Glossary term: Reflecting Telescope
Description: In a reflecting telescope or mirror telescope, the main optical element is a mirror, the "main mirror", which bundles infalling light. Mirror telescopes are often characterized by main mirror diameter, ranging from a dozen centimeters for smaller amateur telescopes to eight meters for the largest solid mirrors used in professional telescopes. Still larger collecting areas can be obtained by combining several mirror segments, which then act in a way similar to that of a larger solid mirror. There are several types of mirror telescopes. For example, in a Newtonian telescope the light coming from the main mirror is reflected sideways by a smaller mirror into an eyepiece. In a Cassegrain telescope, a smaller secondary mirror reflects the light back, through an opening in the main mirror.Related Terms:
See this term in other languages
Term and definition status: 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".
Keck TelescopesCaption: The two Keck telescopes on Mauna Kea on the island of Hawai`i. These two telescopes are reflecting telescopes with primary mirrors 10m across.
Credit: NASA/JPL credit link
License: PD Public Domain icons