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Meteorite Study Published
ICTP junior associate co-authors Science article
A study of a crater recently discovered in southern Egypt concludes that
the Earth may be more vulnerable to large meteorite impacts than
previously thought.
Results of the study have been published in a paper co-authored by ICTP
junior associate Mohamed El Gabry that appears in the 22 July online
version of Science magazine. The paper, titled "The Kamil Crater in
Egypt", analyzes the crater's well-preserved features and concludes that
iron meteorites with a mass of tens of tons can indeed penetrate the
Earth's atmosphere and remain in intact, contrary to geophysical model
predictions.
"Current impact models state that iron meteors around this size and mass
should break into smaller chunks before impact," explained El Gabry,
adding, "Instead, the existence of the new-found crater implies that up
to 35% of these iron giants may actually survive whole, and thus have
greater destructive power."
Based on the average diameter of the impact crater—about 45 meters, with
16 meters depth—scientists estimate that the size of the meteorite was
about 1.3 meters in diameter, weighing about 9,000 kg, and that its
pre-atmospheric mass would have been between 20,000 to 40,000 kg.
Geophysical models have held that meteorites with masses of less than
3x106 kg become fragmented when passing through the Earth's atmosphere.
El Gabry said that the Kamil Crater is the most conserved crater found
yet. "While small meteorite impact craters are common surface structures
on solid planetary bodies in the solar system, they are rare on Earth
due to the relative ease with which smaller structures can be buried by
post-impact sediments or destroyed by erosion. The few identified have
lost many of their primary features. As a consequence, knowledge of
their formation mechanism, their effect on the environment, and of the
hazard small impactors pose to human populations is largely based on
theoretical models and experimental analogs," he said.
El Gabry is a seismologist with the National Research Institute of
Astronomy and Geophysics in Helwan, Egypt. He has been an ICTP junior
associate since 2005.