List of largest infrared telescopes explained

The largest infrared telescopes for infrared astronomy are listed in terms of diameter of primary mirror. The infrared spectrum with its longer wavelength than visible light has a number of challenges, especially for ground-based observatories but also in space. Notably infrared radiation is emitted by all physical objects above Absolute Zero temperature so telescopes are subject to local interference.

Overall

Infrared observations from Earth's surface are possible in a limited way but can be very dependent on location and atmospheric conditions. Water vapour in the Earth's atmosphere blocks much of the infrared band, although some limited observations are possible and there is a number of infrared observatories.

Sometimes other optical telescopes can make infrared observations if they are equipped with the right detectors, even if they are not dedicated infrared observatories. For ground-based observatories, the location can make a big difference in how much observation is possible.

Name Image Effective
aperture
Wavelength
Coverage
Site Year(s) Refs
6.5m (21.3feet) University of Tokyo Atacama Obs., Chile 2024 [1]
James Webb Space Telescope6.5m (21.3feet) 2022-
4.1m (13.5feet) 0.85 – 2.3 μm Paranal Obs., Chile 2008 [2]
150abbr=onNaNabbr=on 0.8 - 20 μm Mauna Kea Obs., Hawaii 1978
3.5m (11.5feet) 60-672 μm 2009-2013 [3]
3.2m (10.5feet) 0.8 - 25 μm 1979 [4]
2.5m (08.2feet) 0.3 - 655 μm 747SP
Stratosphere
2010-2022 [5]
2.3m (07.5feet) 0.4 - 0.8 μm Jelm mountain, 9656 ft. (2943m) 1977 [6]

Space telescopes only

Name Effective
aperture
cm (in)
Wavelength
Coverage
Year Refs
650 cm 2021-
350 cm (138 in) 60-672 μm 2009 - 2013
240 cm 0.2-1.7 μm 2009 -
Euclid NISP 120 cm 0.92-2.02 μm 2023 -
85 cm 3-180 μm 2003 - 2020
68.5 cm 2-200 μm 2006 -2011
60 cm 2.5-240 μm 1995-1998
57 cm 5-100 μm 1983 [7]
50 cm 4–5.2 & 6–10 μm 2028 (planned) [8]
40 cm 3-25 μm 2009-2011 & 2013 -
33 cm 4.3-21 μm 1996 - 1997
15.2 cm 1.7-118 μm 1985 Aug [9]
Human Eye ~1 cm 0.39-0.75 μm -
For comparison

See also

Notes and References

  1. http://www.ioa.s.u-tokyo.ac.jp/TAO/intro/intro3.html
  2. Emerson, J.P., Sutherland, W.J., McPherson, A.M., Craig, S.C., Dalton, G.B., Ward, A.K. (2005). The Visible & Infrared Survey Telescope for Astronomy. The Messenger
  3. News: ESA launches Herschel and Planck space telescopes . BBC . 14 June 2009. 10 November 2011 . Jonathan . Amos.
  4. http://irtfweb.ifa.hawaii.edu/information/about.php IRTF homepage
  5. Alfred . Krabbe . SOFIA telescope . Proceedings of SPIE: Astronomical Telescopes and Instrumentation . 276–281 . March 2007 . SPIE — The International Society for Optical Engineering . Munich, Germany . astro-ph/0004253. 2000SPIE.4014..276K . 10.1117/12.389103 .
  6. http://physics.uwyo.edu/~chip/wiro/ University of Wyoming 2.3-meter Telescope (WIRO)
  7. http://herschel.jpl.nasa.gov/relatedMissions.shtml JPL: Herschel Space Observatory: Related Missions
  8. http://www.planetary.org/blogs/jason-davis/nasa-to-build-asteroid-telescope.html NASA to Build New Asteroid-Hunting Space Telescope 2019
  9. http://adsabs.harvard.edu/full/1992ApJS...78..403K Kent, et al. – Galactic structure from the Spacelab infrared telescope (1992)