Planetary Sciences and Cosmochemistry

  • A CAD diagram of the Chicago Instrument for Laser Ionization (CHILI)

  • Group photo of students, postdocs, and faculty working on planetary science at the University of Chicago.

  • A panoramic view of the Kite Group's Planetary Geoscience Lab

  • Some workstations in Professor Nicolas Dauphas's Origins Lab

The University of Chicago was the cradle of modern planetary science. In the 1940s and 1950s, Gerard Kuiper gave observational planetary science a firm grounding in physics and chemistry. At Chicago, Kuiper discovered Miranda and Nereid, found methane in the atmosphere of Titan and CO2 on Mars, and correctly predicted the existence of a belt of dwarf planets beyond the orbit of Neptune (now called the Kuiper Belt). At the same time, Eugene Parker developed the basic theory of the solar wind, and Harold Urey and Claire Patterson’s work was founding cosmochemistry – using meteorites to probe the birth environment of the Earth (some of this work was covered in the Cosmos: A Spacetime Odyssey television series) . Urey’s work on the chemical prerequisites for the origin of life was an inspiration for Carl Sagan (B.S. ’55, PhD ’60). The isotopic and chemical fingerprints of solar system formation were untangled by University of Chicago cosmochemists including Larry Grossman and Robert Clayton. The first science instrument to fly on a Mars rover, the Sojourner X-ray spectrometer, was built at the University of Chicago. 

Today, planetary research occurring within our department is complemented by and integrated with research elsewhere in the University and in Chicago. For example a cohesive exoplanet group with members from our department and the Department of Astronomy and Astrophysics (including Professors Bean, Fabrycky, Konigl, and Rogers) meets weekly to discuss the latest developments in exoplanet research, and there is a weekly cosmochemistry seminar that includes active participation by Phillip Heck, whose primary appointment is at the Field Museum. We are continuing the legacy of research into planet formation and early evolution (Dauphas, Ciesla, Davis, Campbell, and Heck). We have also expanded into new areas recently, including exoplanets and planetary habitability (Abbot, Bean, Fabrycky, Kite, and Rogers). This expansion has already started to produce successful PhD graduates. Spectroscopic observations of rocky exoplanets require large telescopes, and the University of Chicago has reserved time on the Magellan telescopes and is a founding partner in the Giant Magellan Telescope, which at first light will have five times the light-gathering power of any other telescope. Potential graduate students interested in planetary science should consider the research of the faculty in our department and in the Department of Astronomy and Astrophysics to determine which department they would fit best in and should apply to.