Siding Spring 2.3 M Telescope
Instrumentation includes an integral field spectrograph known as WiFeS, an echelle spectrograph, and a Nasmyth imager. The telescope is a workhorse for numerous large programs where it is used to do follow-up observations on objects of interest before more extensive observations are made at larger telescopes. It is also a valuable tool for training students in the astronomical observing techniques.
History
The telescope was the initiative of Don Mathewson. It was inaugurated Prime Minister, Bob Hawke on 16 May 1984. It was regarded as an achievement in high technology for Australia. In 1985, it won an award from the Institution of Engineers.
In 2023 the telescope was automated to robotically study astrophysical explosions
Mirror
The mirror used in the telescope is much thinner than those typically used in a telescope mirror. Its ratio of diameter to thickness is about 20:1. The light mirror and rotating design allows the telescope to be rapidly moved as observations are made.
See also
References
- ^ Mathewson, Don S. (2013). "The Australian National University's 2.3m New Generation Telescope At Siding Spring Observatory". Journal of Astronomical History and Heritage. 16 (1): 2–28 – via Sciengine.
- ^ "ANU 2.3m Telescope". ANU College of Physical & Mathematical Sciences. The Australian National University. Retrieved 15 April 2013.
- ^ Haynes, Raymond (1996). Explorers of the Southern Sky: A History of Australian Astronomy. Cambridge University Press. pp. 184–185. ISBN 0521365759. Retrieved 15 April 2013.
- ^ "2.3m Automation | The Centre for Gravitational Astrophysics". cga.anu.edu.au. Retrieved 5 January 2024.