How Does the Vis-Viva Equation Explain Orbital Speed Changes to Reach the Moon?

  • Thread starter Lucy Yeats
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In summary, it is more efficient to reach the moon by first putting the spacecraft in a low circular Earth orbit, then boosting the speed to create an elliptical orbit with apogee at the moon's orbit and perigee at the initial orbit's radius. Using the Vis Viva equation, we can find the ratio of the speeds at each point, which simplifies to (2ra-r0)/ra. However, this is incorrect as the semi major axis, not the apogee distance, should be used in the equation. The semi major axis can be found using the relationship between the semi major axis and the apogee distance.
  • #1
Lucy Yeats
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Homework Statement


An efficient way to reach the Moon is to first put the spacecraft in a low circular Earth
orbit (radius r0, speed v0). The speed is then boosted to vp giving an elliptical orbit with
apogee at the Moon’s orbit, ra, and perigee at r0. Show that:

(vp/v0)^2=2ra/(r0+ra)

Homework Equations



http://en.wikipedia.org/wiki/Vis-viva_equation

The Attempt at a Solution



Using the Vis Viva equations, I found:
vp^2=GM((2/r0)-(1/ra))
v0^2=GM((2/r0)-(1/r0))=GM(1/r0)

so (vp/v0)^2=((2/r0)-(1/ra))/(1/r0)
Which simplifies to (2ra-r0)/ra, which isn't right.

Where did I go wrong?
 
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  • #2
The vis viva equation is [itex]v^2 = \mu\left(\frac 2 r - \frac 1 a\right)[/itex], where [itex]\mu=GM[/itex] is the gravitational parameter, [itex]r[/itex] is the radial distance, and [itex]a[/itex] is the semi major axis of the orbit.

Your mistake was using the apogee distance in lieu of the semi major axis.
 
  • #3
I thought in this case the apogee distance was the semi major axis? :-/

If not, how do I find the semi major axis?

Thanks for helping!
 
  • #4
Sorry, I've got it now! Thanks! :-)
 
  • #5


It appears that you have made a computational error in your attempt at a solution. The correct equation for the speed at perigee (vp) is vp^2 = GM((2/r0)-(1/ra)), as you have stated. However, the equation for the speed at apogee (va) is va^2 = GM((2/r0)-(1/ra)), not v0^2 = GM((2/r0)-(1/r0)). This is because the speed at apogee is not equal to the speed at the initial circular orbit, but rather is the speed at the point where the spacecraft is farthest from the Earth.

Using the correct equation for va, we get:

vp^2/v0^2 = (GM((2/r0)-(1/ra)))/(GM((2/r0)-(1/r0))) = ((2/r0)-(1/ra))/((2/r0)-(1/r0)) = (2ra-r0)/(2r0-r0) = (2ra-r0)/r0

This can be simplified to (2ra)/(2r0) = ra/r0

Substituting this into the original equation, we get:

(vp/v0)^2 = 2(ra/r0) / (1 + (ra/r0)) = 2ra/(r0+ra)

This matches the desired result, so it appears that the error was in the equation for va.
 

1. What is an elliptical orbit?

An elliptical orbit is a type of orbit in which an object, such as a planet, satellite, or comet, follows a path that is shaped like an ellipse. This means that the object's distance from the body it is orbiting around changes throughout the orbit.

2. How does an elliptical orbit differ from a circular orbit?

An elliptical orbit differs from a circular orbit in that the shape of the orbit is not perfectly round. In a circular orbit, the object's distance from the body it is orbiting around remains constant, while in an elliptical orbit, the distance varies.

3. What causes an object to have an elliptical orbit?

An object has an elliptical orbit due to the influence of gravity. The strength of gravity depends on the mass of the two objects and the distance between them. If the object is closer to the body it is orbiting, gravity will be stronger, causing the object to have a more elliptical orbit.

4. Can any object have an elliptical orbit?

Yes, any object can have an elliptical orbit as long as it is under the influence of gravity from another object. This can include planets, moons, satellites, and even man-made objects such as spacecraft.

5. What are some real-life examples of elliptical orbits?

Many objects in our solar system have elliptical orbits, including planets such as Mars and Pluto, as well as comets and asteroids. The orbits of satellites, such as those used for communication and navigation, are also often elliptical.

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