McKinnon’s research focuses on the icy satellites of the outer solar system and the physics of impact cratering. The last twenty odd years of planetary exploration can be characterized by both the unveiling of the outer solar system – initially by the Voyager missions, but now by the Galileo mission to Jupiter as well as ground- and space-based telescopes – and the growing realization of the importance of impacts in solar system evolution. Professor McKinnon and his students and colleagues are dedicated to exploring this frontier, concentrating on the origin, structure, evolution, and bombardment history of outer planet satellites and Pluto. This includes understanding the relative importance of large impacts, orbital dynamics, and internal processes for tectonics and other surface modifications, the origin and evolution of impactor populations, and the cratering mechanics in ice and other targets.
William B. McKinnon, professor of earth and planetary sciences in Arts & Sciences at Washington University in St. Louis, led one of three new studies that together provide a far more complete picture of the composition and origin of Arrokoth. The new research published in Science points to the resolution of a longstanding scientific controversy about how such primitive planetary building blocks called planetesimals were formed.
William B. McKinnon, professor of earth and planetary sciences in Arts & Sciences, is a co-investigator on the NASA New Horizons team that published the first comprehensive profile of Ultima Thule in the May 17 issue of the journal Science.
William B. McKinnon, professor of earth and planetary sciences in Arts & Sciences, will deliver the McDonnell Distinguished Lecture on Wednesday, March 29, on the Danforth Campus of Washington University in St. Louis.
What gives Mordor Macula, the red dusted polar region of Pluto’s moon Charon, its color? New Horizons scientists, including Washington University’s Bill McKinnon, answer the question in the current issue of Nature.
Using computer models, New Horizons team members have been able to determine the depth of the layer of solid nitrogen ice within Pluto’s distinctive “heart” feature — a large plain informally known as Sputnik Planum — and how fast that ice is flowing. “For the first time, we can really determine what these strange welts of the icy surface of Pluto really are,” said William B. McKinnon, who led the study.