The deceleration of meteors is computed theorically as a function of the characteristic quantities of evaporation, in particular, of velocity. I+ is shown that for over 3/4 of all meteors, the deceleration increases until the end of evaporation, and that, at the point of maximum rate of evaporation, the deceleration, as a first approximation, may he assumed the same for all meteors.
展开▼