Astronomical observatories

Childhood in Germany and family background — competitive spirit; war years — internment and radar work with Bondi and Hoyle (1942-1945) at Cambridge — development of theory of hearing and steady state theory; at Greenwich (1952-1956) — research on lunar surface and terrestrial dynamics; positions at Harvard and Cornell — involvement with Arecibo; involvement with governmental agencies including NSF and NASA — changes in government funding. A major part of the interview covers the development and reception of the steady date theory.

Born in Flagstaff, Arizona; spends professional life as astronomer in Flagstaff, 1931-1981. Early life in Flagstaff, the Lowell Observatory's place in it, and how he became a research assistant at Lowell, with particular emphasis on V. M. Slipher, the director from 1916-1955. Describes how the Observatory was transformed as a research institution after World War II, due to changing research topics and shifting patterns of patronage.

Early home life in Indiana, and early schooling. Origins of his interest in astronomy and the influence of both family and teachers. College years at Indiana University and contacts with members of the astronomy department there (E.C. and Vesto M. Slipher). Discussion of history of Indiana University Astronomy Department, and its contact with the Lowell Observatory. Graduate school at Harvard University, Peter van de Kamp's influence, work in stellar kinematics, impressions of atmosphere at Harvard. Faculty position at Indiana University, 1937 to present. Origins of Goethe Link Observatory, and the growth of the department. Organizational work in the American Astronomical Society (AAS). Work at National Science Foundation (NSF) as scientific officer for astronomy, 1956, and development of National Radio Astronomy Observatory (NRAO); NSF and AUI; NRAO directors; Sputnik; Kitt Peak Observatory site survey, NSF and Associated Universities for Research in Astronomy (AURA); Aden Meinel; John B. Irwin's proposal for a photoelectric observatory; Flagstaff Conference; Robert McMath Panel; structure of Kitt Peak staff; Chilean observatory and development of Cerro Tololo; Gerard Kuiper's role in southern observatory; European Southern Observatory (ESO), Carnegie Southern Observatory (CARSO) and AURA joint Paris meeting; Russian interests in southern observatory; CARSO application to Ford Foundation; agreements between AURA and CARSO; building telescopes at Kitt Peak and Cerro Tololoth︣e WISCO dispute; policy problems; AURA Board meetings; demise of Space Division at Kitt Peak; Whitford Panel; White Sands rocket project; astronomy and teaching at Indiana. Also prominently mentioned are: Jorge Alessandri Rodríguez, Lawrence Hugh Aller, Bart Jan Bok, William A. Cogshall, James Cuffey, H. T. Davis, Arthur Foley, Paul Herget, Helen Sawyer Hogg, Virgil Hunt, Geoffrey Keller, C. O. Lampland, Robert Reynolds McMath, Edward Arthur Milne, Samuel A. Mitchell, William Wilson Morgan, Jason John Nassau, Henry Norris Russell, Frederico Rutllant, Charles Donald Shane, Harlow Shapley, Jurgen Stock, Otto Struve, Merle Antony Tuve, Herman B. Wells, K. P. Williams, Marshall Wrubel; Associated Universities, Inc., Ford Foundation, Indiana Higher Education Telecommunication System, Lick Observatory, McDonald Observatory, and Yerkes Observatory.

Early home life in Indiana, and early schooling. Origins of his interest in astronomy and the influence of both family and teachers. College years at Indiana University and contacts with members of the astronomy department there (E.C. and Vesto M. Slipher). Discussion of history of Indiana University Astronomy Department, and its contact with the Lowell Observatory. Graduate school at Harvard University, Peter van de Kamp's influence, work in stellar kinematics, impressions of atmosphere at Harvard. Faculty position at Indiana University, 1937 to present. Origins of Goethe Link Observatory, and the growth of the department. Organizational work in the American Astronomical Society (AAS). Work at National Science Foundation (NSF) as scientific officer for astronomy, 1956, and development of National Radio Astronomy Observatory (NRAO); NSF and AUI; NRAO directors; Sputnik; Kitt Peak Observatory site survey, NSF and Associated Universities for Research in Astronomy (AURA); Aden Meinel; John B. Irwin's proposal for a photoelectric observatory; Flagstaff Conference; Robert McMath Panel; structure of Kitt Peak staff; Chilean observatory and development of Cerro Tololo; Gerard Kuiper's role in southern observatory; European Southern Observatory (ESO), Carnegie Southern Observatory (CARSO) and AURA joint Paris meeting; Russian interests in southern observatory; CARSO application to Ford Foundation; agreements between AURA and CARSO; building telescopes at Kitt Peak and Cerro Tololoth︣e WISCO dispute; policy problems; AURA Board meetings; demise of Space Division at Kitt Peak; Whitford Panel; White Sands rocket project; astronomy and teaching at Indiana. Also prominently mentioned are: Jorge Alessandri Rodríguez, Lawrence Hugh Aller, Bart Jan Bok, William A. Cogshall, James Cuffey, H. T. Davis, Arthur Foley, Paul Herget, Helen Sawyer Hogg, Virgil Hunt, Geoffrey Keller, C. O. Lampland, Robert Reynolds McMath, Edward Arthur Milne, Samuel A. Mitchell, William Wilson Morgan, Jason John Nassau, Henry Norris Russell, Frederico Rutllant, Charles Donald Shane, Harlow Shapley, Jurgen Stock, Otto Struve, Merle Antony Tuve, Herman B. Wells, K. P. Williams, Marshall Wrubel; Associated Universities, Inc., Ford Foundation, Indiana Higher Education Telecommunication System, Lick Observatory, McDonald Observatory, and Yerkes Observatory.

Early life in the Cotswolds, England; Bristol University, 1943, and physics program during WWII; teachers include Nevill Mott and Edward Tyndall; effect of WWII; work with Harrie Massey on meson capture; University College, London; meets wife and growing contacts in astronomy, late 1940s; thesis, 1952; work in stellar atmosphere; visit to U.S. at Howard and Terkes, 1951-1953; Cavendish group under Martin Ryle, house theoretician; contact with William Fowler and growing interest in nucleosynthesis, 1954; fellowship at Pasadena, 1955; opinions on operation of major observatories, philosophy of cosmological research, reaction to steady state; problem of high energy sources, synchrotron radiation; belief structure in cosmology; Halton Arp’s work; Nuclear Processes in Astrophysics - B²FH; Yerkes Observatory, 1957; physics of galaxies, 1959. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, Margaret Burbidge, Subrahmanyan Chandrasekhar, Paul A. M. Dirac, Enrico Fermi, William Alfred Fowler, James Edward Gunn, Fred Hoyle, Martin Ryle, Allan Sandage, Maarten Schmidt, and Arthur Wolfe.

Early life and education; research on spectroscopy with Robert A. Millikan at University of Chicago and Caltech; early teaching career at Caltech; work on forbidden lines, 200-inch telescope project; visitors to Caltech during the 1930s include Albert Einstein and Arnold Sommerfeld; effects of the Depression and World War II on astronomy; postwar reorganization, staff and funding at Mt. Wilson and Palomar Observatories; Edwin P. Hubble's role at the observatory; educational aspects of the observatory program (professional and public); research groups and research interests; theorists and observationalists, Jesse Greenstein, Guido Münch, Jan Oort, radio astronomy; recollections and evaluations of own work after retirement. Also prominently mentioned are: Walter Sydney Adams, Harold Delos Babcock, William Alvin Baum, Wilhelm Bjerknes, T. Bowen, Geoffrey R. Burbidge, Margaret Burbidge, Vannevar Bush, J. Carroll, Lee Alvin DuBridge, Theodore Dunham Jr., Edlén, Robley Dunglison Evans, William Alfred Fowler, Henry Gordon Gale, Cecilia Helena Payne Gaposchkin, George Ellery Hale, John L. Hall, Don Hendrix, Alfred H. Joy, Thomas Lauritsen, Ernest Orlando Lawrence, Max Mason, Edwin Mattison McMillan, Merriam, Paul Merrill, Rudolph Leo Bernhard Minkowski, R. Otis, Henry Norris Russell, John Donovan Strong, Richard Chase Tolman, Merle Antony Tuve; Carnegie Corporation of New York, Carnegie Institution of Washington.

Early life and education; research on spectroscopy with Robert A. Millikan at University of Chicago and Caltech; early teaching career at Caltech; work on forbidden lines, 200-inch telescope project; visitors to Caltech during the 1930s include Albert Einstein and Arnold Sommerfeld; effects of the Depression and World War II on astronomy; postwar reorganization, staff and funding at Mt. Wilson and Palomar Observatories; Edwin P. Hubble's role at the observatory; educational aspects of the observatory program (professional and public); research groups and research interests; theorists and observationalists, Jesse Greenstein, Guido Münch, Jan Oort, radio astronomy; recollections and evaluations of own work after retirement. Also prominently mentioned are: Walter Sydney Adams, Harold Delos Babcock, William Alvin Baum, Wilhelm Bjerknes, T. Bowen, Geoffrey R. Burbidge, Margaret Burbidge, Vannevar Bush, J. Carroll, Lee Alvin DuBridge, Theodore Dunham Jr., Edlén, Robley Dunglison Evans, William Alfred Fowler, Henry Gordon Gale, Cecilia Helena Payne Gaposchkin, George Ellery Hale, John L. Hall, Don Hendrix, Alfred H. Joy, Thomas Lauritsen, Ernest Orlando Lawrence, Max Mason, Edwin Mattison McMillan, Merriam, Paul Merrill, Rudolph Leo Bernhard Minkowski, R. Otis, Henry Norris Russell, John Donovan Strong, Richard Chase Tolman, Merle Antony Tuve; Carnegie Corporation of New York, Carnegie Institution of Washington.

Interview discusses, not in chronological order: early home life and schooling; undergraduate at Leiden, influence of Paul Ehrenfest, Jan H. Oort, Jacobus C. Kapteyn, Gerard Kuiper, Antonie Pannekoek, Ejnar Hertzsprung. Recollections of work of Georg Uhlenbeck and Samuel Goudsmit. Assistant to Peter van Rhijn at Groningen ca. 1928, work on various stellar and galactic topics. Move to Harvard, 1929, and atmosphere there under Harlow Shapley. Marriage to Priscilla Fairfield Bok; her contacts with William W. Campbell. Search for and interpretation of spiral auras of our galaxy; studies of stellar density distribution. Activities during World War II. Harvard astronomy group's difficult postwar transition; McCarthyism. Work on nebulae and globules. Comments on astronomy at Mt. Wilson, Tonantziutla, and South Africa. Origins of Harvard radio astronomy and National Radio Astronomy Observatory, and their funding. Move to Australia, 1956, and conditions there. Move to Steward Observatory of University of Arizona, 1964, and conditions there. Location of national observatory at Kitt Peak; management of Kitt Peak. Discussions of astronomy, education, popularization, employment, and organization. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, McGeorge Bundy, Edwin F. Carpenter, Tom Cherry, James Bryant Conant, Arthur Stanley Eddington, Sergei Gaposchkin, Jesse Leonard Greenstein, Haro, David Heeschen, Ejnar Hertzsprung, James Jeans, Ivan Robert King, Bertil Lindblad, Antonia Maury, Nicholas Ulrich Mayall, Joseph McCarthy, Sidney McCuskey, Aden Meinel, Donald Howard Menzel, Robert Menzies, James E. Miller, Edward Arthur Milne, William Wilson Morgan, Edward Charles Pickering, Harry Hemley Plaskett, Nathan Pusey, Martin Schwarzschild, Willem de Sitter, Otto Struve; American Astronomical Society, Associated Universities for Research in Astronomy, Associated Universities, Inc., Boyden Observatory, Case Institute of Technology, Harvard College Observatory, Harvard Series on Astronomy, Indiana University, Mount Stromlo Observatory, National Science Foundation (U.S.), Ohio State University, Princeton University, Rijksuniversiteit te Groningen, Rijksuniversiteit te Leiden, University of Arizona, University of Illinois, University of Michigan, and University of Texas.

Interview discusses, not in chronological order: early home life and schooling; undergraduate at Leiden, influence of Paul Ehrenfest, Jan H. Oort, Jacobus C. Kapteyn, Gerard Kuiper, Antonie Pannekoek, Ejnar Hertzsprung. Recollections of work of Georg Uhlenbeck and Samuel Goudsmit. Assistant to Peter van Rhijn at Groningen ca. 1928, work on various stellar and galactic topics. Move to Harvard, 1929, and atmosphere there under Harlow Shapley. Marriage to Priscilla Fairfield Bok; her contacts with William W. Campbell. Search for and interpretation of spiral auras of our galaxy; studies of stellar density distribution. Activities during World War II. Harvard astronomy group's difficult postwar transition; McCarthyism. Work on nebulae and globules. Comments on astronomy at Mt. Wilson, Tonantziutla, and South Africa. Origins of Harvard radio astronomy and National Radio Astronomy Observatory, and their funding. Move to Australia, 1956, and conditions there. Move to Steward Observatory of University of Arizona, 1964, and conditions there. Location of national observatory at Kitt Peak; management of Kitt Peak. Discussions of astronomy, education, popularization, employment, and organization. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, McGeorge Bundy, Edwin F. Carpenter, Tom Cherry, James Bryant Conant, Arthur Stanley Eddington, Sergei Gaposchkin, Jesse Leonard Greenstein, Haro, David Heeschen, Ejnar Hertzsprung, James Jeans, Ivan Robert King, Bertil Lindblad, Antonia Maury, Nicholas Ulrich Mayall, Joseph McCarthy, Sidney McCuskey, Aden Meinel, Donald Howard Menzel, Robert Menzies, James E. Miller, Edward Arthur Milne, William Wilson Morgan, Edward Charles Pickering, Harry Hemley Plaskett, Nathan Pusey, Martin Schwarzschild, Willem de Sitter, Otto Struve; American Astronomical Society, Associated Universities for Research in Astronomy, Associated Universities, Inc., Boyden Observatory, Case Institute of Technology, Harvard College Observatory, Harvard Series on Astronomy, Indiana University, Mount Stromlo Observatory, National Science Foundation (U.S.), Ohio State University, Princeton University, Rijksuniversiteit te Groningen, Rijksuniversiteit te Leiden, University of Arizona, University of Illinois, University of Michigan, and University of Texas.

Interview discusses, not in chronological order: early home life and schooling; undergraduate at Leiden, influence of Paul Ehrenfest, Jan H. Oort, Jacobus C. Kapteyn, Gerard Kuiper, Antonie Pannekoek, Ejnar Hertzsprung. Recollections of work of Georg Uhlenbeck and Samuel Goudsmit. Assistant to Peter van Rhijn at Groningen ca. 1928, work on various stellar and galactic topics. Move to Harvard, 1929, and atmosphere there under Harlow Shapley. Marriage to Priscilla Fairfield Bok; her contacts with William W. Campbell. Search for and interpretation of spiral auras of our galaxy; studies of stellar density distribution. Activities during World War II. Harvard astronomy group's difficult postwar transition; McCarthyism. Work on nebulae and globules. Comments on astronomy at Mt. Wilson, Tonantziutla, and South Africa. Origins of Harvard radio astronomy and National Radio Astronomy Observatory, and their funding. Move to Australia, 1956, and conditions there. Move to Steward Observatory of University of Arizona, 1964, and conditions there. Location of national observatory at Kitt Peak; management of Kitt Peak. Discussions of astronomy, education, popularization, employment, and organization. Also prominently mentioned are: Wilhelm Heinrich Walter Baade, McGeorge Bundy, Edwin F. Carpenter, Tom Cherry, James Bryant Conant, Arthur Stanley Eddington, Sergei Gaposchkin, Jesse Leonard Greenstein, Haro, David Heeschen, Ejnar Hertzsprung, James Jeans, Ivan Robert King, Bertil Lindblad, Antonia Maury, Nicholas Ulrich Mayall, Joseph McCarthy, Sidney McCuskey, Aden Meinel, Donald Howard Menzel, Robert Menzies, James E. Miller, Edward Arthur Milne, William Wilson Morgan, Edward Charles Pickering, Harry Hemley Plaskett, Nathan Pusey, Martin Schwarzschild, Willem de Sitter, Otto Struve; American Astronomical Society, Associated Universities for Research in Astronomy, Associated Universities, Inc., Boyden Observatory, Case Institute of Technology, Harvard College Observatory, Harvard Series on Astronomy, Indiana University, Mount Stromlo Observatory, National Science Foundation (U.S.), Ohio State University, Princeton University, Rijksuniversiteit te Groningen, Rijksuniversiteit te Leiden, University of Arizona, University of Illinois, University of Michigan, and University of Texas.