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The name J1407b follows the exoplanet naming convention by adding the letter "b" after the host star's name. [5] At the time of J1407b's discovery, V1400 Centauri was known as "J1407", which is the shortened form of the star's full SuperWASP catalogue designation 1SWASP J140747.93–394542.6.
V1400 Centauri, also known as 1SWASP J140747.93−394542.6 or simply J1407, is a young, pre-main-sequence star that was eclipsed by the likely free-floating substellar object J1407b in April–June 2007.
Later studies have since found that J1407b is most likely a free-floating sub-brown dwarf or rogue planet, possibly less than 6 Jupiter masses. [2] 2012 — The confirmed hot Jupiter planet WASP-12b may also possess a moon. [3]
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a (images are tagged and non-free content have non-free use rationales): b (appropriate use with suitable captions): The biggest issue I have right now are the placements and amount of images. I am currently on a Microsoft Edge browser, so it may just look different to me, but the "double images" interfere with the layout of the article.
The following is an archived discussion of the DYK nomination of the article below. Please do not modify this page. Subsequent comments should be made on the appropriate discussion page (such as this nomination's talk page, the article's talk page or Wikipedia talk:Did you know), unless there is consensus to re-open the discussion at this page.
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J1407b is currently a Physics and astronomy good article nominee. Nominated by Nrco0e (talk • contribs) at 02:31, 29 July 2024 (UTC). Any editor who has not nominated or contributed significantly to this article may review it according to the good article criteria to decide whether or not to list it as a good article.