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Childhood; early interest in science (astronomy). Member of Astronomical Society of the Pacific, 1928. Special student at University of California at Berkeley, 1931, with Donald H. Menzel’s help. Regular student from 1932; comments on teachers and fellow students at Berkeley Student Observatory. Summer assistantship at Lick Observatory (Nicholas Mayall, Arthur B. Wyse), life at Lick Observatory. To Harvard University in 1937 for graduate studies; comparison between Harvard and Berkeley/Lick; teaching assistant at Radcliffe; 3-year membership in Harvard Society of Fellows, from 1939, of enormous importance for his development; works with Menzel and James G. Baker on the Theory of Physical Processes in Gaseous Nebulae, 1937; Analysis of the Atmospheres of the A-type Dwarfs Gamma Geminorum and Sirius based on data from Louis Berman; Jesse Greenstein. Comments on Harvard Summer Schools, Harlow Shapley’ s Square.” Volunteer teacher of elementary physics courses from 1942 at Harvard. Lawrence Radiation Laboratory, 1943-1945; work involved evaluation of the chemists and the Counting Group’s output from the electromagnetic separation process. Job offer from University of Indiana (Frank Edmunson) accepted due to cutback at Radiation Laboratory. Indiana years, 1945-1948, very productive (drafts for two astrophysics books); problems getting telescope time at Yerkes Observatory and unsatisfactory living conditions leads to acceptance of a promising tenured position at Michigan, a center with very active research due to Leo Goldberg; Robert McMath’s influence in the department; Keith Pierce and Aller’s work on infrared solar spectrum. Work performed at Mt. Wilson Observatory and Dominion Astrophysical Observatory. Goldberg resigns in 1959; comments on Aller’s decision to leave Michigan; discussions of funding; “over-head” (Aller’s talk at an AAS Meeting); comparison of Lick Observatory and Kitt Peak Observatory policies. Work at Mt. Stromio Observatory, Australia on sabbatical visits, 1960, 1968-1969, 1977-1978. Overview of opinions of the present state of astronomy. Comments on personal life, wife and children.
Childhood in New York; high school experience at Horace Mann; Harvard undergraduate at the age of 15. Impressions of ordeal with Harlow Shapley. Depression years in the family business, return to a very changed Harvard in 1934. Thesis work on Interstellar Absorption (Bart Bok), Ph.D. 1937. Postdoc at Yerkes Observatory (Otto Struve) working on Upsilon Sagittarius. Develops the 140-degree camera (the Greenstein-Louis G. Henyey camera); work with Fred Whipple on radio signals from space (Karl Jansky, Grote Reber), Greenstein and Reber’s review article on classified radio detection work during World War II. Founding of the Astrophysics Department at Caltech. Radio astronomy in the mid-1950s. Work on white dwarfs from 1957 on. Own accomplishments as scientist and in personal life. Impressions of Martin Schwarzschild, Shapley, Reber, Fred Hoyle. Also prominently mentioned are: Walter Sydney Adams, Lloyd Viel Berkner, John Bolton, Leverett Davis, William Alfred Fowler, Leo Goldberg, Louis Henyey, Fred Hoyle, Edwin Powell Hubble, Milton Lasell Humason, Robert Hutchins, Karl Jansky, Gerard Peter Kuiper, Tom R. Matthews, Robert Reynolds McMath, Donald Howard Menzel, Paul Merrill, Rudolph Leo Bernhard Minkowski, William Wilson Morgan, Guido Munch, Beverly Oke, Donald Osterbrock, Cecilia Payne-Gaposchkin, Harry Hemley Plaskett, Robert Richardson, Allan Sandage, Jan Scheldt, Shklovsky, Charlotte Moore Sitterly, Lyman Spitzer, Edward Teller, Richard Chace Tolman, Robert Julius Trumpler, Merle Antony Tuve, Albrecht Otto Johannes Unsold, Immanuel Velikofsky, Frederick Whipple; Carnegie Institution of Washington, Hale Observatories, Harvard College Observatory, Lick Observatory, McDonald Observatory, McDonald Observatory Nebular spectrograph, National Science Foundation (U.S.), 100-inch Telescope, University of Chicago, and Vista Project.