Kepler-1040

Autors(-i): Gliese_504b

Izlaišanas datums:

Kepler-1040, also known as KOI-1989, is a binary star system consisting of a G-type star and a red dwarf, located 1,551.6465 light-years from Earth. It is known that component A has a super-Earth with an orbital period of about 201 days.

Palīdziet mums tulkot šo lapu šeit.

Atvērt programmā Celestia (ieteicams) vai Lejupielādēt

Kā instalēt papildinājumus? Uzziniet šeit.