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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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  • Anverso adaptive optics
    Reverso systems used with telescopes that can compensate for distortions in an image introduced by the atmosphere, thus resulting in sharper images
  • Anverso aperture
    Reverso diameter of the primary lens or mirror of a telescope
  • Anverso charge-coupled device (CCD)
    Reverso 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
  • Anverso chromatic aberration
    Reverso distortion that causes an image to appear fuzzy when each wavelength coming into a transparent material focuses at a different spot
  • Anverso detector
    Reverso device sensitive to electromagnetic radiation that makes a record of astronomical observations

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Licencia
Creative Commons Attribution 4.0 International CC-BY-4.0
Atribución
Source : https://openstax.org/books/astronomy/pages/preface — Licence : Creative Commons Attribution 4.0 International (https://creativecommons.org/licenses/by/4.0/)
Fuente
OpenStax — Astronomy (first edition)
Obtenido el
Tema
Astronomía
Idioma
English
Versión
3
Actualizado el

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