When a large star becomes a supernova, its core may be compressed so tightly that it becomes a neutron star, with a radius of about 20 km (about the size of the San Francisco area). If a neutron star rotates once every second, (a) what is the speed of a particle on the star’s equator and (b) what is the magnitude of the particle’s centripetal acceleration? (c) If the neutron star rotates faster, do the answers to (a) and (b) increase, decrease, or remain the same?

Principles of Physics: A Calculus-Based Text
5th Edition
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Raymond A. Serway, John W. Jewett
Chapter3: Motion In Two Dimensions
Section: Chapter Questions
Problem 24P
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When a large star becomes a supernova, its core may be
compressed so tightly that it becomes a neutron star, with a radius of
about 20 km (about the size of the San Francisco area). If a neutron
star rotates once every second, (a) what is the speed of a particle on
the star’s equator and (b) what is the magnitude of the particle’s centripetal
acceleration? (c) If the neutron star rotates faster, do the answers
to (a) and (b) increase, decrease, or remain the same?

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