Meteorite impacts have shaped the development of the Earth and life repeatedly in the past.
The extinction of the dinosaurs, for instance, is thought to have been brought on by a mega-collision at the end of the Cretaceous period.
In comparison to the more than 300,000 impact craters on Mars, the mere 188 confirmed craters on Earth seem almost negligible, researchers said.
Moreover, 60 of them are buried under sediments. Advances in remote sensing have not led to the expected boom in crater discoveries: An average of only one to two meteorite craters are discovered per year, most of them already heavily eroded.
As a result, the craters remain visible for a much shorter period of time, meaning that many less of them are detectable today.
"The main challenge of the study was to estimate the long-term effect of erosion, which causes craters to disappear over time," said Dr Stefan Hergarten from the University of Freiburg in Germany.
The life span of a crater depends on the rate of erosion and its size. Large craters can achieve a life span of several 100 million years, depending on the region in which they are located.
The solution was to compare the amount of confirmed craters of different sizes, calculate the expected frequency of the impacts on the basis of the known probabilities, and combine this information to infer the rates of erosion.
"A surprising, initially sobering finding we made was that there are not many craters of above six kilometres in diameter left to discover on the Earth's surface," said Hergarten.
In the case of smaller craters, on the other hand, the scientists found the current list to be far from complete: Around 90 craters with a diameter of one to six kilometres and a further 250 with a diameter of 250 to 1000 meters are still awaiting discovery.
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