Calculating Semimajor Axis of Meteor Orbit

In summary, to find the length of the semimajor axis of a meteor's orbit given its observed altitude of 6km, initial velocity of 20 km/s, and deceleration rate of 0.2km/s^2, you would need to estimate the meteor's speed before entering Earth's atmosphere and use the conservation of energy to determine its unperturbed state vector and orbital elements. This could be done by observing the meteor from multiple angles and using Runga-Kutta calculations.
  • #1
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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  • #2
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.
 

1. What is the semimajor axis of a meteor's orbit?

The semimajor axis of a meteor's orbit is the half of the longest diameter of the elliptical orbit that the meteor follows around the Sun.

2. How is the semimajor axis calculated?

The semimajor axis can be calculated using the following formula: a = (p^2)/(T^2), where a is the semimajor axis, p is the meteor's orbital period, and T is the meteor's orbital period in Earth years.

3. Why is the semimajor axis important in studying meteor orbits?

The semimajor axis is important because it provides information about the size and shape of the meteor's orbit. It can also be used to determine the meteor's distance from the Sun at any given point in its orbit.

4. How does the semimajor axis affect a meteor's orbital velocity?

The semimajor axis is directly related to the orbital velocity of a meteor. The larger the semimajor axis, the slower the orbital velocity and vice versa. This is because the speed of an object in an elliptical orbit decreases as it moves further away from the center of mass.

5. Can the semimajor axis change over time?

Yes, the semimajor axis of a meteor's orbit can change over time due to various factors such as gravitational interactions with other objects in the solar system, atmospheric drag, and solar radiation pressure. However, in most cases, these changes are small and can only be observed over long periods of time.

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