Gravitational interaction between three bodies

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SUMMARY

The gravitational interaction between three bodies A, B, and C arranged linearly is analyzed, focusing on whether body A affects the free fall of body B towards body C. The scenario involves calculating the rate at which the distance between B and C decreases, first with A present and then absent. Key formulas utilized include Newton's second law, \(F=ma\), and Newton's universal law of gravitation, \(F=G\frac{m_1m_2}{r^2}\). The conclusion is that the total gravitational force on a mass is the vector sum of the forces from individual masses, indicating that one mass does not interfere with the gravitational effect of another.

PREREQUISITES
  • Understanding of Newton's laws of motion
  • Familiarity with Newton's universal law of gravitation
  • Basic knowledge of calculus for velocity calculations
  • Concept of vector addition in physics
NEXT STEPS
  • Calculate gravitational forces in multi-body systems using vector addition
  • Explore the implications of gravitational interactions in orbital mechanics
  • Study the effects of tidal forces in celestial mechanics
  • Learn about the SUVAT equations for motion under uniform acceleration
USEFUL FOR

Students of physics, astrophysicists, and anyone interested in gravitational dynamics and multi-body interactions in space.

Ranku
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If there are three bodies A, B, and C arranged linearly, and B is free falling towards C, will the gravitational presence of A affect the rate of free fall of B towards C?
 
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Ranku said:
If there are three bodies A, B, and C arranged linearly, and B is free falling towards C, will the gravitational presence of A affect the rate of free fall of B towards C?
Why not set up a situation and calculate it? Put B in the middle at coordinate zero, A on the left at coordinate -1 and C on the right at coordinate 1. Give them all the same mass.

Decide what you want to calculate. The rate at which the distance between B and C decreases?

Calculate. First with A present then with A absent.

Hint: Tides.
 
jbriggs444 said:
Why not set up a situation and calculate it? Put B in the middle at coordinate zero, A on the left at coordinate -1 and C on the right at coordinate 1. Give them all the same mass.

Decide what you want to calculate. The rate at which the distance between B and C decreases?

Calculate. First with A present then with A absent.

Hint: Tides.
What formulas do I use and in what order?
 
Ranku said:
What formulas do I use and in what order?
Newton's second law:$$F=ma$$That'll let you compute the acceleration ##a## of an object of mass ##m## when subject to a force ##F##.

Newton's universal law of gravitation:$$F=G\frac{m_1m_2}{r^2}$$That'll let you compute the force ##F## on an object of mass ##m_1## from an object of mass ##m_2## a distance ##r## away.

It should be enough to look at the accelerations, but you might choose to look at the resulting velocities. You get that from Calculus or the SUVAT equations. In particular:$$v=at$$That'll give you the velocity ##v## of an object with uniform acceleration ##a## after duration ##t## when starting from rest.
 
The answer to your query is that total gravitational force on a given mass by several other masses is the (vector) sum of the forces due to the individual masses. One mass does not "interfere" with the affect of another mass.
 

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