36 Ursae Majoris
Main sequence, Star, Sun, Gas giant, Brown dwarf, Jupiter mass, Brown dwarf, McDonald Observatory
Herausgegeben: Nicolao, Hardmod Carlyle
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 36 Ursae Majoris is a yellowish main sequence star of spectral type F8V. The star is 1.2 times more massive than the Sun and has a 1.2 times larger radius. Its age is around 2 billion years. The star is thought to have a stellar companion B of spectral type K7V at wide separation. An optical companion C is located at 49,000 AUs, but is probably not bound to the system. According to Nelson & Angel, 36 Ursae Majoris could host one or two jovian planets at wide separatio...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 36 Ursae Majoris is a yellowish main sequence star of spectral type F8V. The star is 1.2 times more massive than the Sun and has a 1.2 times larger radius. Its age is around 2 billion years. The star is thought to have a stellar companion B of spectral type K7V at wide separation. An optical companion C is located at 49,000 AUs, but is probably not bound to the system. According to Nelson & Angel, 36 Ursae Majoris could host one or two jovian planets at wide separations from the host star, with orbital periods of 10-15, 25 and 50 years respectively.
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