p37_025 - 25. (a) Using Eq. 37-14, the angular separation...

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25. (a) Using Eq. 37-14, the angular separation is θ R = 1 . 22 λ d = (1 . 22)(550 × 10 9 m) 0 . 76 m =8 . 8 × 10 7 rad . (b) Using the notation of Sample Problem 37-6 (which is in the textbook supplement), the distance between the stars is D = R = (10 ly)(9
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This note was uploaded on 11/12/2011 for the course PHYS 2001 taught by Professor Sprunger during the Fall '08 term at LSU.

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