Calculating Mass and Weight of a Planet

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SUMMARY

The discussion focuses on calculating the total mass and weight of a planet with a density function defined as D(r) = Do*[1-(a*r/Ro)], where Ro = 3.1623×106 m, Do = 3160 kg/m3, and a = 0.16. The correct approach involves integrating the density function using the shell method to find the total mass, which is expressed as the integral of D(r) dV = D(r) r2 sin(θ) dr dθ dφ. Subsequently, the weight of a one-kilogram mass at the planet's surface can be calculated using the formula F = (G m M) / r2.

PREREQUISITES
  • Understanding of calculus, specifically integration techniques.
  • Familiarity with the shell method for volume integration.
  • Knowledge of gravitational force calculations using Newton's law of gravitation.
  • Basic concepts of planetary density variations.
NEXT STEPS
  • Study the shell method for volume integration in spherical coordinates.
  • Learn about the universal law of gravitation and its applications in astrophysics.
  • Explore advanced integration techniques for variable density functions.
  • Investigate the implications of density variations on planetary formation and structure.
USEFUL FOR

Students and professionals in physics, astrophysics, and engineering who are involved in planetary science, gravitational studies, or advanced calculus applications.

whereisccguys
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2 part question

The density of a certain planet varies with radial distance as: D(r) = Do*[1-(a*r/Ro)], where Ro= 3.1623×106 m is the radius of the planet, Do = 3160 kg/m3 is its central density, and a = 0.160. Calculate the total mass of this planet.

Calculate the weight of a one kilogram mass located on the surface of the planet.

i tried integrating D(r) with and plugin in the radius of the planet but it doesn't work

i know this question has somethin to do with integrating through shell method but I'm not sure how to do it

can any1 help me?
 
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Why doesn't it work?

~H
 
whereisccguys said:
2 part question

The density of a certain planet varies with radial distance as: D(r) = Do*[1-(a*r/Ro)], where Ro= 3.1623×106 m is the radius of the planet, Do = 3160 kg/m3 is its central density, and a = 0.160. Calculate the total mass of this planet.

Calculate the weight of a one kilogram mass located on the surface of the planet.

i tried integrating D(r) with and plugin in the radius of the planet but it doesn't work

i know this question has somethin to do with integrating through shell method but I'm not sure how to do it

can any1 help me?

I am not sure what you integrated exactly but here are some thoughts:

First, you must determined the total massof the planet, right? This is given by the integral of D(r) dV = D(r) r^2 sin(\theta) dr d\theta d\phi. The angular integrals are trivial and give 4 \pi. The radial integral is straightforward.

Then, you must use this in the universal law of gravitation to determine the *weight* of 1 kg at the surface of the planet, F= {G m M \over r^2}.

Patrick
 

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