Orbiters, followed by rovers sent to Mars, have yielded a dramatic increase in knowledge about Mars over the past decade. Today thanks to several years of data collected in situ and remotely we have a better understanding of its geology and habitability potential. Three SETI Institute planetary scientists who have dedicated their career to the study of the red planet will tell us what we have learned from those studies, and what the next steps are in the exploration of Mars with the next generation of rovers.
Janice Bishop will introduce the candidate landing sites for upcoming martian rovers. She will focus on the mineralogy determined from the CRISM spectrometer at Mars and what that can tell us about Mars’ early environment.
Ginny Gulick will describe the fluvial morphology/water history of these sites as seen by the HiRISE and CTX cameras.
Finally, Pablo Sobron will address the instruments scheduled for the Mars2020 and ExoMars rovers and how SuperCam, Sherlock and the ExoMars Raman/LIBS instrument will be used to explore mineralogy and organics at the future landing sites.