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Post Info TOPIC: Chicxulub event


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RE: Chicxulub event
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Title: Importance of pre-impact crustal structure for the asymmetry of the Chicxulub impact crater
Authors: Sean P. S. Gulick, Penny J. Barton, Gail L. Christeson, Joanna V. Morgan, Matthew McDonald, Keren Mendoza-Cervantes, Zulmacristina F. Pearson, Anusha Surendra, Jaime Urrutia-Fucugauchi, Peggy M. Vermeesch & Mike R. Warner

Impact craters are observed on the surfaces of all rocky planets and satellites in our Solar System; some impacts on Earth, such as the Cretaceous/Tertiary one that formed the Chicxulub impact crater, have been implicated in mass extinctions. The direction and angle of the impactor its trajectoryis an important determinant of the severity of the consequent environmental damage, both in the downrange direction (direction bolide travels) and in the amount of material that enters the plume of material vaporised on impact. The trajectory of the Chicxulub impact has previously been inferred largely from asymmetries in the gravity anomalies over the crater. Here, we use seismic data to image the Chicxulub crater in three dimensions and demonstrate that the strong asymmetry of its subsurface correlates with significant pre-existing undulations on the end-Cretaceous continental shelf that was the site of this impact. These results suggest that for rocky planets, geological and geomorphological heterogeneities at the target site may play an important role in determining impact crater structure, in addition to impact trajectories. In those cases where heterogeneous targets are inferred, deciphering impact trajectories from final crater geometries alone may be difficult and require further data such as the distribution of ejecta.

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Chicxulub
1996 (black) and 2005 (red) seismic surveys are shown over the Bouguer gravity anomaly map showing the buried Chicxulub impact crater. The black dots are cenotés, the black star is the crater centre and the white line is the coastline. The black dashed line shows the extent of the Cenozoic Chicxulub basin. Faults in the rings (white) can be traced to the near surface, whereas faults in the terrace zone (grey) are buried by breccia. Radial distances to distinct features, such as the start of the ring faults, vary by up to 20 km. .

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The meteorite linked to the mass extinction of dinosaurs and other life forms 65 million years ago was four to six kilometres in diameter. Thats the conclusion of a team of Hawaii University researchers who have evolved a mechanism to measure the size of meteorites that have rammed into earth over millennia.
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Imagine the asteroid impact that killed off the dinosaurs and you may also picture a hellish aftermath of global forest fires. However, soot particles from across the globe now suggest that the smoke that shrouded the world after the collision came from immature oil in rocks at the crater site.
Over 20 years ago, researchers found large volumes of soot in the distinctive layer of iridium-rich sediment that marks the impact, 65 million years ago. Theory had it that the rock from the crater was vaporised, and that the soot came from extensive wildfires sparked by the smash. However, charcoal from burnt plant material is absent in some places, suggesting the fires were not global.

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The asteroid presumed to have wiped out the dinosaurs struck the Earth with such force that carbon deep in the Earth's crust liquefied, rocketed skyward, and formed tiny airborne beads that blanketed the planet, say scientists from the U.S., U.K., Italy, and New Zealand in this month's Geology.
The beads, known to geologists as carbon cenospheres, cannot be formed through the combustion of plant matter, contradicting a hypothesis that the cenospheres are the charred remains of an Earth on fire. If confirmed, the discovery suggests environmental circumstances accompanying the 65-million-year-old extinction event were slightly less dramatic than previously thought.

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Call it extraterrestrial bling. Fossilised sea creatures have been found that coated themselves in tiny diamonds created in the asteroid impact that killed off the dinosaurs.
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It's a cratered spheroid, just the kind of object one imagines striking the Earth about 65 million years ago and wiping out 70 per cent of the planet's species -- including the dinosaurs.

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Scientists have developed a new way of determining the size and frequency of meteorites that have collided with Earth.  Their work shows that the size of the meteorite that likely plummeted to Earth at the time of the Cretaceous-Tertiary (K-T) boundary 65 million years ago was 2.5 to 4 miles in diameter.  The meteorite was the trigger, scientists believe, for the mass extinction of dinosaurs and other life forms.

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The Chicxulub crater
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NASA is advocating that the Mexican zone of Chicxulub, where 65 million years ago a large meteorite impacted, changing the course of evolution on Earth, be declared a World Heritage Site by UNESCO.

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