Glossarbegriffe: Teleskop
Description: Ein Teleskop ist ein Gerät, das Photonen (des sichtbaren Lichts oder anderer Wellenlängen) von weit entfernten Objekten sammelt und so einem Beobachter Informationen (z. B. ein Bild) über diese Objekte liefert. Frühe Teleskope (ab Anfang des 17. Jahrhunderts) verwendeten Linsen als optische Elemente (siehe Fernrohr). Linsen für solche Teleskope können aber nicht beliebig groß hergestellt werden. Deshalb werden stattdessen Spiegel (siehe Spiegelteleskop) benutzt, um das Licht von lichtschwächeren Objekten mit größeren Teleskopen zu fokussieren. Deshalb sind die größten optischen Teleskope Spiegelteleskope. Im 20. Jahrhundert wurden Teleskope zur Untersuchung anderer Bereiche der elektromagnetischen Strahlung erfunden, sodass es heute Radioteleskope, Infrarotteleskope, Röntgenteleskope usw. gibt. Da die Himmelsquellen lichtschwach sind, bauen Astronomen in der Regel Teleskope mit großer Öffnung, um mehr Licht zu sammeln und eine größere Winkelauflösung zu erreichen.
Zugehörige Glossarbegriffe:
- Elektromagnetische Strahlung
- Infrarotteleskop
- Radioteleskop
- Spiegelteleskop
- Fernrohr
- Auflösungsvermögen
- Röntgenteleskop
- Linse
- Spiegel
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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