KMT-2018-BLG-1292L

Autor(es): TOI-700d

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KMT-2018-BLG-1292L is a single F dwarf star with a mass of approximately 1.2 M☉, located about 9,524 light-years away in the constellation Scorpius. A super-Jovian planet, KMT-2018-BLG-1292L b, was discovered orbiting this star via the microlensing method in 2020. The planet has a mass of approximately 4.4–5.0 Jupiter masses and orbits at a semi-major axis of about 6.0 AU. The host star of this system lies physically within about 10 parsecs of the Galactic plane.

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