Optical Telescopes
Optical telescopes are instruments that use lenses or mirrors to collect and focus visible light from distant objects in space. They are designed to capture and magnify the light emitted by celestial bodies, allowing astronomers to study their properties and behavior. Optical telescopes come in a variety of sizes and designs, from small refracting telescopes to large reflecting telescopes with segmented mirrors. They can be used for a wide range of astronomical observations, including studying the surfaces of planets and moons, observing stars and galaxies, and detecting and characterizing exoplanets. Optical telescopes are often equipped with additional instruments, such as spectrographs and cameras, to analyze the light they collect in more detail.
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