A spherical planet has an outer radius R; its density p varies as a function of distance r from the centre, given by the function p(r) = 4 – 3(r2 /R²) (so the density is 4 at the centre, decreasing to 1 at the surface). Calculate the mass of the planet. Select one: 8 T R³ 5 16 T R³ 3 25 T R³ 12 44 T R³ 15

Classical Dynamics of Particles and Systems
5th Edition
ISBN:9780534408961
Author:Stephen T. Thornton, Jerry B. Marion
Publisher:Stephen T. Thornton, Jerry B. Marion
Chapter10: Motion In A Noninertial Reference Frame
Section: Chapter Questions
Problem 10.20P: Calculate the effective gravitational field vector g at Earths surface at the poles and the equator....
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A spherical planet has an outer radius R;
its density p varies as a function of
distance r from the centre, given by the
function p(r) = 4 – 3(r2 /R²) (so the
-
density is 4 at the centre, decreasing to 1
at the surface).
Calculate the mass of the planet.
Select one:
8 T
R3
5
16 T
R³
3
25 T R
12
44 T
R³
15
Transcribed Image Text:A spherical planet has an outer radius R; its density p varies as a function of distance r from the centre, given by the function p(r) = 4 – 3(r2 /R²) (so the - density is 4 at the centre, decreasing to 1 at the surface). Calculate the mass of the planet. Select one: 8 T R3 5 16 T R³ 3 25 T R 12 44 T R³ 15
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