L = ( 0.0813 ) x (Rs) ^2 x 10-0.4m x Ls where L = luminosity of the desired star Rs = distance of the stars in light years m = apparent magnitude of star Ls = Luminosity of Sun = 1.00 The calculated value of Polaris' luminosity is: a. 2382 times Ls b. 6040 times Ls c. 5566 times Ls d. 2612 times Ls
L = ( 0.0813 ) x (Rs) ^2 x 10-0.4m x Ls where L = luminosity of the desired star Rs = distance of the stars in light years m = apparent magnitude of star Ls = Luminosity of Sun = 1.00 The calculated value of Polaris' luminosity is: a. 2382 times Ls b. 6040 times Ls c. 5566 times Ls d. 2612 times Ls
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L = ( 0.0813 ) x (Rs) ^2 x 10-0.4m x Ls
where L = luminosity of the desired star
Rs = distance of the stars in light years
m = apparent magnitude of star
Ls = Luminosity of Sun = 1.00
The calculated value of Polaris' luminosity is:
a. 2382 times Ls
b. 6040 times Ls
c. 5566 times Ls
d. 2612 times Ls
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