List of Solar System objects by size

This is a partial list of Solar System objects by size, arranged in descending order of mean volumetric radius, and divided into several size classes. These lists can also be sorted according to an object's mass and, for the largest objects, volume, density and surface gravity, insofar as these values are available. This list contains the Sun, the planets, dwarf planets, many of the larger small Solar System bodies, all named natural satellites, and a number of smaller objects of historical or scientific interest, such as comets and near-Earth objects.
Objects on this list are ordered by mean radius rather than mass; thus, objects on the lower portions of the table can be more massive than objects higher on the list if they have a higher density.
Many trans-Neptunian objects have been discovered; in many cases their positions in this list are approximate, as there is frequently a large uncertainty in their estimated diameters.
Solar System objects more massive than 10²¹ kilograms are known or expected to be approximately spherical. Astronomical bodies relax into rounded shapes, 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 are not in hydrostatic equilibrium at this time, and a 2019 assessment suggests that many TNOs in the size range of 400-1000 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. 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 for typical objects beyond Saturn. For TNOs there is some confidence in the diameters, but for non-binary TNOs there is no real confidence in the masses/densities. Many TNOs are often just assumed to have Pluto's density of 2.0 g/cm³, but it is just as likely that they have a comet-like density of only 0.5 g/cm³. 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/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 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. 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, 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.

Graphical overview

List of objects by mean radius

Larger than 400 km

It was once expected that any icy body larger than approximately 200 km in radius was likely to be in hydrostatic equilibrium. However, is the smallest body for which detailed measurements are consistent with hydrostatic equilibrium, whereas Iapetus is the largest icy body that has been found to not be in hydrostatic equilibrium.
For simplicity and comparative purposes, the values are manually calculated assuming a sphericity of 1. 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. The radius of Saturn's main rings is 136,775 km.

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. The known densities of TNOs in this size range are remarkably low, implying that the objects retain significant internal porosity from their formation and were never gravitationally compressed into fully solid bodies.

From 100 to 199 km

This list contains a selection of objects estimated to be between 100 and 199 km in radius. 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. Mass switches from 10²¹ kg to 10¹⁸ kg. Main-belt asteroids have orbital elements constrained by according to JPL Solar System Dynamics. Many TNOs are omitted from this list as their sizes are poorly known.

From 50 to 99 km

This list contains a selection of objects 50 and 99 km in radius. 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. Asteroid spectral types are mostly Tholen, but some might be SMASS.

Body	Image	Radius '	Mass	Type	Refs '
Bienor 54598				centaur	M
Themis 24				belt asteroid type C
Larissa Neptune VII				moon of Neptune
Ursula 375				belt asteroid type C
Amphitrite 29				belt asteroid type S
Daphne 41				belt asteroid type C; binary
Aurora 94				belt asteroid type C
Hermione 121				outer belt asteroid type C; binary
Bertha 154				belt asteroid type C
Hebe 6				belt asteroid type S
Metis 9				belt asteroid type S
Elektra 130				belt asteroid type G; trinary
Janus Saturn X				moon of Saturn
Teharonhiawako 88611				cubewano; binary
Aegle 96				belt asteroid type T
S/2015 1 Makemake I				moon of Makemake	M
Galatea Neptune VI				moon of Neptune
Phorcys Ceto I				secondary of 65489 Ceto
Palma 372				belt asteroid type B
Alauda 702				belt asteroid type C; binary
Hilda 153				outer belt asteroid; Hildas	M
Himalia Jupiter VI				moon of Jupiter
Namaka Haumea II				moon of Haumea
Weywot Quaoar I				moon of 50000 Quaoar
Freia 76				outer belt asteroid type P/type X
Kalliope 22				belt asteroid type M; binary
Amalthea Jupiter V				moon of Jupiter
Agamemnon 911				Jupiter trojan type D	M
Elpis 59				belt asteroid type CP/type B
Puck Uranus XV				moon of Uranus	M
Sycorax Uranus XVII				moon of Uranus	M
Despina Neptune V				moon of Neptune	M
Io 85				belt asteroid type FC/type B
Minerva 93				belt asteroid type C; trinary
Alexandra 54				belt asteroid type C
Laetitia 39				belt asteroid type S
Parthenope 11				belt asteroid type S
Manwë 385446				resonant KBO ; binary
Pales 49				belt asteroid type C
Arethusa 95				belt asteroid type C	M
Flora 8				belt asteroid type S
Pulcova 762				belt asteroid type F; binary
Julia 89				belt asteroid type S
Irene 14				belt asteroid type S
Aglaja 47				belt asteroid type C
Patroclus 617				Jupiter trojan type P; binary
Melpomene 18				belt asteroid type S
Nemausa 51				belt asteroid type G
Hesperia 69				belt asteroid type M
Typhon 42355				resonant SDO ; binary
Massalia 20				belt asteroid type S
Portia Uranus XII				moon of Uranus	M
Emma 283				belt asteroid type X; binary
Paha Lempo I				moon of 47171 Lempo
Lucina 146				belt asteroid type C	M
Sawiskera Teharonhiawako I				secondary of 88611 Teharonhiawako	M
Kleopatra 216				belt asteroid type M; trinary
Achilles 588				Jupiter trojan type DU	M
Panopaea 70				belt asteroid type C
Thule 279				belt asteroid type D	M
Borasisi 66652				cubewano; binary
Hestia 46				belt asteroid type P/type Xc
Leto 68				belt asteroid type S
Undina 92				belt asteroid type X
Bellona 28				belt asteroid type S
Diana 78				belt asteroid type C
Anchises 1173				Jupiter trojan type P	M
Galatea 74				belt asteroid type C
Deiphobus 1867				Jupiter trojan type D	M
Äneas 1172				Jupiter trojan type D	M
Diomedes 1437				Jupiter trojan type D	M
Terpsichore 81				belt asteroid type C
Epimetheus Saturn XI				moon of Saturn
Circe 34				belt asteroid type C
Leda 38				belt asteroid type C
Victoria 12				belt asteroid type S
Odysseus 1143				Jupiter trojan type D	M
Alcathous 2241				Jupiter trojan type D	M
Melete 56				belt asteroid type P
Mnemosyne 57				belt asteroid type S
Nestor 659				Jupiter trojan type XC	M
Harmonia 40				belt asteroid type S	M
Leleākūhonua 541132				sednoid	M
Euterpe 27				belt asteroid type S
Antilochus 1583				Jupiter trojan type D	M
Thorondor Manwë I				secondary of 385446 Manwë
Thalia 23				belt asteroid type S
Erato 62				belt asteroid type BU/type Ch	M
Astraea 5				belt asteroid type S
Pabu Borasisi I				secondary of 66652 Borasisi	M
Eos 221				belt asteroid type S/type K
Aegina 91				belt asteroid type C	M
Leukothea 35				belt asteroid type C	M
Menoetius Patroclus I				secondary of 617 Patroclus	M
Isis 42				belt asteroid type S
Klotho 97				belt asteroid type M
Troilus 1208				Jupiter trojan type FCU	M

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. Most mass values of asteroids are assumed.

Body	Image	Radius '	Mass	Type – notes	Refs '
Asterope 233				belt asteroid type T/type K	M
Pholus 5145				centaur	M
Thebe Jupiter XIV				moon of Jupiter	M
Lutetia 21				belt asteroid type M
Kalypso 53				belt asteroid type XC
Proserpina 26				belt asteroid type S
Juliet Uranus XI				moon of Uranus	M
Urania 30				belt asteroid type S
Ausonia 63				belt asteroid type S
Beatrix 83				belt asteroid type X	M
Concordia 58				belt asteroid type C	M
Echidna Typhon I				moon of 42355 Typhon	M
Automedon 2920				Jupiter trojan type D	M
90 Antiope				belt asteroid type C; binary
Prometheus Saturn XVI				moon of Saturn
Danaë 61				belt asteroid type S
Thetis 17				belt asteroid type S
Pandora 55				belt asteroid type M	M
Huenna 379				belt asteroid type B/type C; binary
Virginia 50				belt asteroid type X/type Ch
Feronia 72				belt asteroid type TDG
S/2000 1 Antiope I				secondary of 90 Antiope	M
Poulydamas 4348				Jupiter trojan type C	M
Logos 58534				cubewano; binary
Pandora Saturn XVII				moon of Saturn
Thalassa Neptune IV				moon of Neptune	M
Niobe 71				belt asteroid type S	M
Pomona 32				belt asteroid type S	M
Belinda Uranus XIV				moon of Uranus	M
Elara Jupiter VII				moon of Jupiter	M
Cressida Uranus IX				moon of Uranus	M
Amycus 55576				centaur	M
Hylonome 10370				centaur	M
3708				Jupiter trojan type C	M
Nysa 44				belt asteroid type E	M
Rosalind Uranus XIII				moon of Uranus	M
Maja 66				belt asteroid type C	M
Ariadne 43				belt asteroid type S
Iphigenia 112				belt asteroid type C
Dike 99				belt asteroid type C	M
Echeclus 60558 or 174P				centaur	M
Desdemona Uranus X				moon of Uranus	M
Eurybates 3548				Jupiter trojan type CP	M
Eurynome 79				belt asteroid type S	M
Eurydike 75				belt asteroid type M	M
Halimede Neptune IX				moon of Neptune	M
Phocaea 25				belt asteroid type S
Naiad Neptune III				moon of Neptune	M
Schwassmann– Wachmann 1 29P				comet	M
Neso Neptune XIII				moon of Neptune	M
Angelina 64				belt asteroid type E	M
Pasiphae Jupiter VIII				moon of Jupiter	M
Alkmene 82				belt asteroid type S	M
Nessus 7066				centaur	M
Polana 142				belt asteroid type F	M
Bianca Uranus VIII				moon of Uranus	M
Mathilde 253				belt asteroid type C
Hidalgo 944				centaur	M
Orus 21900				Jupiter trojan type C/type D	M
Amalthea 113				belt asteroid type S; binary	M
Prospero Uranus XVIII				moon of Uranus	M
Setebos Uranus XIX				moon of Uranus	M
Carme Jupiter XI				moon of Jupiter	M
Klytia 73				belt asteroid type S	M
Sao Neptune XI				moon of Neptune	M
Echo 60				belt asteroid type S
Metis Jupiter XVI				moon of Jupiter
Ophelia Uranus VII				moon of Uranus	M
Lysithea Jupiter X				moon of Jupiter	M
Caliban Uranus XVI				moon of Uranus	M
Laomedeia Neptune XII				moon of Neptune	M
Cordelia Uranus VI				moon of Uranus	M
Psamathe Neptune X				moon of Neptune	M

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 moons.

Body	Image	Radius '	Mass	Type – notes	Refs '
Urda 167				belt asteroid type S	M
Hydra Pluto III				moon of Pluto
Siarnaq Saturn XXIX				moon of Saturn	M
Koronis 158				belt asteroid type S	M
Nix Pluto II				moon of Pluto
Ganymed 1036				Amor asteroid type S
Okyrhoe 52872				centaur	M
Helene Saturn XII				moon of Saturn; Dione trojan	M
Sinope Jupiter IX				moon of Jupiter	M
Hippocamp Neptune XIV				moon of Neptune
Leucus 11351				Jupiter trojan type D	M
Stephano Uranus XX				moon of Uranus	M
Arrokoth 486958				cubewano; contact binary	M
Ida 243				belt asteroid type S; binary
Atlas Saturn XV				moon of Saturn
Ananke Jupiter XII				moon of Jupiter	M
Albiorix Saturn XXVI				moon of Saturn	M
Pan Saturn XVIII				moon of Saturn
Linus Kalliope I				asteroid moon of 22 Kalliope
Dioretsa 20461				centaur; damocloid	M
Perdita Uranus XXV				moon of Uranus	M
Telesto Saturn XIII				moon of Saturn; Tethys trojan	M
Mab Uranus XXVI				moon of Uranus	M
Phobos Mars I				moon of Mars
Paaliaq Saturn XX				moon of Saturn	M
Francisco Uranus XXII				moon of Uranus	M
Leda Jupiter XIII				moon of Jupiter	M
Calypso Saturn XIV				moons of Saturn; Tethys trojan	M
Polymele 15094				Jupiter trojan type P	M
Margaret Uranus XXIII				moon of Uranus	M
Ferdinand Uranus XXIV				moon of Uranus	M
Cupid Uranus XXVII				moon of Uranus	M
Ymir Saturn XIX				moon of Saturn	M
Trinculo Uranus XXI				moon of Uranus	M
Eros 433				Amor asteroid type S
Adrastea Jupiter XV				moon of Jupiter	M
Kiviuq Saturn XXIV				moon of Saturn	M
Tarvos Saturn XXI				moon of Saturn	M
Kerberos Pluto IV				moon of Pluto
Gaspra 951				belt asteroid type S
Deimos Mars II				moon of Mars
Skamandrios Hektor I				asteroid moon of 624 Hektor	M
Ijiraq Saturn XXII				moon of Saturn	M
Halley's Comet 1P				comet
Styx Pluto V				moon of Pluto
Romulus Sylvia I				asteroid moon of 87 Sylvia	M
Masursky 2685				belt asteroid type S	M
Erriapus Saturn XXVIII				moon of Saturn	M
Callirrhoe Jupiter XVII				moon of Jupiter	M
Alexhelios Kleopatra I				asteroid moon of 216 Kleopatra	M
Esclangona 1509				inner belt asteroid type S; binary	M
Themisto Jupiter XVIII				moon of Jupiter	M
Daphnis Saturn XXXV				moon of Saturn
Petit-Prince Eugenia I				asteroid moon of 45 Eugenia	M
Praxidike Jupiter XXVII				moon of Jupiter	M
Bestla Saturn XXXIX				moon of Saturn	M
Remus Sylvia II				asteroid moon of 87 Sylvia	M
Kalyke Jupiter XXIII				moon of Jupiter	M
Cleoselene Kleopatra II				asteroid moon of 216 Kleopatra	M
S/2019 1 Euphrosyne I				asteroid moon of 31 Euphrosyne	M
Tempel 1 9P				Jupiter-family comet; Deep Impact flyby and impacted	M
Phaethon 3200				Apollo asteroid type F	M
53319				Apollo asteroid type X	M
Borrelly 19P				Jupiter-family comet	M
Šteins 2867				belt asteroid type E	M
Atira 163693				Atira asteroid type S; binary	M
Annefrank 5535				belt asteroid type S	M
Balam 3749				belt asteroid type S; trinary
Pallene Saturn XXXIII				moon of Saturn	M
Florence 3122				Amor asteroid type S; trinary
Wild 2 81P				Jupiter family comet	M
Litva 2577				Mars-crosser type EU; trinary	M
Churyumov–Gerasimenko 67P				Jupiter-family comet
Donaldjohanson 52246				belt asteroid type C	M
Cuno 4183				Apollo asteroid type S/type Q	M
6178				Amor asteroid type M	M
Pichi üñëm Alauda I				asteroid moon of 702 Alauda	M
Toutatis 4179				Apollo asteroid type S
Methone Saturn XXXII				moon of Saturn	M
285263				Amor asteroid type S; binary	M
Polydeuces Saturn XXXIV				moon of Saturn; Dione trojan	M
153591				Amor asteroid type C; trinary
S/2003 1 Esclangona I				asteroid moon of 1509 Esclangona	M
APL 132524				belt asteroid type S	M
Camillo 3752				Apollo asteroid type S	M
Cruithne 3753				Aten asteroid type Q; quasi-satellite of Earth	M

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 × 10¹⁵ to 10⁹ kg, which is equivalent to one billion kg or 10¹² grams.
Currently most of the objects of mass between 10⁹ kg to 10¹² kg listed here are near-Earth asteroids. The Aten asteroid 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, and interplanetary dust cloud. '
Body Image Radius
' Mass
Type – notes Refs
Ra-Shalom
2100 Aten asteroid type C M
Geographos
1620 Apollo asteroid type S M
Midas
1981 Apollo asteroid type S M
Mithra
4486 Apollo asteroid type S M

12538 Apollo asteroid type S M
Tantalus
2102 Apollo asteroid type Q M
Braille
9969 Mars-crosser type Q M

308242 Aten asteroid type S M
Apollo
1862 Apollo asteroid type Q M

85989 Aten asteroid type K; contact binary M
Icarus
1566 Apollo asteroid type S M
Dactyl
Ida I asteroid moon of 243 Ida M
Castalia
4769 Apollo asteroid type S; contact binary M

214869 Apollo asteroid type Q M
Moshup
66391 Aten asteroid type S; binary

29075 Apollo asteroid type S

394130 Apollo asteroid M
Hartley 2
103P Jupiter-family comet

163899 Aten asteroid type S M
Nyx
3908 Amor asteroid type V M

153814 Apollo asteroid M
Apollo asteroid type S; binary M
Ryugu
162173 Apollo asteroid type Cg

162058 Amor asteroid type S M
Apollo asteroid type S; contact binary M
Hermes
69230 Apollo asteroid type Sq M
Didymos
65803 Apollo asteroid type Xk; binary
Aten
2062 Aten asteroid type S M
Aegaeon
Saturn LIII moon of Saturn M
Apollo asteroid type S M

136617 Apollo asteroid type Sq; trinary

172034 Amor asteroid type S M
Golevka
6489 Apollo asteroid type Q M
Bennu
101955 Apollo asteroid type B

153201 Aten asteroid type X M

163132 Apollo asteroid M
Squannit
asteroid moon of 66391 Moshup M
Aten asteroid type S M
Apollo asteroid M

341843 Aten asteroid type X/type C M

388188 Apollo asteroid type S; contact binary M

6037 Apollo asteroid type S M
Aten asteroid; Earth trojan M

292220 Apollo asteroid

308635 Apollo asteroid type C M
Apollo asteroid; co-orbital with Earth M
Itokawa
25143 Apollo asteroid type S
Apophis
99942 Aten asteroid type Sq
S/2009 S 1 moon of Saturn M
Apollo asteroid type S M

357439 Apollo asteroid type V; binary M
Apollo asteroid type S M
Aten asteroid type X; co-orbital with Venus M

436724 Apollo asteroid type S M
Dimorphos
Didymos I asteroid moon of 65803 Didymos M
Apollo asteroid type S M
YORP
54509 Apollo asteroid type S M
Kamoʻoalewa
469219 Apollo asteroid type S; quasi-satellite of Earth M
Duende
367943 Aten asteroid type L M
Apollo asteroid type X M
Apollo asteroid type E/type Xe M
2014 RC Apollo asteroid type Sq M
Apollo asteroid
2011 MD Apollo asteroid/Amor asteroid type S M
Apollo asteroid type F/type M
Apollo asteroid M
Surface gravity
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
The magnitude of the outward acceleration due to centrifugal force is given by
where
The surface gravity at the equator is then given by:

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Body	Image	Radius '	Mass	Type – notes	Refs
Ra-Shalom 2100				Aten asteroid type C	M
Geographos 1620				Apollo asteroid type S	M
Midas 1981				Apollo asteroid type S	M
Mithra 4486				Apollo asteroid type S	M
12538				Apollo asteroid type S	M
Tantalus 2102				Apollo asteroid type Q	M
Braille 9969				Mars-crosser type Q	M
308242				Aten asteroid type S	M
Apollo 1862				Apollo asteroid type Q	M
85989				Aten asteroid type K; contact binary	M
Icarus 1566				Apollo asteroid type S	M
Dactyl Ida I				asteroid moon of 243 Ida	M
Castalia 4769				Apollo asteroid type S; contact binary	M
214869				Apollo asteroid type Q	M
Moshup 66391				Aten asteroid type S; binary
29075				Apollo asteroid type S
394130				Apollo asteroid	M
Hartley 2 103P				Jupiter-family comet
163899				Aten asteroid type S	M
Nyx 3908				Amor asteroid type V	M
153814				Apollo asteroid	M
				Apollo asteroid type S; binary	M
Ryugu 162173				Apollo asteroid type Cg
162058				Amor asteroid type S	M
				Apollo asteroid type S; contact binary	M
Hermes 69230				Apollo asteroid type Sq	M
Didymos 65803				Apollo asteroid type Xk; binary
Aten 2062				Aten asteroid type S	M
Aegaeon Saturn LIII				moon of Saturn	M
				Apollo asteroid type S	M
136617				Apollo asteroid type Sq; trinary
172034				Amor asteroid type S	M
Golevka 6489				Apollo asteroid type Q	M
Bennu 101955				Apollo asteroid type B
153201				Aten asteroid type X	M
163132				Apollo asteroid	M
Squannit				asteroid moon of 66391 Moshup	M
				Aten asteroid type S	M
				Apollo asteroid	M
341843				Aten asteroid type X/type C	M
388188				Apollo asteroid type S; contact binary	M
6037				Apollo asteroid type S	M
				Aten asteroid; Earth trojan	M
292220				Apollo asteroid
308635				Apollo asteroid type C	M
				Apollo asteroid; co-orbital with Earth	M
Itokawa 25143				Apollo asteroid type S
Apophis 99942				Aten asteroid type Sq
S/2009 S 1				moon of Saturn	M
				Apollo asteroid type S	M
357439				Apollo asteroid type V; binary	M
				Apollo asteroid type S	M
				Aten asteroid type X; co-orbital with Venus	M
436724				Apollo asteroid type S	M
Dimorphos Didymos I				asteroid moon of 65803 Didymos	M
				Apollo asteroid type S	M
YORP 54509				Apollo asteroid type S	M
Kamoʻoalewa 469219				Apollo asteroid type S; quasi-satellite of Earth	M
Duende 367943				Aten asteroid type L	M
				Apollo asteroid type X	M
				Apollo asteroid type E/type Xe	M
2014 RC				Apollo asteroid type Sq	M
				Apollo asteroid
2011 MD				Apollo asteroid/Amor asteroid type S	M
				Apollo asteroid type F/type M
				Apollo asteroid	M