Cis-Neptunian object
A cis-Neptunian object is, literally, any astronomical body found within the orbit of Neptune.[1] However, the term is typically used for those distant minor planets other than trans-Neptunian objects: that is, all sub-planetary bodies orbiting the Sun at or within the distance of Neptune, but outside the orbit of Jupiter. This includes the icy minor planets known as centaurs[2] and the Neptune trojans.[3][lower-alpha 1]
|
Notes
- These are 2001 QR322, 2004 UP10, 2005 TN53, 2005 TO74, 2006 RJ103, 2007 VL305, 2008 LC18, and 2004 KV18.[3]
gollark: Hmm, smelting time.
gollark: !q list <@!258639553357676545>
gollark: !q info <@!258639553357676545>
gollark: !q list
gollark: What can you pay for the clay?
References
- Remo, John L. (2007). "Classifying Solid Planetary Bodies". AIP Conference Proceedings. 886: 284–302. doi:10.1063/1.2710063.
- J Horner; NW Evans; ME Bailey; DJ Asher (2003). "The Populations of Comet-like Bodies in the Solar System" (PDF). Archived from the original (PDF) on 2013-06-01. Retrieved 2007-06-29.
- "List Of Neptune Trojans". Minor Planet Center. Archived from the original on 2012-05-25. Retrieved 2010-10-27.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.