Gravitational potential of two equal stars

In summary, the gravitational potential of the double star system is the sum of the potential of the single stars. The potential in -GM/r units is easy to calculate and sketch.
  • #1
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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  • #2
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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  • #3
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
 
  • #4
Look at the graph ehild has shown and simply look at it as though it were top-down.
 
  • #5
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
 

FAQ: Gravitational potential of two equal stars

What is the gravitational potential of two equal stars?

The gravitational potential of two equal stars is a measure of the amount of work required to move an object from an infinite distance away to a point between the two stars. It is a scalar value that takes into account the masses of the stars and their distance from each other.

How is the gravitational potential of two equal stars calculated?

The gravitational potential of two equal stars can be calculated using the equation V = -Gm/r, where G is the gravitational constant, m is the mass of each star, and r is the distance between the two stars. The potential is negative because it represents the work done by the gravitational force in bringing an object towards the stars.

What is the relationship between gravitational potential and gravitational force?

The gravitational potential between two equal stars is directly proportional to the gravitational force between them. This means that as the potential increases, the force also increases, and vice versa.

Can the gravitational potential of two equal stars be negative?

Yes, the gravitational potential of two equal stars can be negative. This occurs when the distance between the stars is greater than the distance at which the potential becomes zero. In this case, the potential becomes more negative as the distance increases.

How does the gravitational potential of two equal stars affect the motion of objects?

The gravitational potential of two equal stars plays a crucial role in determining the motion of objects in their vicinity. Objects will tend to move towards the stars if they are in a region of lower potential, and away from the stars if they are in a region of higher potential. This is because objects naturally move towards areas of lower energy.

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