What temperature do small meteorites have on impact A question which has haunted me for years. What temperature do small meteorites (which don't evaporate on impact) have if you find them immediately after they hit the surface. I understand that the outer parts are heated by atmospheric friction, but what about the inside? Can the inside keep its low temperature that it inherits from space?

There are some stories on the internet about meteorites that were so cold, that the moisture of the air froze on the surface of the meteorite. Can this really happen?

Subquestion:


Are there numerical simulations that can prove this?


Some of the rumours are summed up here:
"Frosty" meteorite (Wikipedia).
Love &amp; Brownlee (1991) put together numerical models for the experiences of micrometeorites entering the atmosphere. They say:


  The peak temperatures experienced by submillimeter micrometeoroids rarely exceed 1700°C. Maximum temperature and mass loss rate generally occur at altitudes between 85 and 90 km during ∼1 sec of peak heating. A typical melted particle spends ∼2 sec at temperatures above the melting point.


Flynn (1989) discusses interplanetary dust, with figures for peak temperatures given in the abstract.

But I think that what you really want is Sears (1975), Temperature gradients in meteorites produced by atmospheric passage:


  Temperatures in the order of 200°C have usually penetrated no further than 5-10mm, which is consistent with a luminous flight time of the order of 10s.


Using the geologists' rule of thumb for timescales of cooling (I believe $\tau^2 = \ell/\kappa$, where $\tau$ is the timescale, $\ell$ is the thickness of the cooling body, and $\kappa$ is the thermal conductivity - though it's a while since I've had to do this so I may be misremembering...), the information above about the height above the surface at which peak temperature is commonly reached, and an estimate of particle velocity, you can probably back-of-envelope a temperature for a meteorite on impact!