Today’s rare meteorites were once common
Four hundred and sixty-six million years ago, there was a giant collision in outer space. 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.
|Artist's rendering of the space collision 466 million years ago that gave rise to many of the meteorites falling today |
[Credit: © Don Davis, Southwest Research Institute]
"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.
|Co-author Fredrik Terfelt of Lund University collecting rocks containing 467-million-year-old micrometeorites |
at Lynna River in Russia [Credit: © Birger Schmitz, Lund University]
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 2 mm 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."
|An electron microscope image of a polished cross section of chrome spinel from a fossil micrometeorite that scientists |
believe comes from the asteroid 4 Vesta [Credit: © Philipp Heck, The Field Museum]
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."
Source: Field Museum [January 23, 2017]