An international research team has identified the specific origins of most of the Martian meteorites that are now on Earth. They’ve traced the meteorites to five craters where they were launched off Mars after impact. The craters are located within two volcanic regions on the red planet called Tharsis (the region containing Olympus Mons, the largest shield volcano in the solar system) and Elysium.
Western planetary geologist Livio Tornabene is a co-author of the study, recently published in the journal Science Advances.
“Remarkably, with just a few specific clues that the meteorites provide us here on Earth and the abundance of remote data collected by spacecraft missions to Mars, we can narrow down from the tens of millions of craters and identify the very specific ones that some of these meteorites are very likely to originate from,” said Tornabene, an Earth sciences professor and research scientist at Western.
Martian meteorites find their way to Earth when something – a sizeable asteroid or a comet – hits the surface of the red planet with enough energy to blast some of that material into space.
This ejected material then ends up in an orbit around the sun, with some eventually falling to Earth as meteorites. The impact also leaves a crater on Mars’ surface, which is exactly where Tornabene started investigating this mystery nearly two decades ago at the start of his own academic career.
The new study is a renewed effort that builds on the general methodology Tornabene established in 2006 with a paper in Journal of Geophysical Research: Planets that was further advanced through current state-of-the-art analytical techniques, modelling and orbit-based data that wasn’t available at the time.
“It’s a proud moment to see the results of this new effort and to know that what I presented in a paper nearly 20 years ago, stood the test of time. Especially in a field of science where what you write today could turn out to be flawed or even incorrect in a matter of years or less,” said Tornabene, a member of Western’s Institute for Earth and Space Exploration.
Chris Herd, curator of the University of Alberta’s Meteorite Collection and professor in the Faculty of Science, agrees that scientists’ improved understanding of the physics of exactly how the rocks are ejected from Mars was key to this discovery.
Scientists have determined these meteorite-launching events have happened at least 10 times in Mars’ recent history. This estimate is based on the ages, compositional similarities and other common characteristics that enable scientist to classify the approximately 200 known Martian meteorites into 10 groups.
“We think we’ve found the source craters for half of all 10 groups of Martian meteorites,” said Herd, lead author on the study. “Now, we can group these meteorites by their shared history and then their location on the surface prior to coming to Earth.”
Livio Tornabene
Recalibrating Mars’ chronology
This study is a true testament to the resilience of planetary scientists, like Tornabene and Herd, who work to maximize the limited data they use to tell us as much as possible about another planet. “Mars data is certainly not limited with respect to the amount we have, but with respect to how it is collected remotely by robotic surrogates, and not in-person or within a state-of-the-art laboratory,” said Tornabene. Knowing how and where these meteorites are from on Mars gives researchers additional insights into the samples and the planet that spawned them. “We now have the ability to contextualize and position these samples within the Martian geology for the first time, which enables the recalibration of Mars’ chronology,” said Herd. “This has implications for the timing, duration and nature of a wide range of major events through Martian history.” Knowledge about the origin of meteorites, combined with advances in technology like remote sensing, also gives researchers a framework upon which to build future research. The ability to model the ejection process is a major advance. From that, geologists can determine the crater size or range of crater sizes that ultimately could have ejected that group of meteorites, or even one particular meteorite. “I call this the missing link. To be able to say, for example, the conditions under which this meteorite was ejected produced craters between 10 and 30 kilometres across, is really amazing,” said Herd. “It’s the closest thing we have to actually going to Mars and picking up a rock.” In the 1980s, scientists discovered a signature for the Martian atmosphere trapped inside meteorite samples. That signature, or molecular fingerprint, includes a specific combination of trapped gases that match those measured in the atmosphere of Mars by the Viking landers in the 1970s.This image shows lava crumpled against the upstream side of an impact crater in in Elysium Planitia. (NASA/JPL-Caltech/University of Arizona)
