Astronomy optics is a branch of optics and photonics that uses light-controlling components to image celestial objects. It combines precisely machined lenses and mirrors to reduce image distortion and highly sensitive sensors to detect low levels of light. In the optical application, adaptive astronomy optics can be used for astronomical telescopes.
A large size optical mirror is important to the astronomical system. The most common are Newtonian Mirrors and the classic Cassegrain. These mirrors are usually divided into primary and secondary mirrors. The primary mirror is mostly parabolic design
Our hours
Mon 11/21 - Wed 11/23: 9 AM - 8 PM
Thu 11/24: closed - Happy Thanksgiving!
Fri 11/25: 8 AM - 10 PM
Sat 11/26 - Sun 11/27: 10 AM - 9 PM
(all hours are Eastern Time)
English
français
Deutsch
italiano
русский
español
português
Türkçe
ไทย
Tiếng việt
IPv6 network supported