Talk:Kepler-11c
Kepler-11c has been listed as one of the Natural sciences good articles under the good article criteria. If you can improve it further, please do so. If it no longer meets these criteria, you can reassess it. | |||||||||||||
Kepler-11c is part of the Kepler-11 series, a good topic. This is identified as among the best series of articles produced by the Wikipedia community. If you can update or improve it, please do so. | |||||||||||||
| |||||||||||||
A fact from this article appeared on Wikipedia's Main Page in the "Did you know?" column on March 31, 2011. The text of the entry was: Did you know ... that the orbits of exoplanets Kepler-11b, Kepler-11c, Kepler-11d, Kepler-11e, and Kepler-11f (artist's depiction pictured) can fit within the orbit of Mercury? | |||||||||||||
Current status: Good article |
This article is rated GA-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | |||||||||||
|
GA Review
editGA toolbox |
---|
Reviewing |
- This review is transcluded from Talk:Kepler-11c/GA1. The edit link for this section can be used to add comments to the review.
Reviewer: Nergaal (talk) 22:45, 24 March 2011 (UTC)
- " and is most likely a water planet with a thin hydrogen-helium atmosphere" needs a citation
- "its five sister planets formed the first discovered system with more than three planets." same issue as the b one; not accurate
- "being the most compact and the flattest system yet discovered." sounds quite subjective. Who said it?
- I agree (on flatness), unless sourced. The relative inclinations of the orbits are not known to my knowledge. Tom Ruen (talk) 01:24, 26 March 2011 (UTC)
- "In other words, Kepler-11 has the fullest, most compact planetary system yet discovered beyond our own. " It came from this source, which was listed as reference four. --Starstriker7(Talk) 14:42, 26 March 2011 (UTC)
- Ok, but please specify that "in NASA's view" it is the most compact, etc. People outside NASA could disagree. Nergaal (talk) 01:25, 28 March 2011 (UTC)
- "In other words, Kepler-11 has the fullest, most compact planetary system yet discovered beyond our own. " It came from this source, which was listed as reference four. --Starstriker7(Talk) 14:42, 26 March 2011 (UTC)
- I agree (on flatness), unless sourced. The relative inclinations of the orbits are not known to my knowledge. Tom Ruen (talk) 01:24, 26 March 2011 (UTC)
- "The Kepler-11 system is the first known to host more than three planets" see above
- "Follow-up observations were conducted by facilities in California, Arizona, Hawaii, Texas and the Canary Islands." please expand
- why is "Host star" so different from the b one? "With an apparent magnitude of 14.2, Kepler-11 cannot be seen from Earth with the naked eye" is this notable here and not in teh b one?
- Done Section added to Kepler-11b as well. --Starstriker7(Talk) 01:12, 26 March 2011 (UTC)
- "a mass of 13.5 ME and a radius or 3.15 RE" same as for b. please add certainty intervals to be rigurous and not misleading
- "grams/cc" is not a common scientific notation
- "over 3.27 times hotter than the equivalent measurement for Earth" not necessary to have 3 sig figs here. and just say over three times than the average temperature on earth
- "he inclination of Kepler-11c is 89º, and is thus almost edge-on as seen from Earth" super interesting: how was the inclidnation determined for something so far away?
also say that this is similar to Uranus- This is a misunderstanding. It's the orbit that is inclided 89 degrees from the earth's direction of view, nothing to do with the rotational axis, which is unknown. This inclination fact exists because ONLY such planetary systems can be observed by the transit method used. Tom Ruen (talk) 01:21, 26 March 2011 (UTC)
- For clarity say "orbit's inclination" Nergaal (talk) 01:25, 28 March 2011 (UTC)
- This is a misunderstanding. It's the orbit that is inclided 89 degrees from the earth's direction of view, nothing to do with the rotational axis, which is unknown. This inclination fact exists because ONLY such planetary systems can be observed by the transit method used. Tom Ruen (talk) 01:21, 26 March 2011 (UTC)
- How does the density compare to the gas giants in the Solar System?
- again, add an comparative sizes image for the system
Nergaal (talk) 22:52, 24 March 2011 (UTC)
- I'll pass this, but please fix the two issues I replied to. Nergaal (talk) 01:25, 28 March 2011 (UTC)
External links modified
editHello fellow Wikipedians,
I have just modified 2 external links on Kepler-11c. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:
- Added archive https://web.archive.org/web/20110207020029/http://exoplanet.eu/star.php?st=Kepler-11 to http://exoplanet.eu/star.php?st=Kepler-11
- Added archive https://web.archive.org/web/20101205010229/http://zebu.uoregon.edu/ph121/l5.html to http://zebu.uoregon.edu/ph121/l5.html
When you have finished reviewing my changes, you may follow the instructions on the template below to fix any issues with the URLs.
This message was posted before February 2018. After February 2018, "External links modified" talk page sections are no longer generated or monitored by InternetArchiveBot. No special action is required regarding these talk page notices, other than regular verification using the archive tool instructions below. Editors have permission to delete these "External links modified" talk page sections if they want to de-clutter talk pages, but see the RfC before doing mass systematic removals. This message is updated dynamically through the template {{source check}}
(last update: 5 June 2024).
- If you have discovered URLs which were erroneously considered dead by the bot, you can report them with this tool.
- If you found an error with any archives or the URLs themselves, you can fix them with this tool.
Cheers.—InternetArchiveBot (Report bug) 16:24, 4 May 2017 (UTC)