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1
Introduction
2
Apollo 8 Image
3
Exoplanets
4
Key Questions
5
Mars
6
Overview
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Mars Today
8
Phoenix Lander
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Spirit Rover
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Water
11
Time Scale
12
Summary
13
Ice Age
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Comparative Planetology
15
Mars Exploration
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State of Mars Science
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State of the Map
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Rapid Tour
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Early Persistent Environment
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Subsurface Regions
21
Ejecta
22
Iceland
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What does this look like
24
What is the potential analog
25
Carbon sequestration
26
Lakes of Mars
27
Perseverance Rover
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Gale Crater
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Curiosity Exploration
30
Geology Exploration
31
Chlor Chloride Playas
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Sodium Chloride
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Desert Plias
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chloride deposits
35
Amazonian period
36
What sustained the water
37
Global equivalent layers of water
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The fractionation factor
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The modern loss rate
40
Hydration
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Family of Solutions
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Climate Change
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The Frontier
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The Climate
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Questions
Description:
Explore the history of Mars as a habitable world and its implications for terrestrial planet evolution in this Institute for Advanced Study / Princeton University Joint Astrophysics Colloquium talk. Delve into the diverse aqueous environments preserved in Mars' rock record, ranging from lakes and valley networks to groundwaters and hydrothermal systems. Examine the factors that sustained liquid water on Mars, the variability of its environments, and the drivers of long-term environmental change. Gain insights into the processes governing planetary habitability and their relevance to exoplanets beyond our solar system. Investigate the geochemical environments with liquid water on Mars and the impact of aqueous alteration on its atmosphere. Learn about key locations for current and future missions to search for past Martian life and uncover unresolved questions about the planet's evolution. Discover how Mars serves as a crucial linchpin in understanding terrestrial planet evolution and habitability. Read more

Mars- History of a Habitable World and Lessons for Terrestrial Planet Evolution - Bethany Ehlmann

Institute for Advanced Study
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