Light, spectra and telescopes
The electromagnetic spectrum, blackbody radiation, spectral lines and the Doppler effect, then the telescopes and detectors that collect light from radio waves to gamma rays.
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Frente adaptive opticsVerso systems used with telescopes that can compensate for distortions in an image introduced by the atmosphere, thus resulting in sharper images
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Frente apertureVerso diameter of the primary lens or mirror of a telescope
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Frente charge-coupled device (CCD)Verso array of high-sensitivity electronic detectors of electromagnetic radiation, used at the focus of a telescope (or camera lens) to record an image or spectrum
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Frente chromatic aberrationVerso distortion that causes an image to appear fuzzy when each wavelength coming into a transparent material focuses at a different spot
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Frente detectorVerso device sensitive to electromagnetic radiation that makes a record of astronomical observations
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Creative Commons Attribution 4.0 International
CC-BY-4.0 - Atribuição
- Source : https://openstax.org/books/astronomy/pages/preface — Licence : Creative Commons Attribution 4.0 International (https://creativecommons.org/licenses/by/4.0/)
- Fonte
- OpenStax — Astronomy (first edition)
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- Astronomia
- Idioma
- English
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- 3
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