Gravitational potential of two equal stars

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SUMMARY

The discussion focuses on the gravitational potential of a double-star system consisting of two equal stars, A and B, each with mass M and radius r, positioned 6r apart. The gravitational potential is calculated using the formula V = -GM(1/R1 + 1/R2), where R1 and R2 are the distances from each star. The equipotential curves are derived, showing that they are distorted circles around each star, and specific potential values are discussed, including -10GM/11r, -2GM/3r, and -GM/3r. The minimum velocity required for gas emitted from star B to be captured by star A is also addressed.

PREREQUISITES
  • Understanding of gravitational potential and its mathematical representation
  • Familiarity with the concept of equipotential surfaces
  • Knowledge of basic calculus for plotting functions
  • Experience with gravitational equations, specifically U = -GM/R
NEXT STEPS
  • Study the derivation of equipotential surfaces in multi-body gravitational systems
  • Learn about the implications of gravitational potential in astrophysics
  • Explore the mathematical techniques for plotting complex functions
  • Investigate the dynamics of gas emission and capture in binary star systems
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in gravitational interactions in binary star systems will benefit from this discussion.

benf.stokes
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Homework Statement



Two equal spherically symmetrical stars, A and B, each of mass M and radius r have their centers 6r apart. Make a sketch showing the lines on which the gravitational potential takes the values:
1. \frac{-10GM}{11r}

2. \frac{-2GM}{3r}

3. \frac{-GM}{3r}

Accurate plotting is not required but the general shape of the lines must be clear
4. What is the minimum velocity with which gas can be emitted from the surface of B and still be captured by A? Ignore any effects due to the motion of the stars

Homework Equations



U = \frac{-GM}{R}

The Attempt at a Solution



I can't even get started.

Thanks
 
Last edited:
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The potential of the double-star system is the sum of the potential of the single stars:
V=-GM(1/R1+1/R2),
where R1 is the distance from the star on the left and R2 is the distance from the star on the right. We can calculate the potential in -GM/r units, to make sketching equipotential curves easy.

In case of a lonely star, the equipotential curves are circles around the star. These circles will be somewhat distorted in the presence of the other star but they still are a pair of closed curves when we are at the close vicinity of one star.

It is easy to plot the potential values along the line which connects the stars. If the origin is the middle point between the starts, the potential function is V(x) = 1/x+1/(6-x) (multiplied by -GM/r). Drawing horizontal lines at the height of the given potential values, one can find the points where the equipotential curves cross the x axis.
In the middle, the potential of both stars is the same, the equipotential curves around both stars touch here. If the magnitude of the potential is lower than 2/3 the equipotential curve crosses the x-axis outside the two-star system, and encloses both stars.

ehild
 

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  • twostars.jpg
    twostars.jpg
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Thanks for the help but isn't there any general way to determine the equipotential surfaces of the two stars? I happen to have the answer to the problem (I just can't figure it out) and it is like this:
solution.jpg
 
Look at the graph ehild has shown and simply look at it as though it were top-down.
 
You can calculate the equipotential curves, but it was not required.

For r=1, the equation for these curves is :

\frac{1}{\sqrt{(x+3)^2+y^2}}+\frac{1}{\sqrt{(x-3)^2+y^2}}=C

But it is not easy to plot them.

ehild
 

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