Synonyms
Definition
Infrared astronomy is the branch of observational astronomy which studies celestial objects through their infrared radiation, that is, at wavelengths longer than 0.75 μm and shorter than 400 μm. The domain is not strictly defined, and some astronomers consider that it begins at 1 μm where CCDs, the most universally used detectors in the visible domain, are no longer sensitive. Infrared astronomy is considered as part of optical astronomy because technologies and methods (incoherent detection, classical optics, solid-state digital detectors) are globally the same as in the visible domain. One peculiarity of infrared astronomy is the strong background emission of the environment (atmosphere, telescope) that requires dedicated differential techniques. Another one is the absorption by the atmosphere (see Fig. 1) in a large fraction of the wavelength domain: this explains why balloons, airplanes, and satellites are often...
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2023 Springer-Verlag GmbH Germany, part of Springer Nature
About this entry
Cite this entry
Rouan, D. (2023). Infrared Astronomy. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-65093-6_786
Download citation
DOI: https://doi.org/10.1007/978-3-662-65093-6_786
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-662-65092-9
Online ISBN: 978-3-662-65093-6
eBook Packages: Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics