Slowpoke: atmosphere put brakes on meteorite that formed famed crater.The extraterrestrial object that gouged out northeastern Arizona's Meteor Crater about 50,000 years ago struck Earth at a speed much slower than most scientists had previously proposed. When a meteorite meteorite, meteor that survives the intense heat of atmospheric friction and reaches the earth's surface. Because of the destructive effects of this friction, only the very largest meteors become meteorites. slams into Earth, the crater that's created usually contains both Earth and space rocks that were melted by the kinetic energy kinetic energy: see energy. kinetic energy Form of energy that an object has by reason of its motion. The kind of motion may be translation (motion along a path from one place to another), rotation about an axis, vibration, or any combination of of the collision (SN: 6/15/02, p. 378). Meteor Crater holds much less melted rock than expected, says H. Jay Melosh Dr. H. Jay Melosh (born June 23, 1947) is an American geophysicist, renowned as an expert on impact cratering. He earned a degree in physics from Princeton University and a doctoral degree in physics and geology from Caltech in 1972. Dr. of the University of Arizona (body, education) University of Arizona - The University was founded in 1885 as a Land Grant institution with a three-fold mission of teaching, research and public service. in Tucson. Previously, scientists had proposed that groundwater at the impact site vaporized va·por·ize tr. & intr.v. va·por·ized, va·por·iz·ing, va·por·iz·es To convert or be converted into vapor. va and dispersed, taking with it much of the molten rock that had formed when the 40-meter-diameter iron meteorite hit. Now, Melosh and Gareth S. Collins of Imperial College London History Imperial College was founded in 1907, with the merger of the City and Guilds College, the Royal School of Mines and the Royal College of Science (all of which had been founded between 1845 and 1878) with these entities continuing to exist as "constituent colleges". have come up with an alternate theory to explain the missing melted rock. Computer simulations of the aerodynamic forces pummeling meteorites Meteorites See also astronomy. aerolithology the science of aerolites, whether meteoric stones or meteorites. Also called aerolitics. astrolithology the study of meteorites. Also called meteoritics. blazing through Earth's atmosphere indicate that those objects often break up at high altitudes (SN: 7/19/03, p. 36). When Melosh and Collins used similar models to analyze the voyage of the meteorite responsible fur Meteor Crater, they were surprised to find how much the atmospheric drag seemed to have slowed the incoming object before it struck the ground. Most extraterrestrial objects enter Earth's atmosphere at speeds between 15 and 20 kilometers per second, fast enough to cross the United States in 4 to 5 minutes. In the new study, the researchers simulated the brief journey of a 300,000-ton iron meteorite piercing the upper atmosphere at 17 km/sec. At an altitude of about 70 km, where the air is less than 1 percent as dense as it is at sea level, the meteorite began slowing down. Aerodynamic forces began to break apart the meteorite when it reached an altitude of around 14 km. By the time the object reached an altitude of 5 km, its outer layers had fragmented into a cloud measuring about 200 m across and moving at 13 km/sec. A split second later, at a speed of only 12 km/sec, the fragment cloud and the object's 150,000-ton core slammed into the ground. The object's deceleration deceleration /de·cel·er·a·tion/ (de-sel?er-a´shun) decrease in rate or speed. early deceleration , for which scientists hadn't previously accounted, explains the dearth of melted material at Meteor Crater, Melosh and Collins conclude in the March 10 Nature. Philip A. Bland, a planetary scientist also at Imperial College London, concurs with the new analysis. He adds that even though half of the incoming meteorite was battered to fragments, the craters formed by the core and most of those pieces overlapped to create one massive hole about 1.2 km across. Only a few tons of the original meteorite have been found on the plains surrounding the crater. |
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