A reflecting telescope is a type of telescope that uses a curved mirror to gather and focus light. The design of reflecting telescopes allows for larger apertures, which in turn enables greater light-gathering power and higher resolution. This makes them ideal for astronomical observations.
Secondary Mirror: Some reflecting telescopes include a secondary mirror that reflects the focused light out of the side of the telescope, allowing it to be viewed through an eyepiece or a camera.
Focuser: The focuser is the part of the telescope that holds the eyepiece or camera and allows for fine-tuning the focus of the telescope.
Easier and Cheaper to Manufacture:Mirrors are generally easier and cheaper to manufacture than lenses, making reflecting telescopes more cost-effective.
When studying reflecting telescopes, it's important to understand the following key concepts:
Reflecting TelescopeDesigns: Be familiar with the different designs of reflecting telescopes, such as Newtonian, Cassegrain, and Ritchey-Chrétien.
Primary Mirror Properties: Understand how the size and curvature of the primary mirror affect the light-gathering ability and resolution of the telescope.