HIP 38594

Author(en): Karistus

Veröffentlichungsdatum:

HIP 38594, aka Ross 429, is a binary system comprised of a red dwarf and a white dwarf located about 58.05 lightyears from the solar system. two mildly eccentric planets, one sub-Neptune mass planet grazing it's host's habitable zone and an outer sub-Saturn mass planet are currently known to orbit the primary component to the system.

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