In the astronomy, the solar radius is a length unit that lets you express the magnitude of stars. It is equal to the current ray of the sun. The value is: 1 R & # x2299; = 6 , 955 × 10 8 m = 0 , 004 652 {\displaystyle 1\,R_{\odot }=6,955\times 10^{8}\,{\hbox{m}}=0,004\,652} AE {\displaystyle {\hbox{AE}}} .
The solar radius is about 695 500 kilometers or about 110 times the Earth's radius or 10 times the average Jupiter radius. The radius varies slightly from the pole to the equator. That is because of the rotation of the sun. Also see
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