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This interview with A. G. W. Cameron focuses on selected aspects of Cameron's research including nucleosynthesis and use of computers in research. Covers Cameron's different topics of research as well as various institutional appointments. Also comments on style of research and William Fowler's receipt of Nobel prize. Other topics discussed include: his family background and childhood, graduate work at the University of Saskatchewan, Leon Katz, photonuclear reactions, astrophysics, Paul Merrill, galactic evolution, Iowa State teaching nuclear physics, Chalk River, advising work for Atomic Energy Commission (AEC) and Department of Energy (DOE), hydrogen bomb, origin of the moon, Los Alamos National Laboratory, Stirling Colgate, nuclear astrophysics, teaching at Yale University, big bang theory, Harvard Smithsonian Center for Astrophysics, Fred Whipple, Leo Goldberg, Hans Suess, Harold Urey, William Fowler, Fred Hoyle, Geoffrey Burbidge, California Institute of Technology, National Aeronautics and Space Administration (NASA).
Parental background; early interest in science and experience looking through friend's telescope in the fourth grade; feeling of compulsion as a child to go into science; sense of duty inherited from parents; early reading in science; pleasure of solving problems in science; education at Miami University and influential teachers there; experience in the Navy in 1944 and 1945; education at University of illinois; learning observational techniques from Robert Baker; getting into Caltech; attraction of the new 200-inch telescope; attraction of Edwin Hubble and Walter Baade; Sandage's intention of being an apprentice; Sandage's childhood feelings that the world was spirit and magic and the disappearance of those feelings upon entering Caltech; education at Caltech; equations became reality at Caltech; the mystery of science; Ph.D. work with Baade on finding and fitting main sequences in globular clusters; history of motives of work with Martin Schwarzschild on dating globular clusters; apprenticeship with Hubble on the 200-inch telescope; Sandage's later monopoly of the 200-inch after Hubble died; Sandage's feeling of responsibility to carry on Hubble's work; objections to the steady state model; learning about the big bang model; limits of Hubble's understanding of the big bang model; influence of theoretical papers by Mattig; influence of Fred Hoyle; introduction to and early attitude toward the horizon and flatness problems; change in cosmology from finding out what galaxies are like to how galaxies originated; Sandage's change in attitude toward the horizon problem; attitude tow.ard the grand unified theories; Sandage's gradual appreciation for the "new" cosmology, involving particle physics; change in attitude toward the flatness problem; attitude toward dark matter and missing mass; openess to the value of omega; problem of consistent ages in cosmology; many forms of evidence for the big bang model; reaction to de Lapparent, Geller, and Huchra's work on large- scale inhomogeneities and importance of similar work done earlier by Gregory, Thompson, Rood, Chincarini and Tifft; relation between theory and observation; science is not the discovery of absolute truth but only an approximation to reality; lack of good observations at the frontiers of science; the change in cosmology from asking only "where" and "what" to also asking "how;" outstanding problems in cosmology: dark matter and value of omega; ideal design of the universe; question of whether the universe has a point.