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.
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 Telescope | 6.5m (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
| 2010-2022 | [5] | ||
2.3m (07.5feet) | 0.4 - 0.8 μm | Jelm mountain, 9656 ft. (2943m) | 1977 | [6] | ||
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 | - | |