TOI-824 is a K-type main sequence star located about 208.37 lightyears from the solar system. orbiting this star is a single, hot oceanic planet that completes a full orbit every 1.39 days (b= 2.926 Re, 18.467 Me). observations from Spitzer showed that planet had poor heat distribution and likely lacked a hydrogen dominated envelope and was either: a super-Earth with a volatile rich, extended atmosphere or a bare ocean world with a relatively thin atmosphere. Further JWST analysis could constrain where this planet falls into far greater than Spitzer could.
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