Ceres

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Ceres

The Columbia Encyclopedia, Sixth Edition | 2008 | The Columbia Encyclopedia, Sixth Edition. Copyright 2008 Columbia University Press. (Hide copyright information) Copyright

Ceres , in astronomy, a dwarf planet, the first asteroid to be discovered. It was found on Jan. 1, 1801, by G. Piazzi . He took three distinct observations; on the basis of these the mathematician Gauss calculated Ceres' orbit with such accuracy that it was found one year later within 0.5° of the predicted position. Ceres is the largest and most massive of the asteroids; it has a diameter of c.590 mi (949 km) and a mass 1/100,000 that of the earth. Its orbit has a semimajor axis of 2.78 astronomical units and a period of 1,681 days. From its discovery until the 1850s, when many additional asteroids began to be identified, Ceres was regarded by many astronomers as a planet. In 2006 the reconsideration by astronomers of Pluto 's status as a planet also led to the reclassification of Ceres as a dwarf planet.

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Ceres

A Dictionary of Astronomy | 1997 | © A Dictionary of Astronomy 1997, originally published by Oxford University Press 1997. (Hide copyright information) Copyright

Ceres The first asteroid to be discovered, by G.Piazzi on 1801January1, and hence given the number 1. Ceres is by far the largest asteroid, diameter 940 km, mass 9 × 1020 kg (about 1% the mass of the Moon) and mean density c.2.0 g/cm3. Its rotation period is 9.075 hours. Ceres contains roughly one-third the mass of the entire asteroid belt. It is a member of the new class of dwarf planets, along with Eris and Pluto. Its mean magnitude at opposition is 7.4; only Vesta can ever become brighter. Its orbit has a semimajor axis of 2.767 AU, period 4.60 years, perihelion 2.55 AU, aphelion 2.98 AU, and inclination 10°.6. Ceres is of G class, with a reflectance spectrum that implies a composition resembling the carbonaceous chondrite meteorites. Ceres is the largest member of a small family of asteroids with a mean distance of 2.76–2.80 AU from the Sun and orbital inclinations of 9–11°. Other Ceres family members include (39) Laetitia, (264) Libussa, (374) Burgundia (all S-class), and (446) Aeternitas (A-class).

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Ceres

A Dictionary of Earth Sciences | 1999 | | © A Dictionary of Earth Sciences 1999, originally published by Oxford University Press 1999. (Hide copyright information) Copyright

Ceres The largest solar system asteroid (No. 1), diameter 974 km, approximate mass 1021 kg; rotation period 9.078 hours; orbital period 4.6 years. It was discovered in 1801 by G. Piazzi. It accounts for almost half the total estimated mass of all the asteroids.

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AILSA ALLABY and MICHAEL ALLABY. "Ceres." A Dictionary of Earth Sciences. 1999. Encyclopedia.com. 5 Dec. 2009 <http://www.encyclopedia.com>.

AILSA ALLABY and MICHAEL ALLABY. "Ceres." A Dictionary of Earth Sciences. 1999. Encyclopedia.com. (December 5, 2009). http://www.encyclopedia.com/doc/1O13-Ceres.html

AILSA ALLABY and MICHAEL ALLABY. "Ceres." A Dictionary of Earth Sciences. 1999. Retrieved December 05, 2009 from Encyclopedia.com: http://www.encyclopedia.com/doc/1O13-Ceres.html

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