| LSU Geologist and Team Locate Evidence of Earliest
Known Meteor Strike
"There was almost certainly life
at this time. Primitive, bacterial life, and if the
impacts were made by a meteor 20 miles in diameter,
they would have killed everything on the surface of
the Earth."
—Gary Byerly, LSU Professor of
Geology
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A huge meteor, between 12 and 30 miles in diameter, smashed into
the Earth 3.5 billion years ago with the energy of 1 billion atomic
bombs, vaporizing the surface where it struck and creating a tsunami
more than half a mile high that raced around the world at 500 miles
per hour.
This cataclysm is the earliest known meteor strike to hit the
Earth, and one of at least four that has been identified in a geologically
brief 300-million-year period.
LSU
geologist Gary Byerly led an expedition to discover traces of
the impact. While rumors of such an event had lingered for quite
some time, scientists were reluctant to believe the speculations
without proof.
Byerly; Xiaogang Xie, a research associate with LSU’s
Department of Geology & Geophysics; and Donald Lowe and
Joseph Wooden of Stanford University identified traces of the event
in some of the oldest known rocks on Earth—in South Africa
and northwest Australia.
A Cataclysmic Catastrophe
When
the asteroid hit, it was vaporized by the extreme energy of the
impact. Condensation of this vapor produced droplets of melt, called
spherules. Over the next few days, the spherules dropped into the
roiling sea and were deposited in layers on the sea floor.
Byerly said it was not known where the meteor hit, but it was
probably some distance from where they found the spherules and probably
in water rather than on land. He deduced this because the composition
of the spherules lacked the mineral composition that would have
been expected from vaporization of the continental crust, and because
more water covered the Earth’s surface then.
Byerly illustrated his conclusion with a slab of grayish rock.
Measuring about the size of a large hand, the slab consisted of
layers of spherules interlaced with layers of finer sand or silt.
"It would take about 30 hours from impact for
the tsunami to travel all the way around the world. Then, of course,
it wouldn't stop, but bounce all the way back till it met itself
30 hours later, then bounce the other way again, setting up a harmonic."
he said.
Several thin layers of mud within the spherule layer represent
periods of quiet sedimentation between the arrival of tsunami waves.
According to Byerly, the water would likely have inundated everything
but the mountains and eroded the continental land masses, changing
their coastlines dramatically.
The heat of the impact would have evaporated the upper 30 to 300
feet of water in the oceans. It would also have killed everything,
or almost everything, that was alive at that time on land or near
the ocean surface.
"There was almost certainly life at this time.
Primitive, bacterial life, and if the impacts were made by a meteor
20 miles in diameter, they would have killed everything on the surface
of the Earth," he said.
First a hot steam of molten rock and water would have withered
most life, then the tsunamis would have destroyed even more. After
that, years of incredibly cold winters, caused by particles in the
atmosphere blocking out the sun, would have conspired to kill nearly
everything else.
"Anything that survived would have been in
deep rocks or below the surface of the Earth," he said.
Nearly Two Decades of Research
Byerly first came upon evidence of these impacts by chance in
1984 while he was studying ancient volcanism in Australia and South
Africa. He published his first paper on the impacts in 1986.
In 2002, he and his team had four papers published on the subject,
which were featured in an August issue of Science,
and were interviewed by National
Public Radio.
It is now generally accepted that the inner solar system was battered
twice by massive meteor impacts of mysterious origin.
“It is assumed that the solar system was created
by a cloud of dust and rocks that condensed into the sun and planets,
with larger and larger chunks falling near the end. This process
would have finished about 4.5 billion years ago.
"But about 3.8 billion years ago the inner
solar system was torn up by some cataclysmic event. The evidence
is found in the crater basins on the moon and Mars and Venus."
The Earth was probably heavily battered at that time too, but since
the oldest known surface rocks on Earth are about 3.5 billion years
old, no evidence of that exists, Byerly said.
A second battering took place 3.5 billion years ago, and it is
this event that left the record in the rocks Byerly is studying.
This was a smaller series of impacts with a gradual dropoff rate,
he said. That the 3.8 billion-year-old event occurred is accepted
by most scientists. Byerly's work is substantiating the existence
of the second which, up to now, has not been as well accepted.
Byerly
and his team have been able to date the event accurately using SHRIMP
RG, an instrument at Stanford that measures the decay of uranium
into lead.
The uranium was found in zircon crystals at both the Australian
and South African sites and was dated to within 2 million years
of 3.47 billion years ago. The fact that zircons of identical ages
were found in impact strata on two continents shows the worldwide
effects of the impact, Byerly said.
The zircons were not created by the impact but probably by volcanic
action and deposited in the impact layers when the tsunami washed
over the land.
Could it happen again?
These massive, early impacts were similar to the one that killed
the dinosaurs 65 million years ago. But, they were hundreds to thousands
of times more powerful. Probabilities for a similar impact today
are predicted to be about one such strike every 100 million years.
"What that means is, eventually there will
be another such event. We know that large asteroids get disturbed
by interactions with Jupiter and fall into Earth's orbit. When that
happens they will strike the Earth. We can't say when it will happen,
but we can say for certain that it will happen," Byerly said.
The evidence is on a small, grayish slab of rock on his desk.
Back to top
Written by Ronald Brown| University
Relations
April 2003
Related Links
Department of
Geology & Geophysics
Department
of Geology & Geophysics-Byerly’s research
Gary Byerly’s homepage
Stanford
University-Press Release
Stanford University’s
SHRIMP RG
Science
magazine article (August 23, 2002)
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