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planetary science Planetary science (or more rarely, planetology) is the scientific study of planets (including Earth), celestial bodies (such as moons, asteroids, comets) and planetary systems (in particular those of the Solar System) and the processes of ...
, the term unusual minor planet, or ''unusual object'', is used for a
minor planet According to the International Astronomical Union (IAU), a minor planet is an astronomical object in direct orbit around the Sun that is exclusively classified as neither a planet nor a comet. Before 2006, the IAU officially used the term ''minor ...
that possesses an unusual physical or orbital characteristic. For the
Minor Planet Center The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU). Founded in 1947, it operates at the Smithsonian Astrophysical Observatory. Funct ...
(MPC), which operates under the auspices of the
International Astronomical Union The International Astronomical Union (IAU; , UAI) is an international non-governmental organization (INGO) with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach, education, and developmen ...
, any non-classical
main-belt asteroid The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars. It contains a great many solid, irregularly shaped bodies called asteroids ...
, which account for the vast majority of all minor planets, is an unusual minor planet. These include the
near-Earth object A near-Earth object (NEO) is any small Solar System body orbiting the Sun whose closest approach to the Sun ( perihelion) is less than 1.3 times the Earth–Sun distance (astronomical unit, AU). This definition applies to the object's orbit a ...
s and
Trojans Trojan or Trojans may refer to: * Of or from the ancient city of Troy * Trojan language, the language of the historical Trojans Arts and entertainment Music * ''Les Troyens'' ('The Trojans'), an opera by Berlioz, premiered part 1863, part 1890 ...
as well as the
distant minor planet A distant minor planet, or ''distant object'', is any minor planet found beyond Jupiter in the outer Solar System that is not commonly thought of as an "asteroid". The umbrella term is used by IAU's Minor Planet Center (MPC), which is responsib ...
s such as
centaurs A centaur ( ; ; ), occasionally hippocentaur, also called Ixionidae (), is a creature from Greek mythology with the upper body of a human and the lower body and legs of a horse that was said to live in the mountains of Thessaly. In one version o ...
and
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 than Neptune, which has an orbital semi-major axis of 30.1 astronomical units (AU). ...
s. In a narrower sense, the term is used for a group of bodies – including
main-belt asteroid The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars. It contains a great many solid, irregularly shaped bodies called asteroids ...
s,
Mars-crosser A Mars-crossing asteroid (MCA, also Mars-crosser, MC) is an asteroid whose orbit crosses that of Mars. Some Mars-crossers numbered below 100000 are listed here. They include the two numbered Mars trojans 5261 Eureka and . Many databases, for i ...
s, centaurs and otherwise non-classifiable minor planets – that show a high
orbital eccentricity In astrodynamics, the orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values be ...
, typically above 0.5 and/or a
perihelion An apsis (; ) is the farthest or nearest point in the orbit of a planetary body about its primary body. The line of apsides (also called apse line, or major axis of the orbit) is the line connecting the two extreme values. Apsides perta ...
of less than 6  AU. Similarly, an unusual asteroid (UA) is an
inner Solar System The Solar SystemCapitalization of the name varies. The International Astronomical Union, the authoritative body regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed "Sol ...
object with a high eccentricity and/or
inclination Orbital inclination measures the tilt of an object's orbit around a celestial body. It is expressed as the angle between a reference plane and the orbital plane or axis of direction of the orbiting object. For a satellite orbiting the Eart ...
but with a perihelion larger than 1.3 AU, which does exclude the
near-Earth object A near-Earth object (NEO) is any small Solar System body orbiting the Sun whose closest approach to the Sun ( perihelion) is less than 1.3 times the Earth–Sun distance (astronomical unit, AU). This definition applies to the object's orbit a ...
s.


Other unusual objects

According to the MPC, other unusual minor planets are objects, which orbital characteristics do not fit those of the near-Earth and distant populations. These objects typically have high eccentricities, and inclinations often more than 90 degrees (retrograde orbits), a criterion that is common among the members of the
damocloid Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-type or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet, but without showing a cometary coma or tail. David Jewi ...
population. Object in this list have a TJupiter of less than 3 and a
perihelion An apsis (; ) is the farthest or nearest point in the orbit of a planetary body about its primary body. The line of apsides (also called apse line, or major axis of the orbit) is the line connecting the two extreme values. Apsides perta ...
between 1.67 and 5.5  AU, that is, they do not cross the orbit of Mars but cross or at least come close to Jupiter's orbit at 5.2 AU. According to the SSBN07 classification, such objects have cometary dynamics. , the list contains 211 objects, most of which remain unnumbered. A bold designation links to an object's stand-alone article.


Characteristics

*
Extinct comet An extinct comet is a comet that has expelled most of its volatile ice and has little left to form a tail and coma. In a dormant comet, rather than being depleted, any remaining volatile components have been sealed beneath an inactive surface la ...
, are considered unusual minor planets in having the orbital characteristics of a
long period Long may refer to: Measurement * Long, characteristic of something of great duration * Long, characteristic of something of great length * Longitude (abbreviation: long.), a geographic coordinate * Longa (music), note value in early music mens ...
, Jupiter-family or
Halley-type comet A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or Coma (cometary), coma surrounding ...
but showing no sign of cometary activity. *
Damocloid Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-type or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet, but without showing a cometary coma or tail. David Jewi ...
, with typically highly inclined orbits, often being retrograde.


Examples

* (TNO, LPC) * (CEN, HTC) * (NEO) * (CEN)


See also

*
Distant minor planet A distant minor planet, or ''distant object'', is any minor planet found beyond Jupiter in the outer Solar System that is not commonly thought of as an "asteroid". The umbrella term is used by IAU's Minor Planet Center (MPC), which is responsib ...


References

{{Reflist, refs= {{cite web , title = Unusual Minor Planets , work = Minor Planet Center , url = https://www.minorplanetcenter.net/iau/Unusual.html , access-date = 14 November 2018 {{cite web , title = List Of Other Unusual Objects , work = Minor Planet Center , url = https://www.minorplanetcenter.net/iau/lists/t_others.html , access-date= 19 August 2021 {{Cite journal , display-authors = 6 , first1 = John K. , last1 = Davies , first2 = David J. , last2 = Tholen , first3 = Robert J. , last3 = Whiteley , first4 = Simon F. , last4 = Green , first5 = Jon K. , last5 = Hillier , first6 = Michael J. , last6 = Foster , first7 = Neil , last7 = McBride , first8 = Tom. H. , last8 = Kerr , first9 = Erica , last9 = Muzzerall , date = March 2001 , title = The Lightcurve and Colors of Unusual Minor Planet 1998 WU 24 , journal = Icarus , volume = 150 , issue = 1 , pages = 69–77 , bibcode = 2001Icar..150...69D , doi = 10.1006/icar.2000.6554 {{Cite journal , first1 = Yanga R. , last1 = Fernández , first2 = David C. , last2 = Jewitt , first3 = Scott S. , last3 = Sheppard , date = July 2005 , title = Albedos of Asteroids in Comet-Like Orbits , journal = The Astronomical Journal , volume = 130 , issue = 1 , pages = 308–318 , bibcode = 2005AJ....130..308F , doi = 10.1086/430802 , citeseerx = 10.1.1.507.2206 {{cite journal , last1 = Gladman , first1 = B. , last2 = Marsden , first2 = B. G. , last3 = Vanlaerhoven , first3 = C. , title = Nomenclature in the Outer Solar System , journal = The Solar System Beyond Neptune , page = 43 , date = 2008 , url = https://www.lpi.usra.edu/books/ssbn2008/7002.pdf , bibcode = 2008ssbn.book...43G


External links


MPC data page


1996 PW, JPL, August 1996
The lightcurve and colors of unusual minor planet 1996 PW


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