





Monday, November 16, 2026 from to
Seminar Lab Date: November 9, 2026
Seminar Lab Subject: New Mapping of the Baraboo Hills Unravels a More Complex Geologic History for Southern Wisconsin (V)
Seminar Lab Presenter: Esther Stewart, Ph.D., Senior Geologist, WI Geological & Natural History Survey
Seminar Lab Location:
**Virtual Online Lecture**
Participation instructions will be e-mailed to GSM members. If you are not a member of GSM and wish to attend this free seminar online, register as follows by 8 AM CT Monday, Nov 9: Go to the Contact menu above and select “Ask GSM”. In the form that appears, enter your name and e-mail address. Enter “Nov 9 lecture” in the subject line. In the message body, please enter the city and state or country from which you will view the seminar. You will receive instructions by e-mail prior to the lecture. Check your spam folder if the instructions do not appear in your in-box at least one hour prior to the lecture.
Seminar Lab Detail:
Summary: The Baraboo Hills of southern Wisconsin preserve over a billion years of earth history spanning growth of the ancient North American continent, flooding by tropical seas, and more recent glaciation. New geologic mapping of the Baraboo Hills adds detail to the oldest, Precambrian rock units and advances our understanding of how these rocks formed. In this talk I’ll present an overview of the new geologic map and how it contributes to our understanding of Wisconsin geology.
Biography: Esther Stewart has been a geologist with the WGNHS since 2013. Prior to joining WGNHS she worked for ExxonMobil in Houston, TX for several years. She earned her masters in geology from Idaho State University and recently completed her PhD at UW-Madison. Her research interests involve using geologic maps and stratigraphic frameworks to address practical issues in Wisconsin.
Seminar Lab Date: November 23, 2026
Seminar Lab Subject: Mars Demystified: What Everyone Should Know
Seminar Lab Presenter: Protiti Roy, Ph.D. Candidate, Graduate Fellow, University of Iowa
Seminar Lab Location:
In-person only at University of Minnesota, Tate Hall, Room B20
Lecture start time 7:00 PM CT
Seminar Lab Detail:
Summary: Mars provides a unique opportunity to investigate the geological and environmental conditions of the early Solar System because, unlike Earth, much of its ancient surface has remained preserved. Geological evidence from orbital observations, rover missions, and meteorite analyses reveal extensive volcanic activity, a basaltic crust, and localized occurrences of more evolved rocks (SiO2 > 53 wt %), indicating a complex geological history. Landforms such as river deltas, conglomerates, clay-rich sediments, and hydrated mineral deposits demonstrate that liquid water was once abundant on the Martian surface, supporting long-lived fluvial and lacustrine environments. Additional evidence of hydrothermal activity and neutral-pH aqueous conditions suggests that ancient Mars possessed environments favorable for habitability. Recent studies have identified the strongest evidence to date for potential ancient biosignatures, including complex organic molecules and chemical signatures that are consistent with past microbial activity, although these findings have not yet been conclusively confirmed as evidence of life. Continued exploration, advanced in situ analyses, and future sample-return investigations are expected to determine whether these biosignatures represent the first confirmed evidence of ancient life on Mars and to further refine our understanding of the planet’s geological and biological evolution.
Biography: My name is Protiti Roy. I’m a Graduate Fellow and Ph.D. student at the Planetary Exploration Group in the School of Earth, Environment, and Sustainability at The University of Iowa.
Martian mineralogy fascinates me. I use orbital remote sensing data to study minerals on Mars and uncover clues about its igneous and sedimentary history, past water activity, and how Mars may have looked and behaved in the past. My current research focuses on the mineralogy of high thermal inertia regions in Valles Marineris, Mars’s largest canyon system.
In 2025, I received the “Future Investigators in NASA Earth and Space Science and Technology” (FINESST) grant. It is funding my graduate research project entitled “Morphological and Mineralogical Characterization of High Thermal Inertia Regions on the Floor of Valles Marineris, Mars” for 2 years.
Before Iowa, I received my bachelor’s with an Honours in Geology from University of Calcutta, India and my master’s in Applied Geology from Indian Institute of Technology (Indian School of Mines) Dhanbad, India.
In my free time I love painting and sketching, hiking, reading story books, and cooking!
Seminar Lab Date: December 7, 2026
Seminar Lab Subject: Michigan Geology – 3.6 billion Years in the Making (V)
Seminar Lab Presenter: Bob Mahin, M.Sc., CPG, FSEG Economic Geologist/Senior Research Associate, Michigan Geological Survey
Seminar Lab Location:
**Online Lecture**
Seminar Lab Detail:
Summary & biography TBA
TBA
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