Rev5 Phys 1403 Stellar Magnitudes and Parallax Since the minimum brightness visible will be inversely proportional the LGP we can then write: =(2.512) %3D %3D LGP(1) ()7 as long as m>7. Then D =(2.512)" Take the logarithm of both sides of this equation: 2 log D =0.4(m -7) Solve this equation for m: m =7+5 log D (3) This equation represents the limiting magnitude (dimmest star) visible by a telescope of diameter D. Example For a 100-cm telescope, the limiting visual apparent magnitude is m =7+5log(100) =7+5(2) =17 Problems 1. Photometric comparison shows that the star Mizar, magnitude 2.4, is 4.37 times a bright as its companion Alcor. What is the magnitude of Alcor? 2. The variable star Algol declines from a magnitude of 2.2 at a maximum to a magnitude of 3.4 at a minimum. What is the ratio of the brightness at maximum to that at minimum?
Rev5 Phys 1403 Stellar Magnitudes and Parallax Since the minimum brightness visible will be inversely proportional the LGP we can then write: =(2.512) %3D %3D LGP(1) ()7 as long as m>7. Then D =(2.512)" Take the logarithm of both sides of this equation: 2 log D =0.4(m -7) Solve this equation for m: m =7+5 log D (3) This equation represents the limiting magnitude (dimmest star) visible by a telescope of diameter D. Example For a 100-cm telescope, the limiting visual apparent magnitude is m =7+5log(100) =7+5(2) =17 Problems 1. Photometric comparison shows that the star Mizar, magnitude 2.4, is 4.37 times a bright as its companion Alcor. What is the magnitude of Alcor? 2. The variable star Algol declines from a magnitude of 2.2 at a maximum to a magnitude of 3.4 at a minimum. What is the ratio of the brightness at maximum to that at minimum?
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