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* Know anyone interested in [[Andromeda (constellation)]]? – [[User:Ling.Nut3|Ling.Nut3]] ([[User talk:Ling.Nut3|talk]]) 05:38, 24 May 2012 (UTC)
* Know anyone interested in [[Andromeda (constellation)]]? – [[User:Ling.Nut3|Ling.Nut3]] ([[User talk:Ling.Nut3|talk]]) 05:38, 24 May 2012 (UTC)

== Uranus image ==

== Possibly unfree File:File_name.ext ==
A file that you uploaded or altered, [[:File:File_name.ext]], has been listed at [[Wikipedia:Possibly unfree files]] because its copyright status is unclear or disputed. If the file's copyright status cannot be verified, it may be deleted. You may find more information on the [[:File:File_name.ext|file description page]]. You are welcome to add comments to its entry at [[Wikipedia:Possibly unfree files/2012 June 26#File:File_name.ext|the discussion]] if you are interested in it not being deleted. Thank you. <!-- Template:Fdw-puf --> --[[User:Steuard|Steuard]] ([[User talk:Steuard|talk]]) 03:28, 26 June 2012 (UTC)

Revision as of 03:28, 26 June 2012

Main page appearance: Kuiper belt

This is a note to let the main editors of Kuiper belt know that the article will be appearing as today's featured article on May 27, 2012. You can view the TFA blurb at Wikipedia:Today's featured article/May 27, 2012. If you prefer that the article appear as TFA on a different date, or not at all, please ask featured article director Raul654 (talk · contribs) or his delegate Dabomb87 (talk · contribs), or start a discussion at Wikipedia talk:Today's featured article/requests. If the previous blurb needs tweaking, you might change it—following the instructions at Wikipedia:Today's featured article/requests/instructions. If this article needs any attention or maintenance, it would be preferable if that could be done before its appearance on the Main Page. The blurb as it stands now is below:

Known objects in the Kuiper belt

The Kuiper belt is a region of the Solar System beyond the planets extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun. It is similar to the asteroid belt, although it is far larger—20 times as wide and 20 to 200 times as massive. It consists mainly of small bodies, or remnants from the Solar System's formation. While the asteroid belt is composed primarily of rock, ices, and metal, the Kuiper objects are composed largely of frozen volatiles, such as methane, ammonia and water. The classical (low-eccentricity) belt is home to at least three dwarf planets: Pluto, Haumea, and Makemake. Some of the Solar System's moons, such as Neptune's Triton and Saturn's Phoebe, are also believed to have originated in the region. Since the belt was discovered in 1992, the number of known Kuiper belt objects has increased to over a thousand, and more than 70,000 KBOs over 100 km (62 mi) in diameter are believed to exist. Pluto is the largest known member of the Kuiper belt, if the scattered disc is excluded. In Pluto's honour, the four currently accepted dwarf planets beyond Neptune's orbit are called "plutoids".

UcuchaBot (talk) 23:01, 22 May 2012 (UTC)[reply]

Uranus image

Possibly unfree File:File_name.ext

A file that you uploaded or altered, File:File_name.ext, has been listed at Wikipedia:Possibly unfree files because its copyright status is unclear or disputed. If the file's copyright status cannot be verified, it may be deleted. You may find more information on the file description page. You are welcome to add comments to its entry at the discussion if you are interested in it not being deleted. Thank you. --Steuard (talk) 03:28, 26 June 2012 (UTC)[reply]