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(meteorobs) Large Meteor/Atmospheric Collisions



Below is a clarification from Tony Beresford of something that I posted
recently. Just thought Meteorobs list would find it interesting as well.
George Zay
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 WHEN IT COMES TO DETECTING METEORS, LOS ALAMOS RESEARCHER IS ALL EARS
 
 SAN FRANCISCO, Dec. 18, 1996 - Chicken Little might have liked Los Alamos
 National Laboratory researcher Doug ReVelle, a guy who keeps an "ear" to the
 sky listening for falling objects that travel many times faster than the
 speed of sound.
 
 And each year at least one fairly large extraterrestrial object comes
 rumbling into Earth's atmosphere, said ReVelle, who presented information
 about using very low-frequency sound waves to detect meteors today at the
 American Geophysical Union's Fall Meeting in San Francisco.
 
 ReVelle and colleagues Rod Whitaker, Tom Armstrong and Paul Mutschlecner
 work in the Comprehensive Test Ban Treaty International Monitoring System
 infrasound program in Los Alamos' Earth and Environmental Sciences Division.
 
 Using data from Los Alamos listening stations originally set up to monitor
 underground nuclear explosions, ReVelle, a meteorologist in Los Alamos' new
 Atmospheric and Climate Sciences Group, hears the infrasonic signature
 created when meteors enter the atmosphere -- even if no one is around to see
 them.  The Los Alamos stations, around since 1983, still are enlisted in the
 nation's nuclear non-proliferation efforts, but have provided a way for
 scientists to gain insight into the proliferation of bolides,
 larger-than-average space debris that slams into Earth's atmosphere and
 creates brilliant fireballs in the sky.
 
 "Each year, we see at least one object entering the atmosphere that's about
 six meters in diameter," he said.  "These make an infrasonic signal similar
 to what you'd see from a 15-kiloton explosion, an explosion of 15,000 tons
 of TNT, depending on the object's velocity and density.  And each year we
 see around 10 objects entering the atmosphere that are equivalent to a
 one-kiloton blast -- or about two meters in diameter."
 
 ReVelle often speaks of meteor size in terms of explosive yield because
 meteors and nuclear tests have something in common:  Each creates a
 sound/pressure wave in the atmosphere that can be "heard."
 
 "Infrasonic waves are very low frequency sounds that exist somewhere in the
 realm between hearing and meteorology," ReVelle said.  "These sounds are
 well below the range of human hearing, which ends at about 30 Hertz, but
 actually can be detected as small changes in atmospheric pressure.  If you
 had a barometer that was sensitive enough, you'd be able to see fluctuations
 of several microbars when the waves arrive."
 
 The United States Air Force operated a network of stations to listen for
 nuclear weapons tests.  The network was the nation's first line of warning
 during the 1960s and early 1970s -- until the rise of the satellite era --
 ReVelle said.  With the array, scientists could determine the size and
 origin of the infrasonic waves.
 
 And in the early days of listening for nuclear weapons, the arrival of these
 very low-frequency sound waves sometimes put the nation on very high alert.
 "On Aug. 3, 1963, just before the Bay of Pigs, the stations detected a
 one-megaton event south of Africa," ReVelle said.  "As you can imagine, it
 must have created quite a stir.  It turned out to be a bolide that could
 have been as large as 25 meters in diameter."
 
 Since infrasound monitoring stations were set up, a number of large events
 have been recorded, among them:
 
 o On Sept. 26 and 27, 1962, two separate objects with an equivalent
 explosive force of 20 kilotons and 30 kilotons (each at least six to eight
 meters in diameter), respectively, entered the atmosphere above the Middle
 East .
 
 o On April 1, 1965, the network detected the Revelstoke Meteorite, an object
 somewhere around six meters in diameter.  The meteorite yielded enough
 infrasonic and seismic data that researchers were able to plot a trajectory
 and comb an area of Canadian wilderness in search of the crater.  It was
 never found, but scientists did find about two grams of the object on the
 ground.  The Revelstoke Meteorite was the smallest ever recovered and it was
 comprised of a very soft material known as carbonaceous chrondrite, which
 will crumble when lightly squeezed.
 
 o On February 1, 1994, an object that was about 15 meters in diameter
 slammed into the atmosphere over the Marshall Islands in the Pacific at a
 velocity of about 25 kilometers a second.  Luckily, the fireball, reported
 by some witnesses as being brighter than the sun for about a second, most
 likely came down in the ocean, ReVelle said.
 
 Many large events have been recorded since the 1960s, but 1996 was a
 particularly good year for fireballs, particularly the nights of Oct. 2
 through 4, when nearly a dozen bolides were seen over the Earth.
 
 "The Earth ran into a swarm of these things in October," ReVelle said.  "Who
 knows where they came from; perhaps they were the result of a near-Earth
 asteroid that had collided with something, maybe the moon."
 
 During that period, at least five separate fireballs were noticed and
 recorded above California, as well as two above New Mexico and others above
 the Pacific Northwest.  A particularly bright fireball appeared near Little
 Lake, Calif., on Oct. 3 at around 8:45 p.m. PDT, and could be seen above Los
 Angeles and San Francisco; about 105 minutes earlier, a fireball had
 appeared in the skies above New Mexico.
 
 The California bolide -- estimated to be about three-quarters of a meter in
 diameter and detected by three infrasound stations that were nearly 600
 miles away and 31 California seismic stations -- was seen by more than 200
 people.  Many actually heard the object.
 
 "Sometimes you'll actually hear a hissing or a buzzing noise and you'll turn
 around, look and see a fireball," he said.  "What you're hearing is more of
 an electrical disturbance caused by the object interacting with Earth's
 geomagnetic field.  The perturbation travels at nearly the speed of light,
 while the bolide itself only travels 50 to 100 times faster than the speed
 of sound, and that's why people were able to turn around and see the thing
 after they heard it."
 
 The October fireballs above California and New Mexico were the subject of
 plenty of publicity and speculation.  Researchers originally believed that
 one fireball had entered the atmosphere, skipped back into space, orbited
 Earth once and re-entered the skies again.
 
 ReVelle's infrasonic data and subsequent reports from ground observers
 indicate, however, that the fireballs seen that night above New Mexico and
 California came from two different objects -- trajectories indicate that the
 first bolide didn't enter the atmosphere at an angle that would allow it to
 skip back out into space.
 
 Still, the events intrigue ReVelle and other researchers at Los Alamos,
 Sandia National Laboratory, the University of California at Los Angeles and
 the University of Western Ontario.
 
 "There are a number of questions left to be answered about the Oct. 3
 fireballs," he said, "and there are some things which don't quite add up. 
 You know, I'm not really sure what was happening in the sky that night."
 
 The four arrays of listening stations operated by Los Alamos -- the only
 such network left in regular operation in the world -- can detect meteors
 that are as small as a few centimeters in diameter.  The stations are useful
 because they can help validate other non-proliferation and verification
 techniques, and they cost very little to operate and maintain.
 
 "In the realm of non-proliferation, it's a very inexpensive insurance
 policy, and the array gives us a tremendous opportunity to learn about
 meteors and atmospheric phenomena as well," ReVelle said.
 
 
 Los Alamos National Laboratory is operated by the University of California
 for the U.S. Department of Energy.
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