|
|
|||||||||||||||||||||
|
|||||||||||||||||||||
|
|
|||||||||||||||||||||
|
What would happen if a 10-kilometer-diameter asteroid penetrated Earth's crust at a speed of 15 to 20 kilometers per second? The kinetic energy of such an asteroid (more than 6 miles in diameter) would equal the energy of 300 million nuclear weapons and create temperatures hotter than on the sun's surface for several minutes. The expanding fireball of superheated air would immediately wipe out unprotected organisms near the impact and eventually lead to the extinction of many species worldwide. Immediate effects would include an eardrum-puncturing sonic boom, intense blinding light, severe radiation burns, a crushing blast wave, lethal balls of hot glass, winds with speeds of hundreds of kilometers per hour, and flash fires. Longer-term effects would alter Earth's climate. The vapor and debris thrust into the stratosphere would block sunlight for months, lowering global temperatures. Organisms that could not adapt to this impact version of a "nuclear winter" would die. Since plants derive energy from the sun, they would be affected first. As plants die, the decreased food supply and oxygen levels would affect the herbivores first, followed by the carnivores and on up the food chain. Birds, fish, mammals, and small reptiles could survive the cold, desolate "winter" if they could burrow underground or live in caves and consume alternate food sources such as seeds, roots, and decaying matter. Most large reptiles would perish. 3-D Simulation A team from the Applied Physics Division recently announced the results of a three-dimensional (3-D) simulation created with codes developed at Los Alamos. Galen Gisler, Bob Weaver, and Charles Mader, working with Michael Gittings of Science Applications International Corporation, have generated a dynamic picture of the asteroid impact. They collaborated with Jay Melosh and a research team from the University of Arizona, who offered advice on the simulation physics and parameters. [figure: simulating the Chicxulub asteroid impact] Their model focuses on the early-time effects: when the asteroid plunges through Earth's atmosphere and into water and layers of calcite, granite, and mantle. Craters are formed by the explosion of vaporized rock produced as the asteroid's kinetic energy is dissipated through contact with Earth's surface. Steeper impacts result in deeper penetration, but shallower impacts produce larger craters. To understand the importance of the impact angle, Gisler simulated three different angles: 30, 45, and 60 degrees. He discovered that a lower angle of impact is much more efficient at focusing thermal energy into the troposphere, where Earth's weather occurs. "I wasn't smart enough to know this before the simulation," said Gisler. This focusing occurs mainly downrange, carrying the horizontal momentum of the asteroid. Thus, if the Chicxulub asteroid arrived at a low impact angle from a southerly direction, it could have set fire to all the forests in North America. Indeed, soot deposits are found in the continent's iridium layer, formed 65 million years ago (see What Killed the Dinosaurs?). This simulation builds on Gisler's earlier work in modeling giant impact-generated tidal waves, called tsunamis. He and his co-workers completed the largest and most accurate 3-D models of tsunamis caused by asteroids. They simulated six asteroids of varying sizes crashing into the ocean at a speed of 20 kilometers per second. The simulations have potential value in planning emergency response to the huge waves. Beyond Dinosaurs An asteroid impact on land could cause vast forest fires such as the famous Tunguska event of 1908, when such an impact devastated 2,000 square kilometers of Siberian forest. It could also cause global climate changes, possibly severe enough to destroy civilization. A marine impact could generate a tsunami capable of inundating the coasts on both sides of the ocean. Destructive impacts such as Tunguska are likely to happen but once every thousand years. And there is only a 1 in 200,000 chance that a 1-kilometer-diameter asteroid will hit Earth in a given year. Still, scientists do not want to be caught off guard. They would like to be able to identify risks, predict the occurrence of significant impacts, prepare for future impacts, and even mitigate the effects of an impact. Gisler and his team are contributing to this research.
|
Researcher Galen Gisler (left) points out features of the debris
curtain formed in a simulation of the Chicxulub asteroid impact. The complex computation
for the simulation ran on a section of the Q machine A radar image of the southwest portion of the buried Chicxulub
impact crater. Galen Gisler received a B.S. in physics from Yale
University and a Ph.D. in astrophysics from the University of Cambridge.
He has been at Los Alamos since 1981. Before studying asteroid impacts,
he worked in the fields of astrophysics, plasma physics, adaptive
processing, and astronomical transients. | |||||||||||||||||||
|
Operated by the Los Alamos National
Security, LLC for the U.S. Department
of Energy's NNSA
Inside | © Copyright 2007-8 Los Alamos National Security, LLC All rights reserved | Disclaimer/Privacy |