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  2. J1407b - Wikipedia

    en.wikipedia.org/wiki/J1407b

    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.

  3. V1400 Centauri - Wikipedia

    en.wikipedia.org/wiki/V1400_Centauri

    Mamajek's team initially hypothesized that J1407b is a ringed exoplanet or brown dwarf orbiting the star, [3]: 8 but that has since been disfavored by later studies. V1400 Centauri does not show repeating eclipses, telescope observations showed no orbiting companions, and the disk of J1407b would be unstable if it orbited the star, which ...

  4. List of exomoon candidates - Wikipedia

    en.wikipedia.org/wiki/List_of_exomoon_candidates

    2012 — It has been surmised that J1407b, a possibly planetary-mass object that eclipsed the star V1400 Centauri (aka. J1407) in 2007, may have a few moons based on gaps observed in its circumstellar disk or ring system. [1]

  5. Talk:J1407b/GA1 - Wikipedia

    en.wikipedia.org/wiki/Talk:J1407b/GA1

    In fairness, J1407b hasn't received any press releases from academic organizations (in press releases, organizations commission artists to make illustrations that would then become widely used) since its discovery announcement in 2015 (before evidence supporting J1407b being unrelated to V1400 Cen was published), so we're stuck with outdated ...

  6. Comment: The J1407b article was converted from redirect into article as a result of a split from the V1400 Centauri article. I began slowly expanding V1400 Centauri on 8 July 2024, but I did not add much to the J1407b section until 24 July 2024. As of today, it's been 5 days since I significantly expanded the J1407b section.

  7. Ring system - Wikipedia

    en.wikipedia.org/wiki/Ring_system

    The circumstellar disk or ring system of J1407b is about 0.6 astronomical units (90,000,000 km; 56,000,000 mi) in radius. [43] J1407b's transit of V1400 Centauri revealed gaps and density variations within its disk or ring system, which has been interpreted as hints of exomoons or exoplanets forming around J1407b. [43]

  8. Talk:J1407b - Wikipedia

    en.wikipedia.org/wiki/Talk:J1407b

    Comment: The J1407b article was converted from redirect into article as a result of a split from the V1400 Centauri article. I began slowly expanding V1400 Centauri on 8 July 2024, but I did not add much to the J1407b section until 24 July 2024. As of today, it's been 5 days since I significantly expanded the J1407b section.

  9. File:J1407b.ogv - Wikipedia

    en.wikipedia.org/wiki/File:J1407b.ogv

    J1407b.ogv (Ogg multiplexed audio/video file, Theora/Vorbis, length 27 s, 640 × 480 pixels, 3.24 Mbps overall, file size: 10.55 MB) This is a file from the Wikimedia Commons . Information from its description page there is shown below.