Undergrad Solving for Orbital Mechanics

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SUMMARY

This discussion focuses on solving the orbital mechanics of Sputnik 1, specifically using its orbital circumference and period to derive velocity and momentum. The path of a satellite in free-fall around a planet is approximated as an elliptical orbit, described by Kepler's laws. To fully characterize the orbit, seven parameters are required, typically derived from initial position and velocity vectors or orbital elements, such as 2-line elements. The discussion emphasizes the importance of the orbital period in calculating the semi-major axis and relating perigee and apogee.

PREREQUISITES
  • Understanding of Kepler's laws of planetary motion
  • Familiarity with orbital elements and 2-line elements
  • Basic knowledge of momentum and velocity calculations
  • Ability to interpret and apply equations related to orbital mechanics
NEXT STEPS
  • Research how to calculate the semi-major axis from orbital period
  • Study the relationship between perigee and apogee in elliptical orbits
  • Explore the use of initial position and velocity vectors in orbital mechanics
  • Examine the equations provided in the resource on orbital mechanics at Bogan.ca
USEFUL FOR

Aerospace engineers, astrophysicists, students of orbital mechanics, and anyone interested in the calculations related to satellite orbits.

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TL;DR
I'm working on solving for Orbital Mechanics of a satellite. I have the velocity and the momentum and now I'm stuck and don't know what to do next.
I'm working on solving the orbital path of Sputnik 1(even though it's not in orbit any more) and I'm stuck. I have the circumference of the original orbit, and I have the time it took to orbit which gave me the velocity, which I then used to get the momentum. Can anyone tell me what to do next?
 
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Welcome to PF.

In general, the path of a satellite that continues to free-fall around a planet can as a good approximation be described as an elliptical orbit, which is a specialization of a Kepler orbit. For a more complete (3D) description of the orbit of a particular object in relation to the Earth one needs 7 parameters, usually given by the initial position and velocity vectors at epoch or by the set of orbital elements for the object, which historically has been given as 2-line elements.

So if you have the orbital period of a satellite around Earth you should be able to locate the equation that that will yield you, say, the semi-major axis of the orbit. From this you can further relate perigee and apogee if that is what you seek. If this doesn't help, perhaps you can show us what equations and numbers you have so far and what measure it is you seek.
 
I do not have a good working knowledge of physics yet. I tried to piece this together but after researching this, I couldn’t figure out the correct laws of physics to combine to develop a formula to answer this question. Ex. 1 - A moving object impacts a static object at a constant velocity. Ex. 2 - A moving object impacts a static object at the same velocity but is accelerating at the moment of impact. Assuming the mass of the objects is the same and the velocity at the moment of impact...

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