Glossary term: Extinción Atmosférica
Description: La extinción atmosférica es la dispersión o absorción de la luz de los objetos celestes que atraviesan la atmósfera terrestre. Los gases atmosféricos permiten la entrada de luz visible y son transparentes a la luz de radio y a parte de la infrarroja, por lo que este tipo de telescopios terrestres son muy utilizados. Para evitar este fenómeno y observar la luz de otras longitudes de onda, algunos telescopios se sitúan más allá de la atmósfera.
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See this term in other languages
Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
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In Other Languages
- Árabe: التوهين الجوي للضوء
- Alemán: Atmosphärische Extinktion
- Inglés: Atmospheric Extinction
- Francés: Extinction atmosphérique
- Italiano: Estinzione atmosferica
- Japonés: 大気吸収 (external link)
- Coreano: 대기소광
- Portugués de Brasil: Extinção atmosférica
- Chino simplificado: 大气消光
- Chino tradicional: 大氣消光



