HD 16760
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. HD 16760 is a binary star system approximately 150 light-years away in the constellation Perseus. The primary star HD 16760 is a G-type main sequence star similar to our Sun. The secondary, HIP 12635 is 1.521 magnitudes fainter and located at a separation of 14.6 arcseconds from the primary, corresponding to a physical separation of at least 660 AU. Announced in July 2009, HD 16760 has been confirmed to have a substellar object orbiting it.

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. HD 16760 is a binary star system approximately 150 light-years away in the constellation Perseus. The primary star HD 16760 is a G-type main sequence star similar to our Sun. The secondary, HIP 12635 is 1.521 magnitudes fainter and located at a separation of 14.6 arcseconds from the primary, corresponding to a physical separation of at least 660 AU. Announced in July 2009, HD 16760 has been confirmed to have a substellar object orbiting it.