University of Tokyo Atacama Observatory (TAO)
Looking east towards Cerro Chajnantor, site of TAO
OrganizationUniversity of Tokyo
LocationCerro Chajnantor, Atacama Desert, Chile
Coordinates22°59′12″S 67°44′32″W / 22.98667°S 67.74222°W / -22.98667; -67.74222
Altitude5,640 m (18,500 ft)
Established2009
Websitehttp://www.ioa.s.u-tokyo.ac.jp/TAO/
(English translation)
Telescopes
miniTAO1m optical-infrared
(under construction)6.5m optical-infrared
University of Tokyo Atacama Observatory is located in Chile
University of Tokyo Atacama Observatory
Location of University of Tokyo Atacama Observatory (TAO)

The University of Tokyo Atacama Observatory (TAO) is an astronomical observatory located on the summit of Cerro Chajnantor, at an altitude of 5,640 m (18,500 ft) within a lava dome in the Atacama Desert of northern Chile.[1] The site is located less than 5 km (3.1 mi) north-northeast of the Llano de Chajnantor Observatory, where the Atacama Large Millimeter Array (ALMA) is located, but is over 580 m (1,900 ft) higher in elevation. It is also 28 m (92 ft) higher than the Fred Young Submillimeter Telescope proposed for the same peak.

The eventual goal of the project is to construct the TAO telescope (or TAO 6.5m telescope), a 6.5 m (260 in) optical-infrared telescope at the site.[2] A first step towards that goal has been the construction and installation of a 1.0 m (39 in) pilot telescope, called miniTAO, completed in 2009. With miniTAO's first light achieved in March 2009 in the visible region, and in June 2009 for the infrared region, the observatory has become the highest permanent astronomical observatory in the world. The high altitude of the observatory is essential for its mission, for it is an infrared light observatory, and infrared light is absorbed by the water vapor in the atmosphere making it imperative that an infrared observatory be located in high altitude where the atmosphere is sparse. In 2023, TAO was noted as one of only a few major telescopes in the world with light pollution below acceptable levels of interference.[3]

Description

The telescope's primary mirror will have a diameter of 6.5 m (260 in) and will be silver-coated. The secondary mirror will be equipped with adaptive optics to compensate for atmospheric turbulence. A third mirror will allow switching between several instruments. There will be a Cassegrain focus for the mid-infrared range, a Nasmyth focus for the near-infrared range and another Nasmyth focus for far-infrared.

The project started with site studies in the late 1990s and early 2000s. Road construction to the summit of Cerro Chajnantor started in November 2005. Road was opened April 2006. The miniTAO pilot telescope was constructed in 2009. MiniTAO allowed the project to determine the viewing radius of the full-size telescope.[4] The construction of the TAO telescope started in 2013.[5]

The telescope will have two primary instruments, the MIMIZUKU mid-infrared imager and spectrograph, and SWIMS near-infrared spectrograph. Both instruments were tested at the Subaru telescope and achieved first light in the summer of 2018. After testing, the instruments are to be installed into the TAO telescope in 2023. MIMIZUKU has similar spatial resolution to the James Webb Space Telescope's Mid-Infrared Instrument (MIRI) and wider frequency range, although it is less sensitive.[6]

Ground-breaking ceremonies at the site were held at late 2017.[7] In January 2018, the TAO telescope mount construction was completed and the telescope mount assembled in Japan. This was done for testing purposes; the telescope was disassembled and shipped to Chile on multiple vessels in 2020.[8] The observation and operations building was similarly assembled in Kazo, Saitama in May 2020 for testing purposes, and then disassembled and shipped on eight separate vessels over the course of 2021.[9]

First observations are currently planned for the end of 2023.[10]

See also

References

  1. ↑ Yoshii, Yuzuru; et al. (Aug 11, 2009). "The 1m telescope at the Atacama Observatory has Started Scientific Operation, detecting the hydrogen emission line from the Galactic Center in the Infrared Light". Press Release. School of Science, the University of Tokyo. Retrieved 21 December 2009.
  2. ↑ "TAO Project" (PDF). Comisión Nacional de Investigación Científica y Tecnológica - CONICYT. Archived from the original (PDF) on 16 July 2011. Retrieved 21 December 2009.
  3. ↑ Falchi, Fabio; Ramos, Felipe; Bará, Salvador; Sanhueza, Pedro; Jaque Arancibia, Marcelo; Damke, Guillermo; Cinzano, Pierantonio (16 December 2022). "Light pollution indicators for all the major astronomical observatories". Monthly Notices of the Royal Astronomical Society. 519 (1): 26–33. doi:10.1093/mnras/stac2929.
  4. ↑ Kamizuka, Takafumi; Miyata, Takashi; Sako, Shigeyuki; Ohsawa, Ryou; Asano, Kentaro; et al. (13 December 2020). "The University of Tokyo Atacama Observatory 6.5m telescope: On-sky performance evaluations of the mid-infrared instrument MIMIZUKU on the Subaru telescope". In Evans, Christopher J.; Bryant, Julia J.; Motohara, Kentaro (eds.). Ground-based and Airborne Instrumentation for Astronomy VIII. Vol. 11447. pp. 1296–1314. Bibcode:2020SPIE11447E..5XK. doi:10.1117/12.2560789. ISBN 9781510636811. S2CID 230602089.
  5. ↑ "Full start for TAO telescope construction!".
  6. ↑ Sajina, Anna; Lacy, Mark; Pope, Alexandra (27 June 2022). "The Past and Future of Mid-Infrared Studies of AGN". Universe. 8 (7): 356. arXiv:2210.02307. Bibcode:2022Univ....8..356S. doi:10.3390/universe8070356.
  7. ↑ "Ground-breaking ceremony was held at the summit of Co. Chajnantor".
  8. ↑ "Unveiling Ceremony and Commemorative Lectures for Completion of Shop Assembly of TAO 6.5m Telescope Mount".
  9. ↑ "TAO望遠鏡の観測運用棟の仮組試験が完了" (in Japanese).
  10. ↑ Miyata, Takashi; Yoshii, Yuzuru; Doi, Mamoru; Kohno, Kotaro; Tanaka, Masuo; et al. (29 August 2022). "The University of Tokyo Atacama Observatory 6.5m telescope : Project status 2022". In Marshall, Heather K.; Spyromilio, Jason; Usuda, Tomonori (eds.). Ground-based and Airborne Telescopes IX. Vol. 12182. p. 34. Bibcode:2022SPIE12182E..11M. doi:10.1117/12.2628146. ISBN 9781510653450. S2CID 252467157.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.