A reflecting telescope is a type of telescope that uses a combination of curved mirrors to gather and focus light to create an image. It was invented by Sir Isaac Newton in the 17th century.
Reflecting telescopes have several advantages over other types of telescopes, including:
When light enters the telescope, it first strikes the primary mirror, which reflects it to the secondary mirror. The secondary mirror then reflects the light to the focal point, where the eyepiece or camera is located. This creates a magnified image of the object being observed.
Reflecting telescopes are used in a variety of applications, including:
Here are some key points to remember about reflecting telescopes: