Beta Gruis
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Beta Gruis is the second brighest star in the southern constellation of Grus. It was once considered the rear star in the tail of the constellation of the Fish: it, with , , . , and Gru, belonged to Piscis Austrinus in traditional Arabic astronomy. The estimated mass is about three times that of the Sun, and it has a surface temperature of approximately 3,400 K, just over half the surface temperature of the sun. This low temperature accounts for the star's dull red…mehr

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Beta Gruis is the second brighest star in the southern constellation of Grus. It was once considered the rear star in the tail of the constellation of the Fish: it, with , , . , and Gru, belonged to Piscis Austrinus in traditional Arabic astronomy. The estimated mass is about three times that of the Sun, and it has a surface temperature of approximately 3,400 K, just over half the surface temperature of the sun. This low temperature accounts for the star's dull red color. The total luminosity is about 3,800 times that of the Sun, and it has an estimated radius of 0.8 astronomical units, which is about 100 times that of the Sun.