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In this interview, Andrea Dupree discusses topics such as: her family background and childhood; doing her undergraduate studies at Wellesley College; Janet Guernsey; C. P. Snow; becoming interested in astronomy; what is was like being a woman and fitting into the physics profession and dealing with gender inequality; Sarah Hill; Allan Sandage; Hans Bethe; Phil Morrison; Otto Struve; going to the Royal Greenwich Observatory for a summer; Cecilia Payne-Gaposchkin; Dorrit Hoffleit; variable star fields; deciding to go to Berkeley for graduate school; Ivan King; Hyron Spinrad; Lick Observatory; coming back to Harvard University after a year; George Wallerstein; William Liller; Leo Goldberg; her affiliation with the American Astronomical Society (AAS); Don Osterbrock; Simon "Pete" Worden; Owen Chamberlain; Alex Dalgarno; Harvard College Observatory; Harvard-Smithsonian Center for Astrophysics; Ed Lilley; solar physics; ionization rates; Herb Friedman; Dick Tousey; Henry Smith; stellar atmospheres; Fred Whipple; Donald Menzel; Margaret Burbidge; orbiting solar observatories (OSO); Skylab program; Lyman Spitzer; Robert Noyes; Henry Norris Russell; International Astronomical Union (IAU); National Aeronautics and Space Administration (NASA); George Field; Smithsonian Astrophysical Observatory (SAO); Eric Chaisson; Jesse Greenstein; Celescope.
Career of George B. Field, theoretical astrophysicist and administrator of astronomical research at the Harvard-Smithsonian Astrophysical Observatory (SAO). Discussions of education at Massachusetts Institute of Technology, Princeton and Harvard Universities, interest in cosmological problems; possible detection of hot intergalactic matter in 1964; colleagues at University of California at Berkeley; views on popularizing science; reactions to Sputnik launch in 1957; funding of research from the National Aeronautics and Space Administration (NASA); views on the manned space program; effects of Vietnam War on NASA and astronomical research; involvement with the Space Telescope; views of the Space Shuttle; extensive committee work for NASA; astronomical research under NASA; work at SAO; new programs at SAO, such as x-ray astronomy and the Multiple Mirror Telescope; service on the Jesse Greenstein and Allan Bromley survey committees of astronomy and physics; and his view of the universe. Also prominently mentioned are: Kinsey Anderson, Stuart C. Bowyer, Jim Bradley, Tony Calio, Riccardo Giacconi, Thomas Gold, Leo Goldberg, John Hagen, Noel Hinners, Fred Hoyle, Frank Martin, John Earl Naugle, Al Opp, Edward Mills Purcell, Martin Schwarzschild, Dennis William Sciama, Henry Smith, Sylvia Favior Smith, Lyman Spitzer, George Steiner, Frank Sulloway, Pat Thaddeus, James Van Allen, Fred Whipple; American Science and Engineering, Inc., Annual Review of Astronomy and Astrophysics, Congregational Church, Harvard College Observatory, Harvard University Society of Junior Fellows, High Energy Astronomy Observatory, Lick Observatory, National Academy of Sciences (U.S.) Astronomy Survey Committee, National Academy of Sciences (U.S.) Greenstein Committee, National Science Foundation (U.S.), New York Times, Orbiting Astronomical Observatory, Princeton University Matterhorn Project, Project Apollo, Skylab, Smithsonian Astrophysical Observatory Multiple Mirror Telescope, Smithsonian Institution National Air and Space Museum, Space Shuttle, United States Naval Ordnance Laboratory, United States Office of Management and Budget, United States Office of Naval Research, University of California at Berkeley, and Viking (Rocket).
Career of George B. Field, theoretical astrophysicist and administrator of astronomical research at the Harvard-Smithsonian Astrophysical Observatory (SAO). Discussions of education at Massachusetts Institute of Technology, Princeton and Harvard Universities, interest in cosmological problems; possible detection of hot intergalactic matter in 1964; colleagues at University of California at Berkeley; views on popularizing science; reactions to Sputnik launch in 1957; funding of research from the National Aeronautics and Space Administration (NASA); views on the manned space program; effects of Vietnam War on NASA and astronomical research; involvement with the Space Telescope; views of the Space Shuttle; extensive committee work for NASA; astronomical research under NASA; work at SAO; new programs at SAO, such as x-ray astronomy and the Multiple Mirror Telescope; service on the Jesse Greenstein and Allan Bromley survey committees of astronomy and physics; and his view of the universe. Also prominently mentioned are: Kinsey Anderson, Stuart C. Bowyer, Jim Bradley, Tony Calio, Riccardo Giacconi, Thomas Gold, Leo Goldberg, John Hagen, Noel Hinners, Fred Hoyle, Frank Martin, John Earl Naugle, Al Opp, Edward Mills Purcell, Martin Schwarzschild, Dennis William Sciama, Henry Smith, Sylvia Favior Smith, Lyman Spitzer, George Steiner, Frank Sulloway, Pat Thaddeus, James Van Allen, Fred Whipple; American Science and Engineering, Inc., Annual Review of Astronomy and Astrophysics, Congregational Church, Harvard College Observatory, Harvard University Society of Junior Fellows, High Energy Astronomy Observatory, Lick Observatory, National Academy of Sciences (U.S.) Astronomy Survey Committee, National Academy of Sciences (U.S.) Greenstein Committee, National Science Foundation (U.S.), New York Times, Orbiting Astronomical Observatory, Princeton University Matterhorn Project, Project Apollo, Skylab, Smithsonian Astrophysical Observatory Multiple Mirror Telescope, Smithsonian Institution National Air and Space Museum, Space Shuttle, United States Naval Ordnance Laboratory, United States Office of Management and Budget, United States Office of Naval Research, University of California at Berkeley, and Viking (Rocket).
In this interview George Field discusses topics such as: his time at the University of California, Berkeley; Charles Townes; Lick Observatory; working with the National Aeronautics and Space Administration (NASA); radio astronomy work with Ed Purcell; detecting neutral hydrogen gas at big red shifts; Fred Whipple; moving to the Harvard College Observatory; planning for the Harvard-Smithsonian Center for Astrophysics; Charles Lundquist; Riccardo Giacconi; Smithsonian Astrophysical Observatory; Northeast Radio Observatory Corporation (NEROC); orbiting solar observatories (OSOs); Dave Challinor; Bart Bok.
This interview concentrates on Goldberg's involvement in the use of V-2's to obtain solar spectra, while serving as Director of McMath-Hulbert Observatory and Chairman of the Astronomy Department at the University of Michigan (1946-1960). The discussion centers on his contacts with Donald Howard Menzel, Richard Tousey, and Lyman Spitzer, and Naval Research Laboratory and the Office of Naval Research, in an attempt to delineate some of the organizational relationships which arose from the availability of the V-2 rockets. Also discussed is Goldberg's administrative experience with NASA, and his involvement with Kitt Peak National Observatory.
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.
In this interview Joseph Taylor discusses topics such as: his family background and childhood; Haverford College; Fay Ajzenberg-Selove; Tom Benham; going on to do a degree in radio astronomy from Harvard University; working in the summer at the Harvard College Observatory on optical astronomy; quasars; pulsars; Leo Goldberg; Donald Menzel and Bill Lilller; Ed Lilley and Alan Maxwell; radio interferometry; lunar occultation; University of Massachusetts; Bill Irvine; Dick Huguenin; National Science Foundation; National Aeronautics and Space Administration (NASA); Dick Manchester; National Radio Astronomy Observatory's telescopes in Green Bank, West Virginia; Russell Alan Hulse.
Life of his father, Karl Schwarzschild; father's scientific relationships in Göttingen (Felix Klein, David Hilbert); move to Potsdam, 1909; relations with Potsdam and Berlin scientists (Albert Einstein, Karl Sommerfeld); father's Jewish background concealed. M. Schwarzschild's youth in Göttingen and Berlin; early education, interest in astronomy and mathematics. Undergraduate at Göttingen Universität (Hans Kienle, Richard Courant, Neugebauer), 1930-1933; graduate work at Gottingen Observatory, 1933-1935; his reaction to Nazism. Introduction to astrophysics (Arthur Eddington), interest in stellar interiors and stellar evolution; contacts with other astronomers from Gottingen Observatory (Otto Heckmann, Kienle, Rupert Wildt); comments on general relativity; interest in pulsating stars; leaves Göttingen, 1936. Postdoctorate at Oslo (Svein Rosseland); Jan Oort, Ejnar Hertzsprung; mechanical analog computer for computations in astrophysics and celestial mechanics; comments on development of theory of stellar interiors, 1939-1950. To Harvard College Observatory (Harlow Shapley), 1938; C. Payne-Gaposchkin, Bart Bok; comparison of European and American observational style, social scene; Barbara Schwarzschild's difficulties as female astronomer; contacts with S. Chandrasekhar and other astronomers. Tour of the United States; visits Mt. Wilson Observatory (Wilhelm Baade, Rudolph Minkowski, Edwin Hubble, Milton Humason), 1940; Shapley's relationship with Mt. Wilson staff. Harvard (Fred Whipple), 1938-1941; Shapley as a leader; astronomy summer school at Harvard; work on Cepheid variables in M3 (Bok, Chandrasekhar); overall impact on Schwarzschild of Harvard period. Columbia University (Jan Schildt, I. I. Rabi), 1940-1942; difficulties there; origin and funding of Thomas Watson Astronomical Computing Center; discussion of cosmology in the late 1930s; contacts with physicists (Enrico Fermi). In U.S. Army, 1941-1945; enters as private, teaches math to recruits; refuses invitation to Los Alamos; transferred to Aberdeen Proving Ground, dissatisfaction there; to officers training school, does bombing analysis for Italian campaign. Work relating to stellar interiors and evolution, 1938-1946; nuclear energy source ideas (Hans Bethe, Fermi); Eddington, Gerard Kuiper, Chandrasekhar, G. Keller; German astronomers during World War II (Ludwig Biermann). Discussion of wife's career and her role in his career. Early ideas about red giants (Öpik, Herman Bondi, Fred Hoyle), 1946-1950. Work on acoustic wave energy transport (R. Richardson, Gold); work on chemical composition differences in stellar populations. To Princeton University (Spitzer, H. N. Russell), 1947; Project Matterhorn (start of bomb and fusion projects); relationship with Russell. Stellar evolution work in the 1950s; computer work (John Von Neumann, Richard Härm), mid-1950s; collaboration with Allan Sandage evolving a stellar model, 1952; computing towards red giants; observational cluster work, 1951; ages, metallicity, and the Big Bang; beginnings of "astrophysical" cosmology. Evolution theory after late 1950s; effect of computers on theoretical progress; relation of evolution theory to cosmology; general comments on his work in stellar evolution; interactions with Robert Dicke; views on cosmology, general relativity. Need for better solar convection work leads to use of balloons (James Van Allen); post-Sputnik funding; on cooperation with industry and engineers; Stratoscope II (Bob Danielson, Spitzer). Years advising the National Science Foundation, President's Science Advisory Committee, 1959-1976, and National Aeronautics and Space Administration (Von Neumann), to 1969; The International Astronomical Union, 1964-1970; American Asronomical Society, 1967-1973. Informal advisor to various observatories: Kitt Peak National Observatory, Mt. Wilson-Palomar Observatories, Carnegie Southern Observatory. Recent work on galactic structure. Reflects on importance of ethical standards; his feelings about religion and nature.
Life of his father, Karl Schwarzschild; father's scientific relationships in Göttingen (Felix Klein, David Hilbert); move to Potsdam, 1909; relations with Potsdam and Berlin scientists (Albert Einstein, Karl Sommerfeld); father's Jewish background concealed. M. Schwarzschild's youth in Göttingen and Berlin; early education, interest in astronomy and mathematics. Undergraduate at Göttingen Universität (Hans Kienle, Richard Courant, Neugebauer), 1930-1933; graduate work at Gottingen Observatory, 1933-1935; his reaction to Nazism. Introduction to astrophysics (Arthur Eddington), interest in stellar interiors and stellar evolution; contacts with other astronomers from Gottingen Observatory (Otto Heckmann, Kienle, Rupert Wildt); comments on general relativity; interest in pulsating stars; leaves Göttingen, 1936. Postdoctorate at Oslo (Svein Rosseland); Jan Oort, Ejnar Hertzsprung; mechanical analog computer for computations in astrophysics and celestial mechanics; comments on development of theory of stellar interiors, 1939-1950. To Harvard College Observatory (Harlow Shapley), 1938; C. Payne-Gaposchkin, Bart Bok; comparison of European and American observational style, social scene; Barbara Schwarzschild's difficulties as female astronomer; contacts with S. Chandrasekhar and other astronomers. Tour of the United States; visits Mt. Wilson Observatory (Wilhelm Baade, Rudolph Minkowski, Edwin Hubble, Milton Humason), 1940; Shapley's relationship with Mt. Wilson staff. Harvard (Fred Whipple), 1938-1941; Shapley as a leader; astronomy summer school at Harvard; work on Cepheid variables in M3 (Bok, Chandrasekhar); overall impact on Schwarzschild of Harvard period. Columbia University (Jan Schildt, I. I. Rabi), 1940-1942; difficulties there; origin and funding of Thomas Watson Astronomical Computing Center; discussion of cosmology in the late 1930s; contacts with physicists (Enrico Fermi). In U.S. Army, 1941-1945; enters as private, teaches math to recruits; refuses invitation to Los Alamos; transferred to Aberdeen Proving Ground, dissatisfaction there; to officers training school, does bombing analysis for Italian campaign. Work relating to stellar interiors and evolution, 1938-1946; nuclear energy source ideas (Hans Bethe, Fermi); Eddington, Gerard Kuiper, Chandrasekhar, G. Keller; German astronomers during World War II (Ludwig Biermann). Discussion of wife's career and her role in his career. Early ideas about red giants (Öpik, Herman Bondi, Fred Hoyle), 1946-1950. Work on acoustic wave energy transport (R. Richardson, Gold); work on chemical composition differences in stellar populations. To Princeton University (Spitzer, H. N. Russell), 1947; Project Matterhorn (start of bomb and fusion projects); relationship with Russell. Stellar evolution work in the 1950s; computer work (John Von Neumann, Richard Härm), mid-1950s; collaboration with Allan Sandage evolving a stellar model, 1952; computing towards red giants; observational cluster work, 1951; ages, metallicity, and the Big Bang; beginnings of "astrophysical" cosmology. Evolution theory after late 1950s; effect of computers on theoretical progress; relation of evolution theory to cosmology; general comments on his work in stellar evolution; interactions with Robert Dicke; views on cosmology, general relativity. Need for better solar convection work leads to use of balloons (James Van Allen); post-Sputnik funding; on cooperation with industry and engineers; Stratoscope II (Bob Danielson, Spitzer). Years advising the National Science Foundation, President's Science Advisory Committee, 1959-1976, and National Aeronautics and Space Administration (Von Neumann), to 1969; The International Astronomical Union, 1964-1970; American Asronomical Society, 1967-1973. Informal advisor to various observatories: Kitt Peak National Observatory, Mt. Wilson-Palomar Observatories, Carnegie Southern Observatory. Recent work on galactic structure. Reflects on importance of ethical standards; his feelings about religion and nature.
Life of his father, Karl Schwarzschild; father's scientific relationships in Göttingen (Felix Klein, David Hilbert); move to Potsdam, 1909; relations with Potsdam and Berlin scientists (Albert Einstein, Karl Sommerfeld); father's Jewish background concealed. M. Schwarzschild's youth in Göttingen and Berlin; early education, interest in astronomy and mathematics. Undergraduate at Göttingen Universität (Hans Kienle, Richard Courant, Neugebauer), 1930-1933; graduate work at Gottingen Observatory, 1933-1935; his reaction to Nazism. Introduction to astrophysics (Arthur Eddington), interest in stellar interiors and stellar evolution; contacts with other astronomers from Gottingen Observatory (Otto Heckmann, Kienle, Rupert Wildt); comments on general relativity; interest in pulsating stars; leaves Göttingen, 1936. Postdoctorate at Oslo (Svein Rosseland); Jan Oort, Ejnar Hertzsprung; mechanical analog computer for computations in astrophysics and celestial mechanics; comments on development of theory of stellar interiors, 1939-1950. To Harvard College Observatory (Harlow Shapley), 1938; C. Payne-Gaposchkin, Bart Bok; comparison of European and American observational style, social scene; Barbara Schwarzschild's difficulties as female astronomer; contacts with S. Chandrasekhar and other astronomers. Tour of the United States; visits Mt. Wilson Observatory (Wilhelm Baade, Rudolph Minkowski, Edwin Hubble, Milton Humason), 1940; Shapley's relationship with Mt. Wilson staff. Harvard (Fred Whipple), 1938-1941; Shapley as a leader; astronomy summer school at Harvard; work on Cepheid variables in M3 (Bok, Chandrasekhar); overall impact on Schwarzschild of Harvard period. Columbia University (Jan Schildt, I. I. Rabi), 1940-1942; difficulties there; origin and funding of Thomas Watson Astronomical Computing Center; discussion of cosmology in the late 1930s; contacts with physicists (Enrico Fermi). In U.S. Army, 1941-1945; enters as private, teaches math to recruits; refuses invitation to Los Alamos; transferred to Aberdeen Proving Ground, dissatisfaction there; to officers training school, does bombing analysis for Italian campaign. Work relating to stellar interiors and evolution, 1938-1946; nuclear energy source ideas (Hans Bethe, Fermi); Eddington, Gerard Kuiper, Chandrasekhar, G. Keller; German astronomers during World War II (Ludwig Biermann). Discussion of wife's career and her role in his career. Early ideas about red giants (Öpik, Herman Bondi, Fred Hoyle), 1946-1950. Work on acoustic wave energy transport (R. Richardson, Gold); work on chemical composition differences in stellar populations. To Princeton University (Spitzer, H. N. Russell), 1947; Project Matterhorn (start of bomb and fusion projects); relationship with Russell. Stellar evolution work in the 1950s; computer work (John Von Neumann, Richard Härm), mid-1950s; collaboration with Allan Sandage evolving a stellar model, 1952; computing towards red giants; observational cluster work, 1951; ages, metallicity, and the Big Bang; beginnings of "astrophysical" cosmology. Evolution theory after late 1950s; effect of computers on theoretical progress; relation of evolution theory to cosmology; general comments on his work in stellar evolution; interactions with Robert Dicke; views on cosmology, general relativity. Need for better solar convection work leads to use of balloons (James Van Allen); post-Sputnik funding; on cooperation with industry and engineers; Stratoscope II (Bob Danielson, Spitzer). Years advising the National Science Foundation, President's Science Advisory Committee, 1959-1976, and National Aeronautics and Space Administration (Von Neumann), to 1969; The International Astronomical Union, 1964-1970; American Asronomical Society, 1967-1973. Informal advisor to various observatories: Kitt Peak National Observatory, Mt. Wilson-Palomar Observatories, Carnegie Southern Observatory. Recent work on galactic structure. Reflects on importance of ethical standards; his feelings about religion and nature.