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Pasadena, CA · Physics & astronomy

Physics & astronomy at Caltech

Caltech graduates about 30 physics & astronomy majors a year, 14% of its graduating class. That puts it 2nd of 525 schools we score for physics & astronomy, a standout program at 99 out of 100. Research spending in the field runs about $156 million a year, a rough guide to how many labs and projects undergraduates can join.

Graduates a year3014% of the class
Research in the field$156Ma year, NSF
Admit rate3%whole school

Where physics & astronomy happens

Buildings on campus that fit the field: Linde Laboratory for Global Environmental Science, Arms Laboratory of the Geological Sciences, Downs Laboratory of Physics, Bridge Laboratory of Physics West, Bridge Laboratory of Physics Annex, Bridge Laboratory of Physics East, Linde Hall of Mathematics and Physics, Chen Neuroscience Research Building, Powell-Booth Laboratory for Computational Science, Lauritsen Laboratory of High Energy Physics, Firestone Flight Sciences Laboratory, Annenberg Center for Information Science and Technology.

Named buildings on the campus map: Academic 36 · Student housing 22 · Dorm 8 · Athletics 4 · Dining 2 · Library 2.

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Nearby in the physics & astronomy ranking

  1. Massachusetts Institute of Technology 100
  2. Harvard University 99
  3. Princeton University 99
  4. University of Chicago 98
  5. Yale University 97
  6. Stanford University 97
  7. University of Pennsylvania 96

Other strong majors at Caltech

How the score works

The score is out of 100 and compares Caltech with every school we score in physics & astronomy. It weighs the school's overall strength; how many students graduate in the major and what share of the class they are; research spending in the field (NSF); early pay against the same major nationally; how many courses the catalog lists; and test scores. 80+ is a standout program, 65+ strong, 45+ solid. Sources: US Department of Education (College Scorecard, IPEDS), NSF HERD, each school's current course catalog, OpenStreetMap and Wikimedia Commons.

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