KMT-2018-BLG-2602L

Autors(-i): 参宿四and韶山8

Izlaišanas datums:

KMT-2018-BLG-2602L is a single K-type main-sequence star about 14,057 light-years away in the constellation Sagittarius. A super-Jupiter with a mass of approximately 1.15 times that of Jupiter was discovered orbiting this star via the microlensing method in 2022, with a semi-major axis of about 4 AU.

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