Mount Stromlo Observatory
Mount Stromlo Observatory located just outside Canberra, Australia, is part of the Research School of Astronomy and Astrophysics at the Australian National University (ANU).
History
The observatory was established in 1924 as The Commonwealth Solar Observatory. The Mount Stromlo site had already been used for observations in the previous decade, a small observatory being established there by Pietro Baracchi using the Oddie telescope being located there in 1911.[1] The dome built to house the Oddie telescope was the first Commonwealth building constructed in the newly established Australian Capital Territory. In 1911 a delegation for an Australian Solar Observatory went to London seeking Commonwealth assistance. The League of the Empire sought subscriptions to assist raising funds.[2] Survey work to determine the site's suitability had begun as soon as the idea of a new Capital was established. By 1909 the Australian Association for the Advancement of Science was assisted in this effort by Hugh Mahon (Minister for Home Affairs).[3] Until World War II, the observatory specialised in solar and atmospheric observations. During the war the workshops contributed to the war effort by producing gun sights, and other optical equipment. After the war, the observatory shifted direction to stellar and galactic astronomy and was renamed The Commonwealth Observatory. Dr R. Wooley Director of the Observatory, worked to gain support for a larger reflector, arguing that the southern hemisphere should attempt to compete with the effectiveness of American telescopes.[4] The ANU was established in 1946 in nearby Canberra and joint staff appointments and graduate studies were almost immediately undertaken. A formal amalgamation took place in 1957, with Mount Stromlo Observatory becoming part of the Department of Astronomy[5] in the Research School of Physical Sciences at ANU, leading eventually to the formation of the Research School of Astronomy and Astrophysics in 1986.[6]
On 18 January 2003, the devastating Canberra firestorm hit Mount Stromlo (which was surrounded by a plantation pine forest), destroying five telescopes, workshops, seven homes, and the heritage-listed administration building.[7] The only telescope to escape the fires was the 1886 15-centimetre Farnham telescope. Relics from the fire are preserved in the collection of the National Museum of Australia. They include a melted telescope mirror and a piece of melted optical glass (flint). The latter has pieces of charcoal and wire fused into it from the fierce heat of the fire.[8]
Redevelopment is completed and the Observatory is now a major partner in the construction of the Giant Magellan Telescope.[9] The current observatory director is Matthew Colless.[10]
The director's residence, destroyed in the 2003 fire, was rebuilt and opened to the public as a memorial in 2015.[11]
Research
The MACHO project detected the first instance of the gravitational lensing of one star by another, known as gravitational microlensing, in 1993 (Alcock et al. 1993; Paczynski 1996).[12] This discovery was made by repeated imaging of the Magellanic Clouds with the refurbished 50-inch Great Melbourne Telescope which was equipped with a mosaic of 8 2048 by 2048 pixel CCDs.[13] The camera was constructed by the Centre for Particle Astrophysics in California (CFPA), and at the time was the largest digital camera ever built (Frame & Faulkner 2003). Observations began in July 1992 and the project concluded in December 1999. In total, the MACHO project made over 200 billion stellar measurements, with the data processed both at the observatory and at the Lawrence Livermore National Laboratory.
Brian Schmidt organised an international collaboration, known as the High-z Supernova Search Team, to study the rate of change of the Cosmic Expansion using type Ia supernovae. In 1998, the team reach the conclusion that the cosmic expansion was accelerating, contrary to expectations. This universal acceleration implies the existence of dark energy and was named the top science breakthrough of 1998 by Science magazine.[14] In 2011, Brian P. Schmidt shared the Nobel Prize in Physics with Saul Perlmutter and Adam Riess for such observations which provided evidence for the accelerating Universe.[15]
The 2dF Galaxy Redshift Survey, co-led by Matthew Colless, undertook the largest galaxy redshift survey of its time, and was conducted at the Anglo-Australian Observatory (AAO) with the 3.9m Anglo-Australian Telescope between 1997 and 11 April 2002.[16] In total, the survey measured more than 245,000 galaxies, providing, along with the Sloan Digital Sky Survey, the definitive measurements of large scale structure in the low-redshift Universe.
Advanced instrumentation
The instrumentation group at Mount Stromlo Observatory has built two instruments for the Gemini Telescope.[17] This includes the near infrared integral field spectrometer, NIFS, deployed on Gemini-North, and the adaptive optics imager for Gemini-South, GSAOI. NIFS, when nearly completed, was destroyed in the bushfires of 18 January 2003, and rebuilt.
A new rapid survey telescope, SkyMapper, is under construction. SkyMapper will reside at the ANU's other observatory (Siding Spring) and be operated remotely from Mount Stromlo.[18]
Location
Mount Stromlo Observatory is located at an altitude of 770 metres above sea level on Mount Stromlo. Situated west of the centre of Canberra, near the district of Weston Creek. Canberra's main water supply treatment plant is located nearby.[19]
See also
References
- ↑ J. L. Perdrix (1979). "Baracchi, Pietro Paolo Giovanni Ernesto (1851 - 1926)". Australian Dictionary of Biography, Volume 7. MUP. pp. 166–167.
- ↑ "Solar Observatory Commonwealth Aid Sought". The Age. Retrieved 12 October 2013.
- ↑ "Commonwealth Solar Observatory". The Sydney Morning Herald 1909. Retrieved 12 October 2013.
- ↑ "Big Telescope Sought for Australia". The Sydney Morning Herald - Aug 22, 1947. Retrieved 12 October 2013.
- ↑ https://physics.anu.edu.au/fire_in_the_belly/Fire_in_the_Belly07.pdf
- ↑ https://physics.anu.edu.au/fire_in_the_belly/Fire_in_the_Belly04.pdf
- ↑ "Mt Stomlo observatory severely damaged in fires". ABC News. Retrieved 12 October 2013.
- ↑ "NMA Collections Search - Piece of clear optical glass (flint), a relic from the 2003 bush fire that destroyed the Mount Stromlo Observatory". Nma.gov.au. 2003-01-18. Retrieved 2013-10-13.
- ↑ "Giant Magellan Telescope - RSAA - ANU". Rsaa.anu.edu.au. 2012-06-25. Retrieved 2013-10-13.
- ↑ http://rsaa.anu.edu.au/contact-us
- ↑ Louise Maher (30 January 2015). "Mount Stromlo Director's Residence opens to public after being destroyed in 2003 Canberra bushfires". Australian Broadcasting Corporation. Retrieved 31 January 2015.
- ↑ "MACHO project, a search for evidence of dark matter.". The Great Melbourne Telescope [GMT]. Retrieved 12 October 2013.
- ↑ "History". Great Melbourne Telescope Org. Retrieved 12 October 2013.
- ↑ James Glanz (18 December 1998). "Breakthrough of the Year: Astronomy: Cosmic Motion Revealed". Science. 282 (5397): 2156–2157. Bibcode:1998Sci...282.2156G. doi:10.1126/science.282.5397.2156a. Retrieved 2008-07-17.
- ↑ "A look at the winners of the 2011 Nobel Prizes". Associated Press. Retrieved 12 October 2013.
- ↑ Final Status of Survey Observations
- ↑ "North Plains Systems Announces TeleScope Gemini". Information Today Inc. Retrieved 12 October 2013.
- ↑ "Siding Spring Observetory". RSAA-ANU. Retrieved 12 October 2013.
- ↑ "ACT Water Supply". ACTEW Corporation Ltd. Retrieved 12 October 2013.
Further reading
R. Bhathal, R. Sutherland, & H. Butcher (2013), Mt Stromlo Observatory, CSIRO Publishing, Melbourne VIC, ISBN 9781486300754
Bibliography
- Alcock, C. et al. 1993, Nature, 365(6447), 621-623
- Paczynski, B. 1996, Annu. Rev. Astro. Astrophys., 34(1), 419-459
- Stromlo An Australian Observatory by Tom Frame and Don Faulkner, Allen and Unwin 1993, ISBN 1-86508-659-2
External links
Media related to Mount Stromlo Observatory at Wikimedia Commons
- ANU Website
- Research School of Astronomy and Astrophysics at the ANU
- SkyMapper Website.
- Mt. Stromlo. SLR Global Performance Report Card
- Most important of all has been the scientific output of the Observatory
Coordinates: 35°19′13″S 149°00′25″E / 35.32028°S 149.00694°E