Geodigest

Abstract

Tracking meteorite flux A study conducted at Lund University has tracked the meteorite flux to the Earth over the past 500 Myr, finding that, contrary to current theories, major collisions in the asteroid belt (Fig. 1) have not generally affected the number of impacts with the Earth to any great extent (ScienceDaily, 8 June 2021). Researchers have been studying geological sites since the nineteenth century, in order to reconstruct how flora, fauna and the climate have changed over millions of years. Until now, however, almost nothing has been known about ancient meteorite flux—which makes sense since impact is rare, and the battered celestial bodies quickly break down as they encounter Earth’s oxygen. To examine this, the new study has reconstructed meteorite bombardment towards Earth over the past 500 Myr. ‘The research community previously believed that meteorite flux to Earth was connected to dramatic events in the asteroid belt. The new study, however, shows that the flux has instead been very stable,’ says Birger Schmitz (Lund University). To conduct their study, the researchers dissolved almost 10 tonnes of ancient sedimentary rocks in strong acids, so as to discover residue left by meteorites as they fell to Earth. Meteorites contain a small fraction of a mineral, a chromium oxide, which is very resistant to degradation. The microscopic chromium oxide grains were sifted out in the laboratory and serve as time capsules with an abundance of information. ‘The dissolved sediment represents 15 periods over the past 500 Myr. In total, we have extracted chromium oxide from almost 10 000 different meteorites. Chemical analyses then enabled us to determine which types of meteorites the grains represent,’ says Birger Schmitz. A couple of thousand meteorites land on the Earth’s surface every year, and approximately 63 000 of them have been documented by science. They originate from the asteroid belt between Mars and Jupiter where battered celestial bodies from gigantic collisions revolve around the Sun. ‘We were very surprised to learn that only one of the 70 largest asteroid collisions that took place over the past 500 million years resulted in an increased flux of meteorites to Earth. For some reason, most of the rocks stay in the asteroid belt,’ says Birger Schmitz. The study not only upends generally accepted meteorite flux theories; it also provides entirely new perspectives on which types of celestial bodies are at greatest risk of colliding with the Earth, and where in the solar system they originate. From a geological time perspective, kilometre-sized celestial bodies collide with the Earth on a regular basis. One such event took place 66 Ma, when a celestial body stretching over 10 km in diameter hit the Yucatán Peninsula. ‘Future impact from even a small asteroid for example in the sea close to a populated area could lead to disastrous outcomes. This study provides important understanding that we can use to prevent this from happening; for example, by attempting to influence the trajectory of rapidly approaching celestial bodies,’ concluded Birger Schmitz.