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Perth Observatory

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An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy , climatology / meteorology , geophysics , oceanography and volcanology are examples of disciplines for which observatories have been constructed.

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83-557: 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 ). The original Perth Observatory

166-531: A Polar Year, especially considering recent advances in rocketry, radar, and computing. Berkner and Chapman proposed to the International Council of Scientific Unions that an International Geophysical Year (IGY) be planned for 1957–58, coinciding with an approaching period of maximum solar activity. In 1952, the IGY was announced. Joseph Stalin 's death in 1953 opened the way for international collaboration with

249-584: A documentary about the project for the National Snow and Ice Data Center . The participating countries for the IGY included the following: In the end, the IGY was a resounding success, and it led to advancements that live on today. For example, the work of the IGY led directly to the Antarctic Treaty , which called for the use of Antarctica for peaceful purposes and cooperative scientific research. Since then, international cooperation has led to protecting

332-463: A free and open exchange of data among nations. ICSU-WDS goals are to preserve quality-assured scientific data and information, to facilitate open access, and promote the adoption of standards. ICSU World Data System created in 2008 superseded the World Data Centers (WDCs) and Federation of Astronomical and Geophysical data analysis Services (FAGS) created by ICSU to manage data generated by

415-690: A large percentage of clear nights per year, dry air, and are at high elevations. At high elevations, the Earth's atmosphere is thinner, thereby minimizing the effects of atmospheric turbulence and resulting in better astronomical " seeing ". Sites that meet the above criteria for modern observatories include the southwestern United States , Hawaii , Canary Islands , the Andes , and high mountains in Mexico such as Sierra Negra . Major optical observatories include Mauna Kea Observatory and Kitt Peak National Observatory in

498-731: A life member of the Astronomical Association of Western Australia and a member of the IAU 's original Commission 8 (Astrometry) and I (Fundamental Astronomy); he also continued the Observatory's public information services and tours. He retired on 4 January 1985 and died on 8 April 2015. Upon the retirement of Dr I Nikoloff, the governing body of the Perth Observatory at that time, the Department of Science and Technology (Australia) , replaced

581-520: A particular subject (such as public health observatory ) or for a particular geographic area ( European Audiovisual Observatory ). Astronomical observatories are mainly divided into four categories: space-based , airborne , ground-based, and underground-based. Historically, ground-based observatories were as simple as containing an astronomical sextant (for measuring the distance between stars ) or Stonehenge (which has some alignments on astronomical phenomena). Ground-based observatories, located on

664-421: A position he held until 1982 when he was elected president for a 3-year term. At the same time became a working member of International Astronomical Union Commission 20 until 1988 – Positions and Motions of Minor Planets, Satellites and Comets. The Perth Observatory was positioned well for Halley's Comet in 1986/1987 and under Candy the Perth Observatory produced 10% of all Earth based astrometric positions for

747-585: A remote 5,640 m (18,500 ft) mountaintop in the Atacama Desert of Chile. The oldest proto-observatories, in the sense of an observation post for astronomy, The oldest true observatories, in the sense of a specialized research institute , include: Space-based observatories are telescopes or other instruments that are located in outer space , many in orbit around the Earth. Space telescopes can be used to observe astronomical objects at wavelengths of

830-481: A scientific function, however Harris also restarted the public tours on 23 October 1966 and maintained the provision of information services to Western Australia. Harris also continued time and tide services for Western Australia, however as had been the case in 1908 for Meteorology, the move saw seismic monitoring activities being relocated to Mundaring under the Commonwealth Government control. Harris

913-488: A significant number of observations to the Minor Planet Center . He continued the first publication of the Perth Observatory on comet and minor positions, commenced by Mr B Harris, with Communication No. 2, 3, 4 and the last, that of Communication No. 5 in 1986. By 1979 his astrometric abilities and contributions were widely acknowledged and he became Vice President of International Astronomical Union , Commission 6,

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996-620: A two-man camp was installed beside Taylor Glacier, 60 miles (97 km) west of Mawson. Its principal purpose was to enable parallactic photography of the aurora australis (thus locating it in space), but it also permitted studies of Emperor penguins in the adjacent rookery. Two years later, Australia took over the running of Wilkes , a station built for the IGY by the United States. When Wilkes rapidly deteriorated from snow and ice accumulation, plans were made to build Casey Station , known as Repstat ("replacement station"). Opened in 1969, Repstat

1079-419: A week at the absolute reference point calibration measurements are performed. Example magnetic observatories include: Example seismic observation projects and observatories include: Example gravitational wave observatories include: A volcano observatory is an institution that conducts the monitoring of a volcano as well as research in order to understand the potential impacts of active volcanism. Among

1162-833: Is a facility which precisely measures the total intensity of Earth's magnetic field for field strength and direction at standard intervals. Geomagnetic observatories are most useful when located away from human activities to avoid disturbances of anthropogenic origin, and the observation data is collected at a fixed location continuously for decades. Magnetic observations are aggregated, processed, quality checked and made public through data centers such as INTERMAGNET . The types of measuring equipment at an observatory may include magnetometers (torsion, declination-inclination fluxgate, proton precession, Overhauser-effect), variometer (3-component vector, total-field scalar), dip circle , inclinometer , earth inductor, theodolite , self-recording magnetograph, magnetic declinometer, azimuth compass. Once

1245-444: Is a scientific institution whose main task is to make observations in the fields of meteorology, geomagnetism and tides that are important for the navy and civil shipping. An astronomical observatory is usually also attached. Some of these observatories also deal with nautical weather forecasts and storm warnings, astronomical time services, nautical calendars and seismology. Example marine observatories include: A magnetic observatory

1328-648: Is that, because of their location above the Earth's atmosphere, their images are free from the effects of atmospheric turbulence that plague ground-based observations. As a result, the angular resolution of space telescopes such as the Hubble Space Telescope is often much smaller than a ground-based telescope with a similar aperture . However, all these advantages do come with a price. Space telescopes are much more expensive to build than ground-based telescopes. Due to their location, space telescopes are also extremely difficult to maintain. The Hubble Space Telescope

1411-599: Is the Mauna Kea Observatory , located near the summit of a 4,205 m (13,796 ft) volcano in Hawaiʻi. The Chacaltaya Astrophysical Observatory in Bolivia, at 5,230 m (17,160 ft), was the world's highest permanent astronomical observatory from the time of its construction during the 1940s until 2009. It has now been surpassed by the new University of Tokyo Atacama Observatory , an optical-infrared telescope on

1494-466: 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

1577-463: 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. 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

1660-703: 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

1743-467: The Stratospheric Observatory for Infrared Astronomy use airplanes to observe in the infrared , which is absorbed by water vapor in the atmosphere. High-altitude balloons for X-ray astronomy have been used in a variety of countries. Example underground, underwater or under ice neutrino observatories include: Example meteorological observatories include: A marine observatory

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1826-570: The Antarctic continent at Mawson in 1954. It is now the longest continuously operating station south of the Antarctic Circle. Davis was added in 1957, in the Vestfold Hills, 400 miles (640 km) east of Mawson. The wintering parties for the IGY numbered 29 at Mawson and 4 at Davis, all male. (Both stations now have 16 to 18 winterers, including both sexes.) As a part of the IGY activities,

1909-624: The Antarctic environment, preserving historic sites, and conserving the animals and plants. Today, 41 nations have signed the Treaty and international collaborative research continues. The ICSU World Data System (WDS) was created by the 29th General Assembly of the International Council for Science (ICSU) and builds on the 50-year legacy of the former ICSU World Data Centres (WDCs) and former Federation of Astronomical and Geophysical data-analysis Services (FAGS). This World Data System , hosts

1992-664: 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

2075-555: The Department of Conservation and Land Management, now part of the Department of Parks and Wildlife (Western Australia) . In 2005 the Bickley site was heritage listed, being Australia's oldest continuing operating observatory and Australia's only remaining State Government operated astronomical observatory. The Western Australian astronomy almanac was published in the 2000s by the DEC as part of

2158-636: The Directors position until on 22 January 2013 the WA Government announced that all research programs would be cut and the Observatory would only be open for tours. Martin and the remaining staff of the Perth Observatory took voluntary redundancy. As an earthquake observatory in Perth a Milne-Shaw seismograph was utilised between 1923 and 1959 for the recording of earthquakes in Western Australia. After 1959

2241-586: The German expedition work, resulting in the Perth 75 meridian catalogue. In 1967, Harris worked with the University of Western Australia to install a 410-millimetre (16 in) telescope at the Observatory that was built and used by the University of Western Australia staff and students, as well as Perth Observatory astronomers. Harris then moved the astrographic telescope, which had been in storage since August 1963, to

2324-696: The IGY was particularly suited for studying some of these phenomena, since it covered the peak of solar cycle 19 . Both the Soviet Union and the U.S. launched artificial satellites for this event; the Soviet Union's Sputnik 1 , launched on October 4, 1957, was the first successful artificial satellite. Other significant achievements of the IGY included the discovery of the Van Allen radiation belts by Explorer 1 and mid-ocean submarine ridges, an important confirmation of plate-tectonic theory . The origin of

2407-503: The IGY. Although the 1932 Polar Year accomplished many of its goals, it fell short on others because of the advance of World War II. In fact, because of the war, much of the data collected and scientific analyses completed during the 1932 Polar Year were lost forever, something that was particularly troubling to the IGY organizing committee. The committee resolved that "all observational data shall be available to scientists and scientific institutions in all countries." They felt that without

2490-619: The International Geophysical Year can be traced to the International Polar Years held in 1882–1883 , then in 1932–1933 and most recently from March 2007 to March 2009 . On 5 April 1950, multiple scientists (including Lloyd Berkner , Sydney Chapman , S. Fred Singer , and Harry Vestine ) met in James Van Allen 's living room and suggested that the time was ripe to have a worldwide Geophysical Year instead of

2573-412: The International Geophysical Year. The IGY triggered an 18-month year of Antarctic science. The International Council of Scientific Unions , a parent body, broadened the proposals from polar studies to geophysical research. More than 70 existing national scientific organizations then formed IGY committees, and participated in the cooperative effort. Australia established its first permanent base on

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2656-556: The Meridian Section to D. Harwood, but kept a keen involvement in the construction of the subsequent Perth 83 meridian catalogue. While daily administrative duties kept him busy, Nikoloff continued observing on all the Observatory's telescopes at night and on weekends. Nikoloff maintained a good relationship with the University of Western Australia , was a Foundation member and Fellow of the Astronomical Society of Australia ,

2739-625: The Observatory expertise, utilising staff of the Observatory to edit and contribute. The 2002 publication for the 2003 almanac had an extra subtitle which was not utilised in later editions: the really useful guide to the wonders of the night sky . It had been preceded by Astronomical Data (1965–1990) and the Astronomical Handbook (1989–1992 ?). Observatory The term observatoire has been used in French since at least 1976 to denote any institution that compiles and presents data on

2822-590: The Soviet Union. In 1952 the Comité Speciale de l'Année Géophysique Internationale (CSAGI), a special committee of the ICSU, was established to coordinate the International Geophysical Year (IGY) under president Sydney Chapman , a British geophysicist. On 29 July 1955, James C. Hagerty , president Dwight D. Eisenhower 's press secretary, announced that the United States intended to launch "small Earth circling satellites" between 1 July 1957 and 31 December 1958 as part of

2905-550: The Soviet embassy and announced his country's intention to launch a satellite in the "near future". To the surprise of many, the USSR launched Sputnik 1 as the first artificial Earth satellite on 4 October 1957. After several failed Vanguard launches, Wernher von Braun and his team convinced President Dwight D. Eisenhower to use one of their US Army missiles for the Explorer program (there

2988-681: The State Government, the Observatory was moved to its current site at Bickley near Mount Gungin in the Darling Range . Construction of the new observatory cost $ 600,000, and it was opened by the Premier Sir David Brand on 30 September 1966. The Observatory has fought off several attempts to close the facility by the State Government , the most serious being in 1987 when it was part of the Department of State Services. An outcry from

3071-620: The US, Roque de los Muchachos Observatory in Spain, and Paranal Observatory and Cerro Tololo Inter-American Observatory in Chile . Specific research study performed in 2009 shows that the best possible location for ground-based observatory on Earth is Ridge A  — a place in the central part of Eastern Antarctica. This location provides the least atmospheric disturbances and best visibility. Beginning in 1933, radio telescopes have been built for use in

3154-633: The United States contribution to the International Geophysical Year (IGY). Project Vanguard would be managed by the Naval Research Laboratory and to be based on developing sounding rockets , which had the advantage that they were primarily used for non-military scientific experiments. Four days later, at the Sixth Congress of International Astronautical Federation in Copenhagen, scientist Leonid I. Sedov spoke to international reporters at

3237-819: The best known are the Hawaiian Volcano Observatory and the Vesuvius Observatory . Mobile volcano observatories exist with the USGS VDAP (Volcano Disaster Assistance Program), to be deployed on demand. Each volcano observatory has a geographic area of responsibility it is assigned to whereby the observatory is tasked with spreading activity forecasts, analyzing potential volcanic activity threats and cooperating with communities in preparation for volcanic eruption . International Geophysical Year The International Geophysical Year ( IGY ; French : Année géophysique internationale ), also referred to as

3320-525: The city was relocated elsewhere. The house of the chief astronomer of the old observatory remains today, the current tenant is the National Trust. 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

3403-501: The coast of Adelie Land. The first French station, Port Martin , was completed 9 April 1950, but destroyed by fire the night of 22 to 23 January 1952. Belgium established the King Baudouin Base in 1958. The expedition was led by Gaston de Gerlache , son of Adrien de Gerlache who had led the 1897–1899 Belgian Antarctic Expedition . In December 1958, four team members were stranded several hundred kilometers inland when one of

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3486-595: The comet, the largest contribution in the World. Candy was a councillor of the Astronomical Society of Australia from 1988 to 1990, councillor of the Royal Society of Western Australia between 1988 and 1990, and president of the Royal Society of Western Australia in 1989 . He saw the most drastic staff cuts to the Observatory by the Government in 1987 with 50% of the staff redeployed and one whole section closed down. With

3569-441: The compulsory retirement age no longer in place, unlike his predecessor, Candy was able to continue working at the Perth Observatory on projects including the eclipsing binary FO Hydra, a comet hunter telescope, a new theory on comet origins and evolution, the analysis of the lost comet Gale, as well as comparison of a South Australian comet discovered in 1979 with that of a comet from 1770. In 1960 he discovered Comet Candy 1960n and

3652-591: The dogline and survived by killing Adélie penguins in a nearby rookery (which were preserved by the low temperature). The two dogs became instant national heroes in Japan. A Japanese movie about this story was made in 1983, Antarctica . France contributed Dumont d'Urville Station and Charcot Station in Adélie Land . As a forerunner expedition, the ship Commandant Charcot of the French Navy spent nine months of 1949/50 at

3735-500: The earthquake monitoring was taken up by the Mundaring Geophysical Observatory . In the 1960s, light pollution from the city of Perth and a small part of the implementation of the 1955 plan by Stephenson-Hepburn Report saw the land where the Perth Observatory resided make way for what was to initially be five government office blocks, however there was only one ever built, Dumas House . After nearly being closed by

3818-463: The electromagnetic spectrum that cannot penetrate the Earth's atmosphere and are thus impossible to observe using ground-based telescopes. The Earth's atmosphere is opaque to ultraviolet radiation, X-rays , and gamma rays and is partially opaque to infrared radiation so observations in these portions of the electromagnetic spectrum are best carried out from a location above the atmosphere of our planet. Another advantage of space-based telescopes

3901-798: The end of 1974. Harris had to step in to the position of Government Astronomer at a time when the Perth Observatory was on the move to its new site in the Darling Range, Bickley , some 24 kilometres (15 mi) east of its original position in the City of Perth . Clearing of the land in the State Forrest in Bickely commenced in February 1964, with excavations commencing in May 1964 and construction works on buildings continuing through 1965; staff moved in on 19 December 1965. With

3984-406: The entire upper portion of the telescope dome can be rotated to allow the instrument to observe different sections of the night sky. Radio telescopes usually do not have domes. For optical telescopes, most ground-based observatories are located far from major centers of population, to avoid the effects of light pollution . The ideal locations for modern observatories are sites that have dark skies,

4067-521: The expedition on the North Pole. At another point the ice sheet broke up and their fuel tanks started floating away from the base. They had to put pans under the plane engines as soon as they landed as any oil spots would go straight through the ice in the intense sunshine. Their only casualty was a man who got too close to the propeller with the oil pan. Norbert Untersteiner was the project leader for Drifting Station Alpha and in 2008 produced and narrated

4150-665: The field of radio astronomy to observe the Universe in the radio portion of the electromagnetic spectrum. Such an instrument, or collection of instruments, with supporting facilities such as control centres, visitor housing, data reduction centers, and/or maintenance facilities are called radio observatories . Radio observatories are similarly located far from major population centers to avoid electromagnetic interference (EMI) from radio , TV , radar , and other EMI emitting devices, but unlike optical observatories, radio observatories can be placed in valleys for further EMI shielding. Some of

4233-522: The fifteen World Data Centers in the United States. Each World Data Center would eventually archive a complete set of IGY data to deter losses prevalent during the International Polar Year of 1932. Each World Data Center was equipped to handle many different data formats, including computer punch cards and tape—the original computer media. In addition, each host country agreed to abide by the organizing committee's resolution that there should be

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4316-515: The fifth Government Astronomer of the Perth Observatory. After arriving in Australia in 1964, he commenced at the Perth Observatory as an Astronomer Grade II on 1 May 1964 and worked on the Observatory's astrograph ; his previous experience also saw him set up and calibrate the recently acquired Zeiss plate measuring machine. With the relocation of the Perth Observatory from Perth to Bickley, Nikoloff's surveying skills were extensively used in setting up

4399-709: The first Director of the Perth Observatory. In 1969 Candy was offered the position of Director of the British Astronomical Association , however declined due to his plans to emigrate to Australia that year. After arriving in Australia 12 May 1969, he commenced at the Perth Observatory as an Astronomer Grade II and in November 1969 took over the running of the Perth Observatory Astrographic telescope from Dr I Nikoloff. His numerical prowess, gained during his time at HM Nautical Almanac Office ,

4482-401: The fourth, launched on 17 March 1958. The Soviet launches would be followed by considerable political consequences, one of which was the creation of the US space agency NASA on 29 July 1958. The British–American survey of the Atlantic, carried out between September 1954 and July 1959, discovered the full length of the mid-Atlantic ridges ( plate tectonics ); it was a major discovery during

4565-472: The free exchange of data across international borders, there would be no point in having an IGY. In April 1957, just three months before the IGY began, scientists representing the various disciplines of the IGY established the World Data Center system. The United States hosted World Data Center "A" and the Soviet Union hosted World Data Center "B". World Data Center "C" was subdivided among countries in Western Europe, Australia, and Japan. NOAA hosted seven of

4648-499: The icy crust), until it was demolished in December 2010 for safety reasons. Ice Skate 2 was a floating research station constructed and staffed by U.S. scientists. It mapped the bottom of the Arctic Ocean. Zeke Langdon was a meteorologist on the project. Ice Skate 2 was planned to be staffed in 6 month shifts, but due to soft ice surfaces for landing some crew members were stationed for much longer. At one point they lost all communications with anyone over their radios for one month except

4731-407: 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. Upon the death of Spigl on 20 August 1962, John Bertrand Harris, who had been Spigl's assistant since 1957, became the fourth Government Astronomer of the Perth Observatory between 1962 until

4814-452: The limiting magnitude of objects achievable at that time from 14th to 19th. The new processes were to see the recovery of five comets and the positioning of the Observatory to 2nd place between 1973 and 1977 and 4th between 1978 and 1984, resulting in him being awarded the prestigious Merlin Medal of the British Astronomical Association in 1975. Under his direction the Perth Observatory discovered over 100 new asteroids as well as contributing

4897-432: The new Bickely site complete, in 1967, Harris oversaw the installation of a meridian circle telescope at the Observatory as part of an expedition by astronomers from the Hamburg Observatory in Germany. The expedition worked on the international Southern Reference Stars program that resulted in a revised, larger and more accurate meridian catalogue of the Southern Hemisphere : the Perth 70 meridian catalogue. In 1970 Harris

4980-400: The new Observatory during 1965. Nikoloff worked with the German Hamburg Observatory meridian circle telescope expedition on the Perth 70 catalogue, from 1969 until 1971, before the expedition astronomers returned to Germany that Christmas. In 1971, with funding by the Government of Western Australia and negotiations for the loan of the Hamburg telescope, Nikoloff was placed in charge of

5063-400: The new site after arranging its refurbishment; the telescope recommenced observations on 29 March 1968, taking second epoch photographic plates for proper motion studies. In 1968, the Lowell Observatory of Flagstaff Arizona USA, located a 610-millimetre (24 in) Boller and Chivens telescope at the Perth Observatory as part of the International Planetary Patrol Program . The program

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5146-468: The newly formed Perth Observatory Meridian Section. Dr Nikoloff commenced a new observing program of FK4 and FK4 Supplementary stars that would result in the Perth 75 catalogue of 2549 stars. The catalogue not only extended the well revered Perth 70 catalogue, but provided valuable Southern Hemisphere information for the construction of the new FK5 reference frame sought by the international astronomical community. As Government Astronomer, Nikoloff passed on

5229-406: 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 In 1920 and 1921 Curlewis was involved with

5312-447: The primary title of what was previously called the Government Astronomer , with the title of Director Perth Observatory. The reason given was that the title of Government Astronomer "... seemed antiquated to them ", it also reflected similar changes throughout the world with astronomical institutions merging with Universities. With the compulsory retirement age still in place, after Dr I Nikoloff retired, Mr Michael Philip Candy became

5395-411: The public, scientific and amateur communities was helpful in retaining the observatory. As of July 2015, The Perth Observatory Volunteer Group runs the Observatory under a community partnership agreement between the Department of Parks and Wildlife and the Perth Observatory Volunteer Group which was signed in June 2015. In January 1996, the centenary of its foundation, the observatory was transferred to

5478-481: The repositories for data collected during the IGY. Seven of the 15 World Data Centers in the United States are co-located at NOAA National Data Centers or at NOAA affiliates. These ICSU Data Centers not only preserve historical data, but also promote research and ongoing data collection. The fourth International Polar Year on 2007–2008 focused on climate change and its effects on the polar environment. Sixty countries participated in this effort and it included studies in

5561-450: The ship returned a year later, it became beset offshore (stuck in the sea-ice). It was eventually freed with the assistance of the US icebreaker Burton Island but could not resupply the station. The 1957 winterers were retrieved by helicopter, but bad weather prevented going back for the station's 15 sled dogs, which were left chained up. When the ship returned a year later, two of the dogs, Taro and Jiro, were still alive. They had escaped

5644-432: The skis on their light aircraft broke on landing. After a ten-day ordeal, they were rescued by an IL-14 aircraft after a flight of 1,940 miles (3,100 km) from the Soviet base, Mirny Station . The Amundsen–Scott South Pole Station was erected as the first permanent structure at the South Pole in January 1957. It survived intact for 53 years, but was slowly buried in the ice (as all structures there eventually sink into

5727-414: The surface of Earth, are used to make observations in the radio and visible light portions of the electromagnetic spectrum . Most optical telescopes are housed within a dome or similar structure, to protect the delicate instruments from the elements. Telescope domes have a slit or other opening in the roof that can be opened during observing, and closed when the telescope is not in use. In most cases,

5810-402: The third International Polar Year , was an international scientific project that lasted from 1 July 1957 to 31 December 1958. It marked the end of a long period during the Cold War when scientific interchange between East and West had been seriously interrupted. Sixty-seven countries participated in IGY projects, although one notable exception was the mainland People's Republic of China , which

5893-501: The world's major radio observatories include the Very Large Array in New Mexico , United States, Jodrell Bank in the UK , Arecibo in Puerto Rico , Parkes in New South Wales , Australia, and Chajnantor in Chile . A related discipline is Very-long-baseline interferometry (VLBI). Since the mid-20th century, a number of astronomical observatories have been constructed at very high altitudes , above 4,000–5,000 m (13,000–16,000 ft). The largest and most notable of these

5976-476: Was able to be serviced by the Space Shuttles while many other space telescopes cannot be serviced at all. Airborne observatories have the advantage of height over ground installations, putting them above most of the Earth's atmosphere. They also have an advantage over space telescopes: The instruments can be deployed, repaired and updated much more quickly and inexpensively. The Kuiper Airborne Observatory and

6059-409: 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 . Cooke's successor as Government Astronomer was Harold Curlewis who wrote in 1929: Since

6142-404: 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

6225-401: Was designed to collect 35-mm format photographic data on the atmospheric and surface features of Solar System planets, mostly Mars, Jupiter and Venus; Harris was to be a regular observer outside his normal daytime Government Astronomer role. Harris was successful in increasing the technical and astronomical staff numbers at the new Bickley Perth Observatory as its role moved to that of more of

6308-403: 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

6391-517: Was not yet an inhibition about using military rockets to get into space). On 8 November 1957, the US Secretary of Defense instructed the US Army to use a modified Jupiter-C rocket to launch a satellite. The US achieved this goal only four months later with Explorer 1, on 1 February 1958, but after Sputnik 2 on 3 November 1957, making Explorer 1 the third artificial Earth satellite. Vanguard 1 became

6474-678: Was protesting against the participation of the Republic of China ( Taiwan ). East and West agreed to nominate the Belgian Marcel Nicolet as secretary general of the associated international organization. The IGY encompassed fourteen Earth science disciplines: aurora , airglow , cosmic rays , geomagnetism , gravity , ionospheric physics , longitude and latitude determinations (precision mapping), meteorology , oceanography , nuclear radiation , glaciology , seismology , rockets and satellites , and solar activity . The timing of

6557-506: Was replaced by present-day Casey station in 1988. Halley Research Station was founded in 1956 for the IGY by an expedition from the (British) Royal Society . The bay where the expedition set up their base was named Halley Bay, after the astronomer Edmond Halley . Showa Station , the first Japanese base in Antarctica, was set up in January 1957, supported by the ice breaker Sōya . When

6640-510: Was responsible for the August 1973 IAU Symposium No. 61 in Perth on "New Problems of Astrometry". Like his predecessor, he died at an early age, 49, but had raised the standing of the Perth Observatory to a well respected scientific institution within Australia and internationally. With the death of Harris on 23 December 1974, Nikoloff was to act in the role of Government Astronomer of the Perth Observatory until 30 May 1979 when he officially became

6723-594: Was successful in forming a dedicated Perth Observatory Meridian section to assist the German expedition in their work. After the German expedition left over the 1971/72 Christmas/New Year period, Harris successfully negotiated the loan of the Hamburg telescope indefinitely and obtained funding from the Government of Western Australia to increase the Meridian staff numbers. This Perth Observatory Meridian team continued and expanded on

6806-429: Was the first Astronomer to discover, as well as compute, a comets orbit from two more observations within 60 hours of its discovery. Mr M P Candy officially retired on 24 December 1993 and died 2 November 1994. His work was honored by the naming of Minor Planet 3015 Candy in 1980. Dr James D Biggs commenced at the Perth Observatory in May 1994 and resigned in 2010. After Dr J D Biggs resigned, Ralph Martin acted in

6889-411: Was to be a great asset in the astrometric programs of the Perth Observatory, as was his interest in comets. It took little time for Candy to position the Perth Observatory at the forefront of southern cometary astrometry. By 1972, the Perth Observatory was 9th in the world in producing cometary positions. Not content with this, Candy introduced new photographic glass plate processing practices to increase

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