Surface of Equal Gravitational Potential

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SUMMARY

The discussion focuses on deriving the equation of the surface of equal gravitational potential between the Earth and the Sun. The user defines the gravitational potential equations using the masses of the Earth and Sun, denoted as m and M, respectively. The user sets the coordinates for the Sun at (0,0) and the Earth at (0,k), leading to the equation M√(x²+(y-k)²) = m√(x²+y²). The approach is confirmed as valid by another participant in the discussion.

PREREQUISITES
  • Understanding of gravitational potential and forces
  • Familiarity with basic calculus and algebra
  • Knowledge of coordinate systems in physics
  • Concept of level curves in two-dimensional space
NEXT STEPS
  • Explore the derivation of gravitational potential equations in multi-body systems
  • Study the concept of level curves and their applications in physics
  • Learn about gravitational fields and their mathematical representations
  • Investigate the implications of gravitational potential surfaces in astrophysics
USEFUL FOR

Students in introductory physics, educators teaching gravitational concepts, and anyone interested in the mathematical modeling of gravitational interactions between celestial bodies.

amcavoy
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In my introductory physics class, we were given a problem to find the equation of the surface between the Earth and the Sun where the gravitational potential is equal. At first (without working anything out), it seems that it might be some sort of ellipsoid or paraboloid. For now, I'm just going to look at a level curve and try to work it out in two dimensions.

Let M be the mass of the sun, and m be the mass of the earth. Let r1 be the distance from the Earth to a point (x,y) on the graph and r2 be the distance from the sun to the same point (x,y):

[tex]-\frac{GM}{r_2}=-\frac{Gm}{r_1}\implies r_1M=r_2m[/tex]

Now I am going to set the center of the sun as point (0,0) and the Earth as (0,k). Doing so gives:

[tex]M\sqrt{x^2+\left(y-k\right)^2}=m\sqrt{x^2+y^2}[/tex]

I also know that when x=0, r1+r2 is the distance from the Earth to the sun.

I am not finished yet. I would just like to know if my approach is valid. Could someone let me know?

Thank you.
 
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Looks good to me.
 
Great, thank you for the help.
 

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