Working Across Scales

We deploy a broad range of techniques to pursue breakthroughs ranging from the atomic to the galactic

With a vast array of cutting-edge instruments and facilities at their fingertips, Carnegie Earth and planetary scientists advance new frontiers in sample return, planetary history, planetary interior dynamics, geochronology, and more. Carnegie researchers cross disciplinary boundaries to discover distant worlds, illuminate Earth’s inner workings, and reveal the dynamic processes that enabled life to arise and thrive here—and potentially elsewhere in the universe.

protoplanetary disk

protoplanetary disk

Formation of Planetary Systems

During their youth, stars are surrounded by a rotating disk of gas and dust leftover from their formation. Baby planets and other celestial bodies are born from the accretion of this material over time. Revealing this process is critical for understanding planetary habitability and what makes our own Solar System so distinct from the thousands of others we’ve found so far. Carnegie astronomers and planetary scientists use both observing and mathematical modeling to piece together the puzzle of planet formation and early evolution.

New research uses laboratory experiments to demonstrate that water is naturally created during the planet formation process. Credit: Navid Marvi/Carnegie Science

Planetary Dynamics

Carnegie Scientists believe that there are three critical factors for a planet to be considered capable of hosting life: liquid water, plate tectonics, and a magnetic field. Planetary dynamics are the surface expression of these facets, which Carnegie scientists study in the fi eld, in the lab, and at the telescope. The multi-disciplinary Sloan-funded AEThER project, is elucidating fundamental details about the nature of exoplanetary solar systems and the characteristics that could enable life to arise and thrive on rocky planets.

Tissint meteorite courtesy of Kurt Kracher, Museum of Natural History Vienna

Origin & Sustanance of Life

How did life emerge on Earth and what enabled it to thrive? Answering this question requires a deep understanding of both our planet’s geologic history and the raw materials from which the Solar System formed. Carnegie scientists are on the forefront of sample return missions that are enabling a brand-new understanding of organic compounds in our Solar System’s history. This is critical for understanding the origin of life on Earth and how it differentiates us from other bodies within the Solar System.

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