Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Planets beyond Neptune
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Probability=== Even without gravitational evidence, Mike Brown, the discoverer of Sedna, has argued that Sedna's 12,000-year orbit means that probability alone suggests that an Earth-sized object exists beyond Neptune. Sedna's orbit is so eccentric that it spends only a small fraction of its orbital period near the Sun, where it can be easily observed. This means that unless its discovery was a freak accident, there is probably a substantial population of objects roughly Sedna's diameter yet to be observed in its orbital region.<ref name="Mike" /> Mike Brown noted that {{blockquote|Sedna is about three-quarters the size of Pluto. If there are sixty objects three-quarters the size of Pluto [out there] then there are probably forty objects the size of Pluto ... If there are forty objects the size of Pluto, then there are probably ten that are twice the size of Pluto. There are probably three or four that are three times the size of Pluto, and the biggest of these objects ... is probably the size of Mars or the size of the Earth.<ref name="wgbh">{{Cite web |last=Brown |first=Michael |date=11 April 2007 |title=Pluto and the outer solar system |url=http://forum.wgbh.org/wgbh/forum.php?lecture_id=3710 |url-status=dead |archive-url=https://web.archive.org/web/20080103202810/http://forum.wgbh.org/wgbh/forum.php?lecture_id=3710 |archive-date=2008-01-03 |access-date=2008-07-13 |series=Lowell Lectures in Astronomy |publisher=Museum of Science, Boston / WGBH |place=Boston, MA}}</ref><ref>{{cite AV media |first=Mike |last=Brown |date=August 2008 |title=Pluto, Eris, and the dwarf planets of the outer solar system |type=academic talk |publisher=Smithsonian |time=50α΅ |url=https://www.youtube.com/watch?v=WHNO079G1i8&t=3135 |url-status=live |access-date=2 January 2019 |archive-url=https://ghostarchive.org/varchive/youtube/20211114/WHNO079G1i8 |archive-date=2021-11-14 |via=[[YouTube]]}}{{cbignore}} The argument about dwarf planet sizes beyond Neptune is 50α΅ into his talk. The WGBH link doesn't work; view on YouTube.</ref><ref>{{cite web |title=Planet 10? Another Earth-size world may lurk in the outer solar system |date=22 June 2017 |website=[[Space.com]] |url=https://www.space.com/37295-possible-planet-10.html}}</ref>}} However, Brown notes that even though it might approach or exceed Earth in size, should such an object be found it would still be a "dwarf planet" by the current definition, because it would not have cleared its neighbourhood sufficiently.<ref name=wgbh/>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Planets beyond Neptune
(section)
Add topic