Angular momentum problem - what am I doing wrong?

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SUMMARY

The discussion focuses on solving an angular momentum problem related to Hohmann transfer orbits in celestial mechanics. The user attempts to derive the velocity boost required for a spacecraft to transition from an initial circular orbit at radius R1 to a larger orbit at radius R2. The key equations involve conservation of energy and angular momentum, leading to the formula for the velocity change: Δv = vA - v1 = sqrt(GM/R1) [sqrt(2R2/(R1+R2)) - 1]. The user struggles with substituting variables correctly, resulting in negative square roots.

PREREQUISITES
  • Understanding of Hohmann transfer orbits
  • Familiarity with conservation of energy and angular momentum principles
  • Knowledge of gravitational forces and orbital mechanics
  • Ability to manipulate algebraic equations involving square roots
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  • Study the derivation of Hohmann transfer orbits in detail
  • Learn about the implications of conservation laws in orbital mechanics
  • Explore the mathematical treatment of elliptical orbits
  • Practice solving problems involving gravitational forces and orbital speeds
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Aerospace engineers, physics students, and anyone interested in orbital mechanics and spacecraft trajectory planning will benefit from this discussion.

henryc09
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Homework Statement


A hohmann transfer orbit is a way of transferring a spacecraft between two planetary orbits (which we shall assume to be circular) by using one half of an elliptical orbit about the sun.

Suppose the spacecraft is initially moving around the sun with orbital speed v1 of the first planet, at radius R1, and we wish to move it to a larger orbital radius R2. Let their orbital speeds of the spacecraft at perihelion (point A)(sorry I can't show you the diagram) and aphelion (point B) in the elliptical orbit be vA and vB respectively. Write down the conditions on vA and vB assuming the planets have a negligible gravitational effect compared to the sun based on: (i) the conservation of energy (ii) the conservation of angular momentum.

Hence show that that the velocity boost required to accelerate the spacecraft into the transfer orbit is
change in v = vA-v1 = sqrt(GM/R1) [sqrt(2R2/(R1+R2)) - 1]

where M is mass of sun


Homework Equations





The Attempt at a Solution


well I think that conservation of energy would be:

0.5mvA^2 - GmM/R1 = 0.5mvB^2 - GmM/R2

divide through by m

conservation of angular momentum would be:

-mR1vA = -mR2vB

R1vA=R2vB

Then you have that the centripetal force acting on the spacecraft when it's moving in a circular orbit is mv1^2/R1 = GmM/R1^2

giving v1 as sqrt(GM/R1)

but then when I say that Vb = VaR1/R2 and substitute this into the conservation of energy equation I end up with negative square roots and can't get to the result it gives. I'm probably being really stupid but could someone talk me through the steps or point out what I'm doing wrong?
 
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