A uniform distribution of dust in the solar system adds to the gravitational attraction of the Sun on a planet an additional force F = −m C r where m is the mass of the planet, C is a constant proportional to the gravitational constant and the density of the dust, and r is the radius vector from the Sun to the planet (both considered as points). This additional force is very small compared to the direct Sun-planet gravitational force. Calculate the period of radial oscillations for slight disturbances from this circular orbit.
A uniform distribution of dust in the solar system adds to the gravitational attraction of the Sun on a planet an additional force F = −m C r where m is the mass of the planet, C is a constant proportional to the gravitational constant and the density of the dust, and r is the radius vector from the Sun to the planet (both considered as points). This additional force is very small compared to the direct Sun-planet gravitational force. Calculate the period of radial oscillations for slight disturbances from this circular orbit.
Glencoe Physics: Principles and Problems, Student Edition
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ISBN:9780078807213
Author:Paul W. Zitzewitz
Publisher:Paul W. Zitzewitz
Chapter7: Gravitation
Section: Chapter Questions
Problem 5STP
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A uniform distribution of dust in the solar system adds to the gravitational attraction of the Sun on a planet an additional force
F = −m C r
where m is the mass of the planet, C is a constant proportional to the gravitational constant and the density of the dust, and r is the radius vector from the Sun to the planet (both considered as points). This additional force is very small compared to the direct Sun-planet gravitational force.
Calculate the period of radial oscillations for slight disturbances from
this circular orbit.
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