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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.
I've removed the duplicate ALMA image and have split the double image into separate ones, but I personally object to the removal of any of the existing images since I believe they communicate important aspects of J1407b's disk (i.e. eps Aur image helps visualize J1407b as a disk transiting a star, the lightcurve has labeled x and y axes, the ...
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.
August 2021 — astronomers reported an habitable-zone 1.7 R 🜨 exomoon candidate transiting one of the components in the planetary-mass binary 2MASS J1119-1137AB. [ 14 ] January 2022 — an exomoon candidate was reported around the planet Kepler-1708b , and because it is orbiting a planet at approximately 1.6 AU from a star that is slightly ...
J1407b's rings span a radius of about 90 million kilometers (56 million miles) and may eventually form moons over time. Although initially thought to be orbiting V1400 Centauri, later studies suggest J1407b is likely an unbound object passing in front of the star. This is stripped down to what I think is the bare minimum.
The one thing that most agree on is that there is too much racing. The problem is that contraction is great as long as it’s not your business that is contracting. And therein lies another ...
J1407b's rings span a radius of about 90 million kilometers (56 million miles) and may eventually form moons over time. Although initially thought to be orbiting V1400 Centauri, later studies suggest J1407b is likely an unbound object passing in front of the star. This is stripped down to what I think is the bare minimum.
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.