | KBO | unknown | |
| 2004 XR190 | 292[18] | 0.059 | 0.221 | 0.0002 | 0.4416P | 0.00007 | 2.0P | 0.21 | 0.0215 | SDO[18] | unknown | |
| 2004 NT33 | 292[18] | 0.043 | 0.089 | 0.000082 | 0.178P | 0.000029 | 2.0P | 0.155 | 0.0158 | KBO—Cubewano[18] | unknown | |
| 2004 TY364* 120348 |
284,5[18] | 0.043 | 0.089 | 0.000082 | 0.178P | 0.000029 | 2.0P | 0.155 | 0.0158 | KBO[18] | unknown | |
| 2010 VK201 | 284.5[5] | Cubewano[18] | unknown | |||||||||
| 2002 XV93 | 274.6[22] | KBO—Plutino[18] | unknown | |||||||||
| Pallas$ 2 |
272.5[26] | 0.211 | 0.0000353 | 2.8[27] | 0.19 | 0.02 | Asteroid | uncertain | ||||
| 2004 PR107 | 264.5[18] | 0.0345 | 0.0446 | 0.00004 | 0.089P | 0.000014 | 2.0P | 0.123 | 0.0126 | KBO | unknown | |
| Vesta$ 4 |
262.7[28] | 0.259076 | 3.456[28] | 0.252 | Asteroid | regular? | ||||||
| 2003 VS2 84922 |
261.5[22] | KBO—Plutino[18] | unknown | |||||||||
| 2003 QX113 | 252.5[18] | 0.036 | 0.051 | 0.00005 | 0.102P | 0.000017 | 2.0P | 0.129 | 0.013 | SDO[18] | unknown | |
| Enceladus‡ Saturn II |
252.1 | 0.039 | 0.067 | 0.00006 | 0.108 | 0.0000181 | 1.61 | 0.111 | 0.0113 | Satellite of Saturn | regular | |
| 2010 VZ98 | 251.5[5] | SDO[18] | unknown | |||||||||
| 2011 FW62 | 251.5[5] | Classical | unknown | |||||||||
| Varuna* 20000 |
250[5] | 0.049 | 0.125 | 0.000115 | 0.37 | 6.2E-5 | 0.992[14] | 0.258 | 0.028 | KBO | unknown | |
| 2010 TJ | 239[5] | SDO[18] | unknown | |||||||||
| 2010 TY53 | 239[5] | TNO — centaur[18] | unknown | |||||||||
| 2011 GM27 | 239[5] | SDO | unknown | |||||||||
| 2006 HH123 | 239[5] | 0.031 | 0.0335 | 0.000011 | 0.067P | 0.000011 | 2.0 | 0.112 | 0.011 | Centaur[18] | unknown | |
| Miranda‡ Uranus V |
235.8 | 0.037 | 0.055 | 0.00005 | 0.0659 | 0.000011 | 1.20 | 0.0791 | 0.00806 | Satellite of Uranus | regular | |
| 2010 EK139 | 235[17] | SDO | unknown | |||||||||
| 2005 TB190 145480 |
232[13] | TNO—Detached object[18] | unknown | |||||||||
| 1999 DE9 26375 |
230.5[29] | 0.036 | 0.051 | 0.000047 | 0.1026P | 0.000017 | 2.0 | 0.129 | 0.013 | KBO | unknown | |
| 2003 FY128 120132 |
230[13] | SDO[18] | unknown | |||||||||
| 1998 SN165* 35671 |
230[18] | 0.036 | 0.05 | 0.000046 | 0.1P | 0.000017 | 2.0 | 0.128 | 0.013 | KBO | unknown | |
| 2002 VR128 84719 |
224.3[22] | KBO—Plutino[18] | unknown | |||||||||
| HuyaR 38628 |
219.4[22] | KBO—Plutino | unknown | |||||||||
| 1999 CD158 | 210[18] | 0.0345 | 0.0446 | 0.00004 | 0.089P | 0.000014 | 2.0 | 0.123 | 0.0126 | KBO | unknown | |
| Proteus ‡A Neptune VIII (8) |
210 | 0.033 | 0.038 | 0.000035 | 0.050 | 0.00000844 | 1.3[30] | 0.0666 | 0.00678 | Satellite of Neptune | irregular | |
| 2001 QF298 | 204.1[22] | KBO—Plutino[18] | unknown | |||||||||
| 2005 QU1829 303775 |
204[13] | SDO[18] | unknown | |||||||||
| 10 Hygiea$ | 203.6[31] | 0.03 | 0.04 | 3.0E-5 | 0.0885 | 1.0E-5 | 2.5 | 0.143 | 0.02 | Asteroid | irregular | |
| 2000 YW134* 82075 |
202[18] | 0.039 | 0.065 | 0.00006 | 0.13P | 0.000022 | 2.0P | 0.139 | 0.014 | SDO[18] | unknown | |
| 2002 WC19 119979 |
200.5[32] | 0.0315 | 0.034 | 0.00003 | 0.0675P | 0.000011 | 2.0 | 0.113 | 0.0115 | KBO—binary | unknown | |
| 1996 GQ21* 26181 |
200.5[18] | 0.031 | 0.0335 | 0.000011 | 0.067P | 0.000011 | 2.0 | 0.112 | 0.011 | SDO[18] | unknown | |
Objects between 200 and 100 km in radius [edit]
Objects between 200 and 100 km in radius (400 and 200 km in diameter). The largest of these may lie above the boundary for hydrostatic equilibrium, but most are irregular. Most of the trans-Neptunian objects 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. Values relative to Earth are not included beyond this point. 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).[33] This is not complete, missing many poorly known TNOs.[18]
| Satellites of Saturn |
| Satellites of Neptune |
Selected objects between 100 and 50 km in radius [edit]
Objects 100 and 50 km in radius (200 km to 100 km in average diameter). The listed objects currently include most objects in the asteroid belt and moons of the gas giants in this size range, but many newly discovered objects in the outer Solar System are missing, such as those included in the following reference:.[18] Asteroid spectral types are mostly Tholen, but some might be SMASS.
| Satellites of Jupiter |
| Satellites of Saturn |
| Satellites of Uranus |
| Satellites of Neptune |
Examples of objects between 50 km and 20 km in radius [edit]
There are easily tens of thousands of objects 50 km in radius or smaller[clarification needed], but only a fraction have been explored. The number of digits is not an endorsement of significant figures. The table switches from ×1018 kg to ×1015 kg (Eg), and many of these mass values are assumed. (see also List of minor planets)
| Satellites of Jupiter |
| Satellites of Saturn |
| Satellites of Uranus |
| Satellites of Neptune |
| Satellites of Pluto |
Examples of objects between 20 km and 1 km in radius [edit]
| Satellites of Mars |
| Satellites of Jupiter |
| Satellites of Saturn |
| Satellites of Uranus |
| Satellites of Neptune |
| Satellites of Pluto |
Examples of objects below 1 km (1000 m) in radius [edit]
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,[130] 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 viewed by large telescopes. Radius is by mean geometric radius. Number of digits not an endorsement of significant figures. Mass scale shifts from × 1015 to 1012 kg, which is 1015 grams (Petagram - Pg).
| Satellites of Jupiter |
| Satellites of Saturn |
| Satellites of Uranus |
| Satellites of Neptune |
Currently most of the objects of mass between 109 kg to 1012 kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids. (See also: list of NEAs by distance from Sun.) Note that 1994 WR12 possesses less mass than the Great Pyramid of Giza, 5.9 × 109 kg.
For more about really small objects in the Solar System see meteoroid, micrometeoroid, and interplanetary dust cloud.
Surface gravity [edit]
The surface gravity at the equator of a body can in most cases be accurately calculated using Newton's law of universal gravitation and centrifugal force.
The gravitational acceleration at the equator is given by Newton's law of universal gravitation. The formula that follows from this law is:
where
- ag is the magnitude of the gravitational acceleration
- G is the gravitational constant
- m is the mass of the celestial body
- r is the equatorial radius of the celestial body (if this varies significantly, the mean equatorial radius is used)
The magnitude of the outward acceleration due to centrifugal force is given by
where
- T is the rotation period of the celestial body
The surface gravity at the equator is then given by
Closely imaged objects [edit]
| Sun (star) |
Jupiter (planet) |
Saturn (planet) |
Uranus (planet) |
Neptune (planet) |
Earth (planet) |
Venus (planet) |
| Mars (planet) |
Ganymede (moon of Jupiter) |
Titan (moon of Saturn) |
Mercury (planet) |
Callisto (moon of Jupiter) |
Io (moon of Jupiter) |
Moon (moon of Earth) |
| Europa (moon of Jupiter) |
Triton (moon of Neptune) |
Titania (moon of Uranus) |
Rhea (moon of Saturn) |
Oberon (moon of Uranus) |
Iapetus (moon of Saturn) |
Umbriel (moon of Uranus) |
| Ariel (moon of Uranus) |
Dione (moon of Saturn) |
Tethys (moon of Saturn) |
Vesta (asteroid) |
Enceladus (moon of Saturn) |
Miranda (moon of Uranus) |
Proteus (moon of Neptune) |
| Mimas (moon of Saturn) |
Hyperion (moon of Saturn) |
Phoebe (moon of Saturn) |
Janus (moon of Saturn) |
Amalthea (moon of Jupiter) |
Epimetheus (moon of Saturn) |
Thebe (moon of Jupiter) |
| Prometheus (moon of Saturn) |
Pandora (moon of Saturn) |
Mathilde (asteroid) |
Helene (moon of Saturn) |
Ida (asteroid) |
Atlas (moon of Saturn) |
Telesto (moon of Saturn) |
| Calypso (moon of Saturn) |
Phobos (moon of Mars) |
Deimos (moon of Mars) |
Gaspra (asteroid) |
Tempel 1 (comet) |
Borrelly (comet) |
Wild 2 (comet) |
| Methone (moon of Saturn) |
Hartley 2 (comet) |
|||||
Notes [edit]
- † Using equatorial radius and assuming body is spherical
- ‡ Using three radii and assuming body is spheroid
- * Radius is known only very approximately
- R Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft
- 9 Unknown radius, generic assumed albedo of 0.09
- $ Well studied asteroid or moon where the dimensions and mass are very well known. Asteroid sizes and masses taken from James Baer's (Bio) personal website.
- M Mass has been determined by perturbation. For asteroids, see James Baer's personal website.
- A Assumed mass
- P Mass calculated assuming Pluto's density of 2.0 g/cm3
- Note: For many of the well-determined moons, radii were taken from the JPL Solar System Dynamics page.
- O Radius has been determined with Asteroid occultation
- ^ a b Densities of those KBOs whose masses are uncertain are assumed to be 2.0 in line with Pluto
- ^ a b Roman Numerals
- ^ 3000 x 10^9 kg
References [edit]
- ^ Mike Brown. "The Dwarf Planets". CalTech. Archived from the original on 2011-02-12. Retrieved 2008-09-25.
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- ^ Tedesco, Edward; Metcalfe, Leo (April 4, 2002). "New study reveals twice as many asteroids as previously believed" (Press release). European Space Agency. Retrieved 2009-10-20.
- ^ NASA - 2007 PA8
- ^ Minor Planet No. 100,000 Named for Space Age 50th Anniversary (2007) - Space Ref, Quote: "..about a mile in size"
- ^ JPL Small-Body Database Browser: 100000 Astronautica
- ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04.
- ^ "(4769) Castalia." Wikipédia, l'encyclopédie libre. 20 jan 2010, 16:37 UTC. 11 oct 2010, 16:48 <http://fr.wikipedia.org/w/index.php?title=(4769)_Castalia&oldid=49048108>
- ^ a b Lisse, C. M.; Fernandez; Reach; Bauer; A'Hearn; Farnham; et al. (2009). "Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2". Publications of the Astronomical Society of the Pacific 121: 968–975. arXiv:0906.4733. Bibcode:2009PASP..121..968L. doi:10.1086/605546.
- ^ "JPL Small-Body Database Browser: 14827 Hypnos (1986 JK)". Archived from the original on 2011-02-12. Retrieved 2008-02-08.
- ^ Whitman, Kathryn; Alessandro Morbidelli and Robert Jedicke (2006). The Size-Frequency Distribution of Dormant Jupiter Family Comets. arXiv:astro-ph/0603106. Bibcode:2006Icar..183..101W. doi:10.1016/j.icarus.2006.02.016.
- ^ 2062 Aten (this version)[dead link]
- ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04.
- ^ a b c Based on an assumed density of 2.6 g/cm3 as given at the NASA NEO impact risk page http://neo.jpl.nasa.gov/risk/index.html Archived 12 February 2011 at WebCite
- ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04.
- ^ ESA (January 9, 2013). "Herschel intercepts asteroid Apophis". European Space Agency (ESA). Retrieved 2013-01-09.
- ^ BBC - Giant asteroid passes near Earth - 9 November 2011
- ^ The Herschel Space Observatory catches a glimpse of the minor planet during its rendezvous with Earth (November 17, 2011)
- ^ JPL Small-Body Database Browser (2005 YU55)
- ^ "NASA Scientists Get First Images of Earth Flyby Asteroid". NASA/JPL. 2008-01-25. Archived from the original on 2011-02-12. Retrieved 2008-01-26.
- ^ NASA - 1994 WR12 Earth Impact Risk Summary - 2011
- ^ a b 2009 FD Impact Risk
- ^ a b c BBC News - Record spin for newfound asteroid (2008) Archived 12 February 2011 at WebCite
- ^ Alan Chamberlin. "JPL Small-Body Database Browser". Ssd.jpl.nasa.gov. Archived from the original on 2011-02-12. Retrieved 2011-01-04.
Further reading [edit]
- NASA Planetary Data System (PDS)
- Asteroids with Satellites
- Minor Planet discovery circumstances
- Supplemental IRAS Minor Planet Survey (SIMPS) and IRAS Minor Planet Survey (IMPS)
- SIMPS & IMPS (V6, additional, from here)
- Asteroid Data Archive (dead link) Archive Planetary Science Institute
External links [edit]
- Planetary fact sheets
- Asteroid fact sheet
- All (known) Bodies in the Solar System Larger than 200 Miles in Diameter - in an image, put side-by-side.
- Size comparison of asteroids and comets visited by space probe (Parent article of image at The Planetary Society)
- Scaled Solar System montage at TPS Blog
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