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Quaoar

This article is about the trans-Neptunian object. For the Tongva god, see Quaoar (deity).


Quaoar
Quaoar.jpg
Image by G. Bacon of STScI - NASA
Orbital characteristics
Orbit type Kuiper belt
Semimajor axis 43.37 AU
Eccentricity 0.03746
Orbital period 288 Years
Inclination 7.99°
Physical characteristics
Diameter 1280 km
Albedo 0.1
History
Discoverer C. Trujillo & M. Brown, 2002

50000 Quaoar ("kwah-oh-ahr", /kwA o Ar/) is a Trans-Neptunian object circling the Sun in the Kuiper belt. It was discovered on June 4, 2002 by astronomers Chad Trujillo and Mike Brown at the California Institute of Technology in Pasadena, California in images acquired from Palomar Observatory using the JPL Near Earth Asteroid Tracking program.

Quaoar is estimated to have a diameter of about 1,280 kilometres, which would make it the largest Solar System object discovered since Pluto and, indeed, the largest known minor planet. Larger than all the asteroids put together, it is about one tenth the diameter of Earth or one third the diameter of the Moon. It orbits at about 6 billion kilometres from the Sun with an orbital period of 288 years.

The planetoid's name follows International Astronomical Union rules by naming all planetoids after creation deities (see planetary nomenclature). "Quaoar" is the name of a creation deity of the Native American Tongva people, native to the area around Los Angeles, where the discovery was named. The IAU approved the name Quaoar, making it the official name; it also has the systematic name "2002 LM60" and the minor planet number 50000.

The discovery weakens Pluto's case to be counted as a planet, since astronomers expect that there may be as many as a dozen Kuiper Belt objects the size of Quaoar. Some expect to find other planetoids there as large or larger than Pluto. In some ways, Quaoar has more claim to be a planet than Pluto does: it has a more planetary orbit (a near-circular orbit with a radius of somewhat over 40 AU rather than a highly eccentric one like Pluto) and doesn't belong to a binary system with mass ratio more akin to a binary asteroid, of which many are known.

Quaoar belongs to the Kuiper belt, a class of comet like icy objects orbitting beyond Neptune, pristine remnants from the solar nebula with much knowledge to yield. It is believed to be a mixture of rock and ice, like the other Kuiper Belt objects; however its extremely low albedo (estimated at 0.1) indicates that the ice has disappeared from its outer layers. Until the Pluto Express or a similar mission is approved, our knowledge of these worlds will remain vague.

External links

Referenced By

1000km | 1 Ceres | 1 E6 m | 1 E9 s | 1e6 m | 1e6 metres | 1e9 s | 2002 | 2002 in science | As of 2002 | Asteroid Ceres | Ceres (asteroid) | Kuiper Belt | Kuiper Belt Object | List of astronomical topics | List of astronomical topics (N-Z) | October 2002 | Planet Pluto | Pluto (planet) | Quaoar (deity) | The Pluto debate | Tongva | Trans-Neptunian Object | Trans-Neptunian objects

 

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Quaoar
savannah - May 3rd, 2006
I think that Quaoar is a planet not a kuiper belt object. Why do they say it's found in 1932 and seen and just start talking about it in2002?
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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Quaoar".

 

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