Epsilon Reticuli
Constellation, Reticulum, Light-year, Binary star, Subgiant, Extrasolar planet, White dwarf
Herausgegeben: Angelus, Jerold
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Epsilon Reticuli is a binary system approximately 59 light-years away in the constellation of Reticulum. The primary star is an orange subgiant star, while the secondary star is a white dwarf star. The primary star should be easily visible without optical aid under dark skies in the southern hemisphere. In 2000, an extrasolar planet was confirmed to be orbiting the primary star in the system. The primary star, Epsilon Reticuli A, is an orange subgiant 20% more massive...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Epsilon Reticuli is a binary system approximately 59 light-years away in the constellation of Reticulum. The primary star is an orange subgiant star, while the secondary star is a white dwarf star. The primary star should be easily visible without optical aid under dark skies in the southern hemisphere. In 2000, an extrasolar planet was confirmed to be orbiting the primary star in the system. The primary star, Epsilon Reticuli A, is an orange subgiant 20% more massive than our Sun. Being a subgiant it is ceasing or has already ceased fusing hydrogen in its core.