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What makes a planet habitable?
Earth is a dynamic planet: from the surface teeming with life to the deepest interior that maintains the protective magnetic field. For over 4.5 billion years, giant impacts, volcanism, and surface tectonic motions have transformed the surface, oceans, and atmosphere. Despite, or perhaps because of, these extrinsic changes, life has thrived. Why is Earth habitable? Where will life be detected elsewhere? What type of planet is most likely to sustain life? Beyond Earth, what are the characteristics of a habitable planet? In one of the great discoveries of our lifetimes, the Galaxy turns out to be teeming with planets. For the first time in human history, we have a wide range of planets to consider as possible hosts for life.

We are fundamentally interested in what makes a planet habitable. What features of a planet's several-billion-year history create and maintain an environment that is suitable for life? We postulate that one cannot understand the habitability of Earth or constrain the potential for habitability of other planets, particularly terrestrial exoplanets, without studying the role that the internal dynamics and bulk composition of the planet play in establishing and maintaining the surface environment. Whether a planet is hot or cold, wet or dry, active or stagnant, or alive or dead depends critically on the interior in crucial ways. This talk will present more questions than answers, but will show you how we at Carnegie, along with our international collaborators, are tackling these questions in order to understand the origin of habitable planets.

Oct 26, 2021 06:30 PM in Eastern Time (US and Canada)

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