COROT-3
Constellation, G-type main-sequence star, Main sequence, Apparent magnitude, COROT-3b, COROT
Herausgegeben: Toll, Aaron Philippe
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. COROT-3 is a white-yellow dwarf main sequence star hotter than our Sun. This star is located approximately 2200 light-years away in the constellation of Aquila. The apparent magnitude of this star is 13, which means it is not visible to the naked eye but can be seen with a medium sized amateur telescope on a clear dark night. This star is home to object designated COROT-3b. This object was discovered by the COROT Mission spacecraft using the transit method. Measuremen...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. COROT-3 is a white-yellow dwarf main sequence star hotter than our Sun. This star is located approximately 2200 light-years away in the constellation of Aquila. The apparent magnitude of this star is 13, which means it is not visible to the naked eye but can be seen with a medium sized amateur telescope on a clear dark night. This star is home to object designated COROT-3b. This object was discovered by the COROT Mission spacecraft using the transit method. Measurements made using the radial velocity method show that this object is probably a brown dwarf.
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