An impossible Jupiter-sized gas giant, TOI-5205b, the first exoplanet of its kind with an atmosphere containing far fewer heavy elements than similarly sized objects, as well as its own host red dwarf star - TOI-5205, discovered in data from NASA’s alien planet-hunting Transiting Exoplanet Survey Satellite (TESS).
Kanodia described TOI-5205b’s orbit of its host stars as a “pea going around a lemon” as opposed to Jupiter’s orbit of the Sun, which is like a “pea going around a grapefruit.”
Carnegie's Shubham Kanodia quoted in 2023:
TOI-5205b’s existence stretches what we know about the disks in which these planets are born. In the beginning, if there isn’t enough rocky material in the disk to form the initial core, then one cannot form a gas giant planet.
And at the end, if the disk evaporates away before the massive core is formed, then one cannot form a gas giant planet. And yet TOI-5205b formed despite these guardrails. Based on our nominal current understanding of planet formation, TOI-5205b should not exist; it is a “forbidden” planet.
https://futurism.com/space/astronomers-forbidden-size-star
https://www.sciencedaily.com/releases/2023/02/230222141146.htm
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