The ratio of brightness of two stars can be determined by a constant of 2.512 raised to the power of the magnitude difference. The formula b1 b2 = 2.512 (m2 − m1) where b1 and b2 represent the brightness and m1 and m2 refer to the magnitudes of the stars being compared. One star has a magnitude of 0.6, and another star has a magnitude of 2.6.
The ratio of brightness of two stars can be determined by a constant of 2.512 raised to the power of the magnitude difference. The formula b1 b2 = 2.512 (m2 − m1) where b1 and b2 represent the brightness and m1 and m2 refer to the magnitudes of the stars being compared. One star has a magnitude of 0.6, and another star has a magnitude of 2.6.
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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The ratio of brightness of two stars can be determined by a constant of 2.512 raised to the power of the magnitude difference.
The formula
b1
|
b2
|
= 2.512
(m2 − m1)
where b1 and b2 represent the brightness and m1 and m2 refer to the magnitudes of the stars being compared.
One star
has a magnitude of 0.6, and another star has a magnitude of 2.6.
What is
the ratio of brightness of these two stars?
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