Skip to main content
Physics LibreTexts

10.3: The Spectroscope

  • Page ID
    29734
  • \( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}} } \) \( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash {#1}}} \)\(\newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\) \( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\) \( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\) \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\) \( \newcommand{\Span}{\mathrm{span}}\) \(\newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\) \( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\) \( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\) \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\) \( \newcommand{\Span}{\mathrm{span}}\)\(\newcommand{\AA}{\unicode[.8,0]{x212B}}\)

    The Spectroscope

    Light dispersion of a mercury-vapor lamp with a prism made of flint glass.
    When light strikes or enters a prism, it is dispersed into component colors. This is an example of spectroscopy. Light dispersion by D-Kuru is licensed under CC BY-SA 3.0

    A star’s color tells us a lot about the star: its temperature and perhaps even the star’s life cycle. But to dig a bit deeper, scientists use a tool called the spectroscope and spectroscopy. In 1814, Joseph van Fraunhofer invented the modern spectroscope. The spectroscope basically uses a prism or diffraction grating to break light into its component colors, producing a spectrum. There is also a slit, where the light enters, and a telescope-like focuser.

    The heart of the spectroscope — the component which breaks light into its component colors, is either a prism or a diffraction grating. Think of the diffraction grating as many small prisms on a thin sheet of plastic or glass; 500 or more rulings per inch. The CD is a good analogy to a diffraction grating.

    The bottom of a CD is shown with colors illuminated by a light reflection.
    The grooves of a CD can act as a diffraction grating, producing colors when light is reflected off of the CDInterference-colors by Luis Fernández García is licensed under CC BY-SA 2.0

    A spectroscope can be mounted on a telescope, collecting light from one object, such as a star or galaxy, to be passed through the spectroscope for analysis. (1)

    Lick Observatory’s Spectroscope, 1898. The actual spectroscope, which looks like a tube, is attached to the back of the telescope is in the lower left of the illustration.
    Lick Observatory’s Spectroscope, 1898. The actual spectroscope, which looks like a tube, is attached to the back of the telescope is in the lower left of the illustration. Star-Spectroscope by Julius Scheiner is in thePublic Domain
    CC licensed content, Original

    10.3: The Spectroscope is shared under a not declared license and was authored, remixed, and/or curated by LibreTexts.

    • Was this article helpful?