Gravitational potential of two equal stars

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Homework Help Overview

The discussion revolves around the gravitational potential of a system consisting of two equal spherically symmetrical stars, A and B, positioned 6r apart. Participants are tasked with sketching equipotential lines for specific potential values and determining the minimum velocity for gas emitted from one star to be captured by the other.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the potential of the double-star system as a sum of individual star potentials, with considerations on how to sketch equipotential curves. There are questions about general methods for determining these surfaces and how to visualize the potential values along the line connecting the stars.

Discussion Status

Some participants have provided insights into calculating the potential and sketching the curves, while others express uncertainty about the general approach to the problem. There is an ongoing exploration of how to represent the equipotential surfaces accurately, with no clear consensus reached yet.

Contextual Notes

Participants note that accurate plotting is not required, but the general shape of the lines must be clear. There is also mention of the complexity involved in plotting the equipotential curves, indicating a potential challenge in visualizing the problem.

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. [tex]\frac{-10GM}{11r}[/tex]

2. [tex]\frac{-2GM}{3r}[/tex]

3. [tex]\frac{-GM}{3r}[/tex]

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 = [tex]\frac{-GM}{R}[/tex]

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
 

Attachments

  • 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 :

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

But it is not easy to plot them.

ehild
 

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