The Perth Observatory is the name of two astronomical observatories located in Western Australia (WA). In 1896, the original observatory was founded in West Perth on Mount Eliza overlooking the city of Perth (obs. code 319). Due to the city's expansion, the observatory moved to Bickley in 1965. The new Perth Observatory is sometimes referred to as Bickley Observatory (obs. code 322, 323).
History
First Perth Observatory The original Perth Observatory was constructed in 1896 and was officially opened in 1900 by John Forrest, the first premier of Western Australia. The observatory was located at Mount Eliza overlooking the city of Perth. Its chief roles were keeping Standard Time for Western Australia and meteorological data collection. The observatory dome was demolished in the 1960s to make way for Dumas House, after the Observatory of the city was relocated elsewhere. The house of the chief astronomer of the old observatory remains today, the current tenant is the National Trust.
WA Government Astronomers
William Ernest Cooke William Ernest Cooke was appointed the first Western Australian Government Astronomer in 1896 after a similar posting at the Adelaide Observatory. On arrival in Perth, his first task was to determine the exact latitude and longitude of the colony. He was also able to determine the time of day with greater accuracy. Before his arrival clocks could vary by up to half an hour. The time was announced each day by a cannon still present on the grounds. The design was by the government architect, George Temple-Poole, and features a bold combination of styles.
Harold Burnham Curlewis Cooke's successor as Government Astronomer was Harold Curlewis who wrote in 1929:
Since the prevailing winds blow over the huge extent of King's Park, its excellence for astronomical work is not impaired by its proximity to the city, as is so often the case with other observatories. ...A glance from the tower, from which a wonderful panorama of Perth may be obtained, shows that no growth of the city can ever adversely affect observing conditions
Curlewis and the WA border
In 1920 and 1921 Curlewis was involved with the Government Astronomer of South Australia, Dodwell, in determinations to fix positions for marking of the West Australian border on the ground with the South Australian border at Deakin, Western Australia. In 1921 the same group from the Deakin determinations travelled by the State Ship, MV Bambra to Wyndham, where they were guided by M.P. Durack to a point on Rosewood station near Argyle Downs close to the 129th meridian east longitude (129° east). They used the relatively new technology of the day, wireless radio time signals, and other methods to fix a position for the Northern Territory border with Western Australia. These early determinations led to the 1968 agreement for the formation of Surveyor Generals Corner. The WA border is not straight (see Western Australia border); at the 26th parallel south (26° south) there is an approximately 127-metre (417 ft) "sideways" section of the WA/NT border, which runs east–west.
Hyman Solomon Spigl Curlewis's successor as Government Astronomer was Hyman Solomon Spigl between 1940 and 1962. Spigl, who was from a surveying background, progressed rebuilding a post war ravaged Observatory by rejuvenating the time service, seismology services, completing the Astrographic Catalogues, became involved in the International Geophysical Year by installing a Markowitz Moon camera and restarted the publications for the Royal Astronomical Society. Additionally, through a National Science Foundation of America grant, he was in the process of refurbishing the Observatory's 150-millimetre (6 in) meridian transit circle to recommence meridian observations. While he never achieved this before his death, and it was never used again, the instrument sits in the foyer of the Perth Observatory now fully refurbished. In 1958 Spigl was awarded a Gledden Travelling Fellowship by the University of Western Australia; Spigl spent 12 months travelling in the US, UK and Europe. Spigl was actively searching for a new site for the Perth Observatory as a result of the decision for it to be relocated as an outcome of the implementation of the 1955 Stephenson-Hepburn Report. Spigl spent many years lecturing in surveying at the University of Western Australia and was involved in the Astronomical Society of Western Australia.
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