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From the Sun to the Universe—The Woolley and Bok Directorships at Mount Stromlo1

Published online by Cambridge University Press:  25 April 2016

A. R. Hyland
Affiliation:
Mount Stromlo and Siding Spring Observatories, The Australian National University
D. J. Faulkner
Affiliation:
Mount Stromlo and Siding Spring Observatories, The Australian National University

Abstract

The twenty years following the Second World War saw great changes in the research interests of the Observatory at Mount Stromlo, with the early emphasis on solar and geophysical phenomena giving way to stellar and galactic astrophysics. This paper traces the development of the astrophysical research work during the directorships of Woolley, who initiated the change of direction, and of Bok, who continued it. Apart from the shift in the Observatory’s research interests, these years were distinguished by (i) an outstanding period of telescope acquisition, which saw the commissioning of the 74 inch reflector, the 50 inch (formerly the Great Melbourne Telescope), the Yale/Columbia refractor (relocated from South Africa), and the Uppsala Schmidt; (ii) an Australia-wide site-testing programme and the consequent establishment of Siding Spring Observatory with the 40 inch, 24 inch and 16 inch reflectors (the site has subsequently, of course, also become the home of the Anglo-Australian Telescope, the U.K. Schmidt, and the ANU 2.3 m Advanced Technology Telescope); (iii) the incorporation of several major technological developments into the instrument complement of the Observatory, including photo-electric photometry, coudé spectroscopy, spectrum scanners, polarization instruments, and digital computers; (iv) the establishment of the link with the Australian National University and the consequent transformation of the Commonwealth Observatory into the Mount Stromlo Observatory; and (v) the setting up of a large and vigorous graduate school, comprising, at Bok’s departure, about fifteen PhD students on course.

Type
History of Australian Astronomy
Copyright
Copyright © Astronomical Society of Australia 1989

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Footnotes

1

This paper was presented during a symposium entitled ‘Neath Southern Skies–the History of Astronomy in Australia’, held at the University of Sydney on Wednesday, 18 May 1988 as part of the ANZAAS Centenary Congress.

References

References and Notes

2 As, in this account, we are chiefly interested in the development of astrophysical interests at Mount Stromlo, we do not deal with the work of the Time Service (renamed the Section on Positional Astronomy in 1961). This service was active under both Woolley and Bok, but was transferred to the Division of National Mapping in 1968. Nor do we discuss the Ionospheric Prediction Service, which was transferred from the Radio Research Board to the Department of the Interior in 1947 and attached to the Commonwealth Observatory, but which did not accompany the Observatory into the Australian National University in 1957.

3 Woolley was Director of the Commonwealth (Solar) Observatory from 26 October 1939 until 7 December 1955 (and also Commonwealth Astronomer following the name change in 1944). Bok was Director of Mount Stromlo Observatory from 15 January 1957 until 19 March 1966.

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6 Minutes of the 10th meeting of the Board of Visitors, 31 January 1951, Resolution 1. Those present at this meeting were: Prof O. U. Vonwiller, Emeritus Professor of Physics, University of Sydney (Chairman); Prof K. E. Bullen, professor of Mathematics, University of Sydney; Sir Kerr Grant, Emeritus Professor of Physics, University of Adelaide; Prof E. J. Hartung, Professor of Chemistry, Univesity of Melbourne; Sir John Madsen, Chairman, Radio Research Board, Sydney; W. A. McLaren, Secretary Department of the Interior; Fr D. O’Connell, Director, Riverview College Observatory; Prof M. L. Oliphant, Director, Research School of Physical Sciences, ANU; and the Commonwealth Astronomer (Prof R v d R. Woolley). Dr A. R. Hogg was secretary.

7 acting on a suggestion made to him by Fr D. O’Connell at the Dublin General Assembly of the IAU in 1955.

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11 Including 74 inch reflectors at the David Dunlap Observatory at Toronto (1935), the Radcliffe Observatory at Pretoria (1948), the Okayama Astrophysical Observatory in Japan (1960), and the Helwan (Kottamia) Observatory in Egypt (1963); and a 76 inch at Haute Provence in France (1958).

12 The old north pier of the Great Melbourne Telescope, unusable at the different latitude of Mount Stromlo, became the foundation stone of the Australian Academy of Science dome in Canberra, and may be seen in the foyer there.

13 Annual Report of Mount Stromlo Observatory, 1957, pp. 15-16.

14 The Report of the Yale-Columbia work became available in 1959.

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