thumb|[[Parts-per-million chart of the relative mass distribution of the Solar System, each cubelet denoting 2 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. There are uncertainties in the figures for mass and radius, and irregularities in the shape and density, with accuracy often depending on how close the object is to Earth or whether it has been visited by a probe.
Solar System objects more massive than 10<sup>21</sup> 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; however, later studies revealed that icy satellites as large as Iapetus (1,470 kilometers in diameter) are not in hydrostatic equilibrium at this time, 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. Objects that are ellipsoids due to their own gravity are here generally referred to as being "round", whether or not they are actually in equilibrium today, while objects that are clearly not ellipsoidal are referred to as being "irregular".
Spheroidal bodies typically have some polar flattening due to the centrifugal force from their rotation, and can sometimes even have quite different equatorial diameters (scalene ellipsoids such as ). Unlike bodies such as Haumea, the irregular bodies have a significantly non-ellipsoidal profile, often with sharp edges.
There can be difficulty in determining the diameter (within a factor of about 2) for typical objects beyond Saturn . 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/cm<sup>3</sup>, but it is just as likely that they have a comet-like density of only 0.5 g/cm<sup>3</sup>.
For example, if a TNO is incorrectly assumed to have a mass of 3.59 kg based on a radius of 350 km with a density of 2 g/cm<sup>3</sup> but is later discovered to have a radius of only 175 km with a density of 0.5 g/cm<sup>3</sup>, its true mass would be only 1.12 kg.
The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters; however, many of the moons with a radius less than ≈100 km, such as Jupiter's Himalia, have far more uncertain masses. 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 and JPL Solar System Dynamics, However, (r = 470 km) is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium, whereas Iapetus (r = 735 km) is the largest icy body that has been found to not be in hydrostatic equilibrium. 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.
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.
Because Sedna has no known moons, directly determining its mass (estimated to be from 1.7×10<sup>21</sup> to 6.1×10<sup>21</sup> kg) is impossible without sending a probe.
{| class="wikitable sortable"
|-
! rowspan=2 style="font-weight: normal;" | Body
! rowspan=2 class="unsortable"| Image
! colspan=2 style="font-weight: normal;" | Radius
! colspan=2 | Volume
! colspan=2 | Mass
! colspan="2" |Surface area
! data-sort-type="number" | Density
! colspan=2 style="font-weight: normal;" | Gravity
! rowspan=2 | Type
! rowspan=2 data-sort-type="number"|Discovery
|-
! data-sort-type="number" | (km)
! data-sort-type="number" | (R<sub>🜨</sub>)
! data-sort-type="number" | (10<sup>9</sup> km<sup>3</sup>)
! data-sort-type="number" | ()
! data-sort-type="number" | (10<sup>21</sup> kg)
! data-sort-type="number" | (M<sub>🜨</sub>)
!(10<sup>6</sup> km<sup>2</sup>)
!🜨
! data-sort-type="number" | (g/cm<sup>3</sup>)
! data-sort-type="number" | (m/s<sup>2</sup>)
! data-sort-type="number" | (🜨)
|- style="background-color: #FBEC5D;" align=center
|Sun
|bgcolor=black| frameless|center|upright=0.3
! ± ?
|109.2
|1,409,300,000
|333,000
|10.97
|1,431,280
|1,321
!Jupiter mass|
|317.83
|61,419
|120.41
!
|83.54
!
|15.85
!
|14.94
!
|1
!
|0.903
!
|0.283
!
|0.4135
|76.30
|0.0704
!
|0.0248
|86.999
|0.171
!
|0.0225
|83.3054
|0.163
!
|1.354
|0.138
|moon of Saturn (icy)
| 1655
|- style="background-color: #D5D5D5;" align=center
|Mercury
|bgcolor=black| frameless|center|upright=0.3
!
|0.147
!
|0.3783
|58.65
|0.0541
!
|0.018
|73.005
|0.143
!
|0.082
!
|1.797
|0.183
|moon of Jupiter (terrestrial)
| 1610
|- style="background-color: #B0E0E6;" align=center
|Moon <br/>
|bgcolor=black| frameless|center|upright=0.3
!
|0.2727
|21.958
|0.0203
!
|0.0123
|37.937
|0.074
!
|0.06
!
|1.316
|0.134
|moon of Jupiter (terrestrial)
| 1610
|- style="background-color: #DDEEFF;" align=center
|Triton<br/>
|bgcolor=black| frameless|center|upright=0.3
!
|0.045
!
|0.782
|0.0797
|moon of Neptune (icy)
| 1846
|- style="background-color: #E6E6E6;" align="center"
|Pluto<br />
|bgcolor=black| frameless|center|upright=0.3
!
|0.187
|7.057
|0.00651
!
|0.0022
|17.79
|0.034
!
|0.1825
|6.59
|0.0061
!
|-
| Moon of 532037 Chiminigagua
|bgcolor=black|
|align=center |
|align=center |
|moon of 532037 Chiminigagua
|align=center |
|-
|Aegle<br />
|
|align=center |
|align=center |
|belt asteroid type T
|align=center |
|-
|Phorcys<br />
| style="background:black;"| frameless|center|upright=0.2
|align=center |
|align=center |
|secondary of 65489 Ceto
|align=center |
|-
|Palma<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type B
|align=center |
|-
|Hilda<br />
| bgcolor="#181818" | frameless|center|upright=0.2
| align="center" |
| align="center" |
|outer belt asteroid; Hildas
| align="center" |
|-
|Freia<br />
| bgcolor="black" | frameless|center|upright=0.2
| align="center" |
| align="center" |
|outer belt asteroid type P/type X
| align="center" |
|-
|<br />
|
|align=center |
|align=center |
|cubewano
|align=center |
|-
|Io<br />
|bgcolor=black| center|frameless|59x59px
|align=center |
|align=center |
|belt asteroid type FC/type B
|align=center |
|-
|Namaka<br />
| bgcolor=#181818 | frameless|center|upright=0.2
| align="center" |
| align="center" |
|moon of Haumea
| align="center" |
|-
|Flora<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Aglaja<br />
|
|align=center |
|align=center |
|belt asteroid type C
|align=center |
|-
|ǂKá̦gára<br />
| style="background:#181818;"| frameless|center|upright=0.2
|align=center |
|align=center |
|cold classical KBO; binary
|align=center |
|-
|Massalia<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Lucina<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center | ±?
|align=center |
|belt asteroid type C
|align=center |
|-
|Sawiskera<br />
| style="background:#3c3c3c;"| frameless|center|upright=0.2
|align=center |
|align=center |
|secondary of 88611 Teharonhiawako
|align=center |
|-
|Albion<br />
| bgcolor="black" |
| align="center" |
|
|TNO, first KBO discovered
| align="center" |
|-
|Hestia<br />
|
|align=center |
|align=center |
|belt asteroid type P/type Xc
|align=center |
|-
|Leto<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Undina<br />
|
|align=center |
|align=center |
|belt asteroid type X
|align=center |
|-
|Galatea<br />
|
|align=center |
|align=center |
|belt asteroid type C
|align=center |
|-
|Äneas<br />
|
|align=center |
|align=center |
|Jupiter trojan () type D
|align=center |
|-
|Kleopatra<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type M; trinary
|align=center |
|-
|Terpsichore<br />
|
|align=center |
|align=center |
|belt asteroid type C
|align=center |
|-
|Alcathous<br />
|
|align=center |
|align=center |
|Jupiter trojan () type D
|align=center |
|-
|Melete<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type P
|align=center |
|-
|Harmonia<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Euterpe<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Astraea<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Leukothea<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type C
|align=center |
|-
|Menoetius<br />
|bgcolor=#181818| frameless|center|upright=0.2
|align=center |
|align=center |
|secondary of 617 Patroclus
|align=center |
|-
|Isis<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|}
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. Many thousands of objects of this size range have yet to be discovered in the trans-Neptunian region. The number of digits is not an endorsement of significant figures. The table switches from kg to kg (Eg). Most mass values of asteroids are assumed.
{| class="wikitable sortable sticky-header-multi"
|-
! style="font-weight:normal; width:100px;"| Body
! class="unsortable" | Image
! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius<br />
! data-sort- type="number" style="width:75px;"| Mass<br />
! Type – notes
! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs<br />
|-
|Asterope<br />
|
|align=center |
|align=center |
|belt asteroid type T/type K
|align=center |
|-
|Pholus<br />
|
|align=center |
|align=center |
|centaur
|align=center |
|-
|Antiope<br />
|bgcolor=black|<!-- Do not use a non-free file here, per WP:NFLISTS -->
|align=center |
|align=center |
|belt asteroid type C; binary
|align=center |
|-
|Huenna<br />
|
|align=center |
|align=center |
|belt asteroid type B/type C; binary
|align=center |
|-
|Virginia<br />
|
|align=center |
|align=center |
|belt asteroid type X/type Ch
|align=center |
|-
|Logos<br />
|bgcolor=#3c3c3c|frameless|center|upright=0.2
|align=center |
|align=center |
|cubewano; binary
|align=center |
|-
|Belinda<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Uranus
|align=center |
|-
|Cressida<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Uranus
|align=center |
|-
|Socus<br />
|
|align=center |
|align=center |
|Jupiter trojan () type C
|align=center |
|-
|Echeclus<br />
|
|align=center |
|align=center |
|centaur
|align=center |
|-
|Eurydike<br />
|
|align=center |
|align=center |
|belt asteroid type M
|align=center |
|-
|Halimede<br />
| style="background:#6d6d6c;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Neptune
|align=center |
|-
|Neso<br />
| style="background:#181818;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Neptune
|align=center |
|-
|Pasiphae<br />
| style="background:#3c3c3c;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Jupiter
|align=center |
|-
|Nessus<br />
| style="background:#3c3c3c;"| frameless|center|upright=0.2
|align=center |
|align=center |
|centaur
|align=center |
|-
|Polana<br />
|
|align=center |
|align=center |
|belt asteroid type F
|align=center |
|-
|Bianca<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Uranus
|align=center |
|-
|Hidalgo<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|centaur
|align=center |
|-
|Sao<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Neptune
|align=center |
|-
|Ophelia<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Uranus
|align=center |
|-
|Hydra<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Pluto
|align=center |
|-
|Siarnaq<br />
| style="background:#181818;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Nix<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Pluto
|align=center |
|-
|Blarney<br />
|
|align=center |
|align=center |
|belt asteroid
|align=center |
|-
|Helene<br />
| style="background:#616161;"|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn; Dione trojan ()
|align=center |
|-
|Ida<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S; binary
|align=center |
|-
|Atlas<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Ananke<br />
| style="background:#2c2c28;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Jupiter
|align=center |
|-
|Dioretsa<br />
|
|align=center |
|align=center |
|centaur; damocloid
|align=center |
|-
|Pan<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Paaliaq<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Gaspra<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Deimos<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Mars
|align=center |
|-
|Halley's Comet<br />
| style="background:#1f0002;"|frameless|center|upright=0.2
|align=center |
|align=center |
|comet
|align=center |
|-
|Styx<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Pluto
|align=center |
|-
|Masursky<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Erriapus<br />
| style="background:#181818;"|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Esclangona<br />
|
|align=center |
|align=center |
|inner belt asteroid type S; binary
|align=center |
|-
|Themisto<br />
| style="background:#222342;"| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Jupiter
|align=center |
|-
|Praxidike<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Jupiter
|align=center |
|-
|Tempel 1<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Jupiter-family comet;
|align=center |
|-
|Ireland<br />
|
|align=center |
|align=center |
|belt asteroid
|align=center |
|-
|Phaethon<br />
| style="background:#3c3c3c;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type F
|align=center |
|-
|<br />
| style="background:#404040;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type X
|align=center |
|-
|Borrelly<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Jupiter-family comet
|align=center |
|-
|Šteins<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type E
|align=center |
|-
|Annefrank<br />
|bgcolor=black|center|frameless|91x91px
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Balam<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S; trinary
|align=center |
|-
|Pallene<br />
| style="background:#b5b5b5;"|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|Florence<br />
| style="background:#181818;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Amor asteroid type S; trinary
|align=center |
|-
|Wild 2<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Jupiter family comet
|align=center |
|-
|Litva<br />
|
|align=center |
|align=center |
|Mars-crosser type EU; trinary
|align=center |
|-
|Churyumov–Gerasimenko<br />
|bgcolor=black|frameless|center|upright=0.25
|align=center |
|align=center |
|Jupiter-family comet
|align=center |
|-
|Donaldjohanson<br />
|bgcolor=black|center|frameless|60x60px
|align=center |
|align=center |
|belt asteroid type C
|align=center |
|-
|Camelot<br />
|
|align=center |
|align=center |
|belt asteroid
|align=center |
|-
|Cuno<br />
| style="background:#3c3c3c;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S/type Q
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Amor asteroid type M
|align=center |
|-
|Pichi üñëm<br />
|
|align=center |
|align=center |
|asteroid moon of 702 Alauda
|align=center |
|-
|Toutatis<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Methone<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Amor asteroid type S; binary
|align=center |
|-
|Polydeuces<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|moon of Saturn; Dione trojan ()
|align=center |
|-
|S/2003 (1509) 1<br />
|
|align=center |
|align=center |
|asteroid moon of 1509 Esclangona
|align=center |
|-
|APL<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|belt asteroid type S
|align=center |
|-
|Camillo<br />
| style="background:#282828;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|<br />
| style="background:#E6E7E9;"|frameless|center|upright=0.2
| align="center" |1.01
| align="center" |
|Amor asteroid
| align="center" |
|}
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, 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 × 10<sup>15</sup> to 10<sup>9</sup> kg, which is equivalent to one billion kg or 10<sup>12</sup> grams (Teragram – Tg).
Currently most of the objects of mass between 10<sup>9</sup> kg to 10<sup>12</sup> kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids (NEAs). The Aten asteroid has less mass than the Great Pyramid of Giza, 5.9 × 10<sup>9</sup> 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.)
{| class="wikitable sortable sticky-header-multi"
|-
! style="font-weight:normal; width:130px;"| Object
! class="unsortable" | Image
! data-sort- type="number" style="width:85px; font-weight:normal;"| Radius<br />(m)
! data-sort- type="number" style="width:75px;"| Mass<br />(10<sup>9</sup> kg)
! Type – notes
! class="unsortable" style="font-weight: normal; width: 3.8em; text-align: center;" | Refs<br />
|-
|Ra-Shalom<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Aten asteroid type C
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Braille<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Mars-crosser type Q
|align=center |
|-
|<br />
| style="background:#282828;"| frameless|center|upright=0.2
|align=center |
|align=center |
|Aten asteroid type S
|align=center |
|-
|Apollo<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Q
|align=center |
|-
|<br />
| style="background:#646464;"|frameless|center|upright=0.25
|align=center |
|align=center |
|Aten asteroid type K; contact binary
|align=center |
|-
|Icarus<br />
| style="background:#010658;"| frameless|center|upright=0.25
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Dactyl<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|asteroid moon of 243 Ida
|align=center |
|-
|Castalia<br />
|
|align=center |
|align=center |
|Apollo asteroid type S; contact binary
|align=center |
|-
|<br />
| style="background:#181818;"| frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Q
|align=center |
|-
|Moshup<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Aten asteroid type S; binary
|align=center |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid
|align=center |
|-
|Hartley 2<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Jupiter-family comet
|align=center |
|-
|Nyx<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Amor asteroid type V
|align=center |
|-
|Wikipedia<br />
| bgcolor="black" |
| align="center" |475
| align="center" |
|Vestian asteroid
| align="center" |
|-
|Astronautica<br />
| bgcolor=black|
| align="center" |470
| align="center" |
|Hungaria asteroid type E
| align="center" |
|-
|
| style="background:#181818;"| frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S; binary
|align=center |
|-
|Ryugu<br />
|bgcolor=black|centre|frameless|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Cg
|align=center |
|-
|<br />
|bgcolor=black|<!-- Deleted image removed: -->
|align=center |
|align=center |
|Amor asteroid type S
|align=center |
|-
|<br />
| style="background:#282828;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S; contact binary
|align=center |
|-
|Hermes<br />
| style="background:#646464;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Sq
|align=center |
|-
|Didymos<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Xk; binary
|align=center |
|-
|Dinkinesh<br />
| bgcolor=black|frameless|center|upright=0.2
| align="center" |369
| align="center" |
|belt asteroid type Sq
| align="center" |
|-
|Aten<br />
|
|align=center |
|align=center |
|Aten asteroid type S
|align=center |
|-
|<br />
|
| align="center" |
| align="center" |
|Amor asteroid type S
| align="center" |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Sq; trinary
|align=center |
|-
|LINEAR<br />
| bgcolor=black|frameless|center|upright=0.2
| align="center" |
| align="center" |
|Jupiter-family comet
| align="center" |
|-
|Golevka<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Q
|align=center |
|-
|ATLAS<br />
| bgcolor="black" |frameless|center|upright=0.2
| align="center" |260 - 374
| align="center" |
|Interstellar comet
| align="center" |
|-
|<br />
| bgcolor="black" |frameless|center|upright=0.2
| align="center" |
| align="center" |
|Aten asteroid type X
| align="center" |
|-
|Bennu<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type B
|align=center |
|-
|Torifune<br />
| bgcolor=black|
| align="center" |
| align="center" |
|Apollo asteroid
| align="center" |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid
|align=center |
|-
||Squannit<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|asteroid moon of 66391 Moshup <!-- -->
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Aten asteroid; Earth trojan ()
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid
|align=center |
|-
|<br />
|
|align=center |
|align=center |
|Apollo asteroid; co-orbital with Earth
|align=center |
|-
|Itokawa<br />
|bgcolor=black| frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Apophis<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Aten asteroid type Sq
|align=center |
|-
|S/2009 S 1
| style="background:#868686;"|frameless|center|upright=0.25
|align=center |
|align=center |
|moon of Saturn
|align=center |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.25
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type V; binary
|align=center |
|-
|
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Zoozve<br />
|
|align=center |
|align=center |
|Aten asteroid type X; co-orbital with Venus
|align=center |
|-
|<br />
| style="background:#181818;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|Hathor<br />
|
| align="center" |
| align="center" |
|Aten asteroid type S
| align="center" |
|-
|Dimorphos<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|asteroid moon of 65803 Didymos
|align=center |
|-
|
| style="background:#181818;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|
| bgcolor=black|
| align="center" |65
| align="center" |
|Aten asteroid
| align="center" |
|-
|YORP<br />
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type S
|align=center |
|-
|
| bgcolor=black|
| align="center" |28.5 – 165
| align="center" |
|Apollo asteroid
| align="center" |
|-
|Kamooalewa<br />
| bgcolor="black" |
| align="center" |
| align="center" |
|Apollo asteroid type S; quasi-satellite of Earth
| align="center" |
|-
|
|bgcolor=black|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type E/type Xe
|align=center |
|-
|2014 RC
|bgcolor=#181818|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid type Sq
|align=center |
|-
|
| bgcolor="black" |frameless|center|upright=0.2
| align="center" |
| align="center" |
|Apollo asteroid type X
| align="center" |
|-
|
|
|align=center |
|align=center |
|Apollo asteroid
|align=center |
|-
|2011 MD
| style="background:#300409;"|frameless|center|upright=0.2
|align=center |
|align=center |
|Apollo asteroid/Amor asteroid type S
|align=center |
|-
|
| bgcolor=black|
| align="center" |2.5 - 5.5
| align="center" |
|Aten asteroid
| align="center" |
|-
|2023 BU
|bgcolor=#201E1F|frameless|center|upright=0.2
|align=center |
|
|Apollo asteroid
|
|-
|
| bgcolor=#121212|frameless|center|upright=0.2
| align="center" |1
| align="center" |
|Apollo asteroid type E
| align="center" |
|-
|2018 LA
| bgcolor=black|
| align="center" |0.8 - 2.6
| align="center" |
|Apollo asteroid
| align="center" |
|-
|
| bgcolor=black|
| align="center" |0.6 - 1.35
| align="center" |
|Apollo asteroid
| align="center" |
|-
|2020 CW
| bgcolor=black|
| align="center" |0.41 - 0.9
| align="center" |
|Apollo asteroid
| align="center" |
|-
|
| bgcolor=black|
| align="center" |0.25
| align="center" |
|Apollo asteroid
| align="center" |
|-
|
| bgcolor=black|
| align="center" |0.22
| align="center" |
|Apollo asteroid
| align="center" |
|-
|
| bgcolor=black|
| align="center" |0.205 - 0.465
| align="center" |
|Aten asteroid
| align="center" |
|-
|
| bgcolor=black|
| align="center" |0.2 - 0.3
| align="center" |
|Apollo asteroid
| align="center" |
|-
|EN131090
| style="background:#181818;"|frameless|center|upright=0.2
| align="center" |0.1425 - 0.15
| align="center" |0.000000044
|Apollo asteroid
| align="center" |
|}
Gallery
thumb|upright=3|center|Solar system planets, major moons, and 3 stars of different sizes are shown comparatively in three levels of zoom: one for the rocky planets, one for the gas giants, and one for the stars.
thumb|upright=3|center|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 Solar System objects most distant from the Sun
- List of space telescopes
- Lists of astronomical objects
Notes
References
-->
</references>
Further reading
- 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 Archive Planetary Science Institute
External links
- Planetary fact sheets
- Asteroid fact sheet