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| Brian Schmidt (astronomer) | |
|---|---|
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| Name | Brian Schmidt |
| Birth date | 24 February 1967 |
| Birth place | Missoula, Montana, United States |
| Nationality | Australian |
| Fields | Astronomy, Astrophysics |
| Workplaces | Mount Stromlo Observatory, Australian National University, Australian Academy of Science |
| Alma mater | University of Arizona, Harvard University |
| Known for | Discovery of the accelerating expansion of the universe |
| Awards | Nobel Prize in Physics, Breakthrough Prize in Fundamental Physics |
Brian Schmidt (astronomer) is an Australian-American astronomer and astrophysicist noted for leading a team that discovered the accelerating expansion of the universe using observations of Type Ia supernovae. He shared the 2011 Nobel Prize in Physics with Saul Perlmutter and Adam Riess for this discovery, which transformed contemporary understanding of cosmology and led to the widespread adoption of the term dark energy. Schmidt has combined observational astronomy with leadership roles at institutions and national academies, contributing to projects in optical astronomy and time-domain astronomy.
Schmidt was born in Missoula, Montana and raised in Anchorage, Alaska and Bozeman, Montana, later emigrating to Australia where he attended High School — moving through cities that exposed him to observatories such as Mount John Observatory and institutions like the Australian National University. He completed undergraduate studies at the University of Arizona before undertaking graduate research at Harvard University under supervisors connected to projects at Mount Stromlo Observatory and collaborations involving Cerro Tololo Inter-American Observatory and Las Campanas Observatory. Schmidt earned a Ph.D. focused on supernova observations and time-domain surveys, engaging with instrumentation teams at facilities including Anglo-Australian Telescope.
Schmidt led and co-founded the High-Z Supernova Search Team, intersecting with researchers from Harvard-Smithsonian Center for Astrophysics, Lawrence Berkeley National Laboratory, and the Space Telescope Science Institute. The team used observations from telescopes such as the Keck Observatory, Magellan Telescopes, and the European Southern Observatory to measure luminosity distances of Type Ia supernova out to high redshift, comparing results with predictions from Friedmann equations influenced by Einsteinian models and contributions from Lambda (cosmological constant). The empirical finding—that distant supernovae appeared fainter than expected in a decelerating universe—provided evidence for an accelerating expansion attributed to a dominant component later termed dark energy.
Throughout his career Schmidt has been involved in time-domain surveys and instrumentation, contributing to programs at Siding Spring Observatory, collaborations with the Pan-STARRS consortium, and projects involving the Large Synoptic Survey Telescope (now Vera C. Rubin Observatory). His work bridged observational campaigns, data analysis pipelines, and theoretical interpretation, engaging with colleagues from Princeton University, University of California, Berkeley, Carnegie Institution for Science, and CSIRO. Schmidt has supervised students and postdoctoral researchers from institutions including University of Cambridge, University of Oxford, and Massachusetts Institute of Technology.
In 2011 Schmidt, together with Saul Perlmutter and Adam Riess, received the Nobel Prize in Physics for the discovery of cosmic acceleration via measurements of distant supernovae. The recognition followed earlier prizes awarded to members of the discovery teams, such as the Gruber Prize in Cosmology and the Breakthrough Prize in Fundamental Physics, and national honors including appointments to the Order of Australia and membership of the Australian Academy of Science. Schmidt's citations referenced collaborative datasets and methodologies developed alongside teams from Harvard University, Lawrence Berkeley National Laboratory, and the Carnegie Observatories. Other accolades include the Buchalter Prize-style recognitions, honorary doctorates from universities such as Monash University and University of New South Wales, and named lectures at organizations like the Royal Society and the American Astronomical Society.
Schmidt served as Director of the Mount Stromlo Observatory and later as Vice-Chancellor and President of the Australian National University, overseeing links with national facilities such as Pawsey Supercomputing Centre and international collaborations with the European Southern Observatory and National Aeronautics and Space Administration. He has chaired panels for the Australian Research Council and represented Australian science in forums hosted by the Commonwealth Scientific and Industrial Research Organisation and the Group of Eight (Australian universities). Schmidt is active in public science communication, delivering talks at venues including the Royal Institution, participating in media interviews with outlets like the BBC and ABC (Australian Broadcasting Corporation), and contributing to educational initiatives such as outreach programs at Questacon and partnerships with the CSIRO school engagement programs. His policy engagement has included testimony before parliamentary committees and advisory roles for governmental science strategy bodies.
Schmidt holds dual Australian and United States citizenship and resides in Canberra. He is married and has family connections to colleagues and collaborators across institutions such as Australian National University and Mount Stromlo Observatory. Outside academia, Schmidt has participated in public discussions on topics intersecting science and society, has an interest in outdoor activities common in regions like Australian Capital Territory and Alaska, and supports initiatives promoting participation in STEM among young people.
Category:Australian astronomers Category:Nobel laureates in Physics Category:Harvard University alumni Category:University of Arizona alumni