User:Rfassbind/Unusual asteroid

In Planetary science, the term unusual object is used for a minor planet that possesses an unusual physical or orbital characteristic. For the Minor Planet Center (MPC), which operates under the auspices of the International Astronomical Union, any non-classical main-belt asteroid, which account for the vast majority of all minor planets, is an unusual minor planet. These include the near-Earth objects and Trojans as well as the distant minor planets such as centaurs and trans-Neptunian objects.[1]

Other unusual objects

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The MPC also lists a group of other unusual minor planets, which orbital characteristics do not fit those of the near-Earth and distant populations. There 801 of these objects in total, of which 84 are numbered, including 12 named objects:[2]

History

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During the 1930s, two astronomers set up in competition to see who could discover the most unusual asteroid. Those in the main belt usually have more or less circular orbits. However, if the orbit becomes smaller and more elliptical, then asteroids can draw close to - or even collide with - the inner planets. Eugene Delporte, in Belgium, made the first discovery in March 1932 when he discovered asteroid 1221 Amor. This space rock spends over half its orbit outside the main belt and actually crosses Mars's orbit. It comes close to Earth's orbit before heading back out again. The very next month, Karl Reinmuth, in Heidelberg, discovered 1862 Apollo. This asteroid spends much less time in the main belt, spending most of its time inside Mars's orbit. In fact, Apollo crosses the Earth's orbit too.

Characteristics

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Items:

References

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  1. ^ "Unusual Minor Planets". Minor Planet Center. Retrieved 14 November 2018.
  2. ^ "List Of Other Unusual Objects". Minor Planet Center. Retrieved 14 November 2018.
  3. ^ Davies, John K.; Tholen, David J.; Whiteley, Robert J.; Green, Simon F.; Hillier, Jon K.; Foster, Michael J.; et al. (March 2001). "The Lightcurve and Colors of Unusual Minor Planet 1998 WU 24". Icarus. 150 (1): 69–77. Bibcode:2001Icar..150...69D. doi:10.1006/icar.2000.6554. Retrieved 15 November 2018.

Notes

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