List of gravitationally rounded objects of the Solar System

 This is a list of possibly gravitationally rounded objects of the Solar System, which are objects that have a rounded, ellipsoidal shape due to their own gravity (hydrostatic equilibrium). Their sizes range from planetary-mass objects like dwarf planets and some moons to the planets and the Sun. This list does not include small Solar System bodies, but it does include a sample of possible planetary-mass objects whose shapes have yet to be determined. The Sun's orbital characteristics are listed in relation to the Galactic Center, while all other objects are listed in order of their distance from the Sun.

StarEdit

The Sun is a G-type main-sequence star. It contains almost 99.9% of all the mass in the Solar System.[1]

Sun[2][3]
Sun white.jpg
Astronomical symbol[q]Sun symbol.svg
Mean distance
from the Galactic Center
km
light years
~2.5×1017
~26,000
Mean radiuskm
:E[f]
695,508
109.3
Surface areakm2
:E[f]
6.0877×1012
11,990
Volumekm3
:E[f]
1.4122×1018
1,300,000
Masskg
:E[f]
1.9855×1030
332,978.9
Gravitational parameterm3/s21.327×1020
Densityg/cm31.409
Equatorial gravitym/s2274.0
Escape velocitykm/s617.7
Rotation perioddays[g]25.38
Orbital period about Galactic Center[4]million years225–250
Mean orbital speed[4]km/s~220
Axial tilt[i] to the eclipticdeg.7.25
Axial tilt[i] to the galactic planedeg.67.23
Mean surface temperatureK5,778
Mean coronal temperature[5]K1–2×106
Photospheric compositionHHeOCFeS

PlanetsEdit

Key
*
Terrestrial planet
°
Gas giant

Ice giant

The 2006 International Astronomical Union (IAU) defines a planet as a body in orbit around the Sun that was large enough to have achieved hydrostatic equilibrium and to have "cleared the neighbourhood around its orbit".[6] The practical meaning of "cleared the neighborhood" is that a planet is comparatively massive enough for its gravitation to control the orbits of all objects in its vicinity. By the IAU's definition, there are eight planets in the Solar System; four terrestrial planets (Mercury, Venus, Earth and Mars) and four giant planets, which can be divided further into two gas giants (Jupiter and Saturn) and two ice giants (Uranus and Neptune). When excluding the Sun, the four giant planets account for more than 99% of the mass of the Solar System.

 *Mercury[7][8][9]*Venus[10][11][9]*Earth[12][13][9]*Mars[14][15][9]°Jupiter[16][17][9]°Saturn[18][19][9]Uranus[20][21]Neptune[22][23][9]
 Mercury in true color.jpg       
Astronomical symbol[q]Mercury symbol.svg       
Mean distance
from the Sun
km
AU
57,909,175
0.38709893
108,208,930
0.72333199
149,597,890
1.00000011
227,936,640
1.52366231
778,412,010
5.20336301
1,426,725,400
9.53707032
2,870,972,200
19.19126393
4,498,252,900
30.06896348
Equatorial radiuskm
:E[f]
2,440.53
0.3826
6,051.8
0.9488
6,378.1366
1
3,396.19
0.53247
71,492
11.209
60,268
9.449
25,559
4.007
24,764
3.883
Surface areakm2
:E[f]
75,000,000
0.1471
460,000,000
0.9020
510,000,000
1
140,000,000
0.2745
64,000,000,000
125.5
44,000,000,000
86.27
8,100,000,000
15.88
7,700,000,000
15.10
Volumekm3
:E[f]
6.083×1010
0.056
9.28×1011
0.857
1.083×1012
1
1.6318×1011
0.151
1.431×1015
1,321.3
8.27×1014
763.62
6.834×1013
63.102
6.254×1013
57.747
Masskg
:E[f]
3.302×1023
0.055
4.8690×1024
0.815
5.972×1024
1
6.4191×1023
0.107
1.8987×1027
318
5.6851×1026
95
8.6849×1025
14.5
1.0244×1026
17
Gravitational parameterm3/s22.203×10133.249×10143.986×10144.283×10131.267×10173.793×10165.794×10156.837×1015
Densityg/cm35.435.245.523.9401.330.701.301.76
Equatorial gravitym/s23.708.879.83.7124.7910.448.8711.15
Escape velocitykm/s4.2510.3611.185.0259.5435.4921.2923.71
Rotation period[g]days58.646225243.01870.997269681.025956750.413540.444010.718330.67125
Orbital period[g]days
years
87.969
0.2408467
224.701
0.61519726
365.256363
1.000702364
686.971
1.8808476
4,332.59
11.862615
10,759.22
29.447498
30,688.5
84.016846
60,182
164.79132
Mean orbital speedkm/s47.872535.021429.785924.130913.06979.67246.83525.4778
Eccentricity0.205630690.006773230.016710220.093412330.048392660.054150600.047167710.00858587
Inclination[f]deg.7.003.390[12]1.851.312.480.761.77
Axial tilt[i]deg.0.0177.3[h]23.4425.193.1226.7397.86[h]28.32
Mean surface temperatureK440–100730287227152 [j]134 [j]76 [j]73 [j]
Mean air temperature[k]K2881651357673
Atmospheric compositionHe,  Na+
P+ 
CO2N2SO2N2O2Ar, CO2CO2, N2
Ar
H2, HeH2, HeH2, He
CH4
H2, He
CH4
Number of known moons[v]001279822714
Rings?NoNoNoNoYesYesYesYes
Planetary discriminant[l][o]9.1×1041.35×1061.7×1061.8×1056.25×1051.9×1052.9×1042.4×104

Dwarf planetsEdit

Key

asteroid belt

trans-Neptunian

Dwarf planets are bodies that are massive and warm enough to have achieved hydrostatic equilibrium, but have not cleared their neighbourhoods of similar objects. Since 2008, there have been five dwarf planets recognized by the IAU, though of these only Ceres, which orbits in the asteroid belt between the orbits of Mars and Jupiter, has been confirmed.[ae] The others all orbit beyond Neptune. Astronomers generally agree that several other trans-Neptunian objects may be large enough to be dwarf planets, given current uncertainties. It seems that dark, low-density objects like Salacia retain internal porosity from their formation, and thus are not planetary bodies.[24] Both Quaoar and Orcus have moons that have allowed their mass and density to be determined using Kepler's third law, and they are either bright enough to suggest resurfacing and thus planetary geology at least at some point in their past, or are dense enough that they are clearly solid bodies and thus at least potentially dwarf planets.

Ceres[25]Pluto[26][27]Haumea[28][29][30]Makemake[31][32]Eris[33]
Ceres - RC3 - Haulani Crater (22381131691) (cropped).jpg    
Astronomical symbol[q]Ceres symbol.svg 
Minor planet number1134340136108136472136199
Mean distance
from the Sun
km
AU
413,700,000
2.766
5,906,380,000
39.482
6,484,000,000
43.335
6,850,000,000
45.792
10,210,000,000
67.668
Mean radiuskm
:E[f]
473
0.0742
1,188.3[9]
0.186
816
(2100 × 1680 × 1074)
0.13[34][35]
715
0.11[36]
1,163
0.18[37]
Volumekm3
:E[f]
4.21×108
0.00039[b]
6.99×109
0.0065
1.98×109
0.0018
1.7×109
0.0016[b]
6.59×109
0.0061[b]
Surface areakm2
:E[f]
2,770,000
0.0054[a]
17,700,000
0.035
8,140,000
0.016[z]
6,900,000
0.0135[a]
17,000,000
0.0333[a]
Masskg
:E[f]
9.39×1020
0.00016
1.30×1022
0.0022
4.01 ± 0.04×1021
0.0007[38]
< 4.4 ×1021

< 0.0007

1.65×1022
0.0028
Gravitational parameterm3/s26.263 × 10108.710 × 10112.674 × 1011< 2.937 × 10111.108 × 1012
Densityg/cm32.161.872.02[34]2.102.43
Equatorial gravitym/s20.27[d]0.620.63[d]< 0.570.82[d]
Escape velocitykm/s[e]0.511.210.91< 0.911.37
Rotation period[g]days0.37816.38720.16310.951114.560
Orbital period[g]years4.599247.9283.8306.2559
Mean orbital speedkm/s17.8824.754.48[o]4.40[o]3.44[n]
Eccentricity0.0800.2490.1950.1610.436
Inclination[f]deg.10.5917.1428.2128.9844.04
Axial tilt[i]deg.4119.6[h]≈126?≈78
Mean surface temperature[w]K167[39]40[40]<50[41]3030
Atmospheric compositionH2ON2CH4, CO?N2, CH4[42]N2, CH4[43]
Number of known moons[v]052[44]1[45]1[46]
Planetary discriminant[l][o]0.330.0770.0230.020.10

Of the remaining trans-Neptunian objects, the most likely dwarf planets include:

Orcus[47]Salacia[48]Quaoar[49]Gonggong[50]Sedna[51]
Orcus-vanth hst2.jpg    
Minor-planet number904821203475000022508890377
Semi-major axiskm
AU
5,896,946,000
39.419
6,310,600,000
42.18
6,535,930,000
43.69
10,072,433,340
67.33
78,668,000,000
525.86
Mean radius[s]km
:E[f]
458.5[52]
0.0720
423[53]
0.0664
560.5[54]
0.0870
615[55]
0.0982
497.5[56]
0.0780
Surface area[a]km2
:E[f]
2,641,700
0.005179
2,248,500
0.004408
3,948,000
0.007741
4,932,300
0.009671
3,110,200
0.006098
Volume[b]km3
:E[f]
403,744,500
0.000373
317,036,800
0.000396
737,591,000
0.000681
1,030,034,600
0.000951
515,784,000
0.000476
Mass[t]kg
:E[f]
6.32×1020[57]
0.0001
4.9×1020[53]
0.0001
1.41×1021[58]
0.0003
1.75×1021[55]
0.0003
?
Density[t]g/cm31.5±0.3[57]1.50±0.12[53]1.99±0.46[58]1.74±0.16?
Equatorial gravity[d]m/s20.270.180.240.285?
Escape velocity[e]km/s0.500.390.450.604?
Rotation period[g]days??0.36830.93330.4280[59]
Orbital period[g]years247.49273.98287.97552.5212,059
Mean orbital speedkm/s4.684.574.523.631.04
Eccentricity0.2260.1060.0380.5060.855
Inclination[f]deg.20.5923.927.9930.7411.93
Mean surface temperature[w]K~42~43~41~30~12
Number of known moons1[60]11[61]10
Planetary discriminant[l][o]0.003<0.10.0015<0.1?[x]
Absolute magnitude (H)2.34.12.711.81.5

SatellitesEdit

Key
🜨
Satellite of Earth

Satellite of Jupiter

Satellite of Saturn

Satellite of Uranus

Satellite of Neptune

Satellite of Pluto
E
Satellite of Eris


There are at least 19 natural satellites in the Solar System that are known to be massive enough to be close to hydrostatic equilibrium. Alan Stern calls these satellite planets, although the term major moon is more common.

Several of these were once in equilibrium but are no longer: these include Earth's moon[62] and all of the moons listed for Saturn apart from Titan and Rhea.[citation needed] The status of the moons of Uranus, Pluto and Eris are uncertain. Other moons that were once in equilibrium but are no longer very round, such as Saturn's Phoebe, are not included. Satellites are listed first in order from the Sun, and second in order from their parent body.

🜨Moon[63]Io[64]Europa[65]Ganymede[66]Callisto[67]Mimas[p]Enceladus[p]Tethys[p]Dione[p]Rhea[p]
FullMoon2010.jpgIo highest resolution true color.jpg        
Astronomical symbol[q]Moon symbol decrescent.svg
Mean distance
from primary:
km384,399421,600670,9001,070,4001,882,700185,520237,948294,619377,396527,108
Mean radiuskm
:E[f]
1,737.1
0.272
1,815
0.285
1,569
0.246
2,634.1
0.413
2,410.3
0.378
198.30
0.031
252.1
0.04
533
0.084
561.7
0.088
764.3
0.12
Surface area[a]1×106 km237.9341.91030.987.0730.490.7993.573.9657.337
Volume[b]1×109 km32225.315.976590.0330.0670.630.81.9
Mass1×1022 kg7.34778.944.8014.81910.7580.003750.01080.061740.10950.2306
Density[c]g/cm33.34643.5283.011.9361.831.151.610.981.481.23
Equatorial gravity[d]m/s21.6221.7961.3141.4281.2350.06360.1110.1450.2310.264
Escape velocity[e]km/s2.382.562.0252.7412.4400.1590.2390.3930.5100.635
Rotation perioddays[g]27.321582
(sync)[m]
1.7691378
(sync)
3.551181
(sync)
7.154553
(sync)
16.68902
(sync)
0.942422
(sync)
1.370218
(sync)
1.887802
(sync)
2.736915
(sync)
4.518212
(sync)
Orbital period about primarydays[g]27.321581.7691383.5511817.15455316.689020.9424221.3702181.8878022.7369154.518212
Mean orbital speed[o]km/s1.02217.3413.74010.8808.20414.3212.6311.3510.038.48
Eccentricity0.05490.00410.0090.00130.00740.02020.00470.020.0020.001
Inclination to primary's equatordeg.18.29–28.580.040.471.850.21.510.021.510.0190.345
Axial tilt[i][u]deg.6.68000–0.33[68]000000
Mean surface temperature[w]K220130102110[69]1346475648776
Atmospheric compositionArHe
NaKH
SO2[70]O2[71]O2[72]O2CO2[73]H2O, N2
CO2CH4[74]
Rings?NoNoNoNoNoNoNoNoNoYes?
Titan[p]Iapetus[p]Miranda[r]Ariel[r]Umbriel[r]Titania[r]Oberon[r]Triton[75]Charon[26]EDysnomia
[citation needed]
Titan in true color.jpgIapetus true.jpg        
Mean distance
from primary:
km1,221,8703,560,820129,390190,900266,000436,300583,519354,75917,53637,300
Mean radiuskm
:E[f]
2,576
0.404
735.60
0.115
235.8
0.037
578.9
0.091
584.7
0.092
788.9
0.124
761.4
0.119
1,353.4
0.212
603.5
0.095
350
0.057
Surface area[a]1×106 km283.06.70.704.2114.2967.827.28523.0184.5801.5
Volume[b]1×109 km371.61.670.0550.810.842.061.85100.920.18
Mass1×1022 kg13.4520.180530.006590.1350.120.350.30142.140.1520.143
Density[c]g/cm31.881.081.201.671.401.721.632.0611.652.52
Equatorial gravity[d]m/s21.350.220.080.270.230.390.350.780.280.78
Escape velocity[e]km/s2.640.570.190.560.520.770.731.460.580.74
Rotation perioddays[g]15.945
(sync)[m]
79.322
(sync)
1.414
(sync)
2.52
(sync)
4.144
(sync)
8.706
(sync)
13.46
(sync)
5.877
(sync)
6.387
(sync)
15.785
(sync)
Orbital period about primarydays15.94579.3221.41352.5204.1448.70613.465.8776.38715.785
Mean orbital speed[o]km/s5.573.2656.6575.508984.667973.6443.1524.390.20.172
Eccentricity0.02880.02860.00130.00120.0050.00110.00140.000020.00220.0062
Inclination to primary's equatordeg.0.3314.724.220.310.360.140.10157[h]0.0010.15
Axial tilt[i][u]deg.0000000000
Mean surface temperature[w]K93.7[76]130595861606138[77]5334
Atmospheric compositionN2CH4[78]N2CH4[79]

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 Metasyntactic variable, which is released under the 
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