Visible spectrum

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White light is dispersed by a prism into the colors of the optical spectrum.

The visible spectrum is the portion of the electromagnetic spectrum that is visible to (can be detected by) the human eye. Electromagnetic radiation in this range of wavelengths is called visible light or simply light. A typical human eye will respond to wavelengths from about 390 to 700 nm.[1] In terms of frequency, this corresponds to a band in the vicinity of 430–790 THz.

The spectrum does not, however, contain all the colors that the human eyes and brain can distinguish. Unsaturated colors such as pink, or purple variations such as magenta, are absent, for example, because they can be made only by a mix of multiple wavelengths. Colors containing only one wavelength are also called pure colors.

Visible wavelengths pass through the "optical window", the region of the electromagnetic spectrum that allows wavelengths to pass largely unattenuated through the Earth's atmosphere. An example of this phenomenon is that clean air scatters blue light more than red wavelengths, and so the midday sky appears blue. The optical window is also called the visible window because it overlaps the human visible response spectrum. The near infrared (NIR) window lies just out of the human vision, as well as the Medium Wavelength IR (MWIR) window and the Long Wavelength or Far Infrared (LWIR or FIR) window though other animals may experience them.

Many species can see light with frequencies outside the "visible spectrum," which is defined in terms of human vision. Bees and many other insects can detect ultraviolet light, which helps them find nectar in flowers. Plant species that depend on insect pollination may owe reproductive success to their appearance in ultraviolet light rather than how colorful they appear to humans. Birds, too, can see into the ultraviolet (300–400 nm), and some have sex-dependent markings on their plumage that are visible only in the ultraviolet range.[2][3] Many animals that can see into the ultraviolet range, however, cannot see red light or any other reddish wavelengths.[citation needed] Bees' visible spectrum ends at about 590 nm, just before the orange wavelengths start.[citation needed] Birds, however, can see some red wavelengths, but not as many as humans.[citation needed] It is an incorrect popular belief that the common goldfish is the only animal that can see both infrared and ultraviolet light,[4] but goldfish cannot see infrared light.[5]

History[edit]

Visible laser (bottom to top: 445nm, 532nm, 635nm)
Newton's color circle, from Opticks of 1704, showing the colors correlated with musical notes. The spectral colors from red to violet are divided by the notes of the musical scale, starting at D. The circle completes a full octave, from D to D. Newton's circle places red, at one end of the spectrum, next to violet, at the other. This reflects the fact that non-spectral purple colors are observed when red and violet light are mixed.
Illumination with three different coloured light sources; red, green, and blue.

In the 13th century, Roger Bacon theorized that rainbows were produced by a similar process to the passage of light through glass or crystal.[6]

In the 17th century, Isaac Newton discovered that prisms could disassemble and reassemble white light, and described the phenomenon in his book Opticks. He was the first to use the word spectrum (Latin for "appearance" or "apparition") in this sense in print in 1671 in describing his experiments in optics. Newton observed that, when a narrow beam of sunlight strikes the face of a glass prism at an angle, some is reflected and some of the beam passes into and through the glass, emerging as different-colored bands. Newton hypothesized light to be made up of "corpuscles" (particles) of different colors, with the different colors of light moving at different speeds in transparent matter, red light moving more quickly than violet in glass. The result is that red light bends (refracted) less sharply than violet as it passes through the prism, creating a spectrum of colors.

Newton's observation of prismatic colors.

Newton divided the spectrum into seven named colors: red, orange, yellow, green, blue, indigo, and violet. He chose seven colors out of a belief, derived from the ancient Greek sophists, of there being a connection between the colors, the musical notes, the known objects in the solar system, and the days of the week.[7][8] The human eye is relatively insensitive to indigo's frequencies, and some otherwise-well-sighted people cannot distinguish indigo from blue and violet. For this reason, some later commentators, including Isaac Asimov,[9] have suggested that indigo should not be regarded as a color in its own right but merely as a shade of blue or violet. However, the evidence indicates that what Newton meant by "indigo" and "blue" does not correspond to the modern meanings of those color words. Comparing Newton's observation of prismatic colors to a color image of the visible light spectrum shows that "indigo" corresponds to what is today called blue, whereas "blue" corresponds to cyan.

In the 18th century, Goethe wrote about optical spectra in his Theory of Colours. Goethe used the word spectrum (Spektrum) to designate a ghostly optical afterimage, as did Schopenhauer in On Vision and Colors. Goethe argued that the continuous spectrum was a compound phenomenon. Where Newton narrowed the beam of light to isolate the phenomenon, Goethe observed that a wider aperture produces not a spectrum but rather reddish-yellow and blue-cyan edges with white between them. The spectrum appears only when these edges are close enough to overlap.

In the early 19th century, the concept of the visible spectrum became more definite, as light outside the visible range was discovered and characterized by William Herschel (infrared) and Johann Wilhelm Ritter (ultraviolet), Thomas Young, Thomas Johann Seebeck, and others.[10] Young was the first to measure the wavelengths of different colors of light, in 1802.[11]

The connection between the visible spectrum and color vision was explored by Thomas Young and Hermann von Helmholtz in the early 19th century. Their theory of color vision correctly proposed that the eye uses three distinct receptors to perceive color.

Spectral colors[edit]

sRGB rendering of the spectrum of visible light
ColorFrequencyWavelength
violet668–789 THz380–450 nm
blue606–668 THz450–495 nm
green526–606 THz495–570 nm
yellow508–526 THz570–590 nm
orange484–508 THz590–620 nm
red400–484 THz620–750 nm

Colors that can be produced by visible light of a narrow band of wavelengths (monochromatic light) are called pure spectral colors. The various color ranges indicated in the diagram on the right are an approximation: The spectrum is continuous, with no clear boundaries between one color and the next.[12]

Spectroscopy[edit]

Rough plot of Earth's atmospheric opacity (opposite of transmittance) to various wavelengths of electromagnetic radiation, including visible light.

Spectroscopy is the study of objects based on the spectrum of color they emit or reflect. Spectroscopy is an important investigative tool in astronomy, where scientists use it to analyze the properties of distant objects. Typically, astronomical spectroscopy uses high-dispersion diffraction gratings to observe spectra at very high spectral resolutions. Helium was first detected by analysis of the spectrum of the sun. Chemical elements can be detected in astronomical objects by emission lines and absorption lines.

The shifting of spectral lines can be used to measure the Doppler shift (red shift or blue shift) of distant objects. The first exoplanets were discovered by analysis of the Doppler shift of the parent star, revealing variations in radial velocity, the star's speed relative to Earth, caused by the planet's gravitational influence.

Color display spectrum[edit]

Spectrum.svg
Approximation of spectral colors on a display results in somewhat distorted chromaticity.
A rendering of the visible spectrum on a gray background produces non-spectral mixtures of pure spectrum with gray, that fit into the sRGB color space.

Color displays (e.g., computer monitors and televisions) have limited abilities to reproduce all colors discernible by a human eye. Colors outside the color gamut of the device, such as most of spectral colors, have to be approximated. If color accurate reproduction of the spectrum is desired, a spectrum can be projected to a uniform gray field. Resulting mixed colors can have all their R,G,B coordinates non-negative and, hence, reproduced without distortions. This gives an accurate simulation of looking at a spectrum on a gray background.[13]

Visible light may is sometimes abbreviated as VIS.

See also[edit]

References[edit]

  1. ^ Cecie Starr (2005). Biology: Concepts and Applications. Thomson Brooks/Cole. ISBN 0-534-46226-X. 
  2. ^ Cuthill, Innes C (1997). "Ultraviolet vision in birds". In Peter J.B. Slater. Advances in the Study of Behavior 29. Oxford, England: Academic Press. p. 161. ISBN 978-0-12-004529-7. 
  3. ^ Jamieson, Barrie G. M. (2007). Reproductive Biology and Phylogeny of Birds. Charlottesville VA: University of Virginia. p. 128. ISBN 1-57808-386-9. 
  4. ^ "True or False? "The common goldfish is the only animal that can see both infra-red and ultra-violet light." - Skeptive". Retrieved September 28, 2013. 
  5. ^ Neumeyer, Christa (2012). "Chapter 2: Color Vision in Goldfish and Other Vertebrates". In Lazareva, Olga; Shimizu, Toru; Wasserman, Edward. How Animals See the World: Comparative Behavior, Biology, and Evolution of Vision. Oxford Scholarship Online. ISBN 978-0-195-33465-4. 
  6. ^ Coffey, Peter (1912). The Science of Logic: An Inquiry Into the Principles of Accurate Thought. Longmans. 
  7. ^ Hutchison, Niels (2004). "Music For Measure: On the 300th Anniversary of Newton's Opticks". Colour Music. Retrieved 2013-12-05. 
  8. ^ Newton, Isaac (1704). Opticks. 
  9. ^ Asimov, Isaac (1975). Eyes on the universe : a history of the telescope. Boston: Houghton Mifflin. p. 59. ISBN 978-0-395-20716-1. 
  10. ^ Mary Jo Nye (editor) (2003). The Cambridge History of Science: The Modern Physical and Mathematical Sciences 5. Cambridge University Press. p. 278. ISBN 978-0-521-57199-9. 
  11. ^ John C. D. Brand (1995). Lines of light: the sources of dispersive spectroscopy, 1800-1930. CRC Press. pp. 30–32. ISBN 978-2-88449-163-1. 
  12. ^ Thomas J. Bruno, Paris D. N. Svoronos. CRC Handbook of Fundamental Spectroscopic Correlation Charts. CRC Press, 2005.
  13. ^ Reproducing Visible Spectra. Repairfaq.org. Retrieved on 2011-02-09.