TOI-1669

Autor(es): Karistus

Data de lançamento:

TOI-1669 is a G-type main-sequence star located about 364.49 lightyears from the solar system. A single gas giant, a little over half as massive as Jupiter is known to orbit this star on a mildly eccentric orbit throughout its habitable zone. RV analysis shows a linear trend, which could be potentially caused by a planet on a ~2200-day orbit, but more data is needed. A sub-Neptune-sized candidate planet was spotted by TESS, but remains unconfirmed.

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