The signs of the impact are vague, because most of the crater has eroded. Geological processes, such as plate tectonics and volcanism, have almost completely eroded Earth's oldest impact craters.
But the Sudbury and Chicxulub craters, along with a third in Vredefort, South Africa, are still visible enough to provide clues to the planet's formative years.
Today the Sudbury impact basin is about 37 miles (60 kilometers) long and 19 miles (30 kilometers) wide. Mungall and his colleagues believe the crater was originally about 155 miles (250 kilometers) in diameter.
Scientists looking for signs of the impact must cover a large area of ground, and much of the evidence they look for is small.
According to Mungall, the most convincing pieces of evidence are shatter conesconed-shaped fractures in the rock ranging in size from inches to tens of feet across.
"The only way you can get shatter cones is when extremely strong shock waves are passing through material. They don't form any other way," he said. "The only other places you see them on Earth are around nuclear test sites."
Other bits of evidence include microscopic, flaky diamonds formed by the passage of shock waves through carbon-rich rocks. The shock waves also transform tiny mineral crystals into glass.
To make the Sudbury impact crater, the meteorite would have to have been about 6 miles (10 kilometers) in diameter traveling at 89,000 miles per hour (143,232 kilometers per hour), Mungall says.
Shock waves from the meteorite as it plunged into Earth likely caused up to 6,500 cubic miles (27,000 cubic kilometers) of crust to melt, he says.
A plume of superheated rock from the deepest part of the 19- to 25-mile-thick (30- to 40-kilometer-thick) crust then flew upward and landed on top of the impact site, essentially turning the crust there inside out, Mungall explains.
Mungall also suggests that the meteorite vaporized on impact. Its components then condensed and rained back down.
This, he says, would account for the increased concentrations of iridiuma rare metal found mainly in the Earth's mantle and in meteoriteshe and his colleagues found in the upper layers of the crater's crust.
The Sudbury site also has relatively low concentrations of magnesium and nickel, two elements that are common in Earth's mantle. The researchers therefore concluded that the iridium originated from the meteorite.
According to Kring, of the University of Arizona, events like those at Sudbury 1.8 billion years ago and Chicxulub 65 million years ago were tiny compared to those during the period of heavy bombardment in Earth's formative years.
His calculations suggest there were perhaps as many 40 impact events that produced craters at least 620 miles (1,000 kilometers) in diameter during that time.
"That would have redistributed the chemical elements in Earth's crust to a great extent," he said.
Free E-Mail News Updates
Sign up for our Inside National Geographic newsletter. Every two weeks we'll send you our top stories and pictures (see sample).
SOURCES AND RELATED WEB SITES