Solve Orbit Calculations Homework: Find Altitude 30 min After Perigee Passage

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SUMMARY

The discussion focuses on solving orbit calculations for determining the altitude 30 minutes after perigee passage using given parameters: perigee altitude (r_p), apogee altitude (r_a), and orbital period (T). The key equations involved include Kepler's equation for eccentric anomaly (E) and the formula for the radius of the orbit (r). The user seeks clarification on solving for E, with Newton's method suggested as a viable approach for finding the eccentric anomaly from the mean anomaly or time since periapsis.

PREREQUISITES
  • Understanding of orbital mechanics concepts, including perigee and apogee.
  • Familiarity with Kepler's laws and equations.
  • Knowledge of numerical methods, specifically Newton's method for solving equations.
  • Basic proficiency in calculating semi-major axis (a) from orbital parameters.
NEXT STEPS
  • Research how to calculate the semi-major axis (a) from perigee and apogee altitudes.
  • Study Kepler's equation in detail, focusing on its application in orbital mechanics.
  • Learn about Newton's method for solving nonlinear equations, particularly in the context of orbital calculations.
  • Explore alternative methods for solving Kepler's equation, such as the bisection method or fixed-point iteration.
USEFUL FOR

Aerospace engineers, physics students, and anyone involved in orbital mechanics or satellite trajectory analysis will benefit from this discussion.

Logarythmic
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Homework Statement


The given data is the perigee altitude [itex]r_p[/itex], the apogee altitude [itex]r_a[/itex] and the period T. Mission: find the altitude 30 min after perigee passage.


Homework Equations


Semi-major axis a is calculated.
Kepler's equation gives a relation for the eccentric anomaly E:

[tex]E - \epsilon \sin{E} = \frac{2 \pi}{T} \left( t - t_p \right)[/tex]

The radius of the orbit is given by

[tex]r = a \left( 1 - \epsilon \cos{E} \right)[/tex]


The Attempt at a Solution



How do I solve for the eccentric anomaly E so I can use the formula for the radius? Or should I use another approach?
 
Physics news on Phys.org
There are a number of ways to solve Kepler's equation for the eccentric anomaly given either the mean anomaly or time since periapsis, Newton's method being one of them.
 

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