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The human eye is a remarkable biological invention and a shining triumph of the process of evolution. Although it was the detector that started us on mankind's exploration of the Cosmos, it has some shortcomings that ultimately limit that exploration:
1. The eye has limited size and therefore limited light-gathering power.
2. The eye has limited frequency response, since it can only see electromagnetic radiation in the visible wavelengths.
3. The eye distinguishes a new image multiple times a second, so it cannot be used to accumulate light over a long period in order to intensify a faint image.
4. The eye cannot store an image for future reference (like, say a photographic plate or an electronic detector).
Astronomers have developed a variety of instruments and techniques to supplement the human eye and to overcome these limitations.