London, Apr 26 (ANI): Researchers are learning details about asteroid impacts going back to the Earth's early history by using a new method for extracting accurate information from tiny "spherules" embedded in layers of rock.
The spherules were created when asteroids crashed into the Earth, vaporizing rock that expanded into space as a giant vapour plume.
Small droplets of molten and vaporized rock in the plume condensed and solidified, falling back to Earth as a thin layer.
The round or oblong particles were preserved in layers of rock, and now researchers have analysed them to record precise information about asteroids impacting Earth from 3.5 billion to 35 million years ago.
"What we have done is provide the foundation for understanding how to interpret the layers in terms of the size and velocity of the asteroid that made them," said Jay Melosh, an expert in impact cratering and a distinguished professor of earth and atmospheric sciences, physics and aerospace engineering at Purdue University.
The findings, based on geologic observations, support a theory that the Earth endured an especially heavy period of asteroid bombardment early in its history.
The period of heavy asteroid bombardment - from 4.2 to 3.5 billion years ago - is thought to have been influenced by changes in the early solar system that altered the trajectory of objects in an asteroid belt located between Mars and Jupiter, sending them on a collision course with Earth.
"That's the postulate, and this is the first real solid evidence that it actually happened," Melosh said.
"Some of the asteroids that we infer were about 40 kilometers in diameter, much larger than the one that killed off the dinosaurs about 65 million years ago that was about 12-15 kilometers.
"But when we looked at the number of impactors as a function of size, we got a curve that showed a lot more small objects than large ones, a pattern that matches exactly the distribution of sizes in the asteroid belt. For the first time we have a direct connection between the crater size distribution on the ancient Earth and the sizes of asteroids out in space."
Because craters are difficult to study directly, impact history must be inferred either by observations of asteroids that periodically pass near the Earth or by studying craters on the moon. Now, the new technique using spherules offers a far more accurate alternative to chronicle asteroid impacts on Earth, Melosh said.
"We can look at these spherules, see how thick the layer is, how big the spherules are, and we can infer the size and velocity of the asteroid," Melosh said.
"We can go back to the earliest era in the history of the Earth and infer the population of asteroids impacting the planet."
For asteroids larger than about 10 kilometers in diameter, the spherules are deposited in a global layer.
"Some of these impacts were several times larger than the Chicxulub impact that killed off the dinosaurs 65 million years ago," Purdue physics graduate student Brandon Johnson said.
"The impacts may have played a large role in the evolutional history of life. The large number of impacts may have helped simple life by introducing organics and other important materials at a time when life on Earth was just taking hold."
A 40-kilometer asteroid would have wiped out everything on the Earth's surface, whereas the one that struck 65 million years ago killed only land animals weighing more than around 20 kilograms.
"Impact craters are the most obvious indication of asteroid impacts, but craters on Earth are quickly obscured or destroyed by surface weathering and tectonic processes," Johnson said. "However, the spherule layers, if preserved in the geologic record, provide information about an impact even when the source crater cannot be found."
The Purdue researchers studied the spherules using computer models that harness mathematical equations developed originally to calculate the condensation of vapour.
The spherules are about a millimeter in diameter.
The researchers also are studying a different type of artifact similar to spherules but found only near the original impact site. Whereas the globally distributed spherules come from the condensing vaporized rock, these "melt droplets" are from rock that's been melted and not completely vaporized.
Findings from the research may enable Melosh's team to enhance an asteroid impact effects calculator he developed to estimate what would happen if asteroids of various sizes were to hit the Earth.
The calculator, "Impact: Earth!" allows anyone to calculate potential comet or asteroid damage based on the object's mass.
The study has been published online in the journal Nature. (ANI)
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