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Abbreviation | ASV |
---|---|
Formation | 1922 |
Legal status | non-profit Incorporated association |
Location |
|
Region | Victoria, Australia |
Membership | over 1000 people [1] |
Publication | Crux |
Website |
www |
The Astronomical Society of Victoria (ASV) is an amateur astronomy club in the state of Victoria, Australia. It was founded in 1922, making it one of the oldest such clubs in the country, and with some 1500 members it claims to be one of the largest amateur astronomy organisations in the southern hemisphere. [2][ failed verification] Membership is open to all with an interest in astronomy, and the society caters for people with a wide range of ages, backgrounds, abilities and interests.
The society has sections dedicated to providing support for members interested in specific aspects of astronomy, including astro-photography, comets, radio astronomy, solar observing, variable stars, and deep sky observing. It owns a suburban property which is used as the Lodge and Observatory / workshop, and it also runs the Leon Mow ( /ˈliːɒn ˈmaʊ/) Dark Sky Site, located north of Melbourne. Its major project is the restoration of the Great Melbourne Telescope.
The ASV is registered under the Associations Incorporation Reform Act 2012, and its operations are governed by its Constitution. Members elect the officers of the society and the Council at each Annual General Meeting, and that Council is then responsible to control and manage the business and affairs of the society.
The Society's purposes are stated in its constitution as follows: [3]
The society hosts several different types of observing sessions, aimed at different audiences, including:
For over 50 years the ASV has conducted tours and played a major role in the care of the Melbourne Observatory, in the Royal Botanic Gardens. [12] This has now been supplemented with the Great Melbourne Telescope (GMT) Restoration Project, working closely with Museum Victoria and Royal Botanic Gardens to restore the telescope to working order so that it may be used for education and public viewing.
The telescope itself has great historical significance; at 48 inches (120 cm) it was the largest fully steerable telescope in the world when it was built in 1869, and it was the first telescope that large to be placed on an equatorial mounting, [13] enabling it to track the stars accurately as they appeared to move across the sky. It was "hailed as a masterpiece of engineering", requiring only one assistant to control its movement. [14] Even the rival Sydney Observatory referred to it as "one of the most important artefacts in the history of Australian science." [15]
The telescope was upgraded by adding photographic equipment in 1872, [14] moved to Mount Stromlo Observatory near Canberra in 1946, and rebuilt with a modern mirror in the late 1950s. As recently as 1993, it was upgraded again to take part in the world's first observations of MACHOs as evidence for the existence of dark matter. It was badly damaged in the 2003 Canberra bushfires – the temperatures were so high that the aluminium dome itself caught fire and melted onto the telescope, the Pyrex mirror shattered, and steel struts sagged. [16] [17]
In 2008, Museums Victoria brought the telescope's remains to Melbourne and began assembling expert volunteers. [17] In mid 2009 a group of volunteers from the ASV began "Project Phoenix" to restore the telescope. The restoration project has required a worldwide scavenger hunt to find suitable parts. The project will incorporate bringing the telescope's optical, mechanical and electrical systems into line with current best practice. [18] [19]
After nearly five years weighing up different proposals, engineering work commenced in late 2013 thanks to a $70,000 grant from the Copland Foundation. [20] The Victorian government later committed $600,000 for the first stage of the restoration, and private benefactors also provided financial support. Computer models were developed to design the supporting frame under a variety of extraordinary load conditions including wind and earthquake. The telescope-bearing frame was constructed and set up in the workshops in November 2013. [21] [22] [23]
The work started with stripping and cataloguing each component, and documenting the structure in almost 1,000 engineering drawings. This identified nearly 400 components which were missing or destroyed and had to be made bespoke. In November 2019, the main structure of the telescope was reassembled for the first time in 74 years. [17]
The Radio Astronomy section started in 1980 and it has been steadily evolving into an active group of people interested in detecting that part of the electromagnetic spectrum that is invisible to the human eye. In 2013 the ASV acquired an 8.5 metre (28 ft) dish antenna. Two years later saw the dish assembled and placed on top of a 5 metre support structure. It is fully steerable and can track any celestial object. Currently fitted with a hydrogen line receiver, astronomers are conducting research and mapping the Doppler shift in hydrogen throughout the galaxy. Observations of pulsars, quasars, and other molecular lines are planned. The dish can also be used as a transmitting antenna using the society's amateur radio license with call sign VK3EKH. It is planned to reflect a signal off the moon and to communicate with other amateur stations around the world using the moon as a passive reflector.
The society provides the following facilities for members: [9]
The Burwood Club Observatory, Heathcote Observatory and Old Melbourne Observatory are classified as "designated" optical observatories by the Astronomical Society of Australia on the basis that they are judged to be valuable astronomical resources for research, education and community use. [24]
Issues held in the National Library of Australia: Vol. 1, no. 1-v. 37, no. 1 (January 1948 – June 1984)
![]() | |
Abbreviation | ASV |
---|---|
Formation | 1922 |
Legal status | non-profit Incorporated association |
Location |
|
Region | Victoria, Australia |
Membership | over 1000 people [1] |
Publication | Crux |
Website |
www |
The Astronomical Society of Victoria (ASV) is an amateur astronomy club in the state of Victoria, Australia. It was founded in 1922, making it one of the oldest such clubs in the country, and with some 1500 members it claims to be one of the largest amateur astronomy organisations in the southern hemisphere. [2][ failed verification] Membership is open to all with an interest in astronomy, and the society caters for people with a wide range of ages, backgrounds, abilities and interests.
The society has sections dedicated to providing support for members interested in specific aspects of astronomy, including astro-photography, comets, radio astronomy, solar observing, variable stars, and deep sky observing. It owns a suburban property which is used as the Lodge and Observatory / workshop, and it also runs the Leon Mow ( /ˈliːɒn ˈmaʊ/) Dark Sky Site, located north of Melbourne. Its major project is the restoration of the Great Melbourne Telescope.
The ASV is registered under the Associations Incorporation Reform Act 2012, and its operations are governed by its Constitution. Members elect the officers of the society and the Council at each Annual General Meeting, and that Council is then responsible to control and manage the business and affairs of the society.
The Society's purposes are stated in its constitution as follows: [3]
The society hosts several different types of observing sessions, aimed at different audiences, including:
For over 50 years the ASV has conducted tours and played a major role in the care of the Melbourne Observatory, in the Royal Botanic Gardens. [12] This has now been supplemented with the Great Melbourne Telescope (GMT) Restoration Project, working closely with Museum Victoria and Royal Botanic Gardens to restore the telescope to working order so that it may be used for education and public viewing.
The telescope itself has great historical significance; at 48 inches (120 cm) it was the largest fully steerable telescope in the world when it was built in 1869, and it was the first telescope that large to be placed on an equatorial mounting, [13] enabling it to track the stars accurately as they appeared to move across the sky. It was "hailed as a masterpiece of engineering", requiring only one assistant to control its movement. [14] Even the rival Sydney Observatory referred to it as "one of the most important artefacts in the history of Australian science." [15]
The telescope was upgraded by adding photographic equipment in 1872, [14] moved to Mount Stromlo Observatory near Canberra in 1946, and rebuilt with a modern mirror in the late 1950s. As recently as 1993, it was upgraded again to take part in the world's first observations of MACHOs as evidence for the existence of dark matter. It was badly damaged in the 2003 Canberra bushfires – the temperatures were so high that the aluminium dome itself caught fire and melted onto the telescope, the Pyrex mirror shattered, and steel struts sagged. [16] [17]
In 2008, Museums Victoria brought the telescope's remains to Melbourne and began assembling expert volunteers. [17] In mid 2009 a group of volunteers from the ASV began "Project Phoenix" to restore the telescope. The restoration project has required a worldwide scavenger hunt to find suitable parts. The project will incorporate bringing the telescope's optical, mechanical and electrical systems into line with current best practice. [18] [19]
After nearly five years weighing up different proposals, engineering work commenced in late 2013 thanks to a $70,000 grant from the Copland Foundation. [20] The Victorian government later committed $600,000 for the first stage of the restoration, and private benefactors also provided financial support. Computer models were developed to design the supporting frame under a variety of extraordinary load conditions including wind and earthquake. The telescope-bearing frame was constructed and set up in the workshops in November 2013. [21] [22] [23]
The work started with stripping and cataloguing each component, and documenting the structure in almost 1,000 engineering drawings. This identified nearly 400 components which were missing or destroyed and had to be made bespoke. In November 2019, the main structure of the telescope was reassembled for the first time in 74 years. [17]
The Radio Astronomy section started in 1980 and it has been steadily evolving into an active group of people interested in detecting that part of the electromagnetic spectrum that is invisible to the human eye. In 2013 the ASV acquired an 8.5 metre (28 ft) dish antenna. Two years later saw the dish assembled and placed on top of a 5 metre support structure. It is fully steerable and can track any celestial object. Currently fitted with a hydrogen line receiver, astronomers are conducting research and mapping the Doppler shift in hydrogen throughout the galaxy. Observations of pulsars, quasars, and other molecular lines are planned. The dish can also be used as a transmitting antenna using the society's amateur radio license with call sign VK3EKH. It is planned to reflect a signal off the moon and to communicate with other amateur stations around the world using the moon as a passive reflector.
The society provides the following facilities for members: [9]
The Burwood Club Observatory, Heathcote Observatory and Old Melbourne Observatory are classified as "designated" optical observatories by the Astronomical Society of Australia on the basis that they are judged to be valuable astronomical resources for research, education and community use. [24]
Issues held in the National Library of Australia: Vol. 1, no. 1-v. 37, no. 1 (January 1948 – June 1984)