The story of Amazonian climate change on Mars as told by carbonates in Miller Range Nakhlites

This is a story about rocks from Mars, and how they reveal environmental changes on Mars. A specific region of volcanic rocks formed on Mars about 1.3 billion years ago (bya). This region is now known as the Nakhla lava pile. The rocks were likely formed near the surface. Chemical analysis of these rocks confirms that they formed on Mars, because rocks on Earth have different oxygen isotope values. Sometime later, perhaps 0.7 bya, very small amounts of subsurface water on Mars percolated through the lava pile. The water contained dissolved carbon dioxide (CO2) from contact with the atmosphere of Mars. Ions in the water bonded with rock ions to create tiny, white, carbonate minerals along the cracks within the lava pile. The Nakhla subsurface water temperature was likely cool ( 15°C), which is different from the hot water that possibly created minerals on older Mars rocks. About 11 million years ago, an asteroid impacted Mars over the Nakhla lava pile. The impact rebound ejected mass from the surface and subsurface, and some rocks escaped the gravity of Mars. These rocks floated in space for over 10.9 million years before they fell to Earth as meteorites. The most famous of these meteorites, named Nakhla, fell over Egypt in 1911 and fragmented into 40 pieces. A total of 11 similar meteorites, known as Nakhlites, have been collected across the Earth. Four of these meteorites fell into a remote region of Antarctica called the Miller Range (MIL). They were collected by the National Science Foundation (NSF) "Antarctica Search for Meteorite" (ANSMET) program. This study analyzed the stable isotope geochemistry of the carbonates on the four MIL Nakhlites. Antarctica is an analog for carbonate formation on recent Mars because it forms the minerals in a cold environment with a thin film of water. Carbonates from oceans are dominated by the oxygen isotopic values of the water, but in Mars and Antarctica the carbonates are also influenced by the oxygen in the atmospheric CO2. This study reveals that terrestrial carbonates have different carbon isotope values from martian carbonates. The carbon isotope values of the Mars atmospheric CO2 that formed the MIL Nakhlite carbonates was different from the modern atmosphere (as measured by the MSL Curiosity rover). This difference may be due somewhat to loss of atmospheric gas to space over the past billion years.