Under some circumstances, a star can collapse into an extremely dense object made mostly of neutrons and called a neutron star. (The density of a neutron star is roughly 10¹4 times as great as that of ordinary solid matter.) Suppose we represent a star as a uniform, solid, rigid sphere, both before and after the collapse. Also assume that mass of the star is conserved during the collapse. The star's initial radius before collapse is 7.0 ×105 km (comparable to our sun); its final radius after collapse is 16 km. If the original star rotates once in 30 days, what is the angular speed of the neutron star resulting from the collapse?
Under some circumstances, a star can collapse into an extremely dense object made mostly of neutrons and called a neutron star. (The density of a neutron star is roughly 10¹4 times as great as that of ordinary solid matter.) Suppose we represent a star as a uniform, solid, rigid sphere, both before and after the collapse. Also assume that mass of the star is conserved during the collapse. The star's initial radius before collapse is 7.0 ×105 km (comparable to our sun); its final radius after collapse is 16 km. If the original star rotates once in 30 days, what is the angular speed of the neutron star resulting from the collapse?
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...
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