Siding Spring Observatory

The original Mount Stromlo Observatory was set up by the Commonwealth Government in 1924. After duty supplying optical components to the military in World War II, the emphasis on astronomical research changed in the late 1940s from solar to stellar research. Between 1953 and 1974, the 74-inch (1.9 m) reflecting telescope at Mount Stromlo was the largest optical telescope in Australia.

Already in the 1950s, the artificial lights of Canberra, ACT, had brightened the sky at Mount Stromlo to such an extent that many faint astronomical objects had been overwhelmed by light pollution. The search for a new site was initiated by Bart Bok. After a site survey was undertaken the number of possible locations was narrowed down to two – Siding Spring and Mount Bingar near Griffith, also in New South Wales.[3] Siding Spring was first suggested for astronomy by Harley Wood, the New South Wales Government Astronomer at the time. Arthur Hogg did much of the preliminary site testing.

The Siding Spring site was selected by the ANU in 1962 from many other possible locations because of the dark and cloud-free skies. By the mid-1960s the ANU had set up three telescopes, together with supporting facilities, such as sealed roads, staff accommodation, electricity and water. In 1984, the Prime Minister, Bob Hawke, opened the ANU's largest telescope, the low-cost and innovative 2.3-metre (7 ft 7 in) aperture telescope, housed in a simple, co-rotating cuboid dome.

Since the 1950s, and quite independently of developments at Siding Spring, the Australian and British governments had been negotiating about the construction of a very large telescope. When these negotiations finally came to fruition in 1969, the infrastructure of Siding Spring Observatory was already in place, and it was the obvious site at which to locate the 3.9-metre (13 ft) aperture Anglo-Australian Telescope (AAT).

During the construction of the AAT in the early 1970s, the British Science Research Council also built the UK Schmidt Telescope, 1 kilometre (0.62 mi) to the northeast of the AAT dome. The considerably wider field of view of the Schmidt optical design complements the narrower field of the AAT, in that larger areas of sky may be surveyed more quickly. Interesting objects so discovered are then studied in greater detail on the larger instrument. In 1987, the Schmidt Telescope was amalgamated with the AAT.

Siding Spring Observatory also houses many telescopes from institutions across the world including, Korea, America, the UK, Poland, Hungary, Germany and Russia. In 1990, the earth-satellite tracking facility of the Royal Greenwich Observatory was closed down after 10 years of operation.

In 2012 the first publicly accessible Internet based observatory, working in partnership with the RSAA, was commissioned by iTelescope.Net with over 25 telescopes housed in a large roll-off roof (ROR) observatory near the base of the UK Schmidt Telescope.

Las Cumbres Observatory Global Telescope Network operate a 2-metre Ritchey Chretien telescope used for research, citizen science, and education purposes by users across the globe. Also, they operate inside the clam style dome 2 x 0.40 cm telescopes, and a further 2 × 1 metre telescopes housed in individual domes outside the building. Currently there are over one thousand registered users of the Faulkes Telescopes, who vary from schools and community groups to professional astronomers. A global network of robotic optical telescopes will not only provide continuous sky coverage and the ability to treat the network as a single instrument, but also provide the resources for performing cutting edge science in collaboration with other organisations.

ROTSE, Robotic Optical Transient Search Experiment is operated by the University of New South Wales (UNSW), the 0.45 m, 3rd-generation robotic telescope has successfully detected the transient optical emission from several GRB events. The wide field of view and the fast response permit measurements inaccessible to more conventional instruments.

HAT-South is a project to search for transiting extrasolar planets in the Southern Hemisphere. It uses a network of wide-field telescopes to monitor hundreds of thousands of bright stars, searching for the characteristic dip in light that occurs when a planet passes in front of its host star. Hat – South is made up of 3 sites in the Southern hemisphere with two "TH4" units, making that 8 x 0.2-metre telescopes each at every sites. These TH4 units consist of four 0.18 m Takahashi astrographs fitted with Apogee 4k x 4k CCDs. Each TH4 unit monitors 64 square degrees of sky at a time, so each site is capable of monitoring 128 square degrees of sky.

Automated Patrol Telescope (APT) is operated by the University of NSW (UNSW) is a wide-field CCD imaging telescope. The 0.5 m telescope has a 5-degree field of view and can be operated remotely or in a fully automatic mode. The telescope has an optical design that more resembles that of a Schmidt camera, but has a 3-element lens to achieve a wide, corrected field of view. The APT was developed by extensively modifying the optical, mechanical and electronic systems of a Baker-Nunn satellite tracking instrument. The Baker-Nunn telescope had been located at Woomera in South Australia during the 1960s, and afterward was stationed at Orroral Valley near Canberra. The camera was donated by the Smithsonian Institution to UNSW in 1982.

PROMPT (also known as Skynet) is run by the University of North Carolina. The Panchromatic Robotic Optical Monitoring and Polarimetry Telescopes is made up of 4 x 0.41 Ritchey Chretien telescopes is entirely robotic and queue based. They are able to have rapid and simultaneous multi-wavelength observations of gamma ray burst afterglows and other transient objects.

Uppsala Schmidt Telescope was built in 1957 originally located in Sweden, relocated to Mount Stromlo, then finally in 1982 making a home at Siding Spring Observatory. The telescope was used by ANU in many roles such as Near Earth Object studies (NEOs) by famous comet hunter Rob McNaught. It was also the southern hemisphere counterpart of the Catalina Sky Survey (CSS) located in Arizona, USA. The telescope is a 0.5m spherical mirror, with a 0.5m correcting plate, which allows a 6 degree field of view.

The KMT, Korean Microlensing Telescope, is a 1.6 m operated by KASI. The KMTNet aims primarily to discover extrasolar planets based on the analyses of gravitational microlensing phenomena, especially the detection of earth-mass planets in the habitable zone. The KMTNet system has a very competitive power for wide-field photometric survey sciences that study supernovae, asteroids and external galaxies, for instance. Because the observation period of the Galactic bulge focuses on the primary science on extrasolar planets, the other science programs are performed in the season when the Galactic bulge is not observable.

The Skymapper telescope, operated by the ANU, is currently mapping the entire southern sky, completing each map over a period of 3 months. The survey will record more than a billion stars and galaxies. This fully automated telescope also uses a series of filters enabling the camera to record the spectral type of stars, giving astronomers information about their age, mass and temperature. The 1.35m telescope has been used in the hunt for Planet 9 and more trans Neptunian objects, supernovae and also finding the oldest known star in the universe.

Solaris 3, operated by the Nicolaus Copernicus Astronomical Center as part of a network across the Southern hemisphere, is a single 0.5-metre telescope, using a new method referred to as eclipse timing to search for exoplanets. They have also added an astrograph to their telescope, giving it dual purpose.

Jaxa, the Japan Aerospace Exploration Agency, operate four 0.25-metre telescopes, searching and tracking space debris and near earth objects in the Southern hemisphere.

Huntsman Telephoto Array is operated by the AAO & Macquarie University to take images of faint galaxy structures using commercial lenses. Initially it will use a 0.28-metre Celestron Rowe-Ackermann Schmidt Astrograph (RASA) telescope with seven 400 mm Canon f/2.8 camera lenses.

bRing-AU, operated by a collaboration of Universities and astronomers will search for circumplanetary material, studying disks of dust in early history and the formation of icy satellites. They use 2 small modified cameras, with Kodak CCD chips.

There is a visitors' gallery and exhibition area open to the public which also incorporates a café and souvenir shop. During NSW school holidays, guided tours of the site are offered. Groups of over 15 adults may apply for Behind the Scenes walking or bus tours.

An Open Day is held annually in October, offering talks about astronomy and tours inside many of the telescope domes which are open to the public on this one day of the year. These tours include the AAT 3.9M, UK Schmidt, iTelescope.Net, 2.3M ANU and the LCGTN 2M telescope facilities.

• 3.9 m (13 ft) Anglo-Australian Telescope (AAO), operational in 1974
• 1.24 m (4 ft 1 in) UK Schmidt Telescope (AAO)
• 2 m (6 ft 7 in) Faulkes Telescope South (Las Cumbres Observatory)
• 1.3 m (4 ft 3 in) SkyMapper Telescope (ANU), when launched in 2009 was the first new optical, research grade telescope in Australia since 1984.[7]
• 2.3 m (7 ft 7 in) Advanced Technology Telescope (ANU), was built in 1984
• Multiple – iTelescope.Net (iTelescope Network), Internet connected remote telescopes for the Public. Built 2013
• 4 x 0.4 m (1 ft 4 in) PROMPT Telescopes (The University of North Carolina), Built 2013
• HAT-South Telescope Network (ANU, Harvard–Smithsonian Center for Astrophysics, Max Planck Institute for Astronomy) with 8 x 0.2 m telescopes
• SOLARIS Telescope (Nicolaus Copernicus Astronomical Centre – Poland. Built 2012)
• 0.5 m (1 ft 8 in) Uppsala Southern Schmidt Telescope (ANU – decommissioned 2013)
• 0.5 m (1 ft 8 in) Automated Patrol Telescope (UNSW – decommissioned 2012)
• 0.45 m (1 ft 6 in) ROTSE IIIa, Robotic Optical Transit Search Experiment (UNSW)
• Jaxa (Japan Aerospace Exploration Agency) telescopes
• 40 in (100 cm) Telescope (ANU), was first commissioned in 1963 currently decommissioned and moved to Milroy Observatory for use by amateurs.[8]
• 24 in (61 cm) Telescope (ANU – decommissioned)
• 16 in (41 cm) Telescope (ANU currently housing a 14-inch telescope for outreach programs)
• 1.6 m (5 ft 3 in) Korea Microlensing Telescope Network (KMTNet)

The Anglo-Australian Near-Earth Asteroid Survey used the UK Schmidt Telescope between 1990 and 1996.[9] The same telescope was later dedicated for use by the RAVE survey of the Milky Way. The Near-Earth object search program called the Siding Spring Survey (closed 2013) used the Uppsala Southern Schmidt Telescope.[10] The 2dF Galaxy Redshift Survey, one of the largest survey of galaxies ever undertaken used the Anglo-Australian Telescope between 1995 and 2002.[11]

1977, the Vela Pulsar was discovered at Siding Spring. Comets discovered from the observatory include Comet 103P/Hartley, discovered in 1986 by Malcolm Hartley,[12] Comet C/2006 P1, discovered by Robert H. McNaught using the Uppsala Southern Schmidt Telescope on 8 August 2006,[13] and Comet C/2013 A1, also discovered by McNaught, which passed extremely close to Mars on 19 October 2014.[14]

• Australian Astronomical Observatory (AAO), formerly the Anglo-Australian Observatory
• Comet Siding Spring

• Official website
• Anglo-Australian Observatory
• Uppsala Southern Sky NEO Survey Telescope
• Faulkes Telescope South
• iTelescope.Net Observatory
• PROMPT Telescopes
• SkyMapper Telescope
• ROTSE III Project
• UNSW Automated Patrol Telescope (APT)
• 2.3 m Advanced Technology Telescope
• ANU 40-inch (1,000 mm) Telescope
• Bauer, Amanda (January 2013). "Siding-Spring observatory fires". Bushfire coverage and photos. Local astronomer.