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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 5319 is an 8th magnitude star approximately 326 light years away in the constellation Cetus. It is a giant star of spectral type K0, having run out of hydrogen in its core. When it was main-sequence, the spectral type was early F or late A. The radius is more than three times that of the Sun, and the volume is 35 times greater. The star's mass is more than 1.5 times that of the Sun, which suggests much lower density.

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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 5319 is an 8th magnitude star approximately 326 light years away in the constellation Cetus. It is a giant star of spectral type K0, having run out of hydrogen in its core. When it was main-sequence, the spectral type was early F or late A. The radius is more than three times that of the Sun, and the volume is 35 times greater. The star's mass is more than 1.5 times that of the Sun, which suggests much lower density.