Yerkes Observatory

This interview is a focused exploratory interview covering William Van Altena's brief career history as a student at the University of California, Berkeley and Lick Observatory; interests in astrometry and work for van den Bos and Vasilevskis; work at Yerkes Observatory; state of astrometry and role of automation; discussion of names prominent in community; LST program; funding; tenure.

Family background; education at Tubigen Univ.; Schrodinger Theory thesis at Univ. of Munich (1927), influence of Sommerfeld, Heisenberg. Potsdam experiments inspired by K. Schwarzschild, Emden: Local thermodynamic equilibrium and curve of growth. Spent 1928 at Mt. Wilson. Return to Germany to teach physics during Depression; use of microphotometer, Coude spectrograph; analysis of Tau Scorpii. Pre-war professorship at Yerkes with Struve: line profile information, stellar composition. WWII return to Kiel, star temperature detection, solar spectrum analysis, elements/energy production. Isolation and destruction of German physics, anti-German attitude. Remarks on history of science, views on contemporaries and astrophysical (radio) research; fate of Unsold's correspondence.

Early life in Hamburg, Germany; education at Darmstadt; postdoc period in Göttingen, and Bristol, England; setting up his own lab at Darmstadt as Privatdozent; origins of first of his series of books; departure due to Jewish heritage of wife; fresh start in Saskatoon; more books; limited war research; first direct contributions to astrophysics during the war years; three years at the Yerkes Observatory; forty years of work at the National Research Council in Ottawa; Nobel Prize. Experimental techniques include high resolution grating spectroscopy with photographic plates, very long absorption paths, continuous and flash discharge emission and absorption. Contributions in molecular quantum mechanics, quantum chemistry, astronomy and astrophysics, planetary and cometary atmospheres. Leitmotif is hydrogen: H, H2, H3, H3+. Also prominently mentioned are: National Socialism and World War II.

Early life in Hamburg, Germany; education at Darmstadt; postdoc period in Göttingen, and Bristol, England; setting up his own lab at Darmstadt as Privatdozent; origins of first of his series of books; departure due to Jewish heritage of wife; fresh start in Saskatoon; more books; limited war research; first direct contributions to astrophysics during the war years; three years at the Yerkes Observatory; forty years of work at the National Research Council in Ottawa; Nobel Prize. Experimental techniques include high resolution grating spectroscopy with photographic plates, very long absorption paths, continuous and flash discharge emission and absorption. Contributions in molecular quantum mechanics, quantum chemistry, astronomy and astrophysics, planetary and cometary atmospheres. Leitmotif is hydrogen: H, H2, H3, H3+. Also prominently mentioned are: National Socialism and World War II.

Interview discuss John S. Hall's early interest in astronomy; comments about family background and early childhood, schooling in Connecticut and college training at University of Amherst and Yale University. Early contacts and interests in photoelectric photometry, his pioneering efforts in red sensitive cell photometry, work at the Radiation Laboratory at MIT during World War II, postwar research at the Naval Observatory and his co-discovery of interstellar polarization. Also prominently mentioned are: Solon Bailey, A. L. Bennett, Subrahmanyan Chandrasekhar, Thomas Cochran, Robert H. Dicke, Harold Ewen, Fresnell, Green, Jesse Leonard Greenstein, Ejnar Hertzsprung, W. A. Hiltner, Gerald Edward Kron, J. A. Miller, Prescott, Jan Schildt, Frank Schlesinger, Harlow Shapley, Theodore Stoller, Otto Struve, David Todd, Robert Williams Wood; Amherst College Observatory, General Electric Co., Harvard University, Lawrence Radiation Laboratory, Science (journal), Sproul Observatory, United States Navy, and Yerkes Observatory.

Dr. Yoshio Fujita discusses his family background and high school; education at the University of Tokyo, advisor Yuseke Hagihara; textbooks used, courses taken; positions as assistant at the Tokyo Astronomical Observatory then lecturer at the University of Tokyo; weekly colloquium with Toshio Takamine, Hagihara, Fujita and Masao Kotani; equipment used in his research; research interests during his career, including molecular spectra of stars, stellar atmospheres, late-type stars, diatomic molecules; Martin Kellog Fellowship from C. D. Shane to work at Lick Observatory, fellowship from Subrahmanyan Chandrasekhar to work at Yerkes Observatory; in the United States he worked with George Herbig, William P. Bidelman, and Gerard Kuiper; project to build the 74-inch telescope in Japan; trip to use the Victoria 72-inch telescope for training; professional memberships and accomplishments.

In this interview Pierre Demarque discusses topics such as: his early interest in astronomy; listening to radio lectures by Fred Hoyle; study at the University of Toronto; interest in cosmology; work with Leonard Searle; master's thesis on stellar structure; influence of Searle and J. Beverly Oke; move to the United States and Louisiana State University; University of Illinois and the influence of Ivan King; Ludwig Biermann; George McVittie; going to the University of Chicago and contact with Chandrasekhar; stellar evolution; Yerkes Observatory; leaving Chicago for Yale University; Walter Baade philosophy of studying cosmology; globular clusters; John Eddy's work on solar variability; stellar populations and galaxy evolution.

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.

Training and influences on his career during graduate years at University of Chicago and Yerkes Observatory in the late 1920s. Discussion of science education and the growth of astronomy in China, activities of the Purple Mountain Observatory in Nanking, and Chang's directorship. Effects of the war for Liberation; discussion of astronomy during the Japanese occupation. Other topics include contact with Bart Bok, visits to Yerkes after World War II, and research in astronomy in China.