Paleo-environmental Setting of the Murray Formation of Aeolis Mons, Gale Crater, Mars, as Explored by the Curiosity Rover
Kevin W Lewis1, Christopher Fedo2, John P Grotzinger3, Sanjeev Gupta4, Nathaniel Stein3, Dr. Frances Rivera-Hernandez, PhD5, Jessica A Watkins3, Steven Banham4, Kenneth S Edgett6, Michelle Elaine Minitti7, Juergen Schieber8, Lauren A Edgar9, Kirsten Siebach10, Kathryn Stack11, Horton E Newsom12, Christopher H House13, Dawn Y Sumner14, Ashwin R Vasavada11 and the MSL Science Team, (1)Johns Hopkins University, Earth and Planetary Sciences, Baltimore, MD, United States, (2)University of Tennessee, Department of Earth and Planetary Sciences, Knoxville, TN, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Imperial College London, Department of Earth Science and Engineering, London, United Kingdom, (5)University of California Davis, Davis, CA, United States, (6)Malin Space Science Systems, San Diego, CA, United States, (7)Framework, Silver Spring, MD, United States, (8)Indiana University Bloomington, Bloomington, IN, United States, (9)USGS, Astrogeology, Flagstaff, United States, (10)California Institute of Technology, Pasadena, United States, (11)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (12)Univ New Mexico, Albuquerque, NM, United States, (13)Pennsylvania State University, Geosciences and Environmental Systems Institute, University Park, United States, (14)University of California, Davis, Earth and Planetary Sciences, Davis, United States
