This article was nominated for deletion on 2 March 2011 (UTC). The result of the discussion was keep. |
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If one planet appears to hang brightly and permanently in the sky of the other, then surely the same would happen in the opposite sense. Actually, it would only "hang permanently" if the two planets were tidally locked (not impossible), and even then, only from certain regions (about 120deg of longitude) of each planet. If they have rotation, then each planet would remain in approximately the same position in the sky compared to the star. Which is going to be weird enough.
SF authors are going to LOVE this system! Fixed the phrasing of the article.
Can someone else have a go at the final sentence? I've tried to rewrite it but I can't make it scan properly and say what I want... please have a go! Kernalk ( talk) 23:24, 28 February 2011 (UTC)
Why delete? This is the first discovery of a planet sharing the same orbit with another. This is special and a historic event within planetary discovery. If deleted my respect for wikpeida will be diminished.-- Matthurricane ( talk) 03:13, 2 March 2011 (UTC)
If deleted, KOI's with unconfirmed planets may be an appropriate place to move the information present in this article Nstock ( talk) 23:56, 4 March 2011 (UTC)
The current state of the article is contradictory. If two of planets are trojan with each other, then the resonance relationship 8:6:4:3 is impossible, since two of the planets should have the exact same orbital period. 65.95.15.144 ( talk) 21:55, 2 March 2011 (UTC)
I boldy removed the note tags in this edit, replacing them with wikifyed versions, since all the notes did was reference the wiki pages for them. – Ajl talk 22:10, 5 March 2011 (UTC)
Also, I'm considering removing I've removed –
Ajl
talk 22:14, 5 March 2011 (UTC) the TOC, as there's no point in having it on there if this is being classified as a stub if there is no content between the TOC and the sections it links to. –
Ajl
talk
22:10, 5 March 2011 (UTC)
In impetuous boldness, I've removed the one-source banner as now featuring 5 references and many links to other articles it doesn't seem appropriate any more. Please feel free to revert if you feel strongly. Kernalk ( talk) 22:00, 12 March 2011 (UTC)
I can't find this star in SIMBAD; in order to get any results, I had to use a 10arcmin circle around the coordinates from the February release dataset.
65.95.15.144 ( talk) 23:37, 5 March 2011 (UTC)
http://www.ibtimes.com/articles/117984/20110302/kepler-finds-strange-worlds-fastest-planet.htm
Not sure where they got their sources from, but it might be worth including part of it as well? –
Ajl
talk
22:47, 24 March 2011 (UTC)
If you
Google Image Search for KOI-730, there's a lot of the same picture. I'm not 100% sure on the image guidelines, but is it possible to snag one of them and use it in the article? Found
this on NASA's website. Would it be okay to upload a resized version of it? –
Ajl
talk
22:57, 24 March 2011 (UTC)
Regarding: "Fabrycky et al gives the radii as 1.8, 2.1, 2.8, and 2.4 Earth radii with orbital periods of 7.4, 9.8, 14.8, and 19.7 days respectively"
What radii? The planet themselves or their orbits' (semi-major axis or average distance from the star)?
The first source lists 1.8, 2.1, 2.8, and 2.4 and the second 0.31, 0.23, 0.25 and 0.18. Is it the same quantity? Or are one of the sources incorrect?
-- Mortense ( talk) 08:07, 16 September 2011 (UTC)
I found newer information on KOI-730 if someone wants to try to incorporate this into the article. Just reading the summary made my head spin... sorry.
This article was nominated for deletion on 2 March 2011 (UTC). The result of the discussion was keep. |
This article is rated Start-class on Wikipedia's
content assessment scale. It is of interest to the following WikiProjects: | ||||||||||||||
|
It is requested that a map or maps be
included in this article to
improve its quality. Wikipedians in astronomy may be able to help! |
If one planet appears to hang brightly and permanently in the sky of the other, then surely the same would happen in the opposite sense. Actually, it would only "hang permanently" if the two planets were tidally locked (not impossible), and even then, only from certain regions (about 120deg of longitude) of each planet. If they have rotation, then each planet would remain in approximately the same position in the sky compared to the star. Which is going to be weird enough.
SF authors are going to LOVE this system! Fixed the phrasing of the article.
Can someone else have a go at the final sentence? I've tried to rewrite it but I can't make it scan properly and say what I want... please have a go! Kernalk ( talk) 23:24, 28 February 2011 (UTC)
Why delete? This is the first discovery of a planet sharing the same orbit with another. This is special and a historic event within planetary discovery. If deleted my respect for wikpeida will be diminished.-- Matthurricane ( talk) 03:13, 2 March 2011 (UTC)
If deleted, KOI's with unconfirmed planets may be an appropriate place to move the information present in this article Nstock ( talk) 23:56, 4 March 2011 (UTC)
The current state of the article is contradictory. If two of planets are trojan with each other, then the resonance relationship 8:6:4:3 is impossible, since two of the planets should have the exact same orbital period. 65.95.15.144 ( talk) 21:55, 2 March 2011 (UTC)
I boldy removed the note tags in this edit, replacing them with wikifyed versions, since all the notes did was reference the wiki pages for them. – Ajl talk 22:10, 5 March 2011 (UTC)
Also, I'm considering removing I've removed –
Ajl
talk 22:14, 5 March 2011 (UTC) the TOC, as there's no point in having it on there if this is being classified as a stub if there is no content between the TOC and the sections it links to. –
Ajl
talk
22:10, 5 March 2011 (UTC)
In impetuous boldness, I've removed the one-source banner as now featuring 5 references and many links to other articles it doesn't seem appropriate any more. Please feel free to revert if you feel strongly. Kernalk ( talk) 22:00, 12 March 2011 (UTC)
I can't find this star in SIMBAD; in order to get any results, I had to use a 10arcmin circle around the coordinates from the February release dataset.
65.95.15.144 ( talk) 23:37, 5 March 2011 (UTC)
http://www.ibtimes.com/articles/117984/20110302/kepler-finds-strange-worlds-fastest-planet.htm
Not sure where they got their sources from, but it might be worth including part of it as well? –
Ajl
talk
22:47, 24 March 2011 (UTC)
If you
Google Image Search for KOI-730, there's a lot of the same picture. I'm not 100% sure on the image guidelines, but is it possible to snag one of them and use it in the article? Found
this on NASA's website. Would it be okay to upload a resized version of it? –
Ajl
talk
22:57, 24 March 2011 (UTC)
Regarding: "Fabrycky et al gives the radii as 1.8, 2.1, 2.8, and 2.4 Earth radii with orbital periods of 7.4, 9.8, 14.8, and 19.7 days respectively"
What radii? The planet themselves or their orbits' (semi-major axis or average distance from the star)?
The first source lists 1.8, 2.1, 2.8, and 2.4 and the second 0.31, 0.23, 0.25 and 0.18. Is it the same quantity? Or are one of the sources incorrect?
-- Mortense ( talk) 08:07, 16 September 2011 (UTC)
I found newer information on KOI-730 if someone wants to try to incorporate this into the article. Just reading the summary made my head spin... sorry.