| Revision as of 18:48, 12 January 2025 editMblock150 (talk | contribs)54 edits ←Created page with ''''Hyperion''' is a hypothetical trans-Neptunian planet proposed in 2000 to explain certain features of the Kuiper belt's structure. Researchers Collander-Brown, Maran, and Williams suggested that a large, distant tenth planet could have influenced the formation and current distribution of Kuiper Belt Objects (KBOs).<ref name=":0">{{Cite journal |last=Collander-Brown |first=S. |last...'Tag: Visual edit | Latest revision as of 20:14, 12 January 2025 edit undoChaotic Enby (talk | contribs)Autopatrolled, Extended confirmed users, Page movers, New page reviewers, Pending changes reviewers, Rollbackers30,561 edits Added {{Notability}} tagTag: Twinkle | ||
| (One intermediate revision by one other user not shown) | |||
| Line 1: | Line 1: | ||
| {{Notability|date=January 2025}} | |||
| '''Hyperion''' is a hypothetical ] proposed in 2000 to explain certain features of the ] structure. Researchers Collander-Brown, Maran, and Williams suggested that a large, distant tenth ] could have influenced the formation and current distribution of ] (KBOs).<ref name=":0">{{Cite journal |last=Collander-Brown |first=S. |last2=Maran |first2=M. |last3=Williams |first3=I. P. |date=2000-10-11 |title=The effect on the Edgeworth-Kuiper Belt of a large distant tenth planet |url=https://academic.oup.com/mnras/article/318/1/101/1141308?login=false |journal=Monthly Notices of the Royal Astronomical Society |volume=318 |issue=1 |pages=101–108 |doi=10.1046/j.1365-8711.2000.03640.x |issn=0035-8711}}</ref> | '''Hyperion''' is a hypothetical ] proposed in 2000 to explain certain features of the ] structure. Researchers Collander-Brown, Maran, and Williams suggested that a large, distant tenth ] could have influenced the formation and current distribution of ] (KBOs).<ref name=":0">{{Cite journal |last=Collander-Brown |first=S. |last2=Maran |first2=M. |last3=Williams |first3=I. P. |date=2000-10-11 |title=The effect on the Edgeworth-Kuiper Belt of a large distant tenth planet |url=https://academic.oup.com/mnras/article/318/1/101/1141308?login=false |journal=Monthly Notices of the Royal Astronomical Society |volume=318 |issue=1 |pages=101–108 |doi=10.1046/j.1365-8711.2000.03640.x |issn=0035-8711}}</ref> | ||
| Line 6: | Line 7: | ||
| == References == | == References == | ||
| <references /> | <references />{{Solar System}} | ||
| ] | |||
| ] | |||
| ] | |||
| ] | |||
Latest revision as of 20:14, 12 January 2025
 | The topic of this article may not meet Misplaced Pages's general notability guideline. Please help to demonstrate the notability of the topic by citing reliable secondary sources that are independent of the topic and provide significant coverage of it beyond a mere trivial mention. If notability cannot be shown, the article is likely to be merged, redirected, or deleted. Find sources: "Hyperion" hypothetical planet – news · newspapers · books · scholar · JSTOR (January 2025) (Learn how and when to remove this message) |
Hyperion is a hypothetical trans-Neptunian planet proposed in 2000 to explain certain features of the Kuiper belt's structure. Researchers Collander-Brown, Maran, and Williams suggested that a large, distant tenth planet could have influenced the formation and current distribution of Kuiper Belt Objects (KBOs).
The Kuiper belt, a region of the Solar System beyond Neptune, contains numerous small icy bodies. Its structure, including the sudden drop-off in the number of objects beyond 48 AU—known as the "Kuiper cliff"—has puzzled astronomers. The existence of a planet-sized object beyond Neptune was proposed to account for these observations.
Simulations indicated that a Mars-sized object in a circular orbit at 60 AU would lead to a trans-Neptunian object population incompatible with observations, such as a severe depletion of the plutino population. However, an Earth-sized object located farther than 100 AU with an eccentric and inclined orbit could explain the Kuiper cliff and peculiar detached objects like Sedna.
References
- ^ Collander-Brown, S.; Maran, M.; Williams, I. P. (2000-10-11). "The effect on the Edgeworth-Kuiper Belt of a large distant tenth planet". Monthly Notices of the Royal Astronomical Society. 318 (1): 101–108. doi:10.1046/j.1365-8711.2000.03640.x. ISSN 0035-8711.
- ^ Editor, Hannah Osborne Science (2017-06-23). "A Mars-Sized Planet at the Edge of the Solar System?". Newsweek. Retrieved 2025-01-12.
{{cite web}}:|last=has generic name (help)
