Energy principle and circular/ellipse orbits

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SUMMARY

The discussion focuses on calculating the energy required to transition an object with mass M from a circular orbit with radius R_1 to an elliptical orbit with an aphelion radius of R_2. The Total Specific Mechanical Energy, denoted as ξ, is defined as inversely proportional to the size of the major axis, expressed mathematically as ξ = -μ/(2a). The energy change required for this transition is calculated using the formula ΔE = -GMm/(2a) - (1/2)mv_1^2 + GMm/R_1, where assumptions about the perihelion radius are necessary for accurate calculations.

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Uniquebum
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Question is as follows:
How much energy do i need when i move an object with a mass M from a circular orbit with a radius of R_1 to an ellipse orbit with aphelion radius of R_2.

I'm assuming energy principle is the way to go here but it leads to a question i'd like someone to help me out with.

Do i need to assume the perihelion radius of the new orbit (aphelion radius R_2) is the circular orbit's radius R_1?

Thanks in advance.
 
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Uniquebum said:
Question is as follows:
How much energy do i need when i move an object with a mass M from a circular orbit with a radius of R_1 to an ellipse orbit with aphelion radius of R_2.

I'm assuming energy principle is the way to go here but it leads to a question i'd like someone to help me out with.

Do i need to assume the perihelion radius of the new orbit (aphelion radius R_2) is the circular orbit's radius R_1?

Thanks in advance.

You can assume anything you like; The answer you get will depend upon your assumptions :smile:

The Total Specific Mechanical Energy, [itex]\xi[/itex], of an orbit is inversely proportional to the size of its major axis. Thus [itex]\xi = -\frac{\mu}{2 a}[/itex] . The length of the major axis, in turn, is the sum of the perihelion and aphelion distances. Specific Mechanical Energy is the energy per unit mass; Multiply by mass of the orbiting object to get the energy.

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Yea, i presumed as much. To get the energy change needed i'd have to go

[itex]\Delta E = -\frac{GMm}{2a} - \frac{1}{2}mv_1^2 + \frac{GMm}{R_1}[/itex]

So basically ellipse orbit total energy minus circular orbit total energy. Since i wasn't given the semi-major axis but only the aphelion radius of the ellipse orbit, i would think i'd need to assume the perihelion radius is the R_1. Either way, i think I'm going with this.
Whatever the case, thanks for the reply!
 

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