Minor-planet moon

Short description: Natural satellite of a minor planet

See also: Astronomy:Binary asteroid

* Top: 243 Ida and its moon Dactyl as imaged by Galileo in 1993.
* Middle: Three radar images of 66391 Moshup. The 'streaks' on the image are the moon's trail as it moved while the images were created.
* Bottom: Animation of (357439) 2004 BL86 and its moon (left). Animation of (136617) 1994 CC, a triple asteroid with two moons (middle) Dinkinesh and its contact binary satellite Selam (right).

A minor-planet moon is an astronomical object that orbits a minor planet as its natural satellite. As of January 2022[update], there are 457 minor planets known or suspected to have moons.[1] Discoveries of minor-planet moons (and binary objects, in general) are important because the determination of their orbits provides estimates on the mass and density of the primary, allowing insights into their physical properties that are generally not otherwise accessible.[2]

Several of the moons are quite large compared to their primaries: 90 Antiope, Mors–Somnus and Sila–Nunam (95%), Patroclus–Menoetius, Altjira and Lempo–Hiisi (90%, with Lempo–Paha at 50%). The largest known minor-planet moon in absolute size is Pluto's moon Charon, which has about half the diameter of Pluto.

There are also several known ring systems around distant objects (see: Rings of Chariklo and Chiron).

## Contents

* 1 Terminology
* 2 Discovery milestones
* 2.1 Multiple systems
* 3 Commonality
* 4 Origin
* 5 Populations and classes
* 6 List
* 6.1 Near-Earth objects
* 6.2 Mars crossers
* 6.3 Main-belt asteroids
* 6.4 Jupiter trojans
* 6.5 Trans-Neptunian objects
* 7 See also
* 8 References
* 9 External links

## Terminology

See also: Astronomy:Binary asteroid

In addition to the terms satellite and moon, the term "binary" (binary minor planet) is sometimes used for minor planets with one moon, and "triple" for minor planets with two moons. If one object is much bigger it is referred to as the primary and its companion as the secondary. The term double asteroid is sometimes used for systems in which the asteroid and its moon are roughly the same size, while binary tends to be used independently from the relative sizes of the components. When binary minor planets are similar in size, the Minor Planet Center (MPC) refers to them as "binary companions" instead of referring to the smaller body as a satellite.[3] A good example of a true binary is the 90 Antiope system, identified in August 2000.[4] Very small satellites are often referred to as moonlets.[2][5]

## Discovery milestones

Prior to the era of the Hubble Space Telescope and space probes reaching the outer Solar System, attempts to detect satellites around asteroids were limited to optical observations from Earth. For example, in 1978, stellar occultation observations were claimed as evidence of a satellite for the asteroid to 532 Herculina.[6][7] However, later more-detailed imaging by the Hubble Telescope did not reveal a satellite, and the current consensus is that Herculina does not have a significant satellite.[8] There were other similar reports of asteroids having companions (usually referred to as satellites) in the following years. A letter by astronomer Thomas Hamilton in the Sky & Telescope magazine at this time pointed to apparently simultaneous impact craters on Earth (for example, the Clearwater Lakes in Quebec), suggesting that these craters were caused by pairs of gravitationally bound objects.[9]

Also in 1978, Pluto's largest moon Charon was discovered; however, at the time Pluto was still considered to be one of the major planets.

In 1993, the first asteroid moon was confirmed when the Galileo probe discovered the small Dactyl orbiting 243 Ida in the asteroid belt. The second was discovered around 45 Eugenia in 1998.[10] In 2001, 617 Patroclus and its same-sized companion Menoetius became the first known binary asteroids in the Jupiter trojans.[11] The first trans-Neptunian binary after Pluto–Charon, 1998 WW31, was optically resolved in 2002.[12]

In 2021, 130 Elektra was discovered to have three moons, making it the only known quadruple asteroid.[13]

### Multiple systems

In 2005, the asteroid 87 Sylvia was discovered to have two satellites, making it the first known triple system (also called a triple minor planet or triple asteroid).[14] This was followed by the discovery of a second moon orbiting 45 Eugenia.[15] Also in 2005, the dwarf planet Haumea was discovered to have two moons, making it the second trans-Neptunian object after Pluto known to have more than one moon.[16] Additionally, 216 Kleopatra[17] and 93 Minerva[18] were discovered to be triple asteroids in 2008 and 2009 respectively. There has been one discovered quadruple minor planet, that being 130 Elektra. Since the first few triple minor planets were discovered, more continue to be discovered. As of 2025[update], the total number of known multiple systems among minor planets is 18 (including the Pluto and Haumea systems).[1]

The following table lists all satellites of multiple systems, starting with Pluto, which was unnumbered when its first moon was discovered in 1978. The highest known multiplicities are for Pluto (a sextuple system) and 130 Elektra (a quadruple system).

Parent body  | Minor-planet moon

|

Designation  | Orbital class  | Designation  | Discovery
date  | Announcement
date  | Announcement
of triple
Pluto | Kuiper Belt | Charon | 1978/06/22 | 1978/07/07 | 2005/10/31
Nix | 2005/05/15 | 2005/10/31
Hydra
Kerberos | 2011/06/28 | 2013/07/02
Styx | 2012/06/26 | 2013/07/02
45 Eugenia | Asteroid belt | Petit-Prince | 1998/11/01 | 1999/03/20 | 2007/03/07
S/2004 (45) 1[19] | 2004/02/14 | 2007/03/07
87 Sylvia | Asteroid belt | Romulus | 2001/02/18 | 2005/08/11 | 2005/08/11
Remus | 2004/08/09
93 Minerva | Asteroid belt | Aegis | 2009/08/16 | 2013/12/17 | 2013/12/17
Gorgoneion
107 Camilla | Asteroid belt | S/2001 (107) 1[20] | 2001/03/01 | 2001/03/19 | 2016/08/07
S/2016 (107) 1[21] | 2015/05/29 | 2016/08/07
130 Elektra | Asteroid belt | – | 2003/08/15 | 2003/08/17 | 2014/12/16
– | 2014/12/06 | 2014/12/16
– | 2014/12/09 | 2021/11/06
216 Kleopatra | Asteroid belt | Alexhelios | 2008/09/19 | 2011/02/18 | 2011/02/18
Cleoselene
2577 Litva | Mars-crosser | – | 2009/02/28 | 2009/03/11 | 2013/12/22
– | 2012/06/22 | 2013/12/22
3122 Florence | Amor | – | 2017/08/29 | 2017/09/01 | 2017/09/01

3749 Balam | Asteroid belt | – | 2002/02/08 | 2002/02/13 | 2008/03/12
– | 2007/07/15 | 2008/03/12
4666 Dietz | Asteroid belt | – | 2015/09/02 | 2015/10/?? | 2018/07/20
– | 2015/09/02 | 2018/07/20
6186 Zenon | Asteroid belt | – | 2017/01/01 | 2017/01/14 | 2017/01/14

47171 Lempo | Kuiper belt | Paha | 2001/12/08 | 2002/01/10 | 2009/10/??
Hiisi | 2009/10/?? | 2009/10/??
136108 Haumea | Kuiper belt | Hiʻiaka | 2005/01/26 | 2008/09/17 | 2008/09/17
Namaka | 2005/06/30
(136617) 1994 CC | Apollo | Beta (unofficial) | 2009/06/12 | 2009/06/19 | 2009/06/19
Gamma (unofficial)
(153591) 2001 SN263 | Amor | Beta (unofficial) | 2008/02/12 | 2008/02/12 | 2008/02/12
Gamma (unofficial)
(348400) 2005 JF21 | Amor | – | 2015/08/?? | 2015/08/22 | 2020/06/09
– | 2020/05/?? | 2020/06/09
(363027) 1998 ST27 | Aten | – | 2001/10/07 | 2001/10/09 | 2024/10/11
– | 2024/10/?? | 2024/10/11

## Commonality

The data about the populations of binary objects are still patchy. In addition to the inevitable observational bias (dependence on the distance from Earth, size, albedo and separation of the components) the frequency appears to be different among different categories of objects. Among asteroids, an estimated 2% would have satellites. Among trans-Neptunian objects (TNOs), an estimated 11% are thought to be binary or multiple objects, and the majority of the large TNOs have at least one satellite, including all four IAU-listed dwarf planets.

More than 50 binaries are known in each of the main groupings: near-Earth asteroids, belt asteroids, and trans-Neptunian objects, not including numerous claims based solely on light-curve variation.

Two binaries have been found so far among centaurs with semi-major axes smaller than Neptune.[22] Both are double ring systems around 2060 Chiron and 10199 Chariklo, discovered in 1993–2011 and 2013 respectively.

## Origin

The origin of minor-planet moons is not currently known with certainty, and a variety of hypotheses exist. One such model is that minor-planet moons are formed from debris knocked off the primary by an impact. Other pairings may be formed when a small object is captured by the gravity of a larger one.

Formation by collision is constrained by the angular momentum of the components, i.e. by the masses and their separation. Close binaries fit this model (e.g. Pluto–Charon). Distant binaries however, with components of comparable size, are unlikely to have followed this scenario, unless considerable mass has been lost in the event.

The distances of the components for the known binaries vary from a few hundreds of kilometres (243 Ida, 3749 Balam) to more than 3000 km (379 Huenna) for the asteroids. Among TNOs, the known separations vary from 3,000 to 50,000 km.[22]

## Populations and classes

What is "typical" for a binary system tends to depend on its location in the Solar System (presumably because of different modes of origin and lifetimes of such systems in different populations of minor planets).[23]

* Among near-Earth asteroids, satellites tend to orbit at distances of the order of 3–7 primary radii, and have diameters two to several times smaller than the primary. Since these binaries are all inner-planet crossers, it is thought that tidal stresses that occurred when the parent object passed close to a planet may be responsible for the formation of many of them, although collisions are thought to also be a factor in the creation of these satellites.
* Among main-belt asteroids, the satellites are usually much smaller than the primary (a notable exception being 90 Antiope), and orbit around 10 primary radii away. Many of the binary systems here are members of asteroid families, and a good proportion of satellites are expected to be fragments of a parent body whose disruption after an asteroid collision produced both the primary and satellite.

The eight largest TNOs with moons (Pluto, Haumea, Makemake, Eris, Quaoar, Gonggong, Orcus and Salacia), with the Earth to scale. Gonggong is written as its provisional designation, 2007 OR10.

* Among trans-Neptunian objects, it is common for the two orbiting components to be of comparable size, and for the semi-major axis of their orbits to be much larger − about 100 to 1000 primary radii. A significant proportion of these binaries are expected to be primordial.
* Pluto has five known moons. Its largest moon Charon has a radius of more than half that of Pluto, and is large enough to orbit a point outside Pluto's surface. In fact, each orbits the common barycenter between them, with Pluto's orbit entirely enclosed by Charon's; thus they form a binary system informally referred to as a double dwarf planet. Pluto's four other moons, Nix, Hydra, Kerberos, and Styx, are far smaller and orbit the Pluto–Charon system.
* Haumea has two moons with radii estimated around 155 km (Hiʻiaka) and 85 km (Namaka).
* Makemake has one known moon, S/2015 (136472) 1, estimated to be some 160 kilometers (100 mi) in diameter.
* 47171 Lempo is a unique trans-Neptunian triple system: Lempo and its moon of roughly equal mass, Hiisi, form a close-proximity binary, separated by roughly 867 km. A second moon, Paha, orbits the Lempo–Hiisi binary at about 7411 km.
* Eris has one known moon, Dysnomia. Its radius, based on its brightness, is estimated to be roughly between 150 and 350 km.[24]

##  List

As of January 2022[update], there are 457 minor planets (systems) with 477 known companions.[1] The following table is a listing of the total number of these systems by orbital class:

# of Systems | Orbital class | List by class | Multiple satellites

|
|
|

86 | Near-Earth objects | go to list | Three systems with two satellites: 3122 Florence, (136617) 1994 CC, and (153591) 2001 SN263.
31 | Mars-crossing asteroids | go to list | One system with two satellites: 2577 Litva.
212 | Main-belt asteroids | go to list | Eight systems with two satellites: 45 Eugenia, 87 Sylvia, 93 Minerva, 107 Camilla, 216 Kleopatra, 3749 Balam, 4666 Dietz, 6186 Zenon; and one quadruple system with three satellites: 130 Elektra.
6 | Jupiter trojans | go to list | –
122 | Trans-Neptunian objects | go to list | Two systems with two satellites: 47171 Lempo and 136108 Haumea; one system with five satellites: 134340 Pluto.[1][25]

### Near-Earth objects

This is a list of near-Earth asteroids with companions.[1] Candidate binaries with an unconfirmed status are displayed on a dark background.[26] For an overview, see summary and introduction.

System  | Primary  | Secondary  | Refs

|
|
|

Designation  | Class | De
(km)  | s/p-ratio  | YOD  | Dp
(km)  | RTp
(hours)  | Designation  | YOD  | Ds
(km)  | RTs
(hours)  | as
(km)  | Ps
(hours)
1862 Apollo | APO | 1.55  | 0.052  | 1932  | 1.55  | 3.065  | –  | 2005  | 0.08  | –  | 3.75  | 27.36  | BIN JPL LoMP LCDB
1866 Sisyphus | APO  | 8.48  | 0.1  | 1972  | 8.44  | 2.3909  | –  | 1985  | 0.84  | –  | 19  | 27.12  | BIN JPL LoMP LCDB
3122 Florence | AMO | 4.40  | 0.04
0.04  | 1981  | 4.4  | 2.3581  | –  | 2017  | 0.2  | –  | 4.6  | 7.2  | BIN JPL LoMP LCDB
–  | 2017  | 0.3  | –  | 9.8  | 24
3671 Dionysus | AMO  | 1.46  | 0.2  | 1984  | 1.43  | 2.705  | S/1997 (3671) 1[27] | 1997  | 0.29  | –  | 3.4  | 27.744  | BIN JPL LoMP LCDB
5143 Heracles | APO | 3.65  | 0.167  | 1991  | 3.6  | 2.706  | –  | 2011  | 0.6  | –  | 4  | 15.5  | BIN JPL LoMP LCDB
5381 Sekhmet | ATE | 1.04  | 0.3  | 1991  | 1  | 2.7  | –  | 2003  | 0.3  | 10  | 1.54  | 12.5  | BIN JPL LoMP LCDB
(5646) 1990 TR | AMO | 2.72  | 0.18+  | 1990  | 2.68  | 3.1999  | –  | 2012  | 0.48  | –  | 5.1  | 19.4712  | BIN JPL LoMP LCDB
7088 Ishtar | AMO | 1.51  | 0.42  | 1992  | 1.39  | 2.679  | –  | 2006  | 0.33  | –  | 2.8  | 20.6496  | BIN JPL LoMP LCDB
(7888) 1993 UC | APO | 2.72  | –  | 1993  | 2.72  | 2.34  | –  | 2013  | –  | –  | 7.7  | 35.04  | BIN JPL LoMP LCDB
15745 Yuliya | AMO | 1.2  | 0.46+  | 1991  | 0.61+  | 3.2495  | –  | 2018  | 0.28+  | –  | –  | 11.735  | BIN JPL LoMP LCDB
(31345) 1998 PG | AMO  | 0.94  | 0.3  | 1998  | 0.9  | 2.51620  | –  | 2001  | 0.27  | –  | 1.4  | 14.0064  | BIN JPL LoMP LCDB
(31346) 1998 PB1 | AMO | 1.26  | 0.38+  | 1998  | 1.18  | 2.7358  | –  | 2021  | 0.45+  | –  | 4.6  | 55.39  | BIN JPL
LoMP LCDB
(35107) 1991 VH | APO | 1.12  | 0.4  | 1991  | 1.04  | 2.624  | S/2008 (35107) 1[28] | 1997  | 0.42  | –  | 3.26  | 32.64  | BIN JPL LoMP LCDB
(53110) 1999 AR7 | AMO | 1.5  | 0.41+  | 1999  | 1.4  | 2.7375  | –  | 2015  | 0.6+  | –  | 3.8  | 31.32  | BIN JPL LoMP LCDB
65803 Didymos | AMO  | 0.77  | 0.22  | 1996  | 0.75  | 2.259  | Dimorphos
S/2003 (65803) 1  | 2003  | 0.177  | –  | 1.18  | 11.8992  | BIN JPL LoMP LCDB
(66063) 1998 RO1 | ATE | 0.89  | 0.48  | 1998  | 0.8  | 2.492  | –  | 2002  | 0.38  | –  | 1.2  | 14.5392  | BIN JPL LoMP LCDB
66391 Moshup | ATE  | 1.39  | 0.341  | 1999  | 1.317  | 2.7645  | Squannit
S/2001 (66391) 1  | 2001  | 0.451  | 17.4  | 2.548  | 17.4216  | BIN JPL LoMP LCDB
(68063) 2000 YJ66 | AMO | 2.3  | –  | 2000  | 2.3  | 2.1102  | –  | 2014  | –  | –  | 3.8  | 15.7  | BIN JPL LoMP LCDB
69230 Hermes | APO | 0.81  | 0.9  | 1937  | 0.6  | 13.894  | –  | 2003  | 0.54  | 13.892  | 1.1  | 13.8936  | BIN JPL LoMP LCDB
(85275) 1994 LY | AMO | 2.51  | 0.24+  | 1994  | 2.44  | 2.696  | –  | 2020  | 0.59+  | –  | 4.2  | 16.6238  | BIN JPL LoMP LCDB
(85938) 1999 DJ4 | APO  | 0.48  | 0.5  | 1999  | 0.43  | 2.514  | –  | 2004  | 0.21  | –  | 0.8  | 17.7312  | BIN JPL LoMP LCDB
(88710) 2001 SL9 | APO  | 1  | 0.28  | 2001  | 0.96  | 2.4  | –  | 2001  | 0.2  | –  | 1.6  | 16.399  | BIN JPL LoMP LCDB
(136617) 1994 CC | APO  | 0.64  | 0.182
0.129  | 1994  | 0.62  | 2.3886  | Beta (unofficial)  | 2009  | 0.113  | –  | 1.729  | 29.832  | BIN JPL LoMP LCDB
Gamma (unofficial)  | 2009  | 0.08  | –  | 6.130  | 201.024
(136993) 1998 ST49 | APO  | 0.69  | 0.109  | 1998  | 0.69  | 2.302  | –  | 2012  | 0.08  | –  | –  | –  | BIN JPL LoMP LCDB
(137170) 1999 HF1 | ATE | 3.73  | 0.23  | 1999  | 3.64  | 2.319  | –  | 1999  | 0.84  | –  | 7.3  | 14.01696  | BIN JPL LoMP LCDB
(138095) 2000 DK79 | AMO | 2.18  | –  | 2000  | 2.18  | 4.243  | –  | 2013  | –  | –  | –  | –  | BIN JPL LoMP LCDB
(143649) 2003 QQ47 | APO | 0.995  | 0.33  | 2003  | 0.94  | 2.6446  | –  | 2021  | 0.31  | 13.065  | 1.4  | 13.07  | BIN JPL
LoMP LCDB
(152931) 2000 EA107 | ATE | 1.65  | –  | 2000  | 1.65  | 4.1367  | –  | 2019  | –  | 16.079  | –  | –  | BIN JPL
LoMP LCDB
(153591) 2001 SN263 | AMO  | 2.85  | 0.408
0.177  | 2001  | 2.6  | 3.425  | Beta (unofficial)  | 2008  | 1.06  | –  | 16.633  | 149.4  | BIN JPL LoMP LCDB
Gamma (unofficial)  | 2008  | 0.46  | –  | 3.804  | 16.464
(153958) 2002 AM31 | APO | 0.46  | 0.25  | 2002  | 0.45  | 2.817  | –  | 2012  | 0.11  | –  | 1.5  | 26.304  | BIN JPL LoMP LCDB
(162000) 1990 OS | APO  | 0.3  | 0.167  | 1990  | 0.3  | 2.536  | –  | 2003  | 0.05  | –  | 0.6  | 21  | BIN JPL LoMP LCDB
(162483) 2000 PJ5 | ATE | 0.62  | 0.5  | 2000  | 0.55  | 2.642  | –  | 2005  | 0.28  | –  | 1.05  | 14.16  | BIN JPL LoMP LCDB
163693 Atira | ATI | 4.9  | 0.21  | 2003  | 4.8  | 2.9745  | –  | 2017  | 1  | –  | 6  | 15.504  | BIN JPL LoMP LCDB
(164121) 2003 YT1 | APO | 1.12  | 0.191  | 2003  | 1.1  | 2.343  | –  | 2004  | 0.21  | –  | 3.93  | 36.696  | BIN JPL LoMP LCDB
(175706) 1996 FG3 | APO  | 1.69  | 0.28  | 1996  | 1.69  | 3.595195  | –  | 1998  | 0.49  | 16.15  | 3  | 16.1508  | BIN JPL LoMP LCDB
(185851) 2000 DP107 | APO  | 0.85  | 0.41  | 2000  | 0.8  | 2.774  | –  | 2000  | 0.3  | –  | 2.62  | 42.192  | BIN JPL LoMP LCDB
(190166) 2005 UP156 | AMO | 1.05  | –  | 2005  | 1.045  | 40.542  | –  | 2017  | –  | –  | –  | –  | BIN JPL LoMP LCDB
(190208) 2006 AQ | AMO  | 1.06  | –  | 2006  | 1.06  | 182  | –  | 2015  | –  | 2.62  | –  | –  | BIN JPL LoMP LCDB
(226514) 2003 UX34 | APO | 0.28  | 0.5  | 2003  | 0.25  | –  | –  | 2017  | 0.1  | –  | –  | –  | BIN JPL LoMP LCDB
(250162) 2002 TY57 | AMO | 0.38  | 0.18+  | 2002  | 0.37  | 2.5001  | –  | 2018  | 0.07+  | –  | 0.5  | 10.76  | BIN JPL LoMP LCDB
(276049) 2002 CE26 | APO  | 3.46  | 0.087  | 2002  | 3.46  | 3.2931  | –  | 2004  | 0.3  | –  | 4.7  | 15.6  | BIN JPL LoMP LCDB
(285263) 1998 QE2 | AMO | 3.09  | 0.25  | 1998  | 3.2  | 4.751  | –  | 2013  | 0.8  | 1.3046  | 6.212  | 31.3104  | BIN JPL LoMP LCDB
(285571) 2000 PQ9 | AMO | 1  | –  | 2000  | 1  | –  | –  | 2021  | –  | –  | –  | –  | BIN JPL
LoMP LCDB
(310560) 2001 QL142 | APO | 0.92  | –  | 2001  | 0.92  | –  | –  | 2017  | –  | –  | –  | –  | BIN JPL LoMP LCDB
(311066) 2004 DC | APO  | 0.37  | 0.2  | 2004  | 0.36  | 2.6  | –  | 2006  | 0.07  | 7  | 0.75  | 23.04  | BIN JPL LoMP LCDB
(326732) 2003 HB6 | AMO | 0.95  | 0.23  | 2003  | 0.93  | 3.463  | –  | 2021  | 0.21  | 22.92  | 2  | 22.92  | BIN JPL
LoMP LCDB
(348400) 2005 JF21 | AMO | 0.6  | 0.18  | 2005  | 0.6  | 2.4144  | –  | 2015  | 0.11  | –  | 0.9  | 14.736  | BIN JPL LoMP LCDB
(357439) 2004 BL86 | APO | 0.33  | 0.21  | 2004  | 0.32  | 2.6  | –  | 2015  | 0.07  | –  | 0.5  | 14.4  | BIN JPL LoMP LCDB
(363027) 1998 ST27 | ATE | 0.81  | 0.15  | 1998  | 0.8  | 3-  | –  | 2001  | 0.12  | <6  | 4.5  | 98.4  | BIN JPL LoMP LCDB
(363067) 2000 CO101 | APO | 0.62  | 0.065  | 2000  | 0.62  | 5.12  | –  | 2009  | 0.04  | –  | 0.61  | 7.2  | BIN JPL LoMP LCDB
(363599) 2004 FG11 | APO  | 0.17  | 0.533  | 2004  | 0.15  | 4-  | –  | 2012  | 0.08-  | –  | 0.25  | 20  | BIN JPL LoMP LCDB
(374851) 2006 VV2 | APO  | 1.82  | 0.28  | 2006  | 1.06  | 2.41  | –  | 2007  | 0.3+  | –  | 1.5  | 5.52  | BIN JPL LoMP LCDB
(385186) 1994 AW1 | AMO | 1.04  | 0.49  | 1994  | 0.94  | 2.519  | –  | 1994  | 0.46  | –  | 2  | 22.3296  | BIN JPL LoMP LCDB
(399307) 1991 RJ2 | AMO  | 0.55  | 0.47+  | 1991  | 0.5  | 3.4907  | –  | 2014  | 0.24  | 15.917  | 0.86  | 15.91704  | BIN JPL LoMP LCDB
(399774) 2005 NB7 | APO | 0.54  | 0.32+  | 2005  | 0.5  | 3.4883  | –  | 2008  | 0.2  | 15.267  | 0.6  | 15.2808  | BIN JPL LoMP LCDB
(410777) 2009 FD | APO  | 0.17  | 0.6  | 2009  | 0.15  | 4  | –  | 2015  | 0.09  | –  | 0.25  | 14.4  | BIN JPL LoMP LCDB
(450894) 2008 BT18 | APO  | 0.63  | 0.333  | 2008  | 0.6  | 2.726  | –  | 2008  | 0.2+  | –  | 1.5  | 28.8  | BIN JPL LoMP LCDB
(452561) 2005 AB | AMO | 1.95  | 0.24  | 2005  | 1.9+  | 3.339  | –  | 2005  | 0.46  | –  | 3.4  | 17.9304  | BIN JPL LoMP LCDB
(461852) 2006 GY2 | APO | 0.41  | 0.2  | 2006  | 0.4  | 2.27  | –  | 2006  | 0.08  | –  | 0.5  | 11.7  | BIN JPL LoMP LCDB
(481532) 2007 LE | APO  | 0.53  | 0.36  | 2007  | 0.5  | 2.603  | –  | 2012  | 0.18  | –  | 1.4  | 33.504  | BIN JPL LoMP LCDB
(488453) 1994 XD | APO  | 0.62  | 0.25  | 1994  | 0.6  | 2.736  | –  | 2005  | 0.15+  | –  | 0.6  | 17.976  | BIN JPL LoMP LCDB
(489486) 2007 GS3 | APO  | 1.067  | 0.46  | 2007  | 0.97  | 3.497  | –  | 2019  | 0.45  | 41.36  | 3.2  | 41.36  | BIN JPL LoMP LCDB
(494658) 2000 UG11 | APO  | 0.29  | 0.5  | 2000  | 0.26  | 4.44  | –  | 2000  | 0.13  | –  | 0.426  | 18.4  | BIN JPL LoMP LCDB
(523625) 2008 DG17 | APO  | 0.38  | –  | 2008  | 0.38  | –  | –  | 2013  | –  | –  | –  | –  | BIN JPL LoMP LCDB
(523775) 2014 YB35 | APO  | 0.34  | 0.5-  | 2014  | 0.3  | –  | –  | 2015  | 0.15-  | –  | –  | –  | BIN JPL LoMP LCDB
(741081) 2005 LW3 | APO | 0.40  | 0.25  | 2005  | 0.40  | 3.6  | –  | 2022  | 0.1  | –  | 4  | –  | BIN JPL LCDB
(49494) 1994 CJ1 | APO  | 0.21-  | 1  | 1994  | 0.15-  | 30  | –  | 2014  | 0.15-  | –  | 0.525  | 30  | BIN JPL LoMP LCDB
(612098) 1999 RM45 | APO | 0.181  | 0.45  | 1999  | 0.165  | 3.0697  | –  | 2021  | 0.074  | –  | 0.29  | 16.4448  | BIN JPL LoMP LCDB
2002 BM26 | AMO | 0.61  | 0.167  | 2002  | 0.6  | 2.7  | –  | 2002  | 0.1  | –  | 1.4  | 25.8  | BIN JPL LCDB
2002 KK8 | AMO  | 0.51  | 0.2  | 2002  | 0.5  | –  | –  | 2002  | 0.1  | –  | –  | –  | BIN JPL LCDB
2003 SS84 | APO | 0.13  | 0.5  | 2003  | 0.12  | –  | –  | 2003  | 0.06  | –  | 0.27  | 24  | BIN JPL LCDB
(613286) 2005 YQ96 | ATE | 0.27  | –  | 2005  | 0.27  | rot.  | –  | 2014  | –  | –  | –  | –  | BIN JPL LoMP LCDB
2007 DT103 | APO | 0.31  | 0.267  | 2007  | 0.3  | 2.703  | –  | 2007  | 0.08+  | –  | 0.45  | 13.44  | BIN JPL LCDB
2013 PY6 | AMO | 0.53  | 0.24  | 2013  | 0.52  | 3.6246  | –  | 2020  | 0.12  | –  | 1.2  | 27.312  | BIN JPL LCDB
2013 WT44 | APO  | 1.32  | –  | 2013  | 1  | 2.8849  | –  | 2014  | –  | –  | –  | –  | BIN JPL LCDB
2014 WZ120 | APO  | 0.3  | 0.32+  | 2014  | 0.3  | 3.361  | –  | 2014  | 0.1  | –  | 0.5  | 13.665  | BIN JPL LCDB
2015 TD144 | APO  | 0.1  | –  | 2015  | 0.1  | –  | –  | 2015  | –  | –  | –  | –  | BIN JPL LCDB
2016 AZ8 | APO  | 0.47  | 0.43  | 2016  | 0.42  | 7-  | –  | 2019  | 0.18-  | <40  | 0.42+  | 7.2  | BIN JPL LCDB
2017 RV1 | APO  | 0.3  | –  | 2017  | 0.3  | –  | –  | 2017  | –  | –  | –  | –  | BIN JPL LCDB
2017 YE5 | APO  | 1.3  | 1  | 2017  | 0.9  | 20.6  | –  | 2018  | 0.9  | –  | 2.4  | 22.08  | BIN JPL LCDB
2018 EB | APO  | 0.24  | 0.167  | 2018  | 0.24  | 1.2  | –  | 2018  | 0.04  | –  | –  | –  | BIN JPL LCDB
2018 TF3 | APO  | 0.28  | 0.23  | 2018  | 0.27  | 2.4398  | –  | 2018  | 0.06  | 2.3498  | 0.35  | 10.512  | BIN JPL LCDB
2020 AZ2 | AMO  | 0.19  | –  | 2020  | 0.19  | –  | –  | 2020  | –  | –  | –  | –  | BIN JPL LCDB
2020 BX12 | APO  | 0.18  | 0.42  | 2020  | 0.165  | 2.8  | –  | 2020  | 0.07  | <49  | 0.36  | 47.04  | BIN JPL LCDB

back to summary

### Mars crossers

This is a list of Mars-crossing asteroids with companions.[1] Candidate binaries with an unconfirmed status are displayed on a dark background.[26] For an overview, see summary and introduction.

System  | Primary  | Secondary  | Refs

|
|
|

Designation  | Class | De
(km)  | s/p-ratio  | YOD  | Dp
(km)  | RTp
(hours)  | Designation  | YOD  | Ds
(km)  | as
(km)  | Ps
(hours)
1139 Atami | cls.  | 7.81  | 0.833  | 1929  | 6  | 27.45  | –  | 2005  | 5  | 15+  | 27.456  | BIN JPL LoMP LCDB
1656 Suomi | H | 7.86  | 0.26+  | 1942  | 7.61  | 2.5885  | –  | 2020  | 1.98+  | 30  | 57.92  | BIN JPL LoMP LCDB
1727 Mette | cls.  | 10.4  | 0.21  | 1965  | 10.18  | 2.98109  | –  | 2013  | 2.14  | 21  | 20.99  | BIN JPL LoMP LCDB
2044 Wirt | cls.  | 6.66  | 0.25  | 1950  | 6.46  | 3.6898  | –  | 2006  | 1.62  | 12  | 18.9696  | BIN JPL LoMP LCDB
2449 Kenos | cls.  | 6.2  | 0.23  | 1978  | 6  | 3.8481  | –  | 2015  | 1.4  | 10  | 15.84  | BIN JPL LoMP LCDB
2577 Litva | cls.  | 4.4  | 0.35
0.3  | 1975  | 4  | 2.813  | –  | 2009  | 1.4  | 21  | 35.88  | BIN JPL LoMP LCDB
S/2012 (2577) 1[29] | 2012  | 1.2  | 378  | 5136
3873 Roddy | cls.  | 7.51  | 0.27  | 1984  | 7.25  | 2.47900  | –  | 2012  | 1.96  | 14  | 19.24  | BIN JPL LoMP LCDB
4435 Holt | cls.  | 5.03  | 0.34+  | 1983  | 4.76  | 2.867  | –  | 2017  | 1.62+  | 16  | 42.648  | BIN JPL LoMP LCDB
5261 Eureka | cls.  | 1.28  | 0.39+  | 1990  | 1.19  | 2.6902  | –  | 2011  | 0.46  | 2.1  | 16.9296  | BIN JPL LoMP LCDB
(5407) 1992 AX | cls.  | 3.98  | 0.2  | 1992  | 3.9  | 2.549  | –  | 1997  | 0.78  | 5.8  | 13.5192  | BIN JPL LoMP LCDB
7002 Bronshten | cls.  | 3.12  | 0.24+  | 1971  | 3.03  | 2.67025  | –  | 2018  | 0.73+  | 4.5  | 13.32  | BIN JPL LoMP LCDB
7369 Gavrilin | cls.  | 7.92  | 0.32+  | 1975  | 7.54  | 49.12  | –  | 2007  | 2.41  | 27  | 49.128  | BIN JPL LoMP LCDB
8373 Stephengould | unus.  | 5.48  | 0.27-  | 1992  | 5.29  | 4.435  | –  | 2010  | 1.43  | 15  | 34.152  | BIN JPL LoMP LCDB
12008 Kandrup | cls.  | 4.2  | 0.75  | 1996  | 3.4  | 32.9034  | –  | 2016  | 2.6  | 10  | 32.904  | BIN JPL LoMP LCDB
13920 Montecorvino | cls.  | 2.81  | 0.22+  | 1985  | 2.81  | 2.20231  | –  | 2020  | –  | –  | 15.475  | BIN JPL LoMP LCDB
(15700) 1987 QD | cls.  | 4.15  | 0.31  | 1987  | 3.96  | 3.0586  | –  | 2010  | 1.23  | 14  | 50.4  | BIN JPL LoMP LCDB
(16635) 1993 QO | cls.  | 4.77  | 0.27+  | 1993  | 4.61  | 7.622  | –  | 2007  | 1.24  | 12  | 32.256  | BIN JPL LoMP LCDB
(23621) 1996 PA | cls.  | 2.5  | 0.27+  | 1996  | 2.4  | 2.6649  | –  | 2017  | 0.65  | 5  | 20.60  | BIN JPL LoMP LCDB
24495 Degroff | cls.  | 3.5  | –  | 2001  | 3.26  | 24.083  | –  | 2017  | –  | –  | 2.7375  | BIN JPL LoMP LCDB
26074 Carlwirtz | cls.  | 3.62  | –  | 1977  | 3.62  | 2.4593  | –  | 2013  | –  | 6.1  | 16.1112  | BIN JPL LoMP LCDB
26471 Tracybecker | cls.  | 6.05  | 0.36  | 2000  | 5.69  | 2.687  | –  | 2009  | 2.05  | 18  | 39.288  | BIN JPL LoMP LCDB
(32039) 2000 JO23 | cls.  | 4.15  | 0.32+  | 2000  | 3.96  | 6.5979  | –  | 2007  | 1.27  | 53  | 360  | BIN JPL LoMP LCDB
(34706) 2001 OP83 | cls.  | 3.62  | 0.28  | 2001  | 3.48  | 2.5644  | –  | 2005  | 0.98  | 7  | 20.76  | BIN JPL LoMP LCDB
(51356) 2000 RY76 | cls.  | 3.3  | 0.21+  | 2000  | 3.23  | 2.5572  | –  | 2012  | 0.68  | 13  | 62.04  | BIN JPL LoMP LCDB
(53432) 1999 UT55 | cls.  | 2.62  | 0.23+  | 1999  | 2.55  | 3.330  | –  | 2013  | 0.59  | 4  | 14.1  | BIN JPL LoMP LCDB
(54697) 2001 FA70 | cls.  | 3.3  | 0.19+  | 2001  | 3.2  | 2.7077  | –  | 2016  | 0.6  | –  | 16.2648  | BIN JPL LoMP LCDB
(99913) 1997 CZ5 | cls.  | 6.89  | 0.19  | 1997  | 6.77  | 2.83507  | –  | 2010  | 1.29  | 11  | 14.6808  | BIN JPL LoMP LCDB
(100015) 1989 SR7 | cls.  | 2.4  | 0.35  | 1989  | 2.3  | 2.4172  | –  | 2018  | 0.8  | 4.5  | 20.65  | BIN JPL LoMP LCDB
(114319) 2002 XD58 | cls.  | 2.62  | –  | 2002  | 2.19  | 2.9649  | –  | 2005  | –  | –  | 7.954  | BIN JPL LoMP LCDB
(218144) 2002 RL66 | cls.  | 2.97  | –  | 2002  | –  | 587  | –  | 2010  | –  | –  | –  | BIN JPL LoMP LCDB

back to summary

###  Main-belt asteroids

This is a list of main-belt asteroids with companions.[1] Candidate binaries with an unconfirmed status are displayed on a dark background.[26] For an overview, see summary and introduction.

System  | Primary  | Secondary  | Refs

|
|
|

Designation  | Class | De
(km)  | s/p-ratio  | YOD  | Dp
(km)  | RTp
(hours)  | Designation  | YOD  | Ds
(km)  | as
(km)  | Ps
(hours)
22 Kalliope | – | 168.5  | 0.168  | 1852  | 166.2  | 4.1482  | Linus
S/2001 (22) 1  | 2001  | 28  | 1095  | 86.304  | BIN JPL
LoMP LCDB
31 Euphrosyne | EUP | 267.08  | 0.025  | 1854  | 267.08  | 5.53  | –  | 2019  | 6.7  | 677  | 28.8  | BIN JPL
LoMP LCDB
41 Daphne | – | 174  | 0.011  | 1856  | 174  | 5.9880  | Peneius
S/2008 (41) 1  | 2008  | 2-  | 443  | 26.4  | BIN JPL
LoMP LCDB
45 Eugenia | – | 206  | 0.034
0.024  | 1857  | 206  | 5.699  | Petit-Prince
S/1998 (45) 1
(Eugenia I) | 1998  | 7  | 1164  | 113.18  | BIN JPL
LoMP LCDB
S/2004 (45) 1 | 2004  | 5  | 611  | 43.03
87 Sylvia | SYL | 286  | 0.038
0.037  | 1866  | 286  | 5.1836  | Romulus
S/2001 (87)
(Sylvia I) | 2001  | 10.8  | 1351  | 87.696  | BIN JPL
LoMP LCDB
Remus
S/2004 (87)
(Sylvia II) | 2004  | 10.6  | 701.6  | 32.952
90 Antiope | THM | 121  | 0.954  | 1866  | 87.8  | 16.505  | –  | 2000  | 87.8  | 171  | 16.505  | BIN JPL
LoMP LCDB
93 Minerva | GEF | 141.6  | 0.028
0.021  | 1867  | 141.6  | 5.9818  | Aegis
S/2009 (93) 1
(Minerva I) | 2009  | 3.6  | 623.5  | 57.744  | BIN JPL
LoMP LCDB
Gorgoneion
S/2009 (93) 2
(Minerva II) | 2009  | 3.2  | 375  | 26.7528
107 Camilla | SYL | 219.37  | 0.073
0.016  | 1868  | 219.37  | 4.8439  | S/2001 (107) 1[30] | 2001  | 16  | 1250  | 89.328  | BIN JPL
LoMP LCDB
S/2016 (107) 1[31] | 2016  | 3.5  | 340  | 12
121 Hermione | –  | 190  | 0.171  | 1872  | 187  | 5.551  | S/2002 (121) 1[32] | 2002  | 32  | 747  | 61.512  | BIN JPL
LoMP LCDB
130 Elektra | – | 199  | 0.03
0.01
0.008  | 1873  | 199  | 5.2247  | S/2003 (130) 1[33] | 2003  | 6.0  | 1298  | 126.9  | BIN JPL
LoMP LCDB
S/2014 (130) 1[34] | 2014  | 2.0  | 498  | 30.14
–  | 2014  | 1.6  | 345  | 16.8
216 Kleopatra | – | 135  | 0.066
0.051  | 1880  | 135  | 5.38528  | Alexhelios
S/2008 (216) 1
(Kleopatra I) | 2008  | 8.9  | 678  | 55.68  | BIN JPL
LoMP LCDB
Cleoselene
S/2008 (216) 2
(Kleopatra II) | 2008  | 6.9  | 454  | 29.76
243 Ida | KOR | 31.4  | 0.045  | 1884  | 31.4  | 4.6336  | Dactyl (Ida I)  | 1993  | 1.4  | 108  | 36.96  | BIN JPL
LoMP LCDB
283 Emma | EMA | 134.7  | 0.067  | 1889  | 134.7  | 6.888  | S/2003 (283) 1[35] | 2003  | 9  | 581  | 80.472  | BIN JPL
LoMP LCDB
317 Roxane | – | 20.56  | 0.267  | 1891  | 19.86  | 8.169  | Olympias
S/2009 (317) 1
(Roxane I) | 2009  | 5.3  | 257  | 336  | BIN JPL
LoMP LCDB
379 Huenna | THM | 87.47  | 0.066  | 1894  | 87.47  | 7.022  | S/2003 (379) 1[36] | 2003  | 5.8  | 3336  | 2102  | BIN JPL
LoMP LCDB
702 Alauda | ALA | 201.96  | 0.017  | 1910  | 201.96  | 8.354  | Pichi üñëm
S/2007 (702) 1  | 2007  | 3.51  | 1227  | 117.9  | BIN JPL
LoMP LCDB
762 Pulcova | – | 143  | 0.134  | 1913  | 141.72  | 5.839  | –  | 2000  | 19  | 703  | 106.51  | BIN JPL
LoMP LCDB
809 Lundia | FLO | 9.1  | 0.89  | 1915  | 6.9  | 15.418  | –  | 2005  | 6.1  | 15.8  | 15.418  | BIN JPL
LoMP LCDB
854 Frostia | – | 7.84  | 0.724  | 1916  | 6.35  | 37.728  | –  | 2004  | 4.6  | 17  | 37.73  | BIN JPL
LoMP LCDB
939 Isberga | – | 12.9  | 0.29  | 1920  | 12.4  | 2.9170  | –  | 2006  | 3.6  | 33  | 26.630  | BIN JPL
LoMP LCDB
1016 Anitra | FLO | 9.54  | –  | 1924  | 9.54  | 5.9295  | –  | 2016  | –  | –  | –  | BIN JPL
LoMP LCDB
1052 Belgica | FLO | 10.41  | 0.36+  | 1925  | 9.79  | 2.7097  | –  | 2012  | 3.53  | 34  | 47.26  | BIN JPL
LoMP LCDB
1089 Tama | – | 12.92  | 0.685  | 1927  | 10.7  | 16.444  | –  | 2003  | 7.33  | 20.7  | 16.445  | BIN JPL
LoMP LCDB
1313 Berna | – | 13.5  | 0.79  | 1933  | 10.6  | 25.464  | –  | 2004  | 8.37  | 25  | 25.464  | BIN JPL
LoMP LCDB
1333 Cevenola | EUN | 17.15  | 0.35  | 1934  | 17.15  | 4.88  | –  | 2008  | –  | –  | –  | BIN JPL
LoMP LCDB
1338 Duponta | FLO | 7.88  | 0.23  | 1934  | 7.68  | 3.8545  | –  | 2007  | 1.77  | 14  | 17.57  | BIN JPL
LoMP LCDB
1344 Caubeta | – | 5.84  | –  | 1935  | 5.84  | 3.122  | –  | 2011  | –  | –  | –  | BIN JPL
LoMP LCDB
1453 Fennia | H | 7.23  | 0.28+  | 1938  | 6.96  | 4.4121  | –  | 2007  | 1.95  | 15  | 22.9896  | BIN JPL
LoMP LCDB
1509 Esclangona | H | 8.17  | 0.331  | 1938  | 7.76  | 3.253  | S/2003 (1509) 1[37] | 2003  | 2.57  | 140  | 552  | BIN JPL
LoMP LCDB
1526 Mikkeli | – | 5.32  | 0.2  | 1939  | 5.22  | 2.9341  | –  | 2020  | 1.04  | 8.8  | 15.9792  | BIN JPL LoMP LCDB
1626 Sadeya | – | 15.14  | 0.26  | 1927  | 14.65  | 3.4202  | –  | 2020  | 3.81  | 54  | 51.312  | BIN JPL LoMP LCDB
1717 Arlon | – | 9.13  | –  | 1954  | 9.13  | 5.148  | –  | 2005  | –  | 17  | 18.235  | BIN JPL
LoMP LCDB
1770 Schlesinger | – | 10.61  | –  | 1967  | 10.61  | 2.8804  | –  | 2016  | –  | –  | –  | BIN JPL
LoMP LCDB
1798 Watts | FLO | 6.63  | –  | 1949  | 6.63  | –  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
1803 Zwicky | PHO | 9.93  | 0.26  | 1967  | 9.61  | 2.7329  | –  | 2021  | 2.50  | 24  | 28.459  | BIN JPL LoMP LCDB
1830 Pogson | FLO | 8.28  | 0.32+  | 1968  | 7.89  | 2.57  | –  | 2007  | 2.52  | 18  | 24.24  | BIN JPL
LoMP LCDB
1934 Jeffers | PHO | 9.24  | –  | 1972  | 9.24  | 6.0427  | –  | 2020  | –  | 15  | 15.014  | BIN JPL
LoMP LCDB
2006 Polonskaya | FLO | 4.62  | 0.22+  | 1973  | 4.51  | 3.118  | –  | 2005  | 0.99  | 8.5  | 19.1496  | BIN JPL
LoMP LCDB
2019 van Albada | FLO | 7.86  | 0.26+  | 1935  | 7.61  | 2.7294  | –  | 2019  | 1.98+  | 14  | 17.982  | BIN JPL LoMP LCDB
2047 Smetana | H | 3.07  | 0.21+  | 1971  | 3  | 2.497  | –  | 2012  | 0.63  | 6.3  | 22.4304  | BIN JPL
LoMP LCDB
2070 Humason | – | 4.57  | 0.31  | 1964  | 4.37  | 3.1883  | –  | 2018  | 1.35  | 17  | 53.50  | BIN JPL
LoMP LCDB
2121 Sevastopol | FLO | 9.32  | 0.41  | 1971  | 8.62  | 2.9064  | –  | 2010  | 3.54  | 26  | 37.104  | BIN JPL
LoMP LCDB
2131 Mayall | H | 8.56  | 0.26+  | 1975  | 8.28  | 2.568  | –  | 2009  | 2.15  | 18  | 23.4792  | BIN JPL
LoMP LCDB
2178 Kazakhstania | – | 4.31  | 0.26  | 1972  | 4.17  | 3.0183  | –  | 2018  | 1.08  | 8  | 18.50  | BIN JPL
LoMP LCDB
2242 Balaton | – | 6.13  | 0.25+  | 1936  | 5.95  | 2.7979  | –  | 2015  | 1.49+  | 9  | 12.96  | BIN JPL
LoMP LCDB
2337 Boubín | – | 8.01  | 0.16+  | 1976  | 7.91  | 2.53163  | –  | 2018  | 1.27+  | 13  | 16.09  | BIN JPL
LoMP LCDB
2343 Siding Spring | NYS | 5.2  | 0.19+  | 1979  | 5.11  | 2.10637  | –  | 2015  | 0.97+  | 7  | 11.78904  | BIN JPL
LoMP LCDB
2478 Tokai | FLO | 9.98  | 0.72+  | 1981  | 8.1  | 25.885  | –  | 2007  | 5.83  | 21  | 25.896  | BIN JPL
LoMP LCDB
2486 Metsähovi | – | 8.42  | –  | 1939  | 8.42  | 4.4518  | –  | 2007  | –  | –  | –  | BIN JPL
LoMP LCDB
2491 Tvashtri | H | 3.259  | 0.24+  | 1977  | 3.17  | 4.0852  | –  | 2018  | 0.76+  | 7.5  | 26.71  | BIN JPL
LoMP LCDB
2516 Roman | – | 4.408  | 0.23  | 1964  | 4.3  | 2.6266  | –  | 2019  | 0.99  | 7.3  | 16.2192  | BIN JPL LoMP LCDB
2535 Hämeenlinna | – | 9.42  | 0.22+  | 1939  | 9.2  | 3.23106  | –  | 2015  | 2.0+  | 19  | 21.2304  | BIN JPL
LoMP LCDB
2602 Moore | – | 9.6  | 0.28  | 1982  | 9.2  | 3.46723  | –  | 2019  | 2.6  | 22  | 27.455  | BIN JPL LoMP LCDB
2623 Zech | – | 7.92  | 0.29+  | 1919  | 7.61  | 2.7401  | –  | 2014  | 2.21+  | 48  | 117.19  | BIN JPL
LoMP LCDB
2691 Sersic | – | 5.44  | 0.43+  | 1974  | 5  | 3.8811  | –  | 2011  | 2.15  | 12  | 26.808  | BIN JPL
LoMP LCDB
2754 Efimov | – | 6.58  | 0.2  | 1966  | 6.46  | 2.4497  | –  | 2006  | 1.29  | 10  | 14.7648  | BIN JPL
LoMP LCDB
2815 Soma | FLO | 7.16  | 0.25  | 1982  | 6.95  | 2.73325  | –  | 2011  | 1.74  | 13  | 17.916  | BIN JPL
LoMP LCDB
2825 Crosby | – | 5.06  | 0.18+  | 1938  | 4.98  | 2.8135  | –  | 2017  | 0.9+  | –  | 14.3496  | BIN JPL
LoMP LCDB
2873 Binzel | FLO | 6.43  | 0.25+  | 1982  | 6.24  | 2.7037  | –  | 2019  | 1.56+  | n.a.  | 44.58  | BIN JPL
LoMP LCDB
2881 Meiden | – | 5.67  | –  | 1983  | 5.67  | 3.48  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
3034 Climenhaga | – | 9.97  | –  | 1917  | 9.97  | 2.73749  | –  | 2009  | –  | 19  | 18.9552  | BIN JPL
LoMP LCDB
3073 Kursk | FLO | 6.89  | 0.25  | 1979  | 6.69  | 3.4468  | –  | 2006  | 1.67  | 22  | 44.952  | BIN JPL
LoMP LCDB
3169 Ostro | H | 5.15  | 0.87  | 1981  | 3.89  | 6.509  | –  | 2005  | 3.38  | 5.2  | 6.5088  | BIN JPL
LoMP LCDB
3309 Brorfelde | H | 5.04  | 0.26  | 1982  | 4.88  | 2.5041  | –  | 2005  | 1.27  | 9  | 18.48  | BIN JPL
LoMP LCDB
3378 Susanvictoria | – | 6.64  | 0.24+  | 1922  | 6.46  | 2.5621  | –  | 2017  | 1.55+  | 11  | 17.1312  | BIN JPL
LoMP LCDB
3390 Demanet | FLO | 5.06  | 0.26  | 1984  | 4.9  | 2.59457  | –  | 2021  | 1.27  | 14  | 37.14  | BIN JPL LoMP LCDB
3433 Fehrenbach | – | 7.74  | 0.31  | 1963  | 7.4  | 3.916  | –  | 2015  | 2.3  | 14  | 19.6656  | BIN JPL
LoMP LCDB
3523 Arina | – | 9.07  | 0.24+  | 1975  | 8.82  | 2.6742  | –  | 2021  | 2.12+  | 22  | 29.261  | BIN JPL LoMP LCDB
3623 Chaplin | KOR | 11.1  | –  | 1981  | 11.1  | 8.361  | –  | 2008  | –  | –  | –  | BIN JPL
LoMP LCDB
3673 Levy | – | 6.41  | 0.28  | 1985  | 6.17  | 2.688  | –  | 2007  | 1.73  | 13  | 21.6  | BIN JPL
LoMP LCDB
3703 Volkonskaya | V | 3.73  | 0.4  | 1978  | 3.46  | 3.235  | –  | 2005  | 1.39  | 7.8  | 24  | BIN JPL
LoMP LCDB
3749 Balam | FLO | 4.66  | 0.466
0.42  | 1982  | 3.95  | 2.80483  | S/2002 (3749) 1[38] | 2002  | 1.84  | 289  | 1464  | BIN JPL
LoMP LCDB
–  | 2008  | 1.66  | 20  | 33.384
3782 Celle | V | 5.92  | 0.43  | 1986  | 5.44  | 3.839  | –  | 2003  | 2.34  | 18  | 36.576  | BIN JPL
LoMP LCDB
3792 Preston | PHO | 5.16  | –  | 1985  | 5.16  | 2.9277  | –  | 2016  | –  | –  | 46.8  | BIN JPL
LoMP LCDB
3657 Ermolova | V | 6.66  | 0.14  | 1978  | 6.6  | 2.60655  | –  | 2020  | 0.92  | 9.4  | 12.540  | BIN JPL
LoMP LCDB
3841 Dicicco | FLO | 6.25  | 0.28+  | 1983  | 6.02  | 3.5949  | –  | 2014  | 1.67+  | 12  | 21.6288  | BIN JPL
LoMP LCDB
3865 Lindbloom | V | 7.97  | 0.65+  | 1988  | 6.68-  | 26.016  | –  | 2020  | 4.34+  | 17  | 26.016  | BIN JPL LoMP LCDB
3868 Mendoza | – | 9.35  | 0.22  | 1960  | 9.13  | 2.7709  | –  | 2009  | 2.01  | 20  | 24.384  | BIN JPL
LoMP LCDB
3905 Doppler | – | 7.91  | 0.77+  | 1984  | 6.27  | 50.8  | –  | 2013  | 4.83  | 26  | 50.808  | BIN JPL
LoMP LCDB
3912 Troja | – | 5.93  | 0.33  | 1988  | 5.63  | 3.6594  | –  | 2021  | 1.86  | 10  | 17.371  | BIN JPL
LoMP LCDB
3951 Zichichi | – | 6.72  | 0.33+  | 1986  | 6.38  | 3.3942  | –  | 2006  | 2.11  | 16  | 27.6  | BIN JPL
LoMP LCDB
3982 Kastelʹ | – | 6.79  | –  | 1984  | 6.79  | 5.835  | –  | 2005  | –  | –  | –  | BIN JPL
LoMP LCDB
4029 Bridges | – | 8.02  | 0.24  | 1982  | 7.8  | 3.5746  | –  | 2006  | 1.87  | 13  | 16.3104  | BIN JPL
LoMP LCDB
4030 Archenhold | – | 6.97  | 0.31+  | 1984  | 6.66  | 3.27292  | –  | 2020  | 2.06+  | 12  | 15.9739  | BIN JPL
LoMP LCDB
4092 Tyr | – | 7.6  | 0.45+  | 1986  | 7.6  | 16.0875  | –  | 2020  | –  | 14  | 16.0875  | BIN JPL
LoMP LCDB
4272 Entsuji | – | 7.68  | 0.18  | 1977  | 7.56  | 2.8087  | –  | 2015  | 1.36  | 13  | 15.9456  | BIN JPL
LoMP LCDB
4288 Tokyotech | EUN | 12.3  | 0.30+  | 1989  | 11.78  | 3.18  | –  | 2019  | 3.53+  | 30  | 30.276  | BIN JPL LoMP LCDB
4296 van Woerkom | FLO | 7.6  | 0.3  | 1935  | 7.3  | 2.809  | –  | 2016  | 2.2  | 17  | 26.232  | BIN JPL
LoMP LCDB
4337 Arecibo | THM | 19.69  | 0.53  | 1985  | 24.3  | –  | –  | 2021  | 13  | 48  | 19.2  | BIN JPL
LoMP LCDB
4362 Carlisle | FLO | 5.59  | 0.33+  | 1978  | 5.31-  | 2.63289  | –  | 2021  | 1.75+  | 17  | 43.296  | BIN JPL
LoMP LCDB
4383 Suruga | – | 6.47  | 0.21+  | 1989  | 6.33  | 3.4068  | –  | 2013  | 1.33  | 11  | 16.3872  | BIN JPL
LoMP LCDB
4440 Tchantchès | H | 2.09  | 0.25+  | 1984  | 2.03  | 2.78836  | –  | 2005  | 0.51  | 3.8  | 18.6912  | BIN JPL
LoMP LCDB
4492 Debussy | – | 17.36  | 0.643  | 1988  | 14.6  | 26.606  | –  | 2004  | 9.39  | 31  | 26.616  | BIN JPL
LoMP LCDB
4514 Vilen | – | 6.29  | 0.26  | 1972  | 6.09  | 2.8922  | –  | 2015  | 1.58+  | 11  | 16.8504  | BIN JPL
LoMP LCDB
4541 Mizuno | – | 6.29  | –  | 1989  | 6.29  | 5.261  | –  | 2015  | –  | –  | –  | BIN JPL
LoMP LCDB
4607 Seilandfarm | – | 7.39  | 0.29+  | 1987  | 7.1  | 3.9683  | –  | 2009  | 2.06  | 19  | 31.632  | BIN JPL
LoMP LCDB
4666 Dietz | – | 6.83  | 0.34
–  | 1986  | 6.52  | 2.95242  | –  | 2015  | 2.22+  | 18  | 33.192  | BIN JPL
LoMP LCDB
–  | 2015  | –  | –  | –
4674 Pauling | H | 4.68  | 0.32  | 1989  | 4.46  | 2.521  | S/2004 (4674) 1[39] | 2004  | 1.41  | 250  | 3120  | BIN JPL
LoMP LCDB
4765 Wasserburg | H | 1.78  | 0.16+  | 1986  | 1.76  | 3.6231  | –  | 2013  | 0.28  | 2.9  | 15.9696  | BIN JPL
LoMP LCDB
4786 Tatianina | – | 3.28  | 0.19+  | 1985  | 3.22  | 2.9227  | –  | 2006  | 0.61  | 6.6  | 21.6696  | BIN JPL
LoMP LCDB
4788 Simpson | – | 3.58  | 0.17+  | 1986  | 3.53  | 2.81752  | –  | 2020  | 0.6+  | 5.7  | 14.981  | BIN JPL LoMP LCDB
4868 Knushevia | H | 1.535  | 0.13+  | 1989  | 1.52  | 3.1422  | –  | 2015  | 0.2+  | 2.1  | 11.922  | BIN JPL
LoMP LCDB
4951 Iwamoto | – | 5.52  | 0.76+  | 1990  | 4.39  | 118.0  | –  | 2007  | 3.34  | 31  | 118.0  | BIN JPL
LoMP LCDB
5112 Kusaji | FLO | 3.42  | 0.31  | 1987  | 3.27  | 2.7995  | –  | 2016  | 1.01  | 7  | 20.74  | BIN JPL
LoMP LCDB
5135 Nibutani | – | 4.82  | 0.28  | 1990  | 4.64  | 2.818  | –  | 2020  | 1.3  | 9.6  | 21.7368  | BIN JPL LoMP LCDB
5402 Kejosmith | – | 4.19  | 0.18+  | 1989  | 4.12  | 2.69549  | –  | 2018  | –  | 12  | 36.62  | BIN JPL
LoMP LCDB
5425 Vojtěch | V | 7.05  | 0.22  | 1984  | 6.89  | 2.64759  | –  | 2015  | 1.52  | 16  | 25.4304  | BIN JPL
LoMP LCDB
5426 Sharp | H | 2.033  | –  | 1985  | 2.033  | 4.5609  | –  | 2014  | –  | 4.5  | 24.2208  | BIN JPL
LoMP LCDB
5474 Gingasen | V | 5.05  | –  | 1988  | 5.05  | 3.6242  | –  | 2008  | –  | –  | –  | BIN JPL
LoMP LCDB
5477 Holmes | H | 3.15  | 0.37  | 1989  | 2.95  | 2.9943  | –  | 2005  | 1.09  | 6.7  | 24.43  | BIN JPL
LoMP LCDB
5481 Kiuchi | V | 7.92  | 0.33  | 1990  | 7.52  | 3.6196  | –  | 2008  | 2.48  | 15  | 20.90  | BIN JPL
LoMP LCDB
5500 Twilley | FLO | 4.48  | 0.27+  | 1981  | 4.33  | 2.9554  | –  | 2017  | 1.17+  | 7.8  | 17.556  | BIN JPL LoMP LCDB
5536 Honeycutt | – | 9.1  | 0.31  | 1955  | 8.7  | 3.583  | –  | 2016  | 2.7  | 15  | 16.325  | BIN JPL
LoMP LCDB
5674 Wolff | – | 6.04  | 0.8+  | 1986  | 4.72  | 93.7  | –  | 2015  | 3.78+  | 30  | 93.696  | BIN JPL
LoMP LCDB
5772 Johnlambert | – | 8  | 0.22+  | 1988  | 7.81  | 3.0782  | –  | 2021  | 1.72+  | 14  | 17.98  | BIN JPL
LoMP LCDB
5872 Sugano | – | 6.33  | 0.3+  | 1989  | 6.06  | 3.3642  | –  | 2016  | 1.82+  | 11  | 18.84  | BIN JPL
LoMP LCDB
5899 Jedicke | H | 2.67  | 0.32+  | 1986  | 2.54  | 2.748  | –  | 2010  | 0.81  | 4.4  | 16.699  | BIN JPL
LoMP LCDB
5905 Johnson | H | 4.79  | 0.40  | 1989  | 4.45  | 3.7824  | –  | 2005  | 1.78  | 9.3  | 21.785  | BIN JPL
LoMP LCDB
6009 Yuzuruyoshii | – | 10.32  | 0.29+  | 1990  | 9.91  | 3.03067  | –  | 2021  | 2.87+  | 33  | 44.07  | BIN JPL
LoMP LCDB
6016 Carnelli | – | 3.53  | 0.2  | 1991  | 3.46  | 2.8028  | –  | 2016  | 0.69  | 7  | 21.331  | BIN JPL
LoMP LCDB
6084 Bascom | – | 6.35  | 0.37  | 1985  | 5.96  | 2.745  | –  | 2006  | 2.2  | 20  | 43.512  | BIN JPL
LoMP LCDB
6100 Kunitomoikkansai | – | 4.06  | 0.38+  | 1991  | 3.8  | 4.3018  | –  | 2016  | 1.44+  | 7  | 18.46  | BIN JPL
LoMP LCDB
6181 Bobweber | – | 4.49  | –  | 1986  | 4.49  | 2.75796  | –  | 2008  | –  | –  | –  | BIN JPL
LoMP LCDB
6186 Zenon | – | 6  | 0.28  | 1988  | 5.8  | 2.6832  | –  | 2017  | 1.6  | 9.1  | 14.393  | BIN JPL
LoMP LCDB
6244 Okamoto | – | 6.89  | 0.25  | 1990  | 6.69  | 2.8958  | –  | 2006  | 1.67  | 13  | 20.3208  | BIN JPL
LoMP LCDB
6245 Ikufumi | – | 8.1  | 0.23  | 1990  | 7.89  | 2.9222  | –  | 2018  | 1.89  | 13  | 15.44  | BIN JPL
LoMP LCDB
(6265) 1985 TW3 | – | 4.95  | 0.24  | 1985  | 4.81  | 2.709  | –  | 2007  | 1.16  | 8  | 15.8592  | BIN JPL
LoMP LCDB
(6369) 1983 UC | FLO | 5.17  | 0.35  | 1983  | 4.9  | 2.9  | –  | 2013  | 1.7  | 15–  | 39.8  | BIN JPL
LoMP LCDB
6384 Kervin | H | 3.74  | 0.3+  | 1989  | 3.6  | 3.6194  | –  | 2015  | 1.1+  | 6.1  | 15.94  | BIN JPL
LoMP LCDB
6615 Plutarchos | – | 3.14  | 0.25  | 1960  | 3.05  | 2.3247  | –  | 2007  | 0.76  | 9.7  | 40.03  | BIN JPL
LoMP LCDB
6708 Bobbievaile | – | 9.23  | 0.57+  | 1989  | 8.02  | 8.221  | –  | 2009  | 4.57  | 19  | 24.696  | BIN JPL
LoMP LCDB
7187 Isobe | H | 6.05  | 0.17  | 1992  | 5.96  | 4.2427  | –  | 2012  | 1.01  | 16  | 33.1  | BIN JPL
LoMP LCDB
7225 Huntress | – | 6.68  | 0.21  | 1983  | 6.54  | 2.4400  | –  | 2007  | 1.37  | 10  | 14.6712  | BIN JPL
LoMP LCDB
7307 Takei | – | 10.1  | 0.24+  | 1994  | 9.8  | 2.74685  | –  | 2021  | 2.6  | 19  | 20.0064  | BIN JPL LoMP LCDB
7344 Summerfield | – | 6.25  | –  | 1992  | 6.25  | –  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
7393 Luginbuhl | FLO | 5.47  | 0.4+  | 1984  | 5.08  | 2.68763  | –  | 2017  | 2.03+  | 16  | 39.4224  | BIN JPL
LoMP LCDB
(7792) 1995 WZ3 | – | 7.45  | –  | 1995  | 7.45  | 3.16001  | –  | 2021  | –  | –  | –  | BIN JPL
LoMP LCDB
7958 Leakey | H | 2.94  | 0.30  | 1994  | 2.82  | 2.34843  | –  | 2012  | 0.85  | 10  | 50.28  | BIN JPL
LoMP LCDB
8026 Johnmckay | H | 1.69  | –  | 1991  | 1.69  | 372  | –  | 2010  | –  | –  | –  | BIN JPL
LoMP LCDB
8077 Hoyle | – | 12 | –  | 1986  | 12 | 2.7454  | –  | 2000  | –  | –  | –  | BIN JPL
LoMP LCDB
8116 Jeanperrin | FLO | 4.77  | 0.33+  | 1996  | 4.53  | 3.6169  | –  | 2007  | 1.49  | 13  | 36.144  | BIN JPL
LoMP LCDB
8306 Shoko | FLO | 3.46  | 0.40+  | 1995  | 3.21  | 3.350  | –  | 2013  | 1.28  | 9.4  | 36.192  | BIN JPL
LoMP LCDB
8474 Rettig | FLO | 6  | 0.86+  | 1985  | 4.5  | 30.54  | –  | 2015  | 3.9+  | 14  | 30.54  | BIN JPL
LoMP LCDB
9069 Hovland | H | 3.13  | 0.30+  | 1993  | 3  | 4.2175  | –  | 2004  | 0.9  | 7.8  | 30.336  | BIN JPL
LoMP LCDB
9260 Edwardolson | – | 4.12  | 0.27  | 1953  | 3.98  | 3.0852  | –  | 2005  | 1.07  | 7.2  | 17.784  | BIN JPL
LoMP LCDB
(9332) 1990 SB1 | EUN | 6.18  | 0.26  | 1990  | 5.98  | 2.98701  | –  | 2019  | 1.55  | 21  | 48.84  | BIN JPL LoMP LCDB
9617 Grahamchapman | FLO | 2.84  | 0.27  | 1993  | 2.74  | 2.2856  | –  | 2006  | 0.74  | 5.2  | 19.3848  | BIN JPL
LoMP LCDB
9783 Tensho-kan | – | 5.33  | 0.35  | 1994  | 5.1  | 2.9  | –  | 2013  | 1.8  | 13–  | 29.568  | BIN JPL
LoMP LCDB
9972 Minoruoda | – | 9.1  | –  | 1993  | –  | –  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
10123 Fideöja | – | 3.48  | 0.35  | 1993  | 3.3  | 2.87  | –  | 2013  | 1.2  | 13–  | 56.448  | BIN JPL
LoMP LCDB
10132 Lummelunda | – | 3.589  | 0.28+  | 1993  | 3.46  | 2.5099  | –  | 2017  | 0.97+  | 7.3  | 22.44  | BIN JPL
LoMP LCDB
10208 Germanicus | FLO | 3.55  | 0.46  | 1997  | 3.23  | 3.34825  | –  | 2007  | 1.48  | 13  | 58.56  | BIN JPL
LoMP LCDB
(11217) 1999 JC4 | H | 3.3  | –  | 1999  | 3.3  | 4.8219  | –  | 2013  | –  | 6.2  | 19.1712  | BIN JPL
LoMP LCDB
11227 Ksenborisova | – | 2.6  | –  | 1999  | 2.6  | 2.61679  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
11264 Claudiomaccone | – | 4.2  | 0.31+  | 1979  | 4-  | 3.1872  | –  | 2005  | 1.24+  | 6  | 15.1104  | BIN JPL
LoMP LCDB
12326 Shirasaki | FLO | 3.8  | 0.24  | 1992  | 3.7  | 2.7286  | –  | 2016  | 0.9  | 8.4  | 25.056  | BIN JPL
LoMP LCDB
13123 Tyson | PHO | 10.87  | –  | 1994  | 10.87  | 3.3303  | –  | 2015  | –  | –  | –  | BIN JPL
LoMP LCDB
15107 Toepperwein | FLO | 2.86  | 0.19+  | 2000  | 2.81  | 2.5327  | –  | 2021  | 0.53+  | 5.4  | 19.6032  | BIN JPL LoMP LCDB
15268 Wendelinefroger | NYS | 3.97  | 0.27+  | 1990  | 3.83  | 2.4224  | –  | 2008  | 1.03  | 8.7  | 25.08  | BIN JPL
LoMP LCDB
(15430) 1998 UR31 | – | 3.74  | –  | 1998  | 3.74  | 2.5273  | –  | 2010  | –  | 8.2  | 23.9592  | BIN JPL
LoMP LCDB
15822 Genefahnestock | H | 1.72  | 0.19+  | 1994  | 1.69  | 2.96  | –  | 2010  | 0.32  | 3.3  | 20.1312  | BIN JPL
LoMP LCDB
16525 Shumarinaiko | NYS | 5.25  | 0.16+  | 1991  | 5.18  | 2.5932  | –  | 2013  | 0.83  | 8.1  | 14.4096  | BIN JPL
LoMP LCDB
(16694) 1995 AJ | FLO | 4.06  | 0.23+  | 1995  | 3.96  | 3.6421  | –  | 2020  | 0.91+  | 9  | 25.2792  | BIN JPL LoMP LCDB
17081 Jaytee | – | 4.52  | 0.26+  | 1999  | 4.37  | 2.8818  | –  | 2021  | 1.137+  | 7.5  | 16.34  | BIN JPL
LoMP LCDB
17246 Christophedumas | KOR | 4.61  | 0.222  | 2000  | 4.5  | 5+  | S/2004 (17246) 1[40] | 2004  | 1  | 228  | 2160  | BIN JPL
LoMP LCDB
17260 Kušnirák | – | 4.77  | 0.26  | 2000  | 4.62  | 3.1287  | –  | 2006  | 1.2  | 7.4  | 14.7576  | BIN JPL
LoMP LCDB
17700 Oleksiygolubov | – | 3.45  | 0.31+  | 1997  | 3.29  | 3.8382  | –  | 2018  | 1.02+  | 5.4  | 15.49  | BIN JPL
LoMP LCDB
(18303) 1980 PU | – | 4.38  | 0.24  | 1980  | 4.3  | 2.72627  | –  | 2019  | 1  | 6.1  | 12.27  | BIN JPL LoMP LCDB
(18503) 1996 PY4 | PHO | 3.529  | 0.24+  | 1996  | 3.43  | 3.4391  | –  | 2021  | 0.82+  | 6.7  | 19.904  | BIN JPL
LoMP LCDB
(18527) 1996 VJ30 | V | 3.35  | 0.32  | 1996  | 3.19  | 3.3529  | –  | 2018  | 1.02  | 6  | 19.07  | BIN JPL
LoMP LCDB
(18890) 2000 EV26 | H | 4  | 0.27+  | 2000  | 3.86  | 3.8216  | –  | 2014  | 1.04+  | 6  | 14.2896  | BIN JPL
LoMP LCDB
20325 Julianoey | – | 4.94  | 0.3  | 1998  | 4.73  | 3.24474  | –  | 2014  | 1.42  | 10  | 23.5  | BIN JPL
LoMP LCDB
20882 Paulsánchez | NYS | 4.4  | –  | 2000  | 4.4  | 2.5586  | –  | 2018  | –  | 12  | 32.810  | BIN JPL
LoMP LCDB
21436 Chaoyichi | – | 1.95  | –  | 1998  | 1.8  | 2.87  | –  | 2014  | 0.6  | 0.35  | –  | BIN JPL
LoMP LCDB
21527 Horton | EUN | 4.99  | 0.21+  | 1998  | 4.88  | 2.76762  | –  | 2019  | 1.02+  | 8.7  | 17.44  | BIN JPL LoMP LCDB
22899 Alconrad | KOR | 5.68  | 0.222  | 1999  | 5.54  | 4.03  | Juliekaibarreto
S/2003 (22899) 1  | 2003  | 1.23  | 182  | 1344  | BIN JPL
LoMP LCDB
(24106) 1999 VA12 | – | –  | –  | 1999  | –  | –  | –  | 2020  | –  | –  | –  | BIN JPL
LoMP LCDB
(24465) 2000 SX155 | H | 3.18  | 0.22+  | 2000  | 3.1  | 2.66087  | –  | 2016  | 0.68  | 3.6  | 9.252  | BIN JPL
LoMP LCDB
25015 Lairdclose | FLO | 2.899  | –  | 1998  | 2.9  | –  | –  | 2018  | –  | –  | –  | BIN JPL
LoMP LCDB
25021 Nischaykumar | – | 2.1  | 0.28  | 1998  | 2  | 2.5344  | –  | 2019  | 0.56  | n.a.  | 23.496  | BIN JPL
LoMP LCDB
(26416) 1999 XM84 | – | 4.56  | –  | 1999  | 4.56  | 2.907  | –  | 2015  | –  | –  | –  | BIN JPL
LoMP LCDB
(26420) 1999 XL103 | – | 2.02  | 0.34+  | 1999  | 1.91  | 3.2  | –  | 2019  | 0.65+  | n.a.  | 23.899  | BIN JPL
LoMP LCDB
(27568) 2000 PT6 | H | 1.82  | –  | 2000  | 1.82  | 3.4885  | –  | 2013  | –  | 3.1  | 16.356  | BIN JPL
LoMP LCDB
27675 Paulmaley | PHO | 5.09  | –  | 1981  | 5.09  | –  | –  | 2017  | –  | –  | –  | BIN JPL
LoMP LCDB
31450 Stevepreston | – | 10.62  | 0.22  | 1999  | 10.4  | 3.4116  | –  | 2015  | 2.3  | 39  | 53.47  | BIN JPL
LoMP LCDB
32008 Adriángalád | – | 4.56  | 0.4+  | 2000  | 4.23  | 3.0171  | –  | 2007  | 1.69  | 13  | 40.25  | BIN JPL
LoMP LCDB
(38079) 1999 HF | PHO | 3.4  | –  | 1999  | 3.4  | 16.675  | –  | 2020  | –  | –  | –  | BIN JPL
LoMP LCDB
(43008) 1999 UD31 | – | 2.5  | 0.35  | 1999  | 2.4  | 2.9  | –  | 2014  | 0.8  | –  | –  | BIN JPL
LoMP LCDB
(44620) 1999 RS43 | – | 2.62  | 0.35  | 1999  | 0.66  | 2.9  | –  | 2014  | 0.2  | 2  | –  | BIN JPL
LoMP LCDB
46829 McMahon | – | 3.3  | 0.4  | 1998  | 3.06  | 2.6236  | –  | 2015  | 1.22  | 5.4  | 16.833  | BIN JPL
LoMP LCDB
52316 Daveslater | H | 3.3  | 0.16+  | 1992  | 3.26  | 2.7629  | –  | 2012  | 0.52  | 4.9  | 13.44  | BIN JPL
LoMP LCDB
(57202) 2001 QJ53 | – | 2.2  | 0.25+  | 2001  | 2.2  | 2.44482  | –  | 2017  | 0.5+  | 5  | 24  | BIN JPL
LoMP LCDB
69406 Martz-Kohl | H | 3.18  | 0.19+  | 1995  | 3.12  | 4.486  | –  | 2013  | 0.59  | 5.3  | 16.11  | BIN JPL
LoMP LCDB
(72036) 2000 XM44 | PHO | 2.7  | 0.25+  | 2000  | 2.62  | 2.582  | –  | 2019  | 0.66+  | 4.9  | 18.77  | BIN JPL
LoMP LCDB
76818 Brianenke | H | 3.84  | 0.37  | 2000  | 3.6  | 3.166  | –  | 2005  | 1.33  | 5.6  | 14.12  | BIN JPL
LoMP LCDB
79472 Chiorny | H | 3.79  | 0.32  | 1998  | 3.79  | 2.8802  | –  | 2012  | –  | 9  | 25.94  | BIN JPL
LoMP LCDB
(80218) 1999 VO123 | – | 1.58  | 0.3  | 1999  | 0.28  | 2.9  | –  | 2012  | 0.08  | 0.9  | 33.1  | BIN JPL
LoMP LCDB
152830 Dinkinesh | FLO | 0.82  | 0.28  | 1999  | 0.76  | 52.67 ± 0.04  | Selam
(Dinkinesh I)  | 2023  | 0.22  | ?  | ?  | BIN JPL
LoMP LCDB
(300163) 2006 VW139 | – | 2.6  | 1  | 2006  | 1.8  | –  | –  | 2011  | 1.8  | 104  | 3360  | BIN JPL
LoMP LCDB

back to summary

The following binaries are double asteroids, with similarly sized components, and a barycenter outside of the larger object.

1. 90 Antiope – S/2000 (90) 1[41]
2. 854 Frostia – undesignated
3. 1313 Berna – undesignated
4. 2478 Tokai – undesignated
5. 3169 Ostro – undesignated
6. 3749 Balam – S/2002 (3749) 1[42]
7. 3905 Doppler – undesignated
8. 4674 Pauling – S/2004 (4674) 1[43]
9. 4951 Iwamoto – undesignated
10. 5674 Wolff – undesignated
11. 8474 Rettig – undesignated
12. 17246 Christophedumas – S/2004 (17246) 1[44]
13. (300163) 2006 VW139 – undesignated

In addition, these bodies might be double asteroids, but due to errors in their size and orbit, it is uncertain.

1. 809 Lundia – undesignated
2. 1089 Tama – undesignated
3. 1509 Esclangona – S/2003 (1509) 1[45]
4. 4492 Debussy – undesignated
5. 11264 Claudiomaccone – undesignated
6. 22899 Alconrad – (22899) Alconrad I Juliekaibarreto[46]

### Jupiter trojans

This is a list of Jupiter trojans with companions.[1] Candidate binaries with an unconfirmed status are displayed on a dark background.[26] For an overview, see summary and introduction.

System  | Primary  | Secondary  | Refs

|
|
|

Designation  | Class | De
(km)  | s/p-ratio  | YOD  | Dp
(km)  | RTp
(hours)  | Designation  | YOD  | Ds
(km)  | as
(km)  | Ps
(hours)
617 Patroclus | L5 | 145  | 0.924  | 1906  | 106  | 102.79  | Menoetius (Patroclus I) | 2001  | 98  | 680  | 102.792  | BIN JPL LoMP LCDB
624 Hektor | L4 | 250  | 0.048  | 1907  | 184  | 6.921  | Skamandrios (Hektor I) | 2006  | 12  | 957.5  | 71.162  | BIN JPL LoMP LCDB
3548 Eurybates | L4 | 63.9  | 0.013  | 1973  | 63.9  | 8.711  | Queta (Eurybates I) | 2018  | 0.8  | 2310  | 1982.4  | BIN JPL LoMP LCDB
16974 Iphthime | L4 | 57.3  | 0.767  | 1998  | 45.5  | 78.9  | –  | 2013  | 34.9  | 179  | 78.96  | BIN JPL LoMP LCDB
17365 Thymbraeus | L5 | 42.6  | 0.843  | 1978  | 32.6  | 12.672  | –  | 2005  | 27.5  | 43  | 12.672  | BIN JPL LoMP LCDB
29314 Eurydamas | L5 | 40  | 0.737  | 1994  | 32  | 15.035  | –  | 2005  | 24  | 41  | 15.036  | BIN JPL LoMP LCDB
15094 Polymele | L4 |  |  | 1999  | 21  |  | Shaun (temporary designation)[47] | 2022  |  |  |  |

back to summary

### Trans-Neptunian objects

This is a list of trans-Neptunian objects with companions.[1] Candidate binaries with an unconfirmed status are displayed on a dark background.[26] This list gives the companion's orbital period (Ps) in days rather than hours. For an overview, see summary and introduction.

System  | Primary  | Secondary  | Refs

|
|
|

Designation  | Class | De
(km)  | s/p-ratio  | YOD  | Dp
(km)  | RTp
(hours)  | Designation  | YOD  | Ds
(km)  | as
(km)  | Ps
(days)
(26308) 1998 SM165 | 1:2 | 280  | 0.302  | 1998  | 268  | 8.4  | –  | 2001  | 81  | 11377  | 130.158  | BIN JPL LoMP LCDB
38628 Huya | PLU | 458  | 0.525  | 2000  | 406  | 5.28  | Satellite of (38628) Huya  | 2012  | 213  | 1740  | 3.2  | BIN JPL LoMP LCDB
42355 Typhon | SDO | 185  | 0.55  | 2002  | 162  | 9.67  | Echidna (Typhon I)  | 2006  | 89  | 1580  | 18.982  | BIN JPL LoMP LCDB
47171 Lempo | PLU  | 393  | 0.486
0.927  | 1999  | 272  | 45.763  | Paha (Lempo I)  | 2001  | 132  | 7411  | 50.3  | BIN JPL LoMP LCDB
Hiisi (Lempo II)  | 2007  | 251  | 867  | 1.907
(48639) 1995 TL8 | SDO  | 194  | 0.457  | 1995  | 176  | –  | –  | 2002  | 80  | 420  | 1.4  | BIN JPL LoMP LCDB
50000 Quaoar | CUB | 1074  | 0.076  | 2002  | 1070  | 8.839  | Weywot (Quaoar I)  | 2006  | 81  | 13800  | 12.26  | BIN JPL LoMP LCDB
55637 Uni | CUB  | 697  | 0.316  | 2002  | 665  | 14.382  | Tinia (Uni I)  | 2007  | 210  | 4770  | 8.309  | BIN JPL LoMP LCDB
58534 Logos | CUB  | 106  | 0.766  | 1997  | 82  | –  | Zoe (Logos I)  | 2001  | 67  | 8217  | 309.87  | BIN JPL LoMP LCDB
(60458) 2000 CM114 | SDO  | 211  | 0.769  | 2000  | 167  | –  | –  | 2006  | 128  | 2200  | 15  | BIN JPL LoMP LCDB
(60621) 2000 FE8 | 2:5 | 183  | 0.759  | 2000  | 146  | –  | –  | 2007  | 111  | 1180  | 7.5  | BIN JPL LoMP LCDB
65489 Ceto | SDO  | 281  | 0.764  | 2003  | 223  | 4.43  | Phorcys (Ceto I)  | 2006  | 171  | 1840  | 9.554  | BIN JPL LoMP LCDB
66652 Borasisi | CUB  | 163  | 0.817  | 1999  | 126  | 6.4  | Pabu (Borasisi I)  | 2003  | 103  | 4528  | 46.2888  | BIN JPL LoMP LCDB
79360 Sila–Nunam | CUB  | 343  | 0.944  | 1997  | 249  | 300.2388  | Nunam | 2002  | 236  | 2777  | 12.51  | BIN JPL LoMP LCDB
(80806) 2000 CM105 | CUB  | 201  | 0.759  | 2000  | 160  | –  | –  | 2002  | 121  | 2700  | 23  | BIN JPL LoMP LCDB
(82075) 2000 YW134 | 3:8 | 229  | 0.347  | 2000  | 216  | –  | –  | 2002  | 75  | 1900  | 10  | BIN JPL LoMP LCDB
(82157) 2001 FM185 | CUB  | 183  | 0.867  | 2001  | 138  | –  | –  | 2008  | 120  | 3130  | 33  | BIN JPL LoMP LCDB
88611 Teharonhiawako | CUB  | 220  | 0.724  | 2001  | 178  | 9.505  | Sawiskera (Teharonhiawako I)  | 2001  | 129  | 27670  | 828.76  | BIN JPL LoMP LCDB
90482 Orcus | PLU | 958  | 0.31  | 2004  | 917  | 13.18841  | Vanth (Orcus I)  | 2005  | 442  | 9006  | 9.539  | BIN JPL LoMP LCDB
(119067) 2001 KP76 | CUB  | 211  | 0.955  | 2001  | 153  | –  | –  | 2007  | 146  | 8900  | 130  | BIN JPL LoMP LCDB
(119979) 2002 WC19 | 1:2 | 461  | 0.316  | 2002  | 440  | –  | –  | 2006  | 139  | 4090  | 8.403  | BIN JPL LoMP LCDB
120347 Salacia | CUB  | 901  | 0.344  | 2004  | 854  | 6.5  | Actaea (Salacia I)  | 2006  | 286  | 5619  | 5.4938  | BIN JPL LoMP LCDB
(123509) 2000 WK183 | CUB  | 146  | 0.951  | 2000  | 106  | –  | –  | 2005  | 101  | 2366  | 30.917  | BIN JPL LoMP LCDB
134340 Pluto | PLU | 2376  | 0.511
0.018
0.016
0.012
0.0025  | 1930  | 2380  | 153.2935  | Charon (Pluto I)  | 1978  | 1212  | 19573  | 6.3872  | BIN JPL LoMP LCDB
Nix (Pluto II)  | 2005  | 38  | 48694  | 24.8546
Hydra (Pluto III)  | 2005  | 39  | 64738  | 38.2018
Kerberos (Pluto IV)  | 2011  | 13  | 57783  | 32.1676
Styx (Pluto V)  | 2012  | 11  | 42656  | 20.1616
(134860) 2000 OJ67 | CUB  | 175  | 0.783  | 2000  | 138  | –  | –  | 2003  | 108  | 2270  | 22.0584  | BIN JPL LoMP LCDB
136108 Haumea | HAU  | 1425  | 0.232
0.116  | 2003  | 1379  | 3.9154  | Hiʻiaka (Haumea I)  | 2005  | 320  | 49880  | 49.462  | BIN JPL LoMP LCDB
Namaka (Haumea II)  | 2005  | 170  | 25657  | 18.2783
136199 Eris | SDO  | 2326  | 0.301  | 2003  | 2326  | 378.6  | Dysnomia (Eris I)  | 2005  | 700  | 37460  | 15.7859  | BIN JPL LoMP LCDB
136472 Makemake | CUB  | 1440  | 0.122  | 2005  | 1430  | 7.771  | S/2015 (136472) 1 | 2015  | 130  | 21100+  | 12.4  | BIN JPL LoMP LCDB
(139775) 2001 QG298 | PLU | 179  | 0.867  | 2001  | 135  | 13.7744  | –  | 2003  | 117  | 172  | 0.5739  | BIN JPL LoMP LCDB
148780 Altjira | CUB  | 331  | 0.899  | 2001  | 246  | –  | –  | 2006  | 221  | 9904  | 139.56  | BIN JPL LoMP LCDB
(160091) 2000 OL67 | CUB  | 74  | 0.759  | 2000  | 153  | –  | –  | 2007  | 56  | 7695  | 347.085  | BIN JPL LoMP LCDB
(160256) 2002 PD149 | CUB  | 242  | 0.832  | 2002  | 186  | –  | –  | 2007  | 155  | 24400  | 470  | BIN JPL LoMP LCDB
174567 Varda | CUB  | 792  | 0.513  | 2003  | 705  | 5.91  | Ilmarë (Varda I)  | 2009  | 361  | 4800  | 5.7508  | BIN JPL LoMP LCDB
(182933) 2002 GZ31 | SDO  | 231  | 0.631  | 2002  | 195  | –  | –  | 2006  | 123  | 2060  | 12  | BIN JPL LoMP LCDB
208996 Achlys | PLU  | 727  | 0.1  | 2003  | 723  | 13.44  | –  | 2005  | 72  | 7200  | 12  | BIN JPL LoMP LCDB
225088 Gonggong | 3:10 | 1230  | 0.2  | 2007  | 1535  | 44.81  | Xiangliu (Gonggong I)  | 2010  | 95  | 15000  | 6  | BIN JPL LoMP LCDB
229762 Gǃkúnǁʼhòmdímà | SDO  | 599  | 0.175  | 2007  | 590  | 11.05  | Gǃòʼé ǃHú (Gǃkúnǁʼhòmdímà I)  | 2008  | 71  | 3600  | 5.9  | BIN JPL LoMP LCDB
(275809) 2001 QY297 | CUB  | 229  | 0.912  | 2001  | 169  | 11.68  | –  | 2006  | 154  | 9960  | 138.11  | BIN JPL LoMP LCDB
(303712) 2005 PR21 | CUB  | 265  | 0.603  | 2005  | 227  | –  | –  | 2007  | 137  | 3600  | 22  | BIN JPL LoMP LCDB
341520 Mors–Somnus | PLU | 141  | 0.955  | 2007  | 102  | 9.28  | Somnus | 2007  | 97  | 21040  | 971.7  | BIN JPL LoMP LCDB
(364171) 2006 JZ81 | CUB  | 145  | 0.637  | 2006  | 122  | –  | –  | 2006  | 78  | 33000  | 1500  | BIN JPL LoMP LCDB
385446 Manwë | 4:7 | 185  | 0.58  | 2003  | 160  | –  | Thorondor (Manwë I)  | 2006  | 92  | 6674  | 110.176  | BIN JPL LoMP LCDB
(469420) 2001 XP254 | 3:5 | 133  | 0.711  | 2001  | 108  | –  | –  | 2008  | 77  | 1200  | 12  | BIN JPL LoMP LCDB
(469505) 2003 FE128 | 1:2 | 221  | 0.735  | 2003  | 178  | 5.85  | –  | 2010  | 131  | 2140  | 14  | BIN JPL LoMP LCDB
(469509) 2003 HC57 | CUB  | 306  | 0.95  | 2003  | 222  | –  | –  | 2020  | 211  | 1960  | –  | BIN JPL LoMP LCDB
(469514) 2003 QA91 | CUB | 260  | 0.955  | 2003  | 188  | –  | –  | 2006  | 180  | 1900  | 9.1  | BIN JPL LoMP LCDB
(469610) 2004 HF79 | CUB  | 242  | 0.81  | 2004  | 188  | –  | –  | 2019  | 153  | 3820  | 29  | BIN JPL LoMP LCDB
469705 ǂKá̦gára | CUB  | 174  | 0.762  | 2005  | 138  | 9.65  | ǃHãunu (ǂKá̦gára I)  | 2009  | 105  | 7700  | 128.11  | BIN JPL LoMP LCDB
(505447) 2013 SQ99 | CUB  | 231  | 0.81  | 2013  | 180  | –  | –  | 2017  | 146  | 13300  | 200  | BIN JPL LoMP LCDB
(505476) 2013 UL15 | CUB  | 212  | 0.79  | 2013  | 166  | –  | –  | 2019  | 131  | 5370  | 59  | BIN JPL LoMP LCDB
(506121) 2016 BP81 | CUB  | 253  | 0.90  | 2016  | 188  | 6.85  | –  | 2017  | 169  | 11300  | 140  | BIN JPL LoMP LCDB
(508788) 2000 CQ114 | CUB  | 175  | 0.871  | 2000  | 132  | –  | –  | 2003  | 115  | 6930  | 220.7  | BIN JPL LoMP LCDB
(508869) 2002 VT130 | CUB  | 324  | 0.817  | 2002  | 251  | –  | –  | 2008  | 205  | 2490  | 9.8  | BIN JPL LoMP LCDB
(511551) 2014 UD225 | CUB  | 201  | 0.35  | 2013  | 190  | –  | –  | 2017  | 66  | 21400  | 460  | BIN JPL LoMP LCDB
(523624) 2008 CT190 | SDO  | 350  | 0.83  | 2008  | 270  | –  | –  | 2012  | 220  | 1300  | 3.3  | BIN JPL LoMP LCDB
(523764) 2014 WC510 | PLU | 227  | 0.76  | 2011  | 181  | –  | –  | 2018  | 138  | 349  | 0.87  | BIN JPL LoMP LCDB
(523983) 1999 RY214 | CUB  | 146  | 0.605  | 1999  | 125  | –  | –  | 2008  | 76  | 1500  | 15  | BIN JPL LoMP LCDB
(524217) 2001 RZ143 | CUB  | 140  | 0.832  | 2001  | 108  | –  | –  | 2001  | 90  | 1560  | 17  | BIN JPL LoMP LCDB
(524366) 2001 XR254 | CUB  | 221  | 0.826  | 2001  | 171  | –  | –  | 2006  | 140  | 9310  | 125.58  | BIN JPL LoMP LCDB
(524531) 2002 XH91 | CUB  | 350  | 0.619  | 2002  | 298  | –  | –  | 2008  | 185  | 19900  | 190  | BIN JPL LoMP LCDB
(525462) 2005 EO304 | CUB  | 171  | 0.513  | 2005  | 152.4  | –  | –  | 2005  | 78  | 69800  | 3579  | BIN JPL LoMP LCDB
532037 Chiminigagua | SDO  | 765  | 0.25  | 2013  | 740  | –  | –  | 2018  | 190  | 9800  | 15  | BIN JPL LoMP LCDB
1998 WV24 | CUB  | 146  | 0.871  | 1998  | 110  | –  | –  | 2007  | 96  | 1420  | 14  | BIN JPL uTNO LCDB
1998 WW31 | CUB  | 192  | 0.833  | 1998  | 148  | –  | S/2000 (1998 WW31) 1[48] | 2000  | 123  | 22620  | 587.3  | BIN JPL uTNO LCDB
(612095) 1999 OJ4 | CUB  | 104  | 0.96  | 1999  | 75  | –  | –  | 2002  | 72  | 3267  | 84.12  | BIN JPL LoMP LCDB
1999 RT214 | CUB  | 121  | 0.689  | 1999  | 100  | –  | –  | 2006  | 69  | 3310  | 64  | BIN JPL uTNO LCDB
(612141) 1999 XY143 | CUB  | 278  | 0.839  | 1999  | 213  | –  | –  | 2008  | 179  | 2670  | 14  | BIN JPL LoMP LCDB
(612147) 2000 CF105 | CUB  | 81  | 0.78  | 2000  | 63.6  | –  | –  | 2002  | 50  | 33300  | 3989  | BIN JPL LoMP LCDB
(612176) 2000 QL251 | 1:2 | 206  | 0.967  | 2000  | 148  | –  | –  | 2006  | 143  | 5002  | 56.451  | BIN JPL LoMP LCDB
(612203) 2000 WT169 | CUB  | 265  | 0.82  | 2000  | 205  | –  | –  | 2008  | 168  | 2600  | 14  | BIN JPL LoMP LCDB
2001 FL185 | CUB  | 167  | 0.617  | 2001  | 142  | –  | –  | 2006  | 88  | 1900  | 17  | BIN JPL uTNO LCDB
(612239) 2001 QC298 | CUB  | 303  | 0.817  | 2001  | 235  | 7.78  | –  | 2002  | 192  | 3813  | 19.23  | BIN JPL LoMP LCDB
(612242) 2001 QQ322 | CUB  | 231  | 0.912  | 2001  | 171  | –  | –  | 2007  | 156  | 3890  | 32  | BIN JPL LoMP LCDB
2001 QW322 | CUB  | 180  | 0.986  | 2001  | 128  | –  | –  | 2001  | 126  | 102100  | 6280  | BIN JPL uTNO LCDB
2002 VF130 | CUB  | 160  | 0.867  | 2002  | 121  | –  | –  | 2008  | 105  | 22400  | 760  | BIN JPL uTNO LCDB
(612549) 2003 HG57 | CUB  | 221  | 1  | 2003  | 156  | –  | –  | 2010  | 156  | 13200  | 210  | BIN JPL LoMP LCDB
2003 QY90 | CUB  | 114  | 0.986  | 2003  | 81  | 3.4  | –  | 2003  | 80  | 8549  | 309.7  | BIN JPL uTNO LCDB
(612578) 2003 QR91 | CUB  | 280  | 0.912  | 2003  | 207  | –  | –  | 2007  | 189  | 1790  | 7.5  | BIN JPL LoMP LCDB
2003 TJ58 | CUB  | 83  | 0.787  | 2003  | 65  | –  | –  | 2006  | 51  | 3840  | 137.68  | BIN JPL uTNO LCDB
(612687) 2003 UN284 | CUB  | 149  | 0.667  | 2003  | 124  | –  | –  | 2003  | 83  | 54000  | 3180  | BIN JPL LoMP LCDB
(612719) 2003 WU188 | CUB  | 220-  | 0.724  | 2003  | 178  | –  | –  | 2007  | 129  | 1300  | 6.5  | BIN JPL LoMP LCDB
2003 YS179 | CUB  | 167  | 0.871  | 2003  | 126  | –  | –  | 2008  | 110  | 7830  | 150  | BIN JPL uTNO LCDB
(612733) 2003 YU179 | CUB  | 167  | 0.55  | 2003  | 146  | –  | –  | 2008  | 80  | 2000  | 18  | BIN JPL LoMP LCDB
2004 HD79 | CUB  | 319  | 0.85  | 2004  | 243  | 8+  | –  | 2019  | 206  | 2780  | 12  | BIN JPL LCDB
2004 HK79 | CUB  | 183  | 1.0  | 2004  | 129  | –  | –  | 2019  | 129  | 3600  | 41  | BIN JPL LCDB
2004 KB19 | PLU | 146  | 0.95  | 2004  | 105  | –  | –  | 2012  | 100  | 3400  | 53  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 KE19 | CUB  | 221  | 0.67  | 2004  | 184  | –  | –  | 2019  | 123  | 4110  | 36  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 KH19 | CUB  | 221  | 0.721  | 2004  | 179  | –  | –  | 2011  | 129  | 13000  | 210  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 MU8 | CUB  | 175  | 0.89  | 2004  | 131  | 2.5+  | –  | 2019  | 116  | 5840  | 89  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 PB108 | CUB  | 277  | 0.544  | 2004  | 243  | –  | –  | 2006  | 132  | 10400  | 97.02  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 PV117 | CUB  | 221  | 0.44  | 2004  | 203  | –  | –  | 2019  | 89  | 6800  | 73  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 PW117 | CUB  | 242  | 0.72  | 2004  | 196  | –  | –  | 2019  | 141  | 23190  | 430  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2004 PX117 | CUB  | 221  | 0.81  | 2004  | 172  | –  | –  | 2019  | 139  | 5940  | 64  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2005 GD187 | CUB  | 160  | 0.832  | 2005  | 123  | –  | –  | 2009  | 102  | 7600  | 150  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2005 VZ122 | CUB  | 133  | 0.398  | 2005  | 124  | –  | –  | 2008  | 49  | 2300  | 30  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2006 BR284 | CUB  | 114  | 0.794  | 2006  | 89.8  | –  | –  | 2006  | 71  | 25300  | 1501  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2006 CH69 | CUB  | 129  | 0.817  | 2006  | 100  | –  | –  | 2004  | 82  | 27000  | 1420  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2006 JV58 | CUB  | 211  | 0.76  | 2006  | 168  | –  | –  | 2019  | 127  | 4340  | 43  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2006 SF369 | 1:3 | 201  | 0.977  | 2006  | 144  | –  | –  | 2007  | 141  | 3120  | 28  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
(671468) 2014 LQ28 | CUB  | 320  | 0.83  | 2014  | 250  | –  | –  | 2016  | 210  | 24000  | 290  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL Lua error: Internal error: The interpreter has terminated with signal "24". LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2014 OS393 |  |  |  |  |
2015 QL14 | CUB  | 180  | 0.9  | 2015  | 130  | –  | –  | 2017  | 120  | 52000  | 2300  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL uTNO LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2015 RB280 | CUB  | 134  | 0.76  | 2015  | 107  | –  | –  | 2019  | 81  | 6700  | 160  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2015 RP280 | CUB  | 154  | 0.76  | 2015  | 123  | –  | –  | 2019  | 93  | 5080  | 86  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2015 RT245 | CUB  | 222  | 0.95  | 2015  | 161  | –  | –  | 2019  | 153  | 14680  | 250  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2015 VM173 | CUB  | 265  | 0.87  | 2015  | 200  | –  | –  | 2019  | 174  | 5290  | 41  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
2015 VW168 | CUB  | 106  | 0.76  | 2015  | 84  | –  | –  | 2019  | 64  | 5960  | 190  | BINLua error: Internal error: The interpreter has terminated with signal "24". JPL LCDBLua error: Internal error: The interpreter has terminated with signal "24".
HST5  | –  | 190  | 1  | 2005  | 135  | –  | n.a.  | 2005  | 135  | 16400  | 1000  | BINLua error: Internal error: The interpreter has terminated with signal "24". —

back to summary

## See also

* Lists of astronomical objects
* Astronomy:Subsatellite, also known as a moonmoon - Lua error: Internal error: The interpreter has terminated with signal "24". - Lua error: Internal error: The interpreter has terminated with signal "24".
* Astronomy:Yarkovsky–O'Keefe–Radzievskii–Paddack effect, also known as YORP effect - Lua error: Internal error: The interpreter has terminated with signal "24". - Lua error: Internal error: The interpreter has terminated with signal "24".
* Satellite system

## References

1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 Johnston, Wm. Robert (23 January 2022). "Asteroids with Satellites". Johnston's Archive. http://www.johnstonsarchive.net/astro/asteroidmoons.html.
2. ↑ 2.0 2.1 William J. Merline; Maria Martinez (26 October 2000). "Astronomers Image Double Asteroid". SwRI Press Release. http://www.boulder.swri.edu/merline/press/release.txt. (mentions both 90 Antiope and 762 Pulcova)
3. ↑ "Satellites and Companions of Minor Planets". IAU / Minor Planet Center. 17 September 2009. http://www.cbat.eps.harvard.edu/minorsats.html.
4. ↑ "90 Antiope: Raw Keck Image". SWrI Press Release. August 2000. http://www.boulder.swri.edu/merline/press/fig1.html.
5. ↑ "IAUC 8732: S/2006 (624) 1". Central Bureau for Astronomical Telegrams. 21 July 2006. http://www.cbat.eps.harvard.edu/iauc/08700/08732.html#Item1. (Satellite Discovery)
6. ↑ Dunham, David W. (December 1978). "Satellite of Minor Planet 532 Herculina Discovered During Occultation". The Minor Planet Bulletin 6: 13–14. Bibcode: 1978MPBu....6...13D.
7. ↑ Dunham, David W.; Maley, Paul D. (December 1977). "Possible Observation of a Satellite of a Minor Planet". The Minor Planet Bulletin 5: 16–17. Bibcode: 1977MPBu....5...16D.
8. ↑ Storrs, Alex; Weiss, Ben; Zellner, Ben; Burleson, Win; Sichitiu, Rukmini; Wells, Eddie et al. (February 1999). "Imaging Observations of Asteroids with Hubble Space Telescope". Icarus 137 (2): 260–268. doi:10.1006/icar.1999.6047. Bibcode: 1999Icar..137..260S. https://pdfs.semanticscholar.org/ba43/528983a55b0ec70e42a997e13e553ef19b55.pdf.
9. ↑ Hamilton, Thomas Wm. (27 August 2014). Impact Craters of Earth: with Selected Craters Elsewhere. Strategic Book Publishing & Rights Agency. p. 24. ISBN 9781631353536. https://books.google.com/books?id=-ImmBAAAQBAJ. Retrieved 28 February 2021.
10. ↑ "Astronomers Discover Moon Orbiting Asteroid". SwRI. 1998. http://www.boulder.swri.edu/~merline/press_release/. (Eugenia AO image)
11. ↑ Merline, W. J. (29 October 2001). "IAUC 7741: 2001fc; S/2001 (617) 1; C/2001 T1, C/2001 T2". Central Bureau for Astronomical Telegrams. http://www.cbat.eps.harvard.edu/iauc/07700/07741.html.
12. ↑ Chiang, E.; Lithwick, Y.; Buie, M.; Grundy, W.; Holman, M.; A Brief History of Trans-Neptunian Space, to appear in Protostars and Planets V (August 2006) Final preprint on arXiv
13. ↑ Green, Daniel W. E. (6 November 2021). "(130) ELEKTRA". Central Bureau Electronic Telegrams (Central Bureau for Astronomical Telegrams) (5066). http://www.cbat.eps.harvard.edu/iau/cbet/005000/CBET005066.txt. Retrieved 25 October 2025.
14. ↑ Daniel W. E. Green (2005-08-11). "IAUC 8582: Sats OF (87)". Central Bureau for Astronomical Telegrams. http://www.cbat.eps.harvard.edu/iauc/08500/08582.html.
15. ↑ Daniel W. E. Green (2007-03-07). "IAUC 8817: S/2004 (45) 1". Central Bureau for Astronomical Telegrams. http://www.cbat.eps.harvard.edu/iauc/08800/08817.html.
16. ↑ Marchis, Franck. "Franck Marchis Web Page (Principal Investigator, SETI Institute, UC Berkeley)". Department of Astronomy (University of California at Berkeley). http://astro.berkeley.edu/~fmarchis/.
17. ↑ Marchis, Franck (2008-09-19). "Two Companions Found Near Dog-Bone Asteroid". SETI Institute. http://www.seti.org/Page.aspx?pid=1182.
18. ↑ Franck Marchis (2009-08-21). "The discovery of a new triple asteroid – (93) Minerva". Cosmic Diary Blog. http://www.cosmicdiary.org/blogs/nasa/franck_marchis/?p=465.
19. ↑ Marchis, F.; Baek, M.; Descamps, P.; Berthier, J.; Hestroffer, D.; Vachier, F. (2007). "S/2004 (45) 1". IAU Circular (8817): 1. Bibcode: 2007IAUC.8817....1M.
20. ↑ "IAUC 7599: S/2001 (107) 1; 2001ae; V4643 Sgr". http://www.cbat.eps.harvard.edu/iauc/07500/07599.html.
21. ↑ Marsset, M.; Carry, B.; Yang, B.; Marchis, F.; Vernazza, P.; Dumas, C.; Berthier, J.; Vachier, F. (2016-08-01). "S/2016 (107) 1". International Astronomical Union Circular (9282): 1. ISSN 0081-0304. Bibcode: 2016IAUC.9282....1M. https://ui.adsabs.harvard.edu/abs/2016IAUC.9282....1M/abstract.
22. ↑ 22.0 22.1 Noll, Keith S. "Solar System binaries", Asteroids, Comets, Meteors, Proceedings of the 229th Symposium of the IAU, Rio de Janeiro, 2005, Cambridge University Press, 2006., pp. 301–318 Preprint
23. ↑ T. Michałowski (2004). "Eclipsing binary asteroid 90 Antiope". Astronomy & Astrophysics 423 (3): 1159–1168. doi:10.1051/0004-6361:20040449. Bibcode: 2004A&A...423.1159M.
24. ↑ Santos-Sanz, P. (2012). ""TNOs are Cool": A Survey of the Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS". Astronomy & Astrophysics 541: A92. doi:10.1051/0004-6361/201118541. Bibcode: 2012A&A...541A..92S.
25. ↑ Marchis, F.; Baek, M. (2008). "Multiple Asteroid Systems: New Techniques to Study New Worlds". Lunar and Planetary Institute. http://www.lpi.usra.edu/meetings/acm2008/pdf/8321.pdf.
26. ↑ 26.0 26.1 26.2 26.3 26.4 Johnston, Wm. Robert (24 December 2021). "Asteroids/TNOs with Satellites list by type and presumed level of confirmation". Johnston's Archive. http://www.johnstonsarchive.net/astro/asteroidmoonslist3.html.
27. ↑ "GK Per; S/1997 (3671) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 10 June 1997. http://www.cbat.eps.harvard.edu/iauc/06600/06680.html.
28. ↑ "C/2008 S1; S/2008 (35107) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 19 September 2008. http://www.cbat.eps.harvard.edu/iauc/08900/08977.html.
29. ↑ Warner, B. D.; Pravec, P. (22 December 2013). "S/2012 (2577) 1". Central Bureau for Astronomical Telegrams (International Astronomical Union) 3765: 3. Bibcode: 2013CBET.3765....3W. https://ui.adsabs.harvard.edu/abs/2013CBET.3765....3W/abstract. Retrieved 3 February 2025.
30. ↑ "S/2001 (107) 1; 2001ae; V4643 Sgr". Central Bureau for Astronomical Telegrams. International Astronomical Union. 19 March 2001. http://www.cbat.eps.harvard.edu/iauc/07500/07599.html.
31. ↑ Marsset, M.; Carry, B.; Yang, B.; Marchis, F.; Vernazza, P.; Dumas, C.; Berthier, J.; Vachier, F. (7 August 2016). "S/2016 (107) 1". Central Bureau for Astronomical Telegrams (International Astronomical Union) 9282: 1. Bibcode: 2016IAUC.9282....1M. https://ui.adsabs.harvard.edu/abs/2016IAUC.9282....1M/abstract. Retrieved 3 February 2025.
32. ↑ "S/2001 U 1; S/2002 (121) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 30 September 2002. http://www.cbat.eps.harvard.edu/iauc/07900/07980.html.
33. ↑ "S/2003 (130) 1; 2003hd; C/2003 E1; C/2002 Y1; Corr". Central Bureau for Astronomical Telegrams. International Astronomical Union. 17 August 2003. http://www.cbat.eps.harvard.edu/iauc/08100/08183.html.
34. ↑ "S/2014 (130) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 17 December 2014. https://fcaglp.fcaglp.unlp.edu.ar/pipermail/iauc/2014-December/003403.html.
35. ↑ "S/2003 (283) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 27 July 2003. http://www.cbat.eps.harvard.edu/iauc/08100/08165.html.
36. ↑ "S/2003 (379) 1; 2003he, 2003hf; C/2003 H1; C/2001 Q4". Central Bureau for Astronomical Telegrams. International Astronomical Union. 15 August 2003. http://www.cbat.eps.harvard.edu/iauc/08100/08182.html.
37. ↑ "S/2003 (1509) 1; M87". Central Bureau for Astronomical Telegrams. International Astronomical Union. 18 February 2003. http://www.cbat.eps.harvard.edu/iauc/08000/08075.html.
38. ↑ "P/2001 WF_2; S/2002 (3749) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 13 February 2002. http://www.cbat.eps.harvard.edu/iauc/07800/07827.html.
39. ↑ "S/2004 (4674) 1; 2004ak, 2004al,, 2004am; C/2002 T7". Central Bureau for Astronomical Telegrams. International Astronomical Union. 5 March 2004. http://www.cbat.eps.harvard.edu/iauc/08200/08297.html.
40. ↑ "2004ab; S/2004 (17246) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 24 February 2004. http://www.cbat.eps.harvard.edu/iauc/08200/08293.html.
41. ↑ "OCCULTATIONS BY (90) ANTIOPE AND BY S/2000 (90) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 17 February 2008. http://www.cbat.eps.harvard.edu/iau/cbet/001200/CBET001263.txt.
42. ↑ "S/2002 (3749) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 13 February 2002. http://www.cbat.eps.harvard.edu/iauc/07800/07827.html.
43. ↑ "S/2004 (4674) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 5 March 2004. http://www.cbat.eps.harvard.edu/iauc/08200/08297.html.
44. ↑ "S/2004 (17246) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 24 February 2004. http://www.cbat.eps.harvard.edu/iauc/08200/08293.html.
45. ↑ "S/2003 (1509) 1". Central Bureau for Astronomical Telegrams. International Astronomical Union. 18 February 2003. http://www.cbat.eps.harvard.edu/iauc/08000/08075.html.
46. ↑ "WGSBN Bulletin 4, #14". WGSBN Bulletin (International Astronomical Union) 4 (14): 6. 14 October 2024. https://www.wgsbn-iau.org/files/Bulletins/V004/WGSBNBull_V004_014.pdf. Retrieved 14 October 2024.
47. ↑ "Ninth asteroid added to Lucy mission; optimism grows on solar array issue". Spaceflight Now. 14 June 2022. https://spaceflightnow.com/2022/06/14/nasa-making-progress-deploying-stuck-solar-panel-on-lucy-asteroid-probe. Retrieved 15 June 2022.
48. ↑ "S/2000 (1998 WW_31) 1; V382 Vel". Central Bureau for Astronomical Telegrams. International Astronomical Union. 16 April 2001. http://www.cbat.eps.harvard.edu/iauc/07600/07610.html.

Lua error: Internal error: The interpreter has terminated with signal "24".

## External links

* Lua error: Internal error: The interpreter has terminated with signal "24". on YouTubeLua error: Internal error: The interpreter has terminated with signal "24"., Lecture at SETI talk (duration 1:00:02)Lua error: Internal error: The interpreter has terminated with signal "24".
* Orbits of Binary Asteroids with Adaptive Optics (Franck Marchis)
* Satellites and Companions of Minor Planets (CBAT)
* Asteroids with Satellites Johnston's Archive
* The VOBAD database  a web page built and designed by F. Marchis and his collaborators (UC-Berkeley/SETI Institute) which contains the parameters of 169 multiple asteroid systems (last update May 9, 2009)

Lua error: Internal error: The interpreter has terminated with signal "24". Lua error: Internal error: The interpreter has terminated with signal "24". Lua error: Internal error: The interpreter has terminated with signal "24". Lua error: Internal error: The interpreter has terminated with signal "24".

Lua error: Internal error: The interpreter has terminated with signal "24".

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