KMT-2018-BLG-1292L

Yazar(lar): TOI-700d

Yayın tarihi:

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.

Bu sayfayı çevirmemize buradan yardımcı olun.

Celestia'da aç (önerilen) veya İndir

Eklentiler nasıl yüklenir? buradan öğrenin.