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

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Homework Statement


The given data is the perigee altitude r_p, the apogee altitude r_a 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:

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

The radius of the orbit is given by

r = a \left( 1 - \epsilon \cos{E} \right)


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?
 
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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.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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