Posted by James on Thursday, March 19, 2009 at 12:37am.
The sum of potential and kinetic energy is zero. Potential energy per mass (if zero at infinite distance) is -GM/R. Use the fact that the earth's radius is 6378 km. M is the mass of the Earth.
For meteor (1),
-GM/(250,000*10^3)+ (2100)^/2 =
-GM/6378*10^3)+ Vimpact^2/2
For meteor 2,
-GM/(250,000*10^3)+ (2100)^/2 =
-GM/8500*10^3)+ Vmax^2/2
Look up GM and solve.
If Vmax exceeds the escape velocity, it will not return, if this is considered a two-body problem. Because the sun plays a larger role than Earth at large meteor distances, the meteor could return to the same distance from the sun and the ecliptic plane of the Earth's orbit, but the chances are very small the Earth will be there at the time.
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