He rate p at which a star radiates energy in the form of


10. The rate P at which a star radiates energy in the form of electromagnetic waves can be calculated using the equation: P = 4psR2T4 , where R is the radius of the star and T is the temperature of the star's surface.

Calculate a numerical value for the intensity of sunlight (in watts/meter 2) one AU away from the sun.

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Physics: He rate p at which a star radiates energy in the form of
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