There was a recent discussion on a social media forum about a stone from the 
recent Punggur fall being warm enough on impact to melt a synthetic bedsheet.  
I followed the discussion with interest but don't have an account on that 
platform - so wanted to post here.  The original poster also referenced the 
other recent Indonesian fall (Kolang), where a finder reported the stone felt 
as if it had been "cooked with sunlight".  There are many other references to 
freshly fallen meteorites being warm or hot to the touch, or sometimes cold to 
the touch.  The oft-repeated rebuttal is that meteoroids come from the icy void 
of space where they must be extremely cold, and that any brief heating 
experienced during the luminous ablative phase will dissipate during the few 
minutes of dark flight through the atmosphere.  Also, that the human brain will 
trick surprised finders into misinterpreting "very cold" for "very hot".  It 
seems to me that there's an obvious error in this argument - the initial 
condition of a meteoroid being very cold is not (necessarily) true.  In fact 
the opposite can be true - meteoroids (or asteroids) can actually be very hot 
prior to Earth impact.  "Cooked with sunlight" is an extremely good description.
Consider figure 1 from Delbo and Harris "Physical properties of near-Earth 
asteroids from thermal infrared observations and thermal modeling", published 
in 2002 in MAPS:
https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.2002.tb01174.x

The sunlight side of a model asteroid at 1 AU has a temperature of about 400 
Kelvin = 127 C = 260 F.  The side facing away from the sun will be cooler; how 
much cooler will depend on the thermal inertia of the body, pole orientation, 
rotation speed, etc.  There may be steep temperature gradients across an 
asteroid at impact time, or it may be relatively equilibrated.  Most meteorite 
droppers should fall into the latter category, being small (sub-meter), fast 
rotators, and regolith free.
How much heat is gained during ablation, and retained during dark flight, ought 
to depend on the thermal inertia of the meteorite.  Metal-rich meteorites or 
those with low porosity ought to retain more heat, and be less efficiently 
cooled during dark flight.
So - are fresh meteorites hot or cold on impact?  I think the answer is, "it 
depends!".  One could even contrive a set of circumstances where an asteroid 
with a large thermal gradient drops two meteorites of equal sizes right next to 
each other, coming from different parts of the asteroid, where one lands hot 
and the other lands cold.  Tarp-melting hot?  I don't see why not.  Cold enough 
to form frost?  Sure.  Hot enough to ignite a grass fire?  No.
Regards,
Eric Christensen

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