The following tables list all minor planets and comets that have been visited by robotic spacecraft.
A total of 18 minor planets (asteroids, dwarf planets, and Kuiper belt objects) have been visited by space probes. Moons (not directly orbiting the Sun) and planets are not minor planets and thus are not included in the table below.
Minor planet | Space probe | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Name | Image | Dimensions (km)(a) | Discovery year | Name | Closest approach | Remarks | ||||||||
width=60 style="background-color: #ffffcc;" data-sort-type="number" | year | width=60 style="background-color: #ffffcc;" | in km | width=60 style="background-color: #ffffcc; font-weight: normal;" | in radii(b) | |||||||||
bgcolor=black | align=center | align=center | 1916 | Galileo | align=center | 1991 | align=right | align=right | 262 | Flyby; first asteroid visited by a spacecraft. | ||||
bgcolor=black | align=center | align=center | 1884 | Galileo | align=center | 1993 | align=right | align=right | 152 | Flyby; discovered Dactyl; first asteroid with a moon visited by a spacecraft, largest asteroid visited by spacecraft at the time. | ||||
bgcolor=black | align=center | align=center | 1885 | NEAR Shoemaker | align=center | 1997 | align=right | align=right | 49.5 | Flyby; largest asteroid visited by a spacecraft at the time. | ||||
bgcolor=black | align=center | align=center | 1898 | NEAR Shoemaker | align=center | 1998–2001 | align=right | landed | align=right | landed | 1998 flyby; 2000 orbited (first asteroid studied from orbit); 2001 landing; first asteroid landing, first asteroid orbited by a spacecraft, first near-Earth asteroid (NEA) visited by a spacecraft. | |||
bgcolor=black | align=center | align=center | 1992 | align=center | 1999 | align=right | 26 | align=right | 12.7 | Flyby; followed by flyby of Comet Borrelly; failed to image it during closest approach, only taking images 14,000 km from the asteroid. | ||||
bgcolor=black | align=center | align=center | 1942 | Stardust | align=center | 2002 | align=right | align=right | Flyby | |||||
bgcolor=black | align=center | align=center | 1998 | Hayabusa | align=center | 2005 | align=right | landed | align=right | landed | Landed; returned dust samples to Earth in 2010 - first sample return mission from asteroid; smallest asteroid visited by a spacecraft, first asteroid visited by a non-NASA spacecraft. | |||
bgcolor=black | align=center | align=center | 1969 | Rosetta | align=center | 2008 | align=right | 800 | align=right | 302 | Flyby; first asteroid visited by the ESA. | |||
bgcolor=black | align=center | align=center | 1852 | Rosetta | align=center | 2010 | align=right | align=right | 64.9 | Flyby on 10 July 2010; largest asteroid visited by a spacecraft at the time. | ||||
bgcolor=black | align=center | 525.4 | align=center | 1807 | Dawn | align=center | 2011–2012 | align=right | 200 | align=right | 0.76 | Space probe broke orbit on 5 September 2012 and headed to Ceres; first "big four" asteroid visited by a spacecraft, largest asteroid visited by a spacecraft at the time. | ||
bgcolor=black | align=center | align=center | 1934 | Chang'e 2 | align=center | 2012 | align=right | 3.2 | align=right | 0.70 | Flyby;[1] closest asteroid flyby, first asteroid visited by a Chinese probe. | |||
bgcolor=black | align=center | 939.4 | align=center | 1801 | Dawn | align=center | align=right | 35 | align=right | 0.07 | First "close up" picture of Ceres taken in December 2014; probe entered orbit in March 2015; first dwarf planet visited by a spacecraft, largest asteroid visited by a spacecraft. | |||
bgcolor=black | align=center | 2376.6 | align=center | 1930 | New Horizons | align=center | align=right | align=right | 10.5 | Flyby; first trans-Neptunian object visited, most distant object visited by a spacecraft (at the time of the visit). | ||||
bgcolor=black | align=center | align=center | 1999 | Hayabusa2 | align=center | align=right | landed | align=right | landed | Rendezvoused with asteroid from June 2018 to November 2019. Successful touchdowns to collect a sample in February and July 2019.[2] Three landers and an explosive impactor successfully deployed to the surface.[3] Returned dust samples to Earth in December 2020.[4] | ||||
bgcolor=black | align=center | align=center | 1999 | OSIRIS-REx | align=center | align=right | landed | align=right | landed | Arrived on 3 December 2018; entered lowest orbit on 12 June 2019; smallest object to be orbited by spacecraft and closest ever orbit;[5] [6] touchdown on 20 October 2020 to collect sample. | ||||
bgcolor=black | align=center | align=center | 2014 | New Horizons | align=center | align=right | align=right | 380 | Flew by Arrokoth (nicknamed Ultima Thule) on 1 January 2019, currently farthest object to be visited by a spacecraft. | |||||
bgcolor=black | align=center | align=center | 1996 | DART / LICIACube | align=center | 2022 | align=right | 1.19 | align=right | 3.1 | Asteroid of a near-Earth Apollo group; a flyby target; its moon being the kinetic impact target to test asteroid deflection[7] [8] | |||
Dimorphos | bgcolor=black | align=center | align=center | 2003 | DART / LICIACube | align=center | 2022 | align=right | landed | align=right | landed | Moon of a near-Earth asteroid of the Apollo group; flyby target of one and kinetic impact target of another spacecraft to test asteroid deflection | ||
152830 Dinkinesh | bgcolor=black | align=center | align=center | 1999 | Lucy | align=center | 2023 | align=right | 425 | align=right | Flyby; discovered Selam; smallest main-belt asteroid to be visited by a spacecraft[9] [10] | |||
Notes: a A minor planet's dimensions may be described by x, y, and z axes instead of an (average) diameter due to its non-spherical, irregular shape. b Closest approach given in multiples of the minor planet's mean radius | ||||||||||||||
In addition to the above listed objects, three asteroids have been imaged by spacecraft at distances too large to resolve features (over 100,000 km).
Minor planet | Space probe | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Name | Image | Dimensions (km)(a) | Discovery year | Name | Closest approach | Remarks | ||||||||
width=60 style="background-color: #ffffcc;" data-sort-type="number" | year | width=60 style="background-color: #ffffcc;" | in km | width=60 style="background-color: #ffffcc; font-weight: normal;" | in radii(b) | |||||||||
bgcolor=black | align=center | align=center | 1981 | Cassini–Huygens | align=center | 2000 | align=right | align=right | Distant incidental flyby. | |||||
bgcolor=black | align=center | align=center | 2002 | New Horizons | align=center | 2006 | align=right | align=right | Distant incidental flyby. | |||||
align=center | align=center | 2012 | Dawn | align=center | align=right | align=right | Distant incidental flyby; approached Ceres to 200,000 km in September 2017 while Dawn was in orbit.[11] |
Comet | Space probe | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Name | Image | Dimensions (km)(a) | Discovery year | Name | Closest approach | Remarks | ||||||||
width=60 style="background-color:#ffffcc;" | year | width=60 style="background-color:#ffffcc;" | in km | width=60 style="background-color:#ffffcc; font-weight: normal;" | in radii(b) | |||||||||
21P/Giacobini–Zinner | bgcolor=black | align=center | 2 | align=center | 1900 | ICE | align=center | 1985 | align=right | 7,800 | align=right | 7,800 | First flyby of a comet | |
1P/Halley | 15×9 | Vega 1 | align=center | 1986 | align=right | 8,889 | align=right | 1,620 | flyby | |||||
Vega 2 | align=center | 1986 | align=right | 8,030 | align=right | 1,460 | flyby | |||||||
Suisei | align=center | 1986 | align=right | 151,000 | align=right | 27,450 | distant flyby | |||||||
Sakigake | align=center | 1986 | align=right | 6,990,000 | align=right | 1,270,747 | distant flyby | |||||||
Giotto | align=center | 1986 | align=right | 596 | align=right | 108 | flyby; first direct images of a comet nucleus | |||||||
align=center | 1986 | align=right | 31,000,000 | align=right | 5,647,000 | distant flyby | ||||||||
bgcolor=#606060 | align=center | 2.6 | align=center | 1902 | Giotto | align=center | 1992 | align=right | 200 | align=right | 154 | flyby | ||
19P/Borrelly | bgcolor=black | align=center | 8×4×4 | align=center | 1904 | Deep Space 1 | align=center | 2001 | align=right | 2,171 | align=right | 814 | flyby; closest approach in September 2001 when probe entered the comet's coma[12] | |
81P/Wild | bgcolor=black | align=center | 5.5×4.0×3.3 | align=center | 1978 | Stardust | align=center | 2004 | align=right | 240 | align=right | 113 | flyby; first sample return mission from comet to Earth (2006) | |
9P/Tempel | 7.6×4.9 | 1867 | Deep Impact | align=center | 2005 | align=right | 500 | align=right | 80 | flyby; delivered an impactor | ||||
Deep Impacts impactor vehicle | align=center | 2005 | align=right | landed | align=right | landed | first landing on a comet (blasted a crater) | |||||||
Stardust | align=center | 2011 | align=right | 181 | align=right | 57.9 | flyby; imaged the crater created by Deep Impact | |||||||
103P/Hartley | bgcolor=black | align=center | 1.4 | align=center | 1986 | EPOXI (Deep Impact) | align=center | 2010 | align=right | 700 | align=right | 1,000 | flyby; smallest comet visited | |
67P/Churyumov–Gerasimenko | 4.1×3.3×1.8 | 1969 | Rosetta | align=center | 2016 | align=right | landed | align=right | landed | first orbiter of comet (November 2014); impacted surface as of 2016; OSIRIS captured image with 11 cm/px-resolution in Spring 2015[13] | ||||
Philae | align=center | 2014 | align=right | landed | align=right | landed | first soft landing on a comet (November 2014) | |||||||
Notes: (a)Due to a non-spherical, irregular shape, a comet's,, and axes instead of an (average) diameter are often used to describe its dimensions. (b)Closest approach given in multiples of the comet's (average mean) radius |
Comet | Space probe | ||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Name | Image | Dimensions (km)(a) | Discovery year | Name | Closest approach | Remarks | |||||||||
width=60 style="background-color:#ffffcc;" | year | width=60 style="background-color:#ffffcc;" | in km | width=60 style="background-color:#ffffcc; font-weight: normal;" | in radii(b) | ||||||||||
D/1895 Q1 (Swift) | bgcolor=black | align=center | unknown | align=center | 1895 | Mariner 4 | align=center | 1967 | align=right | 20,000,000 | align=right | unknown | Unconfirmed. Reanalysis of the probe's trajectory in 2005 speculated the probe might've approached the comet's shattered nucleus, explaining the "meteor storm" it encountered |
Comet C/2013 A1 passed close by planet Mars in October 2014, closer than the Moon is to Earth.[14] As of early 2014 it was calculated to pass as close as 0.00087abbr=onNaNabbr=on.[14] This was so close that the event was deemed dangerous to spacecraft in orbit around Mars.[15] Spacecraft that were active at that time included 2001 Mars Odyssey, Mars Express, MAVEN, Mars Orbiter Mission, and Mars Reconnaissance Orbiter in Mars orbit – and two on the surface – Mars Exploration Rover Opportunity and the Mars Science Laboratory Curiosity.
width=150 | Name ! | Diameter(a) (km) | Year of discovery | width=110 | Spacecraft ! | width=80 | Year of visit ! | Notes |
---|---|---|---|---|---|---|---|---|
align=center | 186 | align=center | 1852 | Psyche | align=center | 2029 | Large metallic main-belt asteroid[16] | |
617 Patroclus-Menoetius | align=center | 141 | align=center | 1906 | Lucy | align=center | 2033 | Binary Jupiter trojan, Trojan camp, 5th-largest Jupiter trojan |
align=center | 5 | align=center | 1983 | align=center | 2028 | Rock comet and parent body of Geminids meteor shower[17] | ||
align=center | 72 | align=center | 1973 | Lucy | align=center | 2027 | Jupiter trojan with satellite, Greek camp | |
align=center | 42 | align=center | 1997 | Lucy | align=center | 2028 | Jupiter trojan, Greek camp, a slow rotator | |
align=center | 21 | align=center | 1999 | Lucy | align=center | 2027 | Jupiter trojan with satellite, Greek camp | |
align=center | 53 | align=center | 1999 | Lucy | align=center | 2028 | Jupiter trojan, Greek camp | |
align=center | 3.9 | align=center | 1981 | Lucy | align=center | 2025 | Main-belt asteroid and member of the Erigone family[18] | |
align=center | 0.8 | align=center | 1996 | Hera | align=center | 2026 | Probe will study the results obtained by the NASA's DART impactor 4 years after its mission.[19] [20] | |
Dimorphos | align=center | align=center | 2003 | Hera | align=center | 2026 | Probe will study the results obtained by the NASA's DART impactor 4 years after its mission. | |
align=center | 0.5 | align=center | 2001 | Hayabusa2# | align=center | 2026 | Near-Earth asteroid of the Apollo group; extended mission target | |
align=center | 0.370 | align=center | 2004 | align=center | 2029 | Extended mission after sample delivery[21] | ||
align=center | 2.3 | align=center | 1973 | align=center | 2030 | Flyby[22] | ||
align=center | 22 | align=center | 1907 | align=center | 2030 | Flyby | ||
align=center | 5.2 | align=center | 1998 | align=center | 2031 | Flyby | ||
align=center | 5.4 | align=center | 2000 | align=center | 2032 | Flyby | ||
align=center | 6.7 | align=center | 1998 | align=center | 2032 | Flyby | ||
align=center | 8.0 | align=center | 1999 | align=center | 2033 | Flyby | ||
align=center | 53.62 | align=center | 1887 | align=center | 2034 | Orbit and Landing | ||
align=center | 0.041 | align=center | 2016 | Tianwen-2 | align=center | 2025 | Co-orbital near-Earth asteroid; sample return target[23] | |
align=center | 0.030 | align=center | 1998 | Hayabusa2# | align=center | 2031 | Near-Earth asteroid of the Apollo group; extended mission target[24] | |
align=center | 0.03 | align=center | 2015 | Unnamed CNSA mission | align=center | 2029 | Near-Earth asteroid of the Aten group, will be visited by an orbiter and impactor for an asteroid deflection test.[25] | |
align=center | 0.48 | align=center | 2013 | Tianwen-2 | align=center | 2032 | Active asteroid | |
undisclosed | align=center | ? | align=center | ? | Odin | align=center | 2025 | M-type near-Earth asteroid[26] [27] [28] [29] |
(a) given diameters are estimates |
The following table lists minor planets that are proposed to be visited by spacecraft missions that have not yet been approved.
Name | data-sort-type="number" | Diameter (km) | Year of discovery | Spacecraft | Proposed dates | Notes |
---|---|---|---|---|---|---|
1086 | 2002 | Interstellar Express | Launch: 2024 Flyby: 2030s | A Voyager-like mission proposed to be launched in 2024 by the CNSA. A pair of probes would flyby Neptune, Quaoar, and one other KBO.[30] [31] | ||
2.6 | 2001 | Launch: 2025 Flyby: 2027 | Brazilian Space Agency mission to triple near-Earth asteroid system of the Amor group[32] | |||
0.370 | 2004 | Launch: 2028 Flyby: 2029 | ESA proposal[33] [34] |
Former targets for launched spacecraft.
Name | data-sort-type="number" | Diameter (km) | Date of discovery | Spacecraft | Year | Notes | |||
---|---|---|---|---|---|---|---|---|---|
2P/Encke | align=center | 4.8 | CONTOUR | align=center | 1998 | Spacecraft lost while leaving Earth orbit[35] | |||
2P/Encke | align=center | 4.8 | NEAR | align=center | 1998 | Target changed before launch | |||
4 Vesta | align=center | 525 | NEAR | align=center | 1998 | Target changed before launch | |||
6P/d'Arrest | align=center | 3.2 | CONTOUR | align=center | 2008 | Spacecraft lost while leaving Earth orbit | |||
21P/Giacobini–Zinner | align=center | 2 | Suisei | align=center | 1998 | Extended mission, spacecraft ran out of fuel en route.[36] | |||
29 Amphitrite | align=center | 204 | Galileo | align=center | 1986 | Target changed due to launch postponement | |||
46P/Wirtanen | align=center | 1.2 | Rosetta | align=center | 2011 | Initial target, was changed due to delay.[37] [38] | |||
73P/Schwassmann–Wachmann | align=center | 1.1 (before breakup) | CONTOUR | align=center | 2006 | Spacecraft lost while leaving Earth orbit | |||
76P/West–Kohoutek–Ikemura | align=center | 0.66 | Deep Space 1 | align=center | 2000 | Target changed due to launch postponement[39] | |||
85D/Boethin | EPOXI (Deep Impact) | align=center | 2007 | Astronomers were unable to locate the comet, which is too faint to be observed.[40] | |||||
align=center | 103 | Rosetta | align=center | 2007 | Target changed due to launch postponement[41] | ||||
align=center | 151 | Dawn | align=center | 2016 | Abandoned target (not seriously considered)[42] | ||||
align=center | 82.7 | JUICE | align=center | 2029 | Secondary target; abandoned to conserve fuel for primary Jupiter orbiter mission.[43] [44] | ||||
align=center | 35 | NEAR | align=center | 1998 | Target changed before launch | ||||
align=center | 5.1×1.8 | Clementine | align=center | 1995 | Mission failed before retargeting | ||||
align=center | 7.5-9.4 | NEAR | align=center | 1998 | Target changed before launch | ||||
align=center | 0.6 | Vega 2 | align=center | 1987 | Secondary target; insufficient fuel[45] | ||||
align=center | 12.4[46] | Rosetta | align=center | 2007 | Secondary target; changed for better trajectory | ||||
align=center | 9[47] | Rosetta | align=center | 2007 | Target in early mission planning, but not chosen | ||||
align=center | 2–5 | Deep Space 1 | align=center | 1998 | Target changed due to launch postponement | ||||
align=center | 5.2[48] | Rosetta | align=center | 2007 | Target changed | ||||
align=center | 4 | NEAR | align=center | 1998 | Target changed before launch | ||||
align=center | 4 | Deep Space 1 | align=center | 2001 | Secondary target; abandoned due to instrument failure[49] | ||||
align=center | ~1 | NEAR | align=center | 1997 | Target changed before launch[50] | ||||
align=center | ~1 | Hayabusa | align=center | 2002 | Target changed due to launch postponement | ||||
align=center | 5.5 | Rosetta | align=center | 2007 | Target changed due to launch postponement | ||||
(5604) 1992 FE | align=center | 0.6 | OSIRIS-REx | align=center | 2018 | Secondary target abandoned in 2010 during early mission planning | |||
(10302) 1989 ML | align=center | 0.6 | Hayabusa | align=center | 2002 | Target changed due to launch postponement | |||
(163249) 2002 GT | align=center | 0.35-0.5 | EPOXI (Deep Impact) | align=center | 2020 | Communications with spacecraft lost | |||
align=center | 0.66 | Hayabusa2 | align=center | 2023 | Target proposed for extended mission but not selected.[51] | ||||
align=center | ~0.8 | PROCYON | align=center | 2016 | Ion engine failure in heliocentric orbit[52] | ||||
align=center | 0.005-0.012 | NEA Scout | align=center | 2022 | Target changed due to launch postponement | ||||
align=center | 0.03 | Hayabusa2 | align=center | 2029 | Target proposed but not selected[53] | ||||
align=center | 0.018 | align=center | 2020 | NEA Scout | align=center | 2023 | Communications with spacecraft lost |
Name | data-sort-type="number" | Diameter (km) | Date of discovery | Spacecraft | Year | Notes | ||
---|---|---|---|---|---|---|---|---|
align=center | 939 | January 1, 1801 | align=center | [54] | ||||
align=center | 939 | January 1, 1801 | Calathus | align=center | [55] | |||
align=center | 512 | Athena | align=center | 2024 | ||||
4 Vesta | align=center | 525 | AGORA | align=center | 1990-1994 | |||
4 Vesta | align=center | 525 | MAOSEP | align=center | 1990s | |||
4 Vesta | align=center | 525 | Vesta | align=center | 1994 | |||
22P/Kopff | align=center | 3.0 | CRAF | align=center | 2001 | |||
align=center | 65 | 1927 | Centaurus | align=center | Launch: 2026 Flyby: 2030s | not selected[56] | ||
46P/Wirtanen | align=center | 1.2 | Comet Hopper | align=center | 2022 | [57] | ||
99.8 | 1857 | Launch: 2020s Flyby: 2020s | A flyby proposal of 14 asteroids, the largest being 50 Virginia. | |||||
67P/Churyumov–Gerasimenko | align=center | 4.1×3.3×1.8 | CAESAR | align=center | 2024 | [58] | ||
align=center | 4.1×3.3×1.8 | align=center | 2024 | Proposed comet sample-return mission.[59] | ||||
align=center | 4.4 | 1981 | align=center | 2024 | Proposed comet sample-return mission.[60] | |||
align=center | 1898 | Clementine 2 | align=center | 1996 | ||||
align=center | 86 | CRAF | align=center | 1998 | ||||
271 | 1977 | Centaurus | Launch: 2026 Flyby: 2030s | A flyby proposal. | ||||
align=center | 4 | Marco Polo/Hayabusa Mk2 | align=center | 2022 | ||||
align=center | 1934 | Clementine 2 | align=center | 1996 | ||||
align=center | ~1 | NEAP | align=center | 1997 | ||||
7968 Elst–Pizarro or 133P/Elst–Pizarro | align=center | ~0.6 | Castalia | align=center | 2028 | [61] | ||
260.35 | 1997 | Camilla | Launch: 2026 Flyby: 2039 | A mission concept for a flyby and impactor.[62] | ||||
25143 Itokawa | align=center | align=center | 1998 | Asteroid Redirect Mission | align=center | 2021 | [63] | |
align=center | 1.04 | Janus | align=center | 2026 | Launch delayed, target not available[64] | |||
align=center | 0.272 | New Horizons 2 | align=center | [65] | ||||
align=center | ~0.69 | New Horizons 2 | align=center | [66] | ||||
(65679) 1989 UQ | align=center | Marco Polo | align=center | 2018-2020 | ||||
align=center | ~0.1 | New Horizons 2 | align=center | [67] | ||||
99942 Apophis | align=center | 0.37 | Don Quijote | align=center | 2015 | [68] | ||
101955 Bennu | align=center | align=center | 1999 | Asteroid Redirect Mission | align=center | 2021 | ||
101955 Bennu | align=center | align=center | 1999 | HAMMER | align=center | [69] | ||
align=center | 2376 | Pluto Kuiper Express | align=center | 2004 | [70] | |||
162173 Ryugu | align=center | 0.9 | Marco Polo | align=center | 2018-2020 | |||
162173 Ryugu | align=center | 0.9 | Asteroid Redirect Mission | align=center | 2021 | [71] | ||
align=center | Marco Polo | align=center | 2018-2020 | |||||
align=center | 1.69 | Janus | align=center | 2026 | Launch delayed, target not available | |||
align=center | 1.7 | Marco Polo | align=center | 2018-2020 | ||||
align=center | 0.4 | Marco Polo | align=center | 2018-2020 | ||||
align=center | 0.4 | Asteroid Redirect Mission | align=center | 2021 | ||||
align=center | Marco Polo | align=center | 2018-2020 | |||||
align=center | 0.086-0.16 | Don Quijote | align=center | 2015 | ||||
1906 | Launch: 2026 | Proposed multiple flyby mission to Jupiter's Trojan asteroids using solar sail propulsion.[72] |