What is the ratio between the speeds before and after a short rocket thrust?

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SUMMARY

The discussion focuses on calculating the ratio of speeds before and after a short rocket thrust for a satellite transitioning from a circular orbit around the sun to an elliptical orbit with an aphelion at Jupiter's orbital radius. The participant establishes that the thrust is parallel to the velocity and occurs over a short duration, maintaining equal radii before and after the thrust. The eccentricity of the new orbit is calculated as 0.677 using the formula involving the semi-major axis and the distance from the center of the ellipse to the focus. The participant seeks confirmation on using the vis-viva equation to determine the perihelion speed at Earth's orbital radius.

PREREQUISITES
  • Understanding of orbital mechanics, specifically circular and elliptical orbits.
  • Familiarity with the vis-viva equation for orbital speed calculations.
  • Knowledge of eccentricity and its calculation in orbital dynamics.
  • Basic principles of energy conservation in orbital mechanics.
NEXT STEPS
  • Study the vis-viva equation in detail to understand its application in different orbital scenarios.
  • Research the implications of thrust on orbital mechanics, particularly in elliptical orbits.
  • Explore the calculation of perihelion and aphelion speeds in elliptical orbits.
  • Examine the effects of thrust duration on orbital transitions and speed ratios.
USEFUL FOR

Astronomy students, aerospace engineers, and physicists interested in orbital mechanics and satellite trajectory analysis will benefit from this discussion.

alex3
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Homework Statement


A satellite is in a circular orbit around the sun, radius [tex]r_{e}[/tex], the radius of Earth's orbit. After a short rocket thrust parallel to its velocity, it is in a new orbit with aphelion at Jupiter's orbital radius, [tex]r_{j}[/tex]. What is the ratio of the speed's just before and after the thrust?

2. The attempt at a solution

I'm thinking like this:

  • The thrust is parallel to the velocity and is for a very short time, so the radii before and after the thrust are equal.
  • The aphelion is at Jupiter's orbital radius: the satellite is now describing an elliptical orbit, with an aphelion at Jupiter's orbital radius, and an perihelion at the thrust point; Earth's orbital radius.
  • We need the speed just after the thrust, so we need what the speed would be at the perihelion of the orbit.

Ok so far? I've worked out the eccentricity by using the following logic:

  • The sun is at one focus.
  • The major axis is the [tex]A = r_{j} + r_{e}[/tex], semi-major is [tex]a = \frac{A}{2}[/tex].
  • The distance from the centre of the ellipse to the focus is [tex]ae[/tex], so the eccentricity can be calculated using [tex]a - ae = r_{e}[/tex] and solving for [tex]e[/tex].

I calculated 0.677 for [tex]e[/tex], using

[tex]r_{j} = 7.8 \times 10^{11}[/tex]
[tex]r_{e} = 1.5 \times 10^{11}[/tex]

But how can I deduce the perihelion speed with this data?

EDIT

Is it just as simple as, by energy conservation, using the vis viva equation and setting r to r_e, or will I need some additional calculation?
 
Last edited:
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Vis-viva should do fine.
 

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