SkyEye

Dwarf Planets and Small Solar-System Bodies

What is the Definition?

The words asteroid, minor planet and planetoid are (unofficial and) interchangable. They each refer to the small rocky bodies that are mainly confined to the asteroid belt between the planets Mars and Jupiter. The radius of the asteroid belt varies from 2.0 AU to 3.3 AU from the Sun with holes (called Kirkwood gaps) in the distribution of objects. These gaps coincide with orbital periods which are exact fractions of the period of Jupiter. However, these objects can be found elsewhere in the solar system. Some fly alarmingly close to the Earth whilst others inhabit the shadowy realms of the Kuiper Belt out beyond the planet Neptune.

On 24 August 2006, the International Astronomical Union defined a dwarf planet as a celestial body that

Furthermore, on 11 June 2008, the International Astronomical Union defined a plutoid as a celestial body that

Satellites of plutoids are not plutoids themselves.

Ceres, Pluto, Haumea, Eris and Makemake are now classified as dwarf planets and all but Ceres are also classified as plutoids.

A small solar-system body is anything that isn't a planet, a dwarf planet, or a satellite. This includes most asteroids and comets.

Some Interesting Bodies

The table below lists a few characteristics of some of the more interesting bodies. According to current policy, an official number is not given to a small solar-system body until a reliable orbit has been determined for it. Once the object has been numbered, the discoverer may name it.

Dwarf planets are marked with an asterisk *.

Number Name Discovery Semi-Major
Axis (AU)
Period
(years)
Eccentricity Inclination
1 Ceres * 1801 Piazzi 2.768 4.61 0.0757 10.59°
2 Pallas 1802 Olbers 2.773 4.62 0.2308 34.84°
3 Juno 1804 Harding 2.669 4.36 0.2566 12.99°
4 Vesta 1807 Olbers 2.362 3.63 0.0891 7.14°
5 Astraea 1845 Hencke 2.574 4.13 0.1916 5.37°
21 Lutetia 1852 Goldschmidt 2.434 3.80 0.1646 3.06°
243 Ida 1884 Palisa 2.861 4.84 0.0411 1.13°
253 Mathilde 1885 Palisa 2.648 4.31 0.2649 6.74°
298 Baptistina 1890 Charlois 2.264 3.41 0.0956 6.29°
433 Eros 1898 Witt 1.458 1.76 0.2226 10.83°
588 Achilles 1906 Wolf 5.207 11.88 0.1467 10.32°
624 Hektor 1907 Kopff 5.254 12.04 0.0244 18.17°
719 Albert 1911 Palisa 2.636 4.28 0.5495 11.58°
944 Hidalgo 1920 Baade 5.739 13.75 0.6611 42.52°
951 Gaspra 1916 Neujmin 2.210 3.29 0.1732 4.10°
1221 Amor 1932 Delporte 1.919 2.66 0.4355 11.88°
1566 Icarus 1949 Baade 1.078 1.12 0.8269 22.83°
1862 Apollo 1932 Reinmuth 1.470 1.78 0.5599 6.35°
2060 Chiron 1977 Kowal 13.639 50.37 0.3827 6.95°
2062 Aten 1976 Helin 0.967 0.95 0.1827 18.93°
2161 Grissom 1963 Indiana Asteroid Program 2.747 4.55 0.1621 7.30°
2309 Mr. Spock 1971 Gibson 3.016 5.24 0.0902 10.98°
2417 McVittie 1964 Indiana Asteroid Program 3.181 5.67 0.2238 3.11°
2685 Masursky 1981 Bowell 2.569 4.12 0.1096 12.13°
2867 Steins 1969 Chernykh 2.364 3.63 0.1456 9.93°
3200 Phaethon 1983 IRAS 1.271 1.43 0.8899 22.25°
3634 Iwan 1980 Lagerkvist 2.245 3.36 0.0915 4.31°
4179 Toutatis 1989 Pollas 2.535 4.04 0.6294 0.45°
4659 Roddenberry 1981 Bus 2.370 3.65 0.2246 2.47°
4864 Nimoy 1988 Debehogne 2.468 3.88 0.1778 3.62°
5535 Annefrank 1942 Reinmuth 2.213 3.29 0.0635 4.25°
5598 Carlmurray 1991 Holt 2.190 3.24 0.1134 5.04°
7307 Takei 1994 Shimizu, Urata 2.741 4.54 0.0880 6.99°
9777 Enterprise 1994 Shimizu, Urata 2.397 3.71 0.2317 3.27°
9969 Braille 1992 Helin, Lawrence 2.341 3.58 0.4334 29.00°
10199 Chariklo 1997 Spacewatch 15.801 62.81 0.1725 23.40°
10455 Donnison 1978 Lagerkvist 2.360 3.62 0.2219 6.12°
12395 Richnelson 1995 Asher 3.234 5.82 0.0493 21.12°
25143 Itokawa 1998 Lincoln Laboratory Near-Earth Asteroid Research Team 1.324 1.52 0.2801 1.62°
26733 Nanavisitor 2001 Yeung 2.601 4.19 0.1555 2.09°
28978 Ixion 2001 Deep Ecliptic Survey 39.559 248.81 0.2416 19.61°
50000 Quaoar 2002 Trujillo, Brown 43.440 286.31 0.0351 7.99°
68410 Nichols 2001 Collins, White 2.681 4.39 0.0753 4.85°
69230 Hermes 1937 Reinmuth 1.655 2.13 0.6239 6.07°
101955 Bennu 1999 Lincoln Laboratory Near-Earth Asteroid Research Team 1.126 1.20 0.2037 6.03°
134340 Pluto * 1930 Tombaugh 39.445 247.74 0.2502 17.09°
136108 Haumea * 2003 [disputed] 43.336 285.29 0.1890 28.20°
136199 Eris * 2003 Brown, Trujillo, Rabinowitz 67.661 556.56 0.4423 44.18°
136472 Makemake * 2005 Brown, Trujillo, Rabinowitz 45.761 309.57 0.1540 28.99°
155142 Tenagra 2005 Merlin 2.765 4.60 0.084 0.08°

Notes

Ceres is the largest of all the objects in the asteroid belt and is classified as a dwarf planet. Like Pluto, it was originally identified as a planet but was assigned a different classification when it became clear that it was just one of many such objects inhabiting the region between Mars and Jupiter. It has its own artificial satellite, the Dawn spacecraft which arrived and went into orbit in 2015.

Pallas has an unusually high orbital inclination.

Like its neighbours Ceres, Pallas and Vesta, Juno was originally classified as a planet.

Vesta is the brightest of the asteroids and the only one that can reach the limit of naked-eye visibility, sixth magnitude. It is also the second-most massive object in the main asteroid belt. The Dawn spacecraft was in orbit about it during 2011 and 2012 before setting off to visit Ceres in 2015.

After a gap of 38 years, Astraea was discovered. Modern automated methods now mean thousands of such bodies are discovered every year.

Rosetta's ten-year mission provided it the opportunity to fly past two asteroids, Lutetia and the rare E-type asteroid Steins.

Ida was photographed by the Galileo spacecraft in 1994. This historic encounter provided the first conclusive evidence that asteroids could have natural satellites when Dactyl was discovered accompanying its parent body in orbit about the Sun.

In June 1997, NEAR Shoemaker passed by Mathilde on its way to a year 2000 Valentine's Day encounter with Eros, an Earth-grazing asteroid and the first one discovered to come inside the orbit of Mars. One year later, NEAR made history by becoming the first spacecraft to touch down on an asteroid when it made an amazing soft landing on Eros.

Numerical modelling suggests that members of the Baptistina asteroid group, named for Baptistina, may be responsible not only for the large lunar crater Tycho but also the terrestrial impact site at Chicxulub which seems to be implicated in the extinction of the dinosaurs.

The Trojan asteroids are two families of asteroids stationed at the Lagrangian points in Jupiter's orbit. The first one discovered was Achilles but the largest is Hektor.

The last of the 'lost' named and numbered asteroids, Albert was recovered in May 2000, almost 89 years after its original discovery. With its recovery, the position of every numbered asteroid is now known.

Hidalgo has a highly elliptical orbit which carries it from the main asteroid belt between Mars and Jupiter to out beyond Saturn. Some think that Hidalgo is actually an extinct comet.

In October 1991, the Galileo spacecraft took the first ever high-resolution photograph of an asteroid. The object concerned was Gaspra, a member of the Flora group of asteroids.

Amor is the prototype of the Amor group of asteroids. These objects come to perihelion between the orbits of Mars and Earth.

Icarus has an orbit that carries it closer to the Sun than Mercury, the innermost planet in the solar system.

Apollo is the prototype of the Apollo group of asteroids. These objects have perihelion distances of less than 1 AU so they cross the Earth's orbit. Scientists have reconstructed the orbit of the meteroid that exploded in the region of Chelyabinsk, Russia, on 15 February 2013 and have concluded that it was an Apollo asteroid.

Chiron has an orbit entirely outside that of Jupiter. It has been observed to have a coma and may be a giant comet instead of an asteroid.

Aten is the prototype of the Aten group of asteroids. These are Earth-approaching objects with orbits lying mostly within that of the Earth.

Grissom is named in the memory of Apollo astronaut Virgil Ivan 'Gus' Grissom who was killed in the Apollo 1 launchpad fire on 27 January 1967.

Phaethon passes closer to the Sun than any other object in the solar system with the exception of a few comets. It was discovered by the IRAS satellite and is thought to be the parent body of the Geminid meteor shower.

The Astronomy Unit at Queen Mary University of London, is proud to have five of its faculty members represented in the far reaches of the solar system. McVittie is named for the late George McVittie who was appointed as the first Professor of Mathematics at Queen Mary College in 1948. Iwan is named for Prof. Iwan P. Williams, Carlmurray is named for Prof. Carl D. Murray, Donnison is named for Dr. Richard Donnison and Richnelson is named for Prof. Richard P. Nelson.

In 2000, Masursky was examined by Cassini as the spacecraft headed out to its encounters with Jupiter and Saturn.

Toutatis had a close encounter with the Earth in December 1996 and again in September 2004.

Star Trek creator Gene Roddenberry is immortalised in the heavens as Roddenberry. Actors Leonard Nimoy (Mr Spock), George Takei (Lt Sulu) and Nichelle Nichols (Lt Uhura) from the series have been similarly honoured with Nimoy, Takei and Nichols. Nanavisitor is named for the actress who played Major Kira from Star Trek: Deep Space Nine, Nana Visitor. The starship Enterprise is also represented by Enterprise. Tenagra is the name of an island from the Star Trek: The Next Generation episode entitled 'Darmok'. The asteroid called Mr. Spock is actually named for a cat that accompanied the asteroid's discoverer but of course, the cat was named for the beloved Star Trek character.

Stardust was the first mission to return samples from a comet to the Earth. As a prelude to its cometary encounters, Stardust flew past Annefrank, discovering that it was much larger (and much dimmer) than anticipated.

Using stellar occultation data, scientists discovered that Chariklo is surrounded by two rings, the first asteroid to be identified as possessing a ring system. Chariklo is a Centaur, one of a class of small objects which orbit primarily between Jupiter and Neptune.

Deep Space 1, using an innovative ion propulsion system, made a very close fly by of near-Earth asteroid Braille in July 1999. The spacecraft went to on to fly past the coma of comet 19P/Borrelly two years later.

Itokawa is named for Hideo Itokawa, the father of Japanese rocketry. It's entirely appropriate that in 2005, the Japanese spacecraft Hayabusa landed not once but twice on the asteroid, making it the first spacecraft to successfully land and take off from the surface of an asteroid. Despite multiple problems and malfunctions, the spacecraft successfully collected a specimen from the asteroid and the sample capsule landed in Australia in June 2010 with its precious cargo.

When Ixion was discovered it was originally thought to be larger than Ceres. Quaoar turned out to be even bigger although eventually it too was supplanted by other larger trans-Neptunian objects. Quaoar has one known moon called Weywot.

Lost just five days after its initial discovery in 1937 and only recovered in October 2003, Hermes turns out to be a binary object. Two asteroids for the price of one!

Bennu is a member of the Apollo group of asteroids and has an estimated 1-in-2700 chance of striking the Earth next century. The OSIRIS-REx spacecraft intends to visit this asteroid in 2020 and return a sample from it three years later.

Pluto was demoted from planet to dwarf planet status on 24 August 2006 and given the number 134340 a month later. It was the first trans-Neptunian object discovered and is one of the largest. It has five companions: Charon (discovered in 1978 by J. Christy), Hydra and Nix (discovered in 2005 by the Hubble Space Telescope Pluto Companion Search Team), Kerberos (discovered in 2011 by Showalter et al whilst searching for rings around Pluto) and finally Styx (discovered in 2012 by Showalter et al whilst looking for possible hazards to the wildly successful New Horizons flyby mission in 2015). It's surprising that such a small object has such a complicated satellite system.

Like Pluto, Haumea has satellites. They are named Hi'iaka and Namaka, both discovered in 2005 by Brown, Bouchez and the Keck Observatory Adaptive team. Haumea is the Hawaiian goddess of childbirth and fertility, and Hi'iaka and Namaka are two of her children. The minor planet Haumea is accompanied not only by her two satellites but lots of tiny fragments which resulted from an ancient collision.

Eris is the largest of the dwarf planets and the object which ultimately led to the demotion of Pluto! Informally known as 'Xena' since its discovery in 2003, it is appropriately named for the goddess of discord who caused Trojan War. It has a satellite named Dysnomia who, in Greek mythology, embodies the spirit of lawlessness and is the daughter of Eris.

Like other classical Kuiper belt objects, Makemake has the name of a creator deity, in this case, the creator of humanity according to the myths of Easter Islanders. It is pronounced ma kay ma kay.

Sources

Orbital elements are provided by the JPL Small-Body Database Browser.