How life on Earth was boosted by an asteroid collision 446m years ago
Something mysterious happened nearly half a billion years ago that triggered one of the most important changes in the history of life on Earth. Suddenly, there was an explosion of species, with the biodiversity of invertebrate animals increasing from a very low level to something similar to what we see today. The most popular explanation for this “Great Ordovician Biodiversification Event” is that it was a result of an uncomfortably hot Earth cooling and eventually heading into an ice age.
But what actually triggered the change in temperature? In our new paper, published in Science Advances, we show that its onset coincided exactly with the largest documented asteroid breakup in the asteroid belt during the past two billion years, caused by a collision with another asteroid or a comet. Even today, almost a third of all meteorites falling on Earth originate from the breakup of this 150 kilometer-wide asteroid between Jupiter and Mars.
Following this event, enormous amounts of dust would have spread through the solar system. The blocking effect of this dust could have partly stopped sunlight from reaching the Earth – leading to cooler temperatures. We know that this involved the climate changing from being more or less homogeneous to becoming divided into climate zones – from Arctic conditions at the poles to tropical conditions at the equator. The high diversity among invertebrates, including green algae, primitive fish, cephalopods and corals, came as an adaptation to the new climate.
Swedish sea floor
Our evidence comes from detailed studies of sea floor sediments of Ordovician age (485m-443m years ago) exposed at Kinnekulle in southern Sweden and Lynna River near St. Petersburg in Russia. In a quarry at Kinnekulle, we found more than 130 “fossil meteorites” – rocks that fell on Earth in the ancient past, which became embedded in sea floor sediments and were preserved just like animal fossils.
All but one of these fossil meteorites, which are up to 20cm in diameter, have the same composition – they are all debris from the same collision. Indeed, they were made up of the same type of material as the large asteroid that broke up in the asteroid belt at the time. The other meteorite probably originates from the smaller body that hit the large asteroid.
We know that the asteroid collision took place 466m years ago. This can be dated by looking at isotopes (variants of chemical elements with a different number of neutrons in the nucleus) in recently fallen meteorites from the Ordovician asteroid breakup. The fossil meteorites in the quarry must therefore represent the material that was transported to Earth immediately after the breakup. And given the large number of meteorites that we found on the sea floor, we can estimate that the flux of meteorites to Earth must have been orders of magnitude higher back then than it is today.
But how do we know that this bombardment created a huge amount of dust that lowered the temperature? We also studied the distribution of very fine-grained, micrometer-sized dust in the sedimentary strata. We could determine that it had an extraterrestrial origin by detecting helium and other substances incorporated in the sediments that could only be explained by the solar wind having bombarded the dust, enriching it with those elements on its way to Earth.
Our results clearly show that enormous amounts of fine-grained dust reached Earth shortly after the breakup. And the geological record shows that shortly after the dust arrived, the sea level fell dramatically worldwide – the beginning of the ice age. That was because the sea water was transferred to the high latitudes, where large ice sheets formed.
The result was completely unexpected – we have during the last 25 years leaned against very different hypotheses in terms of understanding what happened during this period. For example, while we suspected that the diversification event was somehow linked to the asteroid breakup, we believed that the many small asteroids that also reached Earth from the breakup, rather than the dust, had something to do with the changes. It wasn’t until we got the last helium measurements that everything fell into place.
Lessons for climate research
Global warming continues as a consequence of carbon dioxide emissions, and the temperature rise is greatest at high latitudes. According to the Intergovernmental Panel on Climate Change, we are approaching a situation that is reminiscent of the conditions that prevailed prior to the asteroid collision 466m years ago. Clearly, continuing on that route is not going to be good for biodiversity.
In the last decade or so, researchers have discussed different artificial methods to cool the Earth in case of a major climate catastrophe. One solution would be to place asteroids, much like satellites, in orbits around Earth in such a way that they continuously liberate fine dust and hence partly block the warming sunlight.
Our results show for the first time that such dust at times has cooled Earth dramatically, giving hopes that it could be a viable artificial solution. Our studies can give a more detailed, empirical-based understanding of how this works that can be used to create and evaluate computer models of such events.
But for the foreseeable future, there is no other way to tackle climate change than to reduce our carbon emissions. Ultimately, that is the only way to preserve the spectacular boost in the diversity of life that happened all those 466m years ago.
This article is republished from The Conversation by Birger Schmitz, Professor of Nuclear Physics, Lund University under a Creative Commons license. Read the original article.