Ceres (dwarf planet): Difference between revisions
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'''Ceres''' is a [[dwarf planet]] situated in the [[asteroid belt]]. It was classified as a dwarf planet, along with [[Pluto]] in the [[Kuiper belt]] and [[Eris]] in the [[scattered disc]], when this new category was created by the [[International Astronomical Union|IAU]] in [[2006]]. Ceres was discovered by [[Piazzi]] in the first days of the [[19th century]]. Originally, Piazzi thought that he had discovered a new [[comet]]. Only after Carl Friedrich [[Gauß]] calculated the course of the object did they find out that it was somewhere between the orbit of [[Mars]] and [[Jupiter]]. These calculations enabled [[Franz Xaver von Zach|Zach]] to find Ceres again on 11th February 1801. It was originally classified as a [[planet]], albeit a strangely small one; but after the discovery of [[Pallas|2 Pallas]], [[Juno|3 Juno]], [[Vesta|4 Vesta]] and other small bodies with nearby orbits, it was reclassified as the largest [[asteroid]], '1 Ceres', and some still refer to it as such. | '''Ceres''' is a [[dwarf planet]] situated in the [[asteroid belt]]. It was classified as a dwarf planet, along with [[Pluto]] in the [[Kuiper belt]] and [[Eris]] in the [[scattered disc]], when this new category was created by the [[International Astronomical Union|IAU]] in [[2006]]. Ceres was discovered by [[Piazzi]] in the first days of the [[19th century]]. Originally, on [[1 January]] [[1901]], Piazzi thought that he had discovered a new [[comet]]. Only after Carl Friedrich [[Gauß]] calculated the course of the object did they find out that it was somewhere between the orbit of [[Mars]] and [[Jupiter]]. These calculations enabled [[Franz Xaver von Zach|Zach]] to find Ceres again on 11th February 1801. It was originally classified as a [[planet]], albeit a strangely small one; but after the discovery of [[Pallas|2 Pallas]], [[Juno|3 Juno]], [[Vesta|4 Vesta]] and other small bodies with nearby orbits, it was reclassified as the largest [[asteroid]], '1 Ceres', and some still refer to it as such. | ||
Revision as of 15:13, 23 October 2007
| Epoch: | 2007 Apr 10.0 |
|---|---|
| M | 215.80100 |
| n: | 0.21425752 |
| a: | 2.7659565 |
| e: | 0.0797602 |
| P: | 4.60 |
| Perihelion: | 73.15069 |
| Node: | 80.40696 |
| Inclination: | 10.58671 |
| H: | 3.34 |
| G: | 0.12
|
| M | Mean anomaly at the epoch. |
| n | Mean daily motion (in degrees/day). |
| a | Semimajor axis (in AU). |
| e | Orbital eccentricity. |
| P | Orbital period (in years). |
| Perihelion | The J2000.0 argument of perihelion (in degrees). |
| Node | The J2000.0 longitude of the ascending node (in degrees). |
| Inclination | The J2000.0 inclination (in degrees). |
| H | Absolute visual magnitude. |
| G | Slope parameter. For an explanation of the H,G magnitude system refer to Application of Photometric Models to Asteroids, Bowell et al., in Asteroids II, 524-556 (published by the University of Arizona Press, ISBN 0-8165-1123-3) and the references therein. |
Ceres is a dwarf planet situated in the asteroid belt. It was classified as a dwarf planet, along with Pluto in the Kuiper belt and Eris in the scattered disc, when this new category was created by the IAU in 2006. Ceres was discovered by Piazzi in the first days of the 19th century. Originally, on 1 January 1901, Piazzi thought that he had discovered a new comet. Only after Carl Friedrich Gauß calculated the course of the object did they find out that it was somewhere between the orbit of Mars and Jupiter. These calculations enabled Zach to find Ceres again on 11th February 1801. It was originally classified as a planet, albeit a strangely small one; but after the discovery of 2 Pallas, 3 Juno, 4 Vesta and other small bodies with nearby orbits, it was reclassified as the largest asteroid, '1 Ceres', and some still refer to it as such.