HD 17926

Autorius (-iai): Karistus

Išleidimo data:

HD 17926, aka TOI-396 and HR 858, is a binary system comprised of an F-type main sequence star and a red dwarf located about 104.35 lightyears from the solar system. The primary component of the pair is known to have three transiting, hot mini-Neptunes orbiting around it in a near-resonant structure

Padėkite mums išversti šį puslapį čia.

Atidaryti naudojant Celestia (rekomenduojama) arba Atsisiųsti

Kaip įdiegti priedus? Sužinokite čia.