HAT-P-17

Autor(i): Edasich

Dátum vydania:

HAT-P-17, also known as TOI-1283, is a binary star system consisting of a K-type main-sequence star and a red dwarf about 302.11 light-years away in the constellation Cygnus. Two super-Jovian planets orbit around the primary star, one of which complete an orbit once every 5.9 days

Pomôžte nám preložiť túto stránku tu.

Otvoriť v Celestii (odporúčané) alebo Prevziať

Ako nainštalovať doplnky? Zistite to tu.