Difference between revisions of "Dwarf Planet"
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In 2006, the International Astronomical Union settled the issue. They determined that Eris was not a planet, and neither was Pluto. But the criteria they set also provoked yet another reassessment of the status of [[Ceres]], the largest and first-discovered object in the [[asteroid]] belt. Upon consideration, the IAU declared that Ceres was a dwarf planet as well. | In 2006, the International Astronomical Union settled the issue. They determined that Eris was not a planet, and neither was Pluto. But the criteria they set also provoked yet another reassessment of the status of [[Ceres]], the largest and first-discovered object in the [[asteroid]] belt. Upon consideration, the IAU declared that Ceres was a dwarf planet as well. | ||
| − | Today the list of dwarf planets is limited to these | + | Today the list of dwarf planets is limited to these five: Ceres, Pluto, Haumea, Makemake and Eris. |
== Table == | == Table == | ||
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| 0.218% earth | | 0.218% earth | ||
| -6.387 da | | -6.387 da | ||
| + | |- | ||
| + | | [[Haumea]] | ||
| + | | 29.66 AU | ||
| + | | 35.164 AU | ||
| + | | 0.18874 | ||
| + | | | ||
| + | | 28.19° | ||
| + | | 4.2 ± 0.1)×10<sup>21</sup> kg | ||
| + | | Unknown | ||
| + | |- | ||
| + | | [[Makemake]] | ||
| + | | 38.509 AU | ||
| + | | 53.074 AU | ||
| + | | 0.159 | ||
| + | | 309.88 a | ||
| + | | Unknown | ||
| + | | ~4 × 10<sup>21</sup> kg | ||
| + | | Unknown | ||
|- | |- | ||
| [[Eris]] | | [[Eris]] | ||
| Line 52: | Line 70: | ||
| 0.333 da | | 0.333 da | ||
|} | |} | ||
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| + | ==Plutoids== | ||
| + | |||
| + | The name '''plutoid''' was proposed by the members of the IAU Committee on Small Body Nomenclature (CSBN), to describe celestial bodies "in orbit around the Sun at a semi-major axis greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighborhood around their orbit." <ref>http://solarsystem.nasa.gov/planets/profile.cfm?Object=Dwarf&Display=OverviewLong</ref> | ||
| + | |||
| + | The four known and named plutoids are Pluto, Haumea, Makemake and Eris. | ||
| + | |||
| + | It is important to note that while all plutoids are dwarf planets, not all dwarf planets are plutiods. Ceres, for example, is a dwarf planet, but not a plutoid, as its orbit lies well within that of Neptune. | ||
| + | |||
== References == | == References == | ||
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* [[Pluto]] | * [[Pluto]] | ||
* [[Ceres]] | * [[Ceres]] | ||
| + | * [[Haumea]] | ||
| + | * [[Makemake]] | ||
[[Category:Dwarf planets]] | [[Category:Dwarf planets]] | ||
Revision as of 10:53, September 21, 2008
A dwarf planet is a satellite of the Sun that meets the following criteria now set by the International Astronomical Union:
| “ | (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, (c) has not cleared the neighbourhood around its orbit, and (d)is not a satellite.[1] | ” |
Contents
Eris
- Main Article: Eris
The concept of "dwarf planet" properly dates to the discovery of the scatter-disk object named Eris on January 5, 2005. With the confirmation of the identification of Eris, a formal debate began on the subject of what does, and what does not, constitute a planet. The community of astronomers decided that relying on history and tradition simply would not serve. The eight celestial bodies that now remain under the present definition of planet do not share their orbits with any other objects. The objects now called dwarf planets do not have this distinction. And yet these objects are significantly heavier than mere asteroids, in that they are so heavy that their own weight, and more particularly their own gravity, forces them to assume the round or nearly-round shape that all planets have.
In 2006, the International Astronomical Union settled the issue. They determined that Eris was not a planet, and neither was Pluto. But the criteria they set also provoked yet another reassessment of the status of Ceres, the largest and first-discovered object in the asteroid belt. Upon consideration, the IAU declared that Ceres was a dwarf planet as well.
Today the list of dwarf planets is limited to these five: Ceres, Pluto, Haumea, Makemake and Eris.
Table
List of all known dwarf planets, from the innermost to the outermost:
| Name | Perihelion | Aphelion | Eccentricity | Sidereal year | Inclination | Mass | Sidereal day |
|---|---|---|---|---|---|---|---|
| Ceres | 2.545 AU | 2.987 AU | 0.0798 | 4.599 a | 10.587 ° | 0.0158% earth | 0.378 da |
| Pluto | 29.658 AU | 49.305 AU | 0.249 | 248.09 a | 17.142 ° | 0.218% earth | -6.387 da |
| Haumea | 29.66 AU | 35.164 AU | 0.18874 | 28.19° | 4.2 ± 0.1)×1021 kg | Unknown | |
| Makemake | 38.509 AU | 53.074 AU | 0.159 | 309.88 a | Unknown | ~4 × 1021 kg | Unknown |
| Eris | 37.77 AU | 97.56 AU | 0.442 | 577 a | 44.187 ° | 0.278% earth | 0.333 da |
Plutoids
The name plutoid was proposed by the members of the IAU Committee on Small Body Nomenclature (CSBN), to describe celestial bodies "in orbit around the Sun at a semi-major axis greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighborhood around their orbit." [2]
The four known and named plutoids are Pluto, Haumea, Makemake and Eris.
It is important to note that while all plutoids are dwarf planets, not all dwarf planets are plutiods. Ceres, for example, is a dwarf planet, but not a plutoid, as its orbit lies well within that of Neptune.
References
- ↑ "IAU0602: the Final IAU Resolution on the Definition of 'Planet' Ready for Voting," International Astronomical Union, 2005. Accessed January 14, 2008.
- ↑ http://solarsystem.nasa.gov/planets/profile.cfm?Object=Dwarf&Display=OverviewLong
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