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Infrared astronomy information


Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation. The wavelength of infrared light ranges from 0.75 to 300 micrometers, and falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.

Infrared astronomy began in the 1830s, a few decades after the discovery of infrared light by William Herschel in 1800. Early progress was limited, and it was not until the early 20th century that conclusive detections of astronomical objects other than the Sun and Moon were made in infrared light. After a number of discoveries were made in the 1950s and 1960s in radio astronomy, astronomers realized the information available outside the visible wavelength range, and modern infrared astronomy was established.

Infrared and optical astronomy are often practiced using the same telescopes, as the same mirrors or lenses are usually effective over a wavelength range that includes both visible and infrared light. Both fields also use solid state detectors, though the specific type of solid state photodetectors used are different. Infrared light is absorbed at many wavelengths by water vapor in the Earth's atmosphere, so most infrared telescopes are at high elevations in dry places, above as much of the atmosphere as possible. There have also been infrared observatories in space, including the Spitzer Space Telescope, the Herschel Space Observatory, and more recently the James Webb Space Telescope.

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Infrared astronomy

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Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation...

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Stratospheric Observatory for Infrared Astronomy

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The Stratospheric Observatory For Infrared Astronomy (SOFIA) was a 80/20 joint project of NASA and the German Aerospace Center (DLR) to construct and maintain...

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Astronomy

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pulsars, and active galactic nuclei. Infrared astronomy is founded on the detection and analysis of infrared radiation, wavelengths longer than red...

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Infrared

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using active near-infrared illumination allow people or animals to be observed without the observer being detected. Infrared astronomy uses sensor-equipped...

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James Webb Space Telescope

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Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy. Its high-resolution and high-sensitivity instruments allow it to...

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Infrared telescope

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infrared astronomy, far-infrared astronomy, to submillimetre astronomy. Ground based : Infrared Telescope Facility, Hawaii, 1979– Gornergrat Infrared...

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Observational astronomy

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wavelengths used by X-ray astronomy, gamma-ray astronomy, UV astronomy and (except for a few wavelength "windows") far infrared astronomy, so observations must...

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IRAS

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launched in 2003. The success of early infrared space astronomy led to further missions, such as the Infrared Space Observatory (1990s) and the Hubble Space...

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National Optical Astronomy Observatory

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Optical Astronomy Observatory (NOAO) was the United States national observatory for ground-based nighttime ultraviolet-optical-infrared (OUVIR) astronomy. The...

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Airborne observatory

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perform infrared astronomy; among other discoveries are "the first measurement of the internal energies of Jupiter and Saturn, far-infrared observations...

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NASA Infrared Telescope Facility

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The NASA Infrared Telescope Facility (NASA IRTF) is a 3-meter (9.8 ft) telescope optimized for use in infrared astronomy and located at the Mauna Kea...

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JAXA

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also gave ground support for the ESA Infrared Space Observatory (ISO) infrared mission. JAXA's first infrared astronomy satellite was the Akari spacecraft...

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Amy Mainzer

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astrophysical instrumentation and infrared astronomy. She is the deputy project scientist for the Wide-field Infrared Survey Explorer and the principal...

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Outline of astronomy

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Submillimetre astronomy – 200 μm to 1 mm Infrared astronomy – 0.7–350 μm Optical astronomy – 380–750 nm Ultraviolet astronomy – 10–320 nm X-ray astronomy – 0.01–10 nm...

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Submillimetre astronomy

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Horizon Telescope Terahertz radiation Far infrared astronomy SCUBA-2 All Sky Survey Radio window Infrared window Optical window Category:Submillimetre...

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List of largest infrared telescopes

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The largest infrared telescopes for infrared astronomy are listed in terms of diameter of primary mirror. The infrared spectrum with its longer wavelength...

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Infrared spectroscopy

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engineering Infrared astronomy Infrared microscopy Infrared multiphoton dissociation Infrared photodissociation spectroscopy Infrared spectroscopy correlation...

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Dark nebula

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obscures are visible only using radio waves in radio astronomy or infrared in infrared astronomy. Dark clouds appear so because of sub-micrometre-sized...

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Infrared photography

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emulsions from Kodak and other manufacturers became useful to infrared astronomy. Infrared photography became popular with photography enthusiasts in the...

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Spitzer Space Telescope

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January 2020. Spitzer was the third space telescope dedicated to infrared astronomy, following IRAS (1983) and ISO (1995–1998). It was the first spacecraft...

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Galactic astronomy

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regions of cosmic dust. The development of radio astronomy, infrared astronomy and submillimetre astronomy in the 20th century allowed the gas and dust of...

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Radio astronomy

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radio astronomy service as follows. Radio portal Astronomy portal Atacama Large Millimeter Array Channel 37 Gamma-ray astronomy Infrared astronomy Radar...

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Ian Glass

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Technology in 1968 for work in x-ray astronomy under George W. Clark. Since 1970 he has worked in infrared astronomy and instrumentation and he has written...

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Boeing 747

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Stratospheric Observatory for Infrared Astronomy (SOFIA) – A former Pan Am Boeing 747SP modified to carry a large infrared-sensitive telescope, in a joint...

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Infrared cirrus

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were first detected by the Infrared Astronomy Satellite at wavelengths of 60 and 100 micrometres. Galaxy filament Cosmic infrared background Low, F. J.; et al...

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Pleiades

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"The distance to the Pleiades. Main sequence fitting in the near infrared". Astronomy and Astrophysics. 429 (3): 887–894. arXiv:astro-ph/0409362. Bibcode:2005A&A...

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