Evidence of Water on Ancient Mars
Research indicates that the meteorite shows evidence of alteration by water beneath the Martian surface. This provides details about ancient interactions between water and rocks. A separate study published in Science Advances in June examined the water content of Teghaza 001, offering further insight into how water interacted with the Martian surface during the planet's early history.
“This is really our first piece of Martian crust from a part of Mars we’ve never had a sample of before,” said Lee Saper, the paper’s second author, who conducted research while at JPL as a postdoctoral scholar.
“It records interactions of water and rock and maybe even an imprint of the Martian atmosphere as it was losing water,” Lee added.
Evidence derived from chemical composition, microstructural features, and oxygen isotope ratios suggests that early Mars had a "substantially more active hydrological cycle."