Meteor Wake in High Frame-Rate Images-Implications for the Chemistry of Ablated Organic Compounds

Details Meteor Wake in High Frame-Rate Images-Implications for the Chemistry of Ablated Organic Compounds Meteor Wake in High Frame-Rate Images-Implications for the Chemistry of Ablated Organic Compounds

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asbio...4...95j&link_type=abstract

Astrobiology, Volume 4, Issue 1, pp. 95-108.

Biology

4

Scientific paper

Extraterrestrial organic matter may have been chemically altered into forms more ameanable for prebiotic chemistry in the wake of a meteor after ablation. We measured the rate of cooling of the plasma in the meteor wake from the intensity decay just behind a meteoroid by freezing its motion in high frame-rate 1,000 frames/s video images, with an intensified camera that has a short phosphor decay time. Though the resulting cooling rate was found to be lower than theoretically predicted, our calculations indicated that there would have been insufficient collisions to break apart large organic compounds before most reactive radicals and electrons were lost from the air plasma. Organic molecules delivered from space to the early Earth via meteors might therefore have survived in a chemically altered form. In addition, we discovered that relatively small meteoroids generated far-ultraviolet emission that is absorbed in the immediate environment of the meteoroid, which may chemically alter the atmosphere over a much larger region than previously recognized.

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