HD 114082

Autors(-i): Karistus

Izlaišanas datums:

HD 114082, aka TOI-6697, is an F-type main sequence star located about 310.03 lightyears from the solar system, at least one gas giant is known to orbit this star, an eccentric transiting 8Mjup planet on a 109.75 day orbit, this star is also known to have a small debris disk extending from around 29 to 35 AU. an additional transit signal was spotted by TESS, possibly indicative of another gas giant is this system with a potential orbital period roughly double that of the confirmed planet.

HD 114082 and its disk

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