Diagenetic Concretions in the Murray Formation, Gale Crater, Mars
Vivian Zheng Sun1, Kathryn Stack1, Linda C Kah2, Amy J Williams3, Lucy M Thompson4, Roger C Wiens5, Scott VanBommel6, Sarah Johnson7, Christopher H House8, Marion Nachon9, Woodward W Fischer10, Rachel E. Kronyak11, Michelle Elaine Minitti12, Kirsten Siebach13 and Dawn Y Sumner14, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)University of Tennesse, Knoxville, United States, (3)University of Florida, Department of Geological Sciences, Ft Walton Beach, FL, United States, (4)University of New Brunswick, Fredericton, NB, Canada, (5)Space Science and Applications, Los Alamos, United States, (6)University of Guelph, Guelph, Canada, (7)Georgetown University, Washington, DC, United States, (8)Pennsylvania State University, Geosciences and Environmental Systems Institute, University Park, United States, (9)University of Nantes, Nantes, France, (10)Caltech, Division of Geological and Planetary Sciences, Pasadena, United States, (11)University of Tennessee, Knoxville, TN, United States, (12)Framework, Silver Spring, MD, United States, (13)California Institute of Technology, Pasadena, United States, (14)University of California, Davis, Earth and Planetary Sciences, Davis, United States
