TOI-1338

Yazar(lar): Karistus trappistplanets fyr02

Yayın tarihi:

Son güncelleme:

TOI-1338 is an eclipsing binary comprised of an F-type main sequence star and a red dwarf located about 1,320 lightyears from the solar system. Two planets are currently known to orbit both stars in this system, the inner one being a transiting Neptune mass, sub-Saturn sized gas giant and the outer being a sub-Saturn mass, non-transiting gas giant. TOI-1338 is the first confirmed circumbinary system discovered by TESS, with TOI-1338 c being the first circumbinary planet confirmed solely by the Radial Velocity method.

Bu sayfayı çevirmemize buradan yardımcı olun.

Celestia'da aç (önerilen) veya İndir

Eklentiler nasıl yüklenir? buradan öğrenin.