By looking at an ancient Martian meteorite that landed in the Sahara Desert, Lawrence Livermore National Laboratory (LLNL) scientists and collaborators have determined how and when the red planet’s crustal topographic and geophysical divide formed.
Northwest Africa (NWA) 7034 is the oldest Martian meteorite discovered to date, at approximately 4.4 billion years old. The meteorite is a breccia (it contains a variety of different crustal rocks that were mixed together and then sintered by heating) and is the only sample from Mars with a composition that is representative of the average Martian crust. The meteorite provided the researchers a unique opportunity to study the ancient crust on Mars.
The team applied a number a radioisotopic dating techniques to determine that the divide (or dichotomy) between the heavily cratered southern highlands of the planet and the smoother plains of the northern lowlands formed prior to the formation of NWA 7034 at 4.4 billion years ago. This ancient age is consistent with a giant impact origin for the crustal dichotomy. The research appears in the May 23 edition of the journal Science Advances.
“If the Martian crustal dichotomy formed as a result of a giant impact, and available data and modeling suggest this is likely, the history of NWA 7034 requires that it formed very early in the planet’s history, before 4.4 billion years ago,” said LLNL cosmochemist Bill Cassata, lead author of the paper.
The team set out to determine when and how the crustal dichotomy formed.
Based on new radioisotopic measurements and in conjunction with other published data, the team determined that all the rocks that eventually were incorporated into the NWA 7034 breccia were emplaced about 4.4 billion years ago in the “source terrain” (the crustal source region that the different breccia components are derived from). The results show that this terrain was subject to prolonged metamorphism associated with a large plume-fed volcanic center from ~1.7 to 1.3 billion years ago. The areal extents of large, plume-fed volcanic centers on Mars are thousands of square kilometers, and the source terrain was likely comparable in size. Finally, they showed the rock was brought together ~200 million years ago or more recently. When viewed together, the data from NWA 7034 demonstrated that large volcanic terrains survived within a few km of the Martian surface since >4400 million years ago. This indicates that the dichotomy formed prior to 4.4 billion years ago, as near surface rocks would have been buried or destroyed by the dichotomy-forming event.
“This multi-disciplinary study, combining both traditional and innovative geochemical techniques has provided us with some exciting new insights into the timings of major processes that shaped young Mars,” said Caroline Smith, head of Earth Sciences Collections, principal curator of meteorites at the Natural History Museum and another author on the paper.
This team’s results have important implications for our understanding of when and how one of the oldest, and most distinctive, global geologic features on Mars was formed.
“This study demonstrates that multiple radioisotopic dating systems that are reset by different metamorphic processes can be used to tease out the thermal history of a sample over billions of years,” Cassata said.
Other Livermore researchers involved in the study include Reto Trappitsch, Carolyn Crow and Joshua Wimpenny. Scottish Universities Environmental Research Centre, the University of Glasgow, the University of St. Andrews and the Natural History Museum also contributed to the research.