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211 relations: Adeona family, Alinda asteroid, Asteroid, Asteroid belt, Asteroid family, Asteroid spectral types, Astronomer, Augusta family, B-type asteroid, Baptistina family, C-type asteroid, Ceres (dwarf planet), Collisional family, Cybele asteroid, Dwarf planet, E-type asteroid, Eos family, Eunomia family, F-type asteroid, Flora family, Gefion family, Geometric albedo, Griqua asteroid, Haumea, Haumea family, Hierarchical clustering, Hilda asteroid, Hirayama family, Homogeneity and heterogeneity, Hungaria asteroid, Hygiea family, Iron meteorite, Japan, Juno clump, K-type asteroid, Karin family, Kirkwood gap, Kiyotsugu Hirayama, Koronis family, L-type asteroid, List of minor planets, List of minor planets: 10001–11000, List of minor planets: 1001–2000, List of minor planets: 12001–13000, List of minor planets: 16001–17000, List of minor planets: 20001–21000, List of minor planets: 2001–3000, List of minor planets: 3001–4000, List of minor planets: 40001–41000, List of minor planets: 4001–5000, ..., List of minor planets: 5001–6000, List of minor planets: 6001–7000, List of minor planets: 7001–8000, List of minor planets: 8001–9000, List of minor planets: 9001–10000, List of minor-planet groups, Maria family, Massalia family, Meanings of minor planet names: 17001–18000, Meanings of minor planet names: 4001–5000, Michael E. Brown, Minor planet, Nysa family, Orbital eccentricity, Orbital elements, Orbital inclination, Orbital resonance, Osculating orbit, P-type asteroid, Padua family, Pallas family, Parent body, Phocaea family, Planetary differentiation, Proper orbital elements, S-type asteroid, Semi-major and semi-minor axes, T-type asteroid, Themis family, Trans-Neptunian object, Trojan (astronomy), V-type asteroid, Vesta family, X-type asteroid, Yarkovsky effect, (9799) 1996 RJ, 10 Hygiea, 1101 Clematis, 1117 Reginita, 1118 Hanskya, 1128 Astrid, 113 Amalthea, 1189 Terentia, 1222 Tina, 125 Liberatrix, 1270 Datura, 1272 Gefion, 128 Nemesis, 1298 Nocturna, 1303 Luthera, 13062 Podarkes, 1332 Marconia, 1338 Duponta, 135 Hertha, 1362 Griqua, 137 Meliboea, 1400 Tirela, 144 Vibilia, 145 Adeona, 14627 Emilkowalski, 148 Gallia, 1484 Postrema, 15 Eunomia, 153 Hilda, 157 Dejanira, 158 Koronis, 159 Aemilia, 163 Erigone, 1644 Rafita, 1647 Menelaus, 170 Maria, 1726 Hoffmeister, 173 Ino, 1749 Telamon, 17492 Hippasos, 1911 Schubart, 194 Prokne, 2 Pallas, 20 Massalia, 2085 Henan, 2148 Epeios, 21509 Lucascavin, 221 Eos, 2384 Schulhof, 24 Themis, 25 Phocaea, 254 Augusta, 260 Huberta, 27 Euterpe, 2732 Witt, 283 Emma, 293 Brasilia, 298 Baptistina, 3 Juno, 302 Clarissa, 3063 Makhaon, 31 Euphrosyne, 313 Chaldaea, 322 Phaeo, 329 Svea, 331P/Gibbs, 3548 Eurybates, 3556 Lixiaohua, 363 Padua, 369 Aëria, 375 Ursula, 396 Aeolia, 4 Vesta, 4007 Euryalos, 410 Chloris, 4138 Kalchas, 43 Ariadne, 434 Hungaria, 44 Nysa, 46 Hestia, 4709 Ennomos, 480 Hansa, 490 Veritas, 5 Astraea, 5026 Martes, 507 Laodica, 5436 Eumelos, 569 Misa, 589 Croatia, 606 Brangäne, 618 Elfriede, 623 Chimaera, 624 Hektor, 627 Charis, 63 Ausonia, 65 Cybele, 656 Beagle, 668 Dora, 686 Gersuind, 702 Alauda, 709 Fringilla, 729 Watsonia, 751 Faïna, 752 Sulamitis, 778 Theobalda, 780 Armenia, 8 Flora, 808 Merxia, 81 Terpsichore, 816 Juliana, 832 Karin, 84 Klio, 845 Naëma, 847 Agnia, 87 Sylvia, 871 Amneris, 883 Matterania, 887 Alinda, 89 Julia, 895 Helio, 9 Metis, 909 Ulla, 918 Itha, 926 Imhilde, 945 Barcelona, 96 Aegle. Expand index (161 more) »
Adeona family
The Adeona or Adeonian family is a large asteroid family that formed from the parent body 145 Adeona.
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Alinda asteroid
The Alinda asteroids are a dynamical group of asteroids with a semi-major axis of about 2.5 AU and an orbital eccentricity approximately between 0.4 and 0.65.
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Asteroid
Asteroids are minor planets, especially those of the inner Solar System.
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Asteroid belt
The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter.
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Asteroid family
An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination.
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Asteroid spectral types
An asteroid spectral type is assigned to asteroids based on their emission spectrum, color, and sometimes albedo (reflectivity).
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Astronomer
An astronomer is a scientist in the field of astronomy who concentrates their studies on a specific question or field outside the scope of Earth.
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Augusta family
The Augusta family is a small asteroid family in the inner asteroid belt according to a HCM-study conducted by Italian astronomer Vincenzo Zappalà and colleges in 1995.
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B-type asteroid
B-type asteroids are a relatively uncommon type of carbonaceous asteroid, falling into the wider C-group.
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Baptistina family
The Baptistina family (FIN: 403) is an asteroid family of more than 2500 members that was probably produced by the breakup of an asteroid across 80 million years ago following an impact with a smaller body.
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C-type asteroid
C-type (carbonaceous) asteroids are the most common variety, forming around 75% of known asteroids.
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Ceres (dwarf planet)
Ceres (minor-planet designation: 1 Ceres) is the largest object in the asteroid belt that lies between the orbits of Mars and Jupiter, slightly closer to Mars' orbit.
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Collisional family
In astronomy, a collisional family is a group of objects that are thought to have a common origin in an impact (collision).
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Cybele asteroid
Cybele asteroids (also known as the "Cybeles") are a dynamical group of asteroids, named after the asteroid 65 Cybele.
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Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.
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E-type asteroid
E-type asteroids are asteroids thought to have enstatite (MgSiO3) achondrite surfaces.
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Eos family
The Eos family (adj. Eoan; FIN: 606) is a very large asteroid family located in the outer region of the asteroid belt.
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Eunomia family
The Eunomia or Eunomian family is a large asteroid family of S-type asteroids named after the asteroid 15 Eunomia.
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F-type asteroid
F-type asteroids are a relatively uncommon type of carbonaceous asteroid, falling into the wider C-group.
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Flora family
The Flora or Florian '''family''' of asteroids is a large grouping of S-type asteroids in the inner main belt, whose origin and properties are relatively poorly understood at present.
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Gefion family
The Gefion family (FIN: 516; adj. Gefionian; also known as Ceres family and Minerva family) is an asteroid family located the in intermediate asteroid belt between 2.74 and 2.82 AU at inclinations of 7.4° to 10.5°.
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Geometric albedo
In astronomy, the geometric albedo of a celestial body is the ratio of its actual brightness as seen from the light source (i.e. at zero phase angle) to that of an idealized flat, fully reflecting, diffusively scattering (Lambertian) disk with the same cross-section.
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Griqua asteroid
The Griqua asteroids (also known as the "Griquas") are a dynamical group of asteroids with marginally unstable orbits.
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Haumea
Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit.
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Haumea family
The Haumea or Haumean family is the only identified trans-Neptunian collisional family; that is, the only group of trans-Neptunian objects (TNOs) with similar orbital parameters and spectra (nearly pure water-ice) that suggest they originated in the disruptive impact of a progenitor body.
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Hierarchical clustering
In data mining and statistics, hierarchical clustering (also called hierarchical cluster analysis or HCA) is a method of cluster analysis which seeks to build a hierarchy of clusters.
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Hilda asteroid
The Hilda asteroids (adj. Hildian) are a dynamical group of asteroids in a 3:2 orbital resonance with Jupiter.
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Hirayama family
A Hirayama family of asteroids is a group of minor planets that share similar orbital elements, such as semimajor axis, eccentricity, and orbital inclination.
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Homogeneity and heterogeneity
Homogeneity and heterogeneity are concepts often used in the sciences and statistics relating to the uniformity in a substance or organism.
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Hungaria asteroid
The Hungaria group is a dynamical group of asteroids in the asteroid belt.
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Hygiea family
The Hygiea or Hygiean '''family''' of asteroids is a grouping of dark, carbonaceous C-type and B-type asteroids in outer asteroid belt, the largest member of which is 10 Hygiea.
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Iron meteorite
Iron meteorites are meteorites that consist overwhelmingly of an iron–nickel alloy known as meteoric iron that usually consists of two mineral phases: kamacite and taenite.
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Japan
Japan (日本; Nippon or Nihon; formally 日本国 or Nihon-koku, lit. "State of Japan") is a sovereign island country in East Asia.
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Juno clump
The Juno clump is a probable main-belt asteroid family in the vicinity of 3 Juno.
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K-type asteroid
K-type asteroids are relatively uncommon asteroids with a moderately reddish spectrum shortwards of 0.75 μm, and a slight bluish trend longwards of this.
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Karin family
The Karin family or Karin cluster is an asteroid family and sub-group of the Koronis family.
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Kirkwood gap
A Kirkwood gap is a gap or dip in the distribution of the semi-major axes (or equivalently of the orbital periods) of the orbits of main-belt asteroids.
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Kiyotsugu Hirayama
was a Japanese astronomer, best known for his discovery that many asteroid orbits were more similar to one another than chance would allow, leading to the concept of asteroid families, now called "Hirayama families" in his honour.
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Koronis family
The Koronis or Koronian family is a family of asteroids in the main belt between Mars and Jupiter.
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L-type asteroid
L-type asteroids are relatively uncommon asteroids with a strongly reddish spectrum shortwards of 0.75 μm, and a featureless flat spectrum longwards of this.
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List of minor planets
This is a list of numbered minor planets in numerical order.
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List of minor planets: 10001–11000
No description.
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List of minor planets: 1001–2000
No description.
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List of minor planets: 12001–13000
#fefefe | 12448 Mr.
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List of minor planets: 16001–17000
#fefefe | 16731 Mitsumata || || April 17, 1996 || Saji || Saji Obs.
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List of minor planets: 20001–21000
No description.
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List of minor planets: 2001–3000
#FA8072 | 2078 Nanking || 1975 AD || January 12, 1975 || Nanking || Purple Mountain Obs.
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List of minor planets: 3001–4000
#d6d6d6 | 3089 Oujianquan || || December 3, 1981 || Nanking || Purple Mountain Obs.
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List of minor planets: 40001–41000
No description.
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List of minor planets: 4001–5000
#C2FFFF | 4063 Euforbo || || February 1, 1989 || Bologna || San Vittore Obs.
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List of minor planets: 5001–6000
#fefefe | 5390 Huichiming || || December 19, 1981 || Nanking || Purple Mountain Obs.
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List of minor planets: 6001–7000
No description.
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List of minor planets: 7001–8000
No description.
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List of minor planets: 8001–9000
#fefefe | 8193 Ciaurro || 1993 SF || September 17, 1993 || Stroncone || Santa Lucia Obs.
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List of minor planets: 9001–10000
No description.
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List of minor-planet groups
A minor-planet group is a population of minor planets that share broadly similar orbits.
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Maria family
The Maria family (adj. Marian; FIN: 506; also known as Roma family) is a collisional asteroid family located in the inner parts of the intermediate asteroid belt, near the 1:3 Kirkwood gap.
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Massalia family
The Massalia family (adj. Massalian; FIN: 404) is a family of asteroids in the inner asteroid belt, named after its parent body, 20 Massalia.
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Meanings of minor planet names: 17001–18000
032 | 17032 Edlu || || Edward Tsang Lu (born 1963), a physicist specializing in solar physics.
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Meanings of minor planet names: 4001–5000
009 | 4009 Drobyshevskij || || Edward Drobyshevski, Russian astro- and plasma physicist at Ioffe Institute in St.
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Michael E. Brown
Michael E. Brown (born June 5, 1965) is an American astronomer, who has been professor of planetary astronomy at the California Institute of Technology (Caltech) since 2003.
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Minor planet
A minor planet is an astronomical object in direct orbit around the Sun (or more broadly, any star with a planetary system) that is neither a planet nor exclusively classified as a comet.
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Nysa family
The Nysa family (adj. Nysian; FIN: 405) is part of the Nysa–Polana complex, the largest cluster of asteroid families in the asteroid belt.
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Orbital eccentricity
The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle.
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Orbital elements
Orbital elements are the parameters required to uniquely identify a specific orbit.
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Orbital inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body.
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Orbital resonance
In celestial mechanics, an orbital resonance occurs when orbiting bodies exert a regular, periodic gravitational influence on each other, usually because their orbital periods are related by a ratio of small integers.
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Osculating orbit
In astronomy, and in particular in astrodynamics, the osculating orbit of an object in space at a given moment in time is the gravitational Kepler orbit (i.e. ellipse or other conic) that it would have about its central body if perturbations were not present.
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P-type asteroid
P-type asteroids have low albedo and a featureless reddish spectrum.
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Padua family
The Padua family (FIN: 507), also known as the Lydia family, is a mid-sized family of asteroids of more than a thousand members.
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Pallas family
The Pallas or Palladian '''family''' of asteroids is a grouping of B-type asteroids at very high inclinations in the intermediate asteroid belt (Cellino et al. (2002)).
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Parent body
In meteoritics, a parent body is the celestial body from which originates a meteorite or a class of meteorites.
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Phocaea family
The Phocaea family (FIN: 701) is a collisional family of asteroids located between 2.25 and 2.5 AU in the inner region of the asteroid belt.
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Planetary differentiation
In planetary science, planetary differentiation is the process of separating out different constituents of a planetary body as a consequence of their physical or chemical behaviour, where the body develops into compositionally distinct layers; the denser materials of a planet sink to the center, while less dense materials rise to the surface, generally in a magma ocean.
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Proper orbital elements
The proper orbital elements of an orbit are constants of motion of an object in space that remain practically unchanged over an astronomically long timescale.
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S-type asteroid
S-type asteroids are asteroids with a spectral type that is indicative of a silicaceous (i.e. stony) mineralogical composition, hence the name.
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Semi-major and semi-minor axes
In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the widest points of the perimeter.
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T-type asteroid
T-type asteroids are rare inner-belt asteroids of unknown composition with dark, featureless and moderately red spectra, and a moderate absorption feature shortwards of 0.85 µm.
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Themis family
The Themis or Themistian asteroid family is a Hirayama family (having similar orbital elements) of asteroids found in the outer portion of the asteroid belt, between the orbits of Mars and Jupiter.
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Trans-Neptunian object
A trans-Neptunian object (TNO, also written transneptunian object) is any minor planet in the Solar System that orbits the Sun at a greater average distance (semi-major axis) than Neptune, 30 astronomical units (AU).
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Trojan (astronomy)
In astronomy, a trojan is a minor planet or moon that shares the orbit of a planet or larger moon, wherein the trojan remains in the same, stable position relative to the larger object.
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V-type asteroid
A V-type asteroid or Vestoid is an asteroid whose spectral type is that of 4 Vesta.
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Vesta family
The Vesta or Vestian family of asteroids is a large and prominent grouping of mostly V-type asteroids ("vestoids") in the inner asteroid belt in the vicinity of 4 Vesta.
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X-type asteroid
The X-group of asteroids collects together several types with similar spectra, but probably quite different compositions.
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Yarkovsky effect
The Yarkovsky effect is a force acting on a rotating body in space caused by the anisotropic emission of thermal photons, which carry momentum.
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(9799) 1996 RJ
, provisional designation, is a large Jupiter trojan from the Greek camp and the parent body of a small, unnamed asteroid family, approximately in diameter.
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10 Hygiea
10 Hygiea is the fourth-largest asteroid in the Solar System by volume and mass, and it is located in the asteroid belt.
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1101 Clematis
1101 Clematis, provisional designation, is an Alauda asteroid from the outermost regions of the asteroid belt, approximately 37 kilometers in diameter.
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1117 Reginita
1117 Reginita, provisional designation, is a stony background asteroid from the inner regions of the asteroid belt, approximately 10 kilometers in diameter.
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1118 Hanskya
1118 Hanskya, provisional designation, is a dark background asteroid from the outer regions of the asteroid belt, approximately 77 kilometers in diameter.
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1128 Astrid
1128 Astrid, provisional designation, is a carbonaceous Astridian asteroid from the central region of the asteroid belt.
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113 Amalthea
113 Amalthea is a fairly typical rocky main-belt asteroid orbiting in the inner regions of the belt.
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1189 Terentia
1189 Terentia, provisional designation, is a carbonaceous Terentian asteroid from the outer regions of the asteroid belt, approximately 56 kilometers in diameter and the namesake of its family.
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1222 Tina
1222 Tina, provisional designation, is a metallic asteroid and parent body of the Tina family located in the intermediate asteroid belt, approximately 25 kilometers in diameter.
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125 Liberatrix
125 Liberatrix is a main-belt asteroid.
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1270 Datura
1270 Datura (1930 YE) is a S-type main-belt asteroid discovered on December 17, 1930, by George Van Biesbroeck at Yerkes Observatory.
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1272 Gefion
1272 Gefion, provisional designation, is a stony asteroid and parent body of the Gefion family from the central region of the asteroid belt, approximately 7 kilometers in diameter.
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128 Nemesis
128 Nemesis is a large 188 km main-belt asteroid, of carbonaceous composition.
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1298 Nocturna
1298 Nocturna, provisional designation, is a dark asteroid from the outer regions of the asteroid belt, approximately 40 kilometers in diameter.
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1303 Luthera
1303 Luthera, provisional designation, is a dark asteroid and the parent body of the Luthera family, located in the outermost regions of the asteroid belt.
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13062 Podarkes
13062 Podarkes, provisional designation, is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter.
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1332 Marconia
1332 Marconia, provisional designation, is a dark asteroid and the parent body of the Marconia family located in the outer regions of the asteroid belt.
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1338 Duponta
1338 Duponta, provisional designation, is a stony Florian asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 7.8 kilometers in diameter.
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135 Hertha
135 Hertha is a large main-belt asteroid named Hertha, another name for Nerthus, a Germanic fertility goddess.
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1362 Griqua
1362 Griqua, provisional designation is a dark, Jupiter-resonant background asteroid on an eccentric, cometary-like orbit and the namesake of the Griqua group, located in the Hecuba gap in the outermost region of the asteroid belt.
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137 Meliboea
137 Meliboea is a large, dark main-belt asteroid that was discovered by Austrian astronomer J. Palisa at the Austrian Naval Observatory on 21 April 1874, the second of his many asteroid discoveries.
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1400 Tirela
1400 Tirela, provisional designation, is an asteroid and the parent body of the Tirela family, located in the outer regions of the asteroid belt, approximately 16 kilometers in diameter.
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144 Vibilia
144 Vibilia is carbonaceous asteroid from the central region of the asteroid belt, approximately 140 kilometers in diameter.
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145 Adeona
145 Adeona is a rather large main-belt asteroid.
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14627 Emilkowalski
14627 Emilkowalski, provisional designation, is a stony asteroid from the central region of the asteroid belt, approximately 7 kilometers in diameter.
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148 Gallia
148 Gallia (as Greek Γαλλία) is an asteroid from the central regions of the asteroid belt, approximately in diameter.
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1484 Postrema
1484 Postrema, provisional designation, is a carbonaceous Postremian asteroid and namesake of the Postrema family from the central regions of the asteroid belt, approximately 41 kilometers in diameter.
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15 Eunomia
15 Eunomia is a very large asteroid in the inner asteroid belt.
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153 Hilda
153 Hilda is a large asteroid in the outer main belt, with a diameter of 170 km.
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157 Dejanira
157 Dejanira is a main belt asteroid that was discovered by Alphonse Borrelly on December 1, 1875, and named after the warlike princess Deianira in Greek mythology (Δηιάνειρα in Greek).
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158 Koronis
158 Koronis is a main-belt asteroid that was discovered by Russian astronomer Viktor Knorre on January 4, 1876, from the Berlin observatory.
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159 Aemilia
159 Aemilia is a large main-belt asteroid.
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163 Erigone
163 Erigone is an asteroid from the asteroid belt and the namesake of the Erigone family of asteroids that share similar orbital elements and properties.
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1644 Rafita
1644 Rafita, provisional designation, is a stony asteroid from the middle region of the asteroid belt, approximately 15 kilometers in diameter.
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1647 Menelaus
1647 Menelaus, provisional designation, is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter.
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170 Maria
170 Maria is a Main belt asteroid that was discovered by French astronomer Henri Joseph Perrotin on January 10, 1877.
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1726 Hoffmeister
1726 Hoffmeister, provisional designation, is a carbonaceous asteroid and namesake of the Hoffmeister family from the central region of the asteroid belt, approximately 23 kilometers in diameter.
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173 Ino
173 Ino is a large asteroid and the parent body of the Ino family, located in the central regions of the asteroid belt, approximately in diameter.
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1749 Telamon
1749 Telamon, provisional designation, is a dark Jupiter Trojan from the Greek camp, approximately in diameter.
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17492 Hippasos
17492 Hippasos, provisional designation, is a Jupiter trojan and member of the Ennomos family from the Trojan camp, approximately in diameter. It was discovered on 10 December 1991, by astronomer Freimut Börngen at the Karl Schwarzschild Observatory in Tautenburg, Germany. The Jovian asteroid belongs to the 80 largest Jupiter trojans has a rotation period of 17.8 hours. It was named after the Trojan prince Hippasus (Hippasos) from Greek mythology.
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1911 Schubart
1911 Schubart, provisional designation, is a dark Hildian asteroid and parent body of the Schubart family, located in the outermost region of the asteroid belt, approximately 70 kilometers in diameter.
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194 Prokne
194 Prokne is a main-belt asteroid that was discovered by German-American astronomer C. H. F. Peters on March 21, 1879, in Clinton, New York, and named after Procne, the sister of Philomela in Greek mythology.
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2 Pallas
Pallas, minor-planet designation 2 Pallas, is the second asteroid to have been discovered (after Ceres), and is one of the largest asteroids in the Solar System.
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20 Massalia
20 Massalia is a stony asteroid and the parent body of the Massalia family located in the inner region of the asteroid belt, approximately in diameter.
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2085 Henan
2085 Henan, provisional designation, is a potentially slow rotating asteroid and the parent body of the Henan family in the central regions of the asteroid belt, approximately 15 kilometers in diameter.
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2148 Epeios
2148 Epeios, provisional designation, is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter.
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21509 Lucascavin
21509 Lucascavin (1998 KL35) is a main-belt asteroid and parent body of the Lucascavin family.
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221 Eos
221 Eos is a large main-belt asteroid that was discovered by Johann Palisa on January 18, 1882, in Vienna.
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2384 Schulhof
2384 Schulhof, provisional designation, is a stony Eunomia asteroid from the middle region of the asteroid belt, approximately 12 kilometers in diameter.
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24 Themis
24 Themis is one of the largest asteroids in the asteroid belt.
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25 Phocaea
25 Phocaea is a stony asteroid from the inner regions of the asteroid belt, approximately 75 kilometers in diameter.
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254 Augusta
254 Augusta is a main-belt asteroid, discovered on 31 March 31, 1886 by astronomer Johann Palisa at Vienna Observatory, Austria.
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260 Huberta
260 Huberta is a large asteroid orbiting near the outer edge of the Main belt.
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27 Euterpe
27 Euterpe is a stony asteroid and parent body of the Euterpe family, located in the inner asteroid belt, approximately 100 kilometers in diameter.
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2732 Witt
2732 Witt, provisional designation, is a bright asteroid and namesake of the Witt family located in the central regions of the asteroid belt, approximately in diameter.
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283 Emma
283 Emma is a large asteroid of the asteroid belt.
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293 Brasilia
293 Brasilia is a large Main belt asteroid that was discovered by French astronomer Auguste Charlois on 20 May 1890 in Nice.
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298 Baptistina
298 Baptistina is an asteroid orbiting in the asteroid belt.
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3 Juno
Juno, minor-planet designation 3 Juno in the Minor Planet Center catalogue system, is an asteroid in the asteroid belt.
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302 Clarissa
302 Clarissa is a typical Main belt asteroid.
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3063 Makhaon
3063 Makhaon, provisional designation, is a large Jupiter trojan from the Greek camp, approximately in diameter.
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31 Euphrosyne
31 Euphrosyne is the 12th-largest and the 5th-most-massive asteroid in the asteroid belt, discovered by James Ferguson on September 1, 1854.
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313 Chaldaea
313 Chaldaea is a large Main belt asteroid.
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322 Phaeo
322 Phaeo is a large Main belt asteroid.
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329 Svea
329 Svea is a large Main belt asteroid.
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331P/Gibbs
331P/Gibbs (P/2012 F5) is a small periodic Encke-type and rare main-belt comet, discovered by American amateur astronomer Alex Gibbs.
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3548 Eurybates
3548 Eurybates, provisional designation, is a carbonaceous Jupiter trojan from the Greek camp and the parent body of the Eurybates family, approximately in diameter.
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3556 Lixiaohua
3556 Lixiaohua, provisional designation, is a dark Lixiaohua asteroid from the outer region of the asteroid belt, approximately 20 kilometers in diameter.
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363 Padua
363 Padua a main belt asteroid that was discovered by Auguste Charlois on 17 March 1893 in Nice.
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369 Aëria
369 Aëria, provisional designation, is a metallic asteroid and the parent body of the Aeria family.
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375 Ursula
375 Ursula, provisional designation, is a dark asteroids and parent body of the Ursula family from the outer regions of the asteroid belt.
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396 Aeolia
396 Aeolia is a typical main belt asteroid.
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4 Vesta
Vesta, minor-planet designation 4 Vesta, is one of the largest objects in the asteroid belt, with a mean diameter of.
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4007 Euryalos
4007 Euryalos, provisional designation, is a larger Jupiter trojan from the Greek camp, approximately in diameter.
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410 Chloris
410 Chloris is a very large main-belt asteroid that was discovered by Auguste Charlois on January 7, 1896, in Nice.
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4138 Kalchas
4138 Kalchas, provisional designation, is a large Jupiter trojan from the Greek camp, approximately in diameter.
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43 Ariadne
43 Ariadne is a fairly large and bright main-belt asteroid.
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434 Hungaria
434 Hungaria is a relatively small asteroid orbiting in the inner asteroid belt.
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44 Nysa
44 Nysa is a large and very bright main-belt asteroid, and the brightest member of the Nysian asteroid family.
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46 Hestia
46 Hestia is a large, dark main-belt asteroid.
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4709 Ennomos
4709 Ennomos, provisional designation, is a large Jupiter trojan from the Trojan camp and the namesake of the small Ennomos family, approximately in diameter.
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480 Hansa
480 Hansa, provisional designation, is a stony asteroid and the namesake of the Hansa family located in the central region of the asteroid belt, approximately in diameter.
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490 Veritas
490 Veritas is a carbonaceous Veritasian asteroid, which may have been involved in one of the more massive asteroid-asteroid collisions of the past 100 million years.
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5 Astraea
5 Astraea is a large asteroid from the asteroid belt.
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5026 Martes
5026 Martes, provisional designation, is a carbonaceous asteroid from the inner region of the asteroid belt, approximately 9 kilometers in diameter.
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507 Laodica
507 Laodica is a minor planet orbiting the Sun.
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5436 Eumelos
5436 Eumelos, provisional designation, is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter.
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569 Misa
569 Misa is a minor planet orbiting the Sun.
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589 Croatia
589 Croatia, provisional designation, is a dark asteroid and parent body of the Croatia family, located in the outer regions of the asteroid belt, approximately 88 kilometers in diameter.
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606 Brangäne
606 Brangäne is a minor planet orbiting the Sun.
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618 Elfriede
618 Elfriede is a minor planet orbiting the Sun.
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623 Chimaera
623 Chimaera is a minor planet orbiting the Sun.
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624 Hektor
624 Hektor is the largest Jupiter trojan and the namesake of the Hektor family, with a highly elongated shape equivalent in volume to a sphere of approximately 225 to 250 kilometers diameter. It was discovered on 10 February 1907, by astronomer August Kopff at Heidelberg Observatory in southwest Germany, and named after the Trojan prince Hector, from Greek mythology. It has one small 12-kilometer sized satellite, Skamandrios, discovered in 2006.
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627 Charis
627 Charis, provisional designation, is an asteroid and the parent body of the Charis family, located in the outer regions of the asteroid belt, approximately 49 kilometers in diameter.
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63 Ausonia
63 Ausonia is a stony Vestian asteroid from the inner region of the asteroid belt, approximately 100 kilometers (60 miles) in diameter.
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65 Cybele
65 Cybele is one of the largest asteroids in the Solar System and is located in the outer asteroid belt.
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656 Beagle
656 Beagle is a Themistian asteroid.
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668 Dora
668 Dora is an asteroid orbiting in the asteroid belt located roughly between the orbits of the planets Mars and Jupiter.
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686 Gersuind
686 Gersuind is a minor planet orbiting the Sun that was discovered by German astronomer August Kopff on 15 August 1909 from Heidelberg.
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702 Alauda
702 Alauda, provisional designation, is a carbonaceous asteroid and binary system from the outer asteroid belt, approximately 190 kilometers in diameter.
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709 Fringilla
709 Fringilla is a minor planet orbiting the Sun.
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729 Watsonia
729 Watsonia is a rare-type asteroid and namesake of the Watsonia family from the central region of the asteroid belt.
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751 Faïna
751 Faïna is a minor planet orbiting the Sun.
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752 Sulamitis
752 Sulamitis is a minor planet orbiting the Sun.
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778 Theobalda
778 Theobalda is a minor planet orbiting the Sun, in the main asteroid belt.
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780 Armenia
780 Armenia is a minor planet in the asteroid belt orbiting the Sun.
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8 Flora
8 Flora is a large, bright main-belt asteroid.
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808 Merxia
808 Merxia is a minor planet orbiting the Sun.
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81 Terpsichore
81 Terpsichore is a large and very dark main-belt asteroid.
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816 Juliana
816 Juliana is a minor planet orbiting the Sun.
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832 Karin
832 Karin is a minor planet orbiting the Sun.
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84 Klio
84 Klio is a quite large and very dark main-belt asteroid.
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845 Naëma
845 Naëma is a minor planet orbiting the Sun.
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847 Agnia
847 Agnia is a minor planet orbiting the Sun.
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87 Sylvia
87 Sylvia is the 8th-largest asteroid in the asteroid belt.
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871 Amneris
871 Amneris is a minor planet orbiting the Sun.
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883 Matterania
883 Matterania is an S-type asteroid belonging to the Flora family in the Main Belt.
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887 Alinda
887 Alinda is a very eccentric, near-Earth asteroid with an Earth minimum orbit intersection distance (MOID) of 0.092 AU.
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89 Julia
89 Julia is a large main-belt asteroid that was discovered by French astronomer Édouard Stephan on August 6, 1866.
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895 Helio
895 Helio is a large dark outer main-belt asteroid about 150 km in diameter.
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9 Metis
9 Metis is one of the larger main-belt asteroids.
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909 Ulla
909 Ulla is a minor planet orbiting the Sun.
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918 Itha
918 Itha is a minor planet orbiting the Sun.
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926 Imhilde
926 Imhilde is a minor planet orbiting the Sun.
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945 Barcelona
945 Barcelona is a minor planet orbiting the Sun in the Asteroid belt.
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96 Aegle
96 Aegle, is a carbonaceous asteroid and the namesake of the Aegle family located in the outer regions of the asteroid belt, approximately in diameter.
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Aegle family, Aeolia family, Aeria family, Agnia family, Alauda family, Amneris family, Anfimov family, Arkesilaos family, Armenia family, Asteroid families, Astraea family, Astrid family, Ausonia family, Aëria family, Background asteroid, Barcelona family, Beagle family, Bower family, Brangane family, Brasilia family, Brucato family, Brugmansia family, Chaldaea family, Charis family, Chimaera family, Chloris family, Clarissa family, Clematis family, Croatia family, Datura family, Dejanira family, Dora family, Durisen family, Elfriede family, Emilkowalski family, Emma family, Ennomos family, Epeios family, Erigone family, Eumelos family, Euphrosyne family, Euryalos family, Eurybates family, Euterpe family, FIN tbl, Family identification number, Family of asteroids, Faïna family, Fringilla family, Gallia family, Gersuind family, Gibbs family, Hanna family, Hansa family, Hektor family, Henan family, Hestia family, Hierarchical Clustering Method (asteroids), Hoffmeister family, Huberta family, Iannini family, Imhilde family, Inarradas family, Ino family, Interloper (asteroid), Itha family, Jones family (asteroids), Julia family (asteroids), Juliana family, Kalchas family, Karma family, Kartivelia family, Kartvelia family, Kazuya family, Klio family, Klytaemnestra family, König family, Laodica family, Lau family, Leonidas family, Liberatrix family, List of asteroid families, Lixiaohua family, Lorre family, Lucascavin family, Lucienne family, Luthera family, Makhaon family, Marconia family, Martes family, Melanthios family, Meliboea family, Menelaus family, Merxia family, Misa family, Mitidika family, Naëma family, Nemesis family, Nohavica family, Phaeo family, Podarkes family, Postrema family, Rafita family, Reginita family, Salli family, San Marcello family, Schubart family, Schulhof family, Sulamitis family, Svea family, Sylvia family, Telamon family, Telramund family, Terentia family, Terpsichore family, Theobalda family, Tina family, Tirela family, Ulla family, Ursula family, Veritas family, Vibilia family, Watsonia family, Witt family, Xizang family, Yakovlev family.
References
[1] https://en.wikipedia.org/wiki/Asteroid_family
