Calculating Semimajor Axis of Meteor Orbit

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SUMMARY

The discussion focuses on calculating the semimajor axis of a meteor's orbit given specific parameters: an altitude of 6 km, an initial velocity of 20 km/s, and a deceleration rate of 0.2 km/s². To derive the semimajor axis, one must first estimate the meteor's speed at Earth's position without gravitational interference. Utilizing the Runga-Kutta method allows for accurate back-calculation of the meteor's velocity prior to atmospheric entry. Finally, applying the conservation of energy principle enables the determination of the meteor's hypothetical unperturbed state vector, from which the semimajor axis can be calculated.

PREREQUISITES
  • Understanding of orbital mechanics and semimajor axis calculations
  • Familiarity with the Runga-Kutta numerical method for solving differential equations
  • Knowledge of conservation of energy principles in physics
  • Basic concepts of meteor dynamics and atmospheric entry effects
NEXT STEPS
  • Study the Runga-Kutta method for numerical integration in orbital mechanics
  • Research conservation of energy applications in celestial mechanics
  • Explore methods for estimating unperturbed state vectors in astrodynamics
  • Investigate the effects of atmospheric drag on meteor trajectories
USEFUL FOR

Astronomers, astrophysicists, and aerospace engineers involved in meteor trajectory analysis and orbital calculations will benefit from this discussion.

crystalplane
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if i know a meter is observed at an altitude of 6km, to be traveling with an initial velocity of 20 km/s and the decelerating at a rate dv/dt=0.2km/s^2, which formula i should use to get the length of the semimajor axis of the meteor'orbit?
 
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crystalplane said:
if i know a meter is observed at an altitude of 6km, to be traveling with an initial velocity of 20 km/s and the decelerating at a rate dv/dt=0.2km/s^2, which formula i should use to get the length of the semimajor axis of the meteor'orbit?

You would have to estimate the speed the meteor would have at Earth's position if Earth had not been in the way to accelerate it with gravity and then decelerate it with atmosphere. Probably you'd want multiple observers with multiple exposures on film so that you could know the direction of meteor flight and deduce the speed of the meteor between each observed position. Then use Runga-Kutta to back out the velocity before it hit the atmosphere. Then apply the conservation of energy to get the speed in the absence of Earth's gravitational acceleration. Then you can infer what the hypothetical unperturbed state vector of the meteor would have been, and from there you can derive the elements of the meteor's former orbit.
 

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