Escape velocity and formulas for circular orbits

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SUMMARY

The discussion focuses on the formulas for circular orbits, specifically the relationship between energy (E), mass (m), gravitational constant (G), and radius (r). The formula E/m=1/2v²-GM/r=constant is established as applicable to all types of orbits, including circular, elliptical, parabolic, and hyperbolic. Escape velocity is defined as the velocity at which E=0, specifically for parabolic orbits. The energy equations for circular and elliptical orbits are confirmed as E=-GMm/2r and E=-GMm/2a, respectively, where 'a' represents the semi-major axis of the ellipse.

PREREQUISITES
  • Understanding of gravitational potential energy in orbital mechanics
  • Familiarity with the concepts of circular and elliptical orbits
  • Knowledge of the gravitational constant (G) and its significance
  • Basic algebra and calculus for manipulating orbital equations
NEXT STEPS
  • Study the derivation of escape velocity in detail
  • Explore the differences between bound and unbound orbits in celestial mechanics
  • Learn about the semi-major axis and its role in elliptical orbits
  • Investigate the implications of energy conservation in orbital dynamics
USEFUL FOR

Astronomy students, physicists, and anyone interested in understanding the mechanics of orbits and escape velocity in celestial bodies.

StephenPrivitera
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In my class, we developed a list of formulas for circular orbits. One of them is E/m=1/2v2-GM/r=constant. To derive escape velocity we find for what v does E=0. But an orbit of this nature is certainly not circular! How can we apply the formula?
 
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Bound orbits are those with E < 0.

- Warren
 
The formula given is true for all orbits; whether they be circular, eliptical, parabolic or hyperbolic.

As Warren pointed out, circular or eliptical orbits will have E<0

A parabolic orbit (the one followed by an object traveling exactly at escape velocity) E=0

For E > 0, you get a hyperbolic orbit.

One thing about circular orbits:

v= [squ](GM/r) at all points. if you substitute this for v in the formula you have it reduces to

E=-GMm/2r

Now, this turns out to be also true for eliptcal orbits if you substitute the semi-major axis(a) for r. (the semi-major axis is half of the longest dimension of the ellipse. It is also the Average length of the radius vector over the course of an orbit. )

This gives

E = -GMm/2a
 

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