Recent from talks
List of minor planets
Knowledge base stats:
Talk channels stats:
Members stats:
List of minor planets
The following is a list of minor planets in ascending numerical order. Minor planets are small bodies in the Solar System: asteroids, distant objects, and dwarf planets, but not comets. As of 2022, the vast majority (97.3%) are asteroids from the asteroid belt. Their discoveries are certified by the Minor Planet Center, which assigns them numbers on behalf of the International Astronomical Union. Every year, the Center publishes thousands of newly numbered minor planets in its Minor Planet Circulars (see index). As of October 2025[update], the 875,150 numbered minor planets made up more than half of the 1,474,903 observed small Solar System bodies, of which the rest were unnumbered minor planets and comets.
The catalog's first object is 1 Ceres, discovered by Giuseppe Piazzi in 1801, while its best-known entry is Pluto, listed as 134340 Pluto. Both are among the 3.1% of numbered minor planets with names, mostly of people, places, and figures from mythology and fiction. (4596) 1981 QB and 841529 Jonahwoodhams are currently the lowest-numbered unnamed and highest-numbered named minor planets, respectively.
There are more than a thousand minor-planet discoverers observing from a growing list of registered observatories. The most prolific discoverers are Spacewatch, LINEAR, MLS, NEAT and CSS. It is expected that the upcoming survey by the Vera C. Rubin Observatory will discover another 5 million minor planets during the next ten years—almost a tenfold increase from current numbers. While all main-belt asteroids with a diameter above 10 km (6.2 mi) have been discovered, there might be as many as 10 trillion 1 m (3.3 ft)-sized asteroids or larger out to the orbit of Jupiter; and more than a trillion minor planets in the Kuiper belt. For minor planets grouped by a particular aspect or property, see § Specific lists.
The list of minor planets consists of more than 700 partial lists, each containing 1000 minor planets grouped into 10 tables. The data is sourced from the Minor Planet Center (MPC) and expanded with data from the JPL SBDB (mean-diameter), Johnston's archive (sub-classification) and others (see detailed field descriptions below). For an overview of all existing partial lists, see § Main index.
The information given for a minor planet includes a permanent and provisional designation (§ Designation), a citation that links to the meanings of minor planet names (only if named), the discovery date, location, and credited discoverers (§ Discovery and § Discoverers), a category with a more refined classification than the principal grouping represented by the background color (§ Category), a mean-diameter, sourced from JPL's SBDB or otherwise calculated estimates in italics (§ Diameter), and a reference (Ref) to the corresponding pages at MPC and JPL SBDB.
The MPC may credit one or several astronomers, a survey or similar program, or even the observatory site with the discovery. In the first column of the table, an existing stand-alone article is linked in boldface, while (self-)redirects are never linked. Discoverers, discovery site and category are only linked if they differ from the preceding catalog entry.
The example above shows five catalog entries from one of the partial lists. All five asteroids were discovered at Palomar Observatory by the Palomar–Leiden survey (PLS). The MPC directly credits the survey's principal investigators, that is, the astronomers Cornelis van Houten, Ingrid van Houten-Groeneveld and Tom Gehrels. (This is the only instance where the list of minor planets diverges from the Discovery Circumstances in the official MPC list.) 189004 Capys, discovered on 16 October 1977, is the only named minor planet among these five. Its background color indicates that it is a Jupiter trojan (from the Trojan camp at Jupiter's L5), estimated to be approximately 12 kilometers in diameter. All other objects are smaller asteroids from the inner (white), central (light-grey) and outer regions (dark grey) of the asteroid belt. The provisional designation for all objects is an uncommon survey designation.
After discovery, minor planets generally receive a provisional designation, e.g. 1989 AC, then a leading sequential number in parentheses, e.g. (4179) 1989 AC, turning it into a permanent designation (numbered minor planet). Optionally, a name can be given, replacing the provisional part of the designation, e.g. 4179 Toutatis. (On Wikipedia, named minor planets also drop their parentheses.)
Hub AI
List of minor planets AI simulator
(@List of minor planets_simulator)
List of minor planets
The following is a list of minor planets in ascending numerical order. Minor planets are small bodies in the Solar System: asteroids, distant objects, and dwarf planets, but not comets. As of 2022, the vast majority (97.3%) are asteroids from the asteroid belt. Their discoveries are certified by the Minor Planet Center, which assigns them numbers on behalf of the International Astronomical Union. Every year, the Center publishes thousands of newly numbered minor planets in its Minor Planet Circulars (see index). As of October 2025[update], the 875,150 numbered minor planets made up more than half of the 1,474,903 observed small Solar System bodies, of which the rest were unnumbered minor planets and comets.
The catalog's first object is 1 Ceres, discovered by Giuseppe Piazzi in 1801, while its best-known entry is Pluto, listed as 134340 Pluto. Both are among the 3.1% of numbered minor planets with names, mostly of people, places, and figures from mythology and fiction. (4596) 1981 QB and 841529 Jonahwoodhams are currently the lowest-numbered unnamed and highest-numbered named minor planets, respectively.
There are more than a thousand minor-planet discoverers observing from a growing list of registered observatories. The most prolific discoverers are Spacewatch, LINEAR, MLS, NEAT and CSS. It is expected that the upcoming survey by the Vera C. Rubin Observatory will discover another 5 million minor planets during the next ten years—almost a tenfold increase from current numbers. While all main-belt asteroids with a diameter above 10 km (6.2 mi) have been discovered, there might be as many as 10 trillion 1 m (3.3 ft)-sized asteroids or larger out to the orbit of Jupiter; and more than a trillion minor planets in the Kuiper belt. For minor planets grouped by a particular aspect or property, see § Specific lists.
The list of minor planets consists of more than 700 partial lists, each containing 1000 minor planets grouped into 10 tables. The data is sourced from the Minor Planet Center (MPC) and expanded with data from the JPL SBDB (mean-diameter), Johnston's archive (sub-classification) and others (see detailed field descriptions below). For an overview of all existing partial lists, see § Main index.
The information given for a minor planet includes a permanent and provisional designation (§ Designation), a citation that links to the meanings of minor planet names (only if named), the discovery date, location, and credited discoverers (§ Discovery and § Discoverers), a category with a more refined classification than the principal grouping represented by the background color (§ Category), a mean-diameter, sourced from JPL's SBDB or otherwise calculated estimates in italics (§ Diameter), and a reference (Ref) to the corresponding pages at MPC and JPL SBDB.
The MPC may credit one or several astronomers, a survey or similar program, or even the observatory site with the discovery. In the first column of the table, an existing stand-alone article is linked in boldface, while (self-)redirects are never linked. Discoverers, discovery site and category are only linked if they differ from the preceding catalog entry.
The example above shows five catalog entries from one of the partial lists. All five asteroids were discovered at Palomar Observatory by the Palomar–Leiden survey (PLS). The MPC directly credits the survey's principal investigators, that is, the astronomers Cornelis van Houten, Ingrid van Houten-Groeneveld and Tom Gehrels. (This is the only instance where the list of minor planets diverges from the Discovery Circumstances in the official MPC list.) 189004 Capys, discovered on 16 October 1977, is the only named minor planet among these five. Its background color indicates that it is a Jupiter trojan (from the Trojan camp at Jupiter's L5), estimated to be approximately 12 kilometers in diameter. All other objects are smaller asteroids from the inner (white), central (light-grey) and outer regions (dark grey) of the asteroid belt. The provisional designation for all objects is an uncommon survey designation.
After discovery, minor planets generally receive a provisional designation, e.g. 1989 AC, then a leading sequential number in parentheses, e.g. (4179) 1989 AC, turning it into a permanent designation (numbered minor planet). Optionally, a name can be given, replacing the provisional part of the designation, e.g. 4179 Toutatis. (On Wikipedia, named minor planets also drop their parentheses.)
Recent media