Daniel K. Inouye Solar Telescope

Daniel K. Inouye Solar Telescope
Daniel K. Inouye Solar Telescope on the left hand side
Alternative namesDKIST Edit this at Wikidata
Named afterDaniel Inouye Edit this on Wikidata
Part ofHaleakalā Observatory Edit this on Wikidata
Location(s)Haleakalā Observatory, Haleakalā, Maui County, Hawaii
Coordinates20°42′17″N 156°10′36″W / 20.7047°N 156.1767°W / 20.7047; -156.1767 Edit this at Wikidata
OrganizationNational Solar Observatory Edit this on Wikidata
Altitude3,084 m (10,118 ft) Edit this at Wikidata
Wavelength380 nm (790 THz)–5,000 nm (60 THz)
First lightDecember 2019 Edit this on Wikidata
Telescope styleGregorian telescope
optical telescope
solar telescope Edit this on Wikidata
Diameter4.24 m (13 ft 11 in) Edit this at Wikidata
Secondary diameter0.65 m (2 ft 2 in) Edit this at Wikidata
Illuminated diameter4 m (13 ft 1 in) Edit this at Wikidata
Collecting area12.5 m2 (135 sq ft) Edit this at Wikidata
Mountingaltazimuth mount Edit this on Wikidata
Websitewww.nso.edu/telescopes/dki-solar-telescope Edit this at Wikidata
Daniel K. Inouye Solar Telescope is located in Pacific Ocean
Daniel K. Inouye Solar Telescope
Location of Daniel K. Inouye Solar Telescope
  Related media on Commons

The Daniel K. Inouye Solar Telescope (DKIST) is a scientific facility for studies of the Sun at Haleakala Observatory on the Hawaiian island of Maui. Known as the Advanced Technology Solar Telescope (ATST) until 2013, it was named after Daniel K. Inouye, a US Senator for Hawaii.[1] It is the world's largest solar telescope, with a 4-meter aperture.[2][3] The DKIST is funded by National Science Foundation and managed by the National Solar Observatory. The total project cost is $344.13 million.[4] It is a collaboration of numerous research institutions. Some test images were released in January 2020.[5] The end of construction and transition into scientific observations was announced in November 2021.[6]

The DKIST can observe the Sun in visible to near-infrared wavelengths and has a 4.24-meter primary mirror in an off-axis Gregorian configuration that provides a 4-meter clear, unobstructed aperture. Adaptive optics correct for atmospheric distortions and blurring of the solar image, which enables high-resolution observations of features on the Sun as small as 20 km (12 miles). The off-axis, clear aperture design avoids a central obstruction, minimizing scattered light. It also eases operation of adaptive optics and digital image reconstruction such as speckle imaging.

The site on the Haleakalā volcano was selected for its clear daytime weather and favourable atmospheric seeing conditions.[7]

It commenced its first science observations on February 23, 2022, signaling the start of its year-long operations commissioning phase.[8]

  1. ^ "Solar Telescope Named for Late Senator Inouye". National Solar Observatory. 16 December 2013. Retrieved 21 October 2015.
  2. ^ Witze, A. (29 January 2020). "World's most powerful solar telescope is up and running". Nature. doi:10.1038/d41586-020-00224-z. PMID 33504997. S2CID 213261911.
  3. ^ Hannah Devlin (29 January 2020). "Telescope captures most detailed pictures yet of the sun". The Guardian.
  4. ^ "NSF FY2019 Report" (PDF). National Science Foundation. 2019. Retrieved 16 December 2022.
  5. ^ Crockett, C. (29 January 2020). "These are the most detailed images of the sun ever taken". Science News. Retrieved 30 January 2020.
  6. ^ Cite error: The named reference Nov2021 was invoked but never defined (see the help page).
  7. ^ Raftery, Claire (18 December 2019). "Why Build the Inouye Solar Telescope on Haleakalā". NSO - National Solar Observatory. Retrieved 24 December 2022.
  8. ^ U.S. NSF's Daniel K. Inouye Solar Telescope Begins Science Operations Commissioning Phase