Studying the meteorites in historic giant space collision

There was a giant collision in outer space, four hundred and sixty-six million years ago. Something hit an asteroid and broke it apart, sending chunks of rock falling to Earth as meteorites since before the time of the dinosaurs. But what kinds of meteorites were making their way to Earth before that collision? In a new study in Nature Astronomy, scientists have tackled that question by creating the first reconstruction of the distribution of meteorite types before the collision. They discovered that most of the meteorites we see today are, in the grand scheme of things, rare, while many meteorites that are rare today were common before the collision.

The paper’s lead author, Philipp Heck of The Field Museum in Chicago, says, “We found that the meteorite flux, the variety of meteorites falling to Earth, was very, very different from what we see today.”

“Looking at the kinds of meteorites that have fallen to Earth in the last hundred million years doesn’t give you a full picture,” explains Heck. “It would be like looking outside on a snowy winter day and concluding that every day is snowy, even though it’s not snowy in the summer.”

Meteorites are pieces of rock that have fallen to Earth from outer space. They’re formed from the debris of collisions between bodies like asteroids, moons, and even planets. There are many different types of meteorites, which reflect the different compositions of their parent bodies. By studying the different meteorites that have made their way to Earth, scientists can develop a better understanding of how the basic building blocks of the Solar System formed and evolved.

“We knew almost nothing about the meteorite flux to Earth in geological deep time before this study,” says coauthor Birger Schmitz of Sweden’s Lund University. “The conventional view is that the solar system has been very stable over the past 500 million years. So it is quite surprising that the meteorite flux at 467 million years ago was so different from the present.”

To learn what the meteorite flux was like before the big collision event, Heck and his colleagues had to analyze meteorites that fell more than 466 million years ago. Such finds are rare, but the team was able to look at micrometeorites—tiny specks of space-rock less than 2mm in diameter that fell to Earth, which are a little more widespread. Heck’s Swedish and Russian colleagues retrieved samples of rock from an ancient seafloor exposed today in a Russian river valley that contained micrometeorites, and then dissolved the rocks in acid so that only microscopic chromite crystals remained.

“Chrome-spinels, crystals that contain the mineral chromite, remain unchanged even after hundreds of millions of years,” explains Heck. “Since they were unaltered by time, we could use these spinels to see what the original parent body that produced the micrometeorites was made of.”

Analysis of the chemical makeup of the spinels showed that the meteorites and micrometeorites that fell earlier than 466 million years ago are different from the ones that have fallen since. A full 34 percent of the pre-collision meteorites belong to a meteorite type called primitive achondrites; today, only 0.45 percent of the meteorites that land on Earth are this type. Other ancient micrometeorites sampled turned out to be relics from Vesta, the brightest asteroid visible from Earth, which underwent its own collision event over a billion years ago.

A contributor to the paper, William Bottke of the Southwest Research Institute, says, “Meteorite delivery from the asteroid belt to the Earth is a little like observing landslides started at different times on a mountainside. Today, the rocks reaching the bottom of the mountain might be dominated by a few recent landslides. Going back in time, however, older landslides should be much more important. The same is true for asteroid breakup events; some younger ones dominate the current meteorite flux, while in the past older ones dominated.”

“Knowing more about the different kinds of meteorites that have fallen over time gives us a better understanding of how the Asteroid Belt evolved and how different collisions happened,” says Heck. “Ultimately, we want to study more windows in time, not just the area before and after this collision during the Ordovician period, to deepen our knowledge of how different bodies in Solar System formed and interact with each other.”

More information: Phys.org