Omega Serpentis

Autor(i): Gurren Lagann

Dátum vydania:

Omega Serpentis is a binary star system consisting of a G-type giant star and a K-type main-sequence star about 251 light-years away in the constellation Serpens Caput. A planet candidate the size of Jupiter was announced orbiting the larger star of the two in 2005, but its existence wasn't confirmed until 2013

Pomôžte nám preložiť túto stránku tu.

Otvoriť v Celestii (odporúčané) alebo Prevziať

Ako nainštalovať doplnky? Zistite to tu.