Calculating the Kinetic Energy of a Meteor: What Factors Influence its Velocity?

Click For Summary

Discussion Overview

The discussion revolves around calculating the kinetic energy of a meteor and the factors that influence its velocity. Participants explore the relevant variables, typical velocities, and the dynamics of meteors and comets in relation to their orbits.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant suggests using the formula for kinetic energy, E = 1/2 mv², where m is mass and v is velocity relative to Earth, noting typical meteor velocities of 10 to 30 km/s.
  • Another participant mentions that ~11 km/s is the minimal velocity corresponding to Earth's escape velocity, while ~30 km/s is the orbital velocity of Earth, with the possibility of higher velocities for objects from the outer solar system.
  • Some participants express surprise at the velocities mentioned, indicating a perception that meteors might be faster.
  • A participant highlights that comets can have varying approach speeds depending on their orbits, specifically noting the difference between prograde and retrograde orbits and referencing Kepler's laws regarding increased speeds at perihelion.

Areas of Agreement / Disagreement

Participants express differing views on the typical velocities of meteors and the factors influencing their speeds, indicating that multiple competing perspectives remain without a clear consensus.

Contextual Notes

The discussion includes assumptions about relative velocities and the influence of orbital dynamics, which are not fully resolved. The specific conditions under which meteors achieve their velocities are not detailed.

Numeriprimi
Messages
135
Reaction score
0
How can I calculate kinetic energy of a meteor? On what variables it depends?

Thanks and sorry for my bad English.
 
Astronomy news on Phys.org
You can use the usual formula for kinetic energy: ##E=\frac{1}{2}mv^2## with the mass m and the velocity v (relative to earth). Typical velocities are 10 to 30 km/s.
 
I thought meteors were faster. :smile:
 
Well, ~11km/s is the minimal velocity, and corresponds to the escape velocity of earth. ~30km/s is the orbital velocity of earth, but most objects nearby have similar orbits, so their relative velocity is lower. Objects from the outer solar system can have higher relative velocities, up to ~75km/s should be possible (but really rare). To get even more speed, you need objects not bound to the solar system.
 
tade said:
I thought meteors were faster. :smile:
30 kms/second is pretty damn fast. That would get them from space to ground in about 3 seconds, if they came in vertically and were not slowed by air resistance.
 
as mbf said 'relative velocity' . comets can have either a prograde or retrograde orbit. so the approach speed of a retrograde is going to be pretty high...
also taking into account keplers second(?) law ...the comet will be most likely at its perihelion when approaching the Sun and so will have an increased speed.
 
Last edited:

Similar threads

  • · Replies 8 ·
Replies
8
Views
4K
  • · Replies 17 ·
Replies
17
Views
3K
  • · Replies 15 ·
Replies
15
Views
1K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
3
Views
1K
Replies
7
Views
11K
  • · Replies 10 ·
Replies
10
Views
924
  • · Replies 33 ·
2
Replies
33
Views
3K
  • · Replies 13 ·
Replies
13
Views
3K