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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