50000 Quaoar (pronounced kwaa'·waar or kwow'·ər, Tongva ) * is a Trans-Neptunian object orbiting the Sun in the Edgeworth-Kuiper belt. It was discovered on June 4, 2002 by astronomers Chad Trujillo and Michael Brown at the California Institute of Technology in Pasadena, California from images acquired at the Samuel Oschin Telescope at Palomar Observatory. This discovery was announced on October 7, 2002, at a meeting of the American Astronomical Society. The earliest precovery turned out to be a May 25, 1954 plate from Palomar Observatory.
Quaoar was the first trans-Neptunian object to be measured directly from Hubble Space Telescope images, using a new sophisticated method (see Brown’s pages for a non-technical description and his paper cited in references for details). Given its distance Quaoar is on the limit of the HST resolution (40 milliarcseconds) and its image is consequently smeared on a few adjacent pixels. By comparing carefully this image with the images of stars in the background and using a sophisticated model of HST optics (PSF), Brown and Troujillo were able to find the best fit disk's size which would give a similar blurred image. This method was recently applied by the same authors to measure the size of the biggest TNO so far: .
Quaoar's volume is somewhat more than all of the asteroids put together, it is about one tenth the diameter of Earth, one third the diameter of the Moon or about half the size of Pluto. It orbits at about 6 thousand million kilometres from the Sun with an orbital period of 287 years.
The planetoid's name is not to be confused with Qo'noS, the fictitious homeworld of the Klingon Empire in the Star Trek universe.
Quaoar is classified as a classical trans-Neptunian object. Its cold orbit is however unusual for large classical objects that typically follow more eccentric and more inclined orbits (see cubewanos for the comparison and the definition of cold and hot families).
At 43 AU and a near-circular orbit, unlike Pluto which is in 2:3 orbital resonance with Neptune, Quaoar is not significantly perturbed by Neptune.
The ecliptic view illustrates the comparison of Quaoar' near-circular, moderately-inclined orbit with Pluto's highly inclined (~17°), highly eccentric (e=0.25) orbit.
Pluto's aphelion is beyond (and below) Quaoar's orbit, so that Pluto is closer to the Sun than Quaoar at some times of its orbit, and farther at others.
In 2004, scientists were surprised to find signs of crystalline ice on Quaoar, indicating that the temperature rose to at least −160 °C (110 K or −260 °F) sometime in the last ten million years. Speculation began as to what could have caused Quaoar to heat up from its natural temperature of −220 °C (55 K or −360 °F). Some have theorized that a barrage of mini-meteors may have raised the temperature, but the most discussed theory speculates that cryovolcanism may be occurring, spurred by the decay of radioactive elements within Quaoar's core (Jewitt & Luu, 2004).
Since then (2006), crystalline water ice was also found on but present in larger quantities and thought to be responsible for the very high albedo of that object (0.7).
If the New Horizons mission visits several Kuiper Belt Objects after visiting Pluto in 2015, our knowledge of the surfaces of small KBOs should improve but encounters with large objects seem unlikely.
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