HD 206893

Συντάκτης(-ες): SolHorizon

Ημερομηνία κυκλοφορίας:

Τελευταία ενημέρωση:

HD 206893, also known as HIP 107412, is about 132.953 light-years away from Earth. It is a binary star system consisting of an F-type main-sequence star and an L-type brown dwarf. Component A is known to be orbited by a gas giant with a mass of about 12.7 times that of Jupiter. In November 2025, a report indicated tentative astrometric residuals for HD 206893 B. If interpreted as signs of an exomoon, these residuals correspond to a candidate moon (HD 206893 B I) with an orbital period of about 0.76 years and a mass of roughly 0.4 times that of Jupiter. However, these residuals could also be due to systematic errors, and it cannot be confirmed at present.

Βοηθήστε μας να μεταφράσουμε αυτή τη σελίδα εδώ.

Άνοιγμα στο Celestia (Συνιστάται) ή Λήψη

Πώς να εγκαταστήσετε πρόσθετα; Μάθετε περισσότερα εδώ.