Kepler-1520

Autor(i): LukeCEL Gurren Lagann

Dátum vydania:

Kepler-1520, also known as KOI-3794, is a K-type main sequence star about 2,017 light-years away in the constellation Cygnus. Its sole planet is one of a few known to have dust tails around it, which is caused by its surface evaporating from its very tight proximity to its host star

Kepler-1520 b

Pomôžte nám preložiť túto stránku tu.

Otvoriť v Celestii (odporúčané) alebo Prevziať

Ako nainštalovať doplnky? Zistite to tu.