3 Centauri
Constellation, Centaurus, Binary star, Light-year, Apparent magnitude, Variable star, Stellar classification
Herausgegeben: Horst, Kristen Nehemiah
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3 Centauri is a binary star in the constellation Centaurus. It is approximately 298 light years from Earth. The primary component, 3 Centauri A, is a blue-white B-type giant with a mean apparent magnitude of +4.56. It is a variable star, and its brightness varies from magnitude +4.27 to +4.32 It is suspected the variations in luminosity are a result of the primary being an eclipsing binary, which would mean the system would consist of at least three objects. Its more ...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3 Centauri is a binary star in the constellation Centaurus. It is approximately 298 light years from Earth. The primary component, 3 Centauri A, is a blue-white B-type giant with a mean apparent magnitude of +4.56. It is a variable star, and its brightness varies from magnitude +4.27 to +4.32 It is suspected the variations in luminosity are a result of the primary being an eclipsing binary, which would mean the system would consist of at least three objects. Its more distant companion, 3 Centauri B, is located 7.9 arcseconds away. It is a blue-white B-type main sequence dwarf and has an apparent magnitude of +6.06.
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