HD 88133 b
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Script error: No such module "infobox".Script error: No such module "Check for unknown parameters". HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected.[1]
In 2016 the direct detection of the planetary thermal emission spectrum was claimed,[2] but the detection was questioned in 2021.[3]
References
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External links
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