by kovil » Sat Nov 25, 2006 6:12 pm
Fascinating , hadn't really thought in depth about all that.
Time and force. How fast is the meteor moving, how much resistance does the atmosphere generate, how long does the descent take.
Can any heat generated have time in a 'heat flow diagram' approach to reach very far into the interior of the meteor ?
Will the atmospheric resistance force, vector into the meteor and cause structural fracture lines to develop and tear it apart in chunks ?
The composition of the meteor will affect these results, metallic or stoney or aggregate conglomerate; vastly different results to atmospheric interaction.
Yes, the meteor will be ambient temperature at arrival, plus the suns heating, minus its own ability to radiate.
My feeling is the descent, 3 to 13 seconds before impact is not enough for heat to penetrate much from its surface. Its surface could be 500 F up to 30 seconds after landing, even while its interior is -390 F. This is assuming a stoney meteorite 24" in diameter. (All a wild intuitive guess)
The blackened thin crust in the photo, suggests a very hot skin, with a cool interior. The intense heat of entry may cause spalling, like when an oxyacetylene torch is held close to concrete, and it boils the water out of hydration with the limestone, causing pops and flying chunks of concrete !
Fascinating , hadn't really thought in depth about all that.
Time and force. How fast is the meteor moving, how much resistance does the atmosphere generate, how long does the descent take.
Can any heat generated have time in a 'heat flow diagram' approach to reach very far into the interior of the meteor ?
Will the atmospheric resistance force, vector into the meteor and cause structural fracture lines to develop and tear it apart in chunks ?
The composition of the meteor will affect these results, metallic or stoney or aggregate conglomerate; vastly different results to atmospheric interaction.
Yes, the meteor will be ambient temperature at arrival, plus the suns heating, minus its own ability to radiate.
My feeling is the descent, 3 to 13 seconds before impact is not enough for heat to penetrate much from its surface. Its surface could be 500 F up to 30 seconds after landing, even while its interior is -390 F. This is assuming a stoney meteorite 24" in diameter. (All a wild intuitive guess)
The blackened thin crust in the photo, suggests a very hot skin, with a cool interior. The intense heat of entry may cause spalling, like when an oxyacetylene torch is held close to concrete, and it boils the water out of hydration with the limestone, causing pops and flying chunks of concrete !