Sunset (color)

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The Sun, about a minute before astronomical sunset. Sunset 2007-1.jpg
The Sun, about a minute before astronomical sunset.
Sunset
 
Gtk-dialog-info.svg    Color coordinates
Hex triplet #FAD6A5
sRGB B (r, g, b)(250, 214, 165)
HSV (h, s, v)(35°, 34%, 98%)
CIELChuv (L, C, h)(88, 47, 56°)
Source ISCC-NBS
ISCC–NBS descriptor Light yellow
B: Normalized to [0–255] (byte)

The color sunset is a pale tint of orange. It is a representation of the average color of clouds when the sunlight from a sunset is reflected from them.

Contents

The first recorded use of sunset as a color name in English was in 1916. [1]

Origin

Evening twilight in Joshua Tree, California, displaying the separation of yellow colors in the direction from the Sun below the horizon to the observer, and the blue components scattered from the surrounding sky Majestic Twilight.jpg
Evening twilight in Joshua Tree, California, displaying the separation of yellow colors in the direction from the Sun below the horizon to the observer, and the blue components scattered from the surrounding sky

As a ray of white sunlight travels through the atmosphere to an observer, some of the colors are scattered out of the beam by air molecules and airborne particles, changing the final color of the beam the viewer sees. Because the shorter wavelength components, such as blue and green, scatter more strongly, these colors are preferentially removed from the beam. [2] At sunrise and sunset, when the path through the atmosphere is longer, the blue and green components are removed almost completely, leaving the longer wavelength orange and red hues we see at those times. The remaining reddened sunlight can then be scattered by cloud droplets and other relatively large particles to light up the horizon red and orange. [3] The removal of the shorter wavelengths of light is due to Rayleigh scattering by air molecules and particles much smaller than the wavelength of visible light (less than 50 nm in diameter). [4] [5] The scattering by cloud droplets and other particles with diameters comparable to or larger than the sunlight's wavelengths (> 600 nm) is due to Mie scattering and is not strongly wavelength-dependent. Mie scattering is responsible for the light scattered by clouds, and also for the daytime halo of white light around the Sun (forward scattering of white light). [6] [7] [8]

Sunset colors are typically more brilliant than sunrise colors, because the evening air contains more particles than morning air. [2] [3] [5] [8] Sometimes just before sunrise or after sunset a green flash can be seen. [9]

Ash from volcanic eruptions, trapped within the troposphere, tends to mute sunset and sunrise colors, while volcanic ejecta that is instead lofted into the stratosphere (as thin clouds of tiny sulfuric acid droplets), can yield beautiful post-sunset colors called afterglows and pre-sunrise glows. A number of eruptions, including those of Mount Pinatubo in 1991 and Krakatoa in 1883, have produced sufficiently high stratus clouds containing sulfuric acid to yield remarkable sunset afterglows (and pre-sunrise glows) around the world. The high altitude clouds serve to reflect strongly reddened sunlight still striking the stratosphere after sunset, down to the surface.

Some of the most varied colors at sunset can be found in the opposite or eastern sky after the Sun has set during twilight. Depending on weather conditions and the types of clouds present, these colors have a wide spectrum, and can produce unusual results.[ citation needed ]

Variations of sunset

Sunglow

Sunglow
 
Gtk-dialog-info.svg    Color coordinates
Hex triplet #FFCC33
sRGB B (r, g, b)(255, 204, 51)
HSV (h, s, v)(45°, 80%, 100%)
CIELChuv (L, C, h)(84, 93, 63°)
Source Crayola
ISCC–NBS descriptor Vivid yellow
B: Normalized to [0–255] (byte)

The color sunglow is displayed at right.

The first recorded use of sunglow as a color name in English was in 1924. [10] The Crayola crayon color was formulated in 1990.

Sunray

Sunray
 
Gtk-dialog-info.svg    Color coordinates
Hex triplet #E3A857
sRGB B (r, g, b)(227, 168, 87)
HSV (h, s, v)(35°, 62%, 89%)
CIELChuv (L, C, h)(73, 73, 50°)
Source ISCC-NBS
ISCC–NBS descriptor Moderate orange yellow
B: Normalized to [0–255] (byte)

At right is displayed the color sunray.

The first recorded use of sunray as a color name in English was in 1926. [11]

Sunset orange

Sunset Orange
 
Gtk-dialog-info.svg    Color coordinates
Hex triplet #FD5E53
sRGB B (r, g, b)(253, 94, 83)
HSV (h, s, v)(4°, 67%, 99%)
CIELChuv (L, C, h)(61, 127, 14°)
Source Crayola
ISCC–NBS descriptor Vivid red
B: Normalized to [0–255] (byte)

The color sunset orange is displayed at right.

Sunset orange was formulated as a Crayola color in 1997.

Sun colors in human culture

Interior Design

Sports

Related Research Articles

<span class="mw-page-title-main">Afterglow</span> Whitish or rosy light during twilight or after sunset

An afterglow in meteorology consists of several atmospheric optical phenomena, with a general definition as a broad arch of whitish or pinkish sunlight in the twilight sky, consisting of the bright segment and the purple light. Purple light mainly occurs when the Sun is 2–6° below the horizon, from civil to nautical twilight, while the bright segment lasts until the end of the nautical twilight. Afterglow is often in cases of volcanic eruptions discussed, while its purple light is discussed as a different particular volcanic purple light. Specifically in volcanic occurrences it is light scattered by fine particulates, like dust, suspended in the atmosphere. In the case of alpenglow, which is similar to the Belt of Venus, afterglow is used in general for the golden-red glowing light from the sunset and sunrise reflected in the sky, and in particularly for its last stage, when the purple light is reflected. The opposite of an afterglow is a foreglow, which occurs before sunrise.

<span class="mw-page-title-main">Rayleigh scattering</span> Scattering of electromagnetic radiation by particles smaller than the radiations wavelength

Rayleigh scattering, named after the 19th-century British physicist Lord Rayleigh, is the predominantly elastic scattering of light or other electromagnetic radiation by particles much smaller than the wavelength of the radiation. For light frequencies well below the resonance frequency of the scattering particle, the amount of scattering is inversely proportional to the fourth power of the wavelength.

<span class="mw-page-title-main">Sunrise</span> Time of day when the sun appears above the horizon

Sunrise is the moment when the upper rim of the Sun appears on the horizon in the morning. The term can also refer to the entire process of the solar disk crossing the horizon and its accompanying atmospheric effects.

<span class="mw-page-title-main">Sunset</span> Daily falling of the Sun below the horizon

Sunset is the disappearance of the Sun below the horizon due to Earth's rotation. As viewed from everywhere on Earth, it is a phenomenon that happens once every 24 hours except in areas close to the poles. The equinox Sun sets due west at the moment of both the spring and autumn equinoxes. As viewed from the Northern Hemisphere, the Sun sets to the northwest in the spring and summer, and to the southwest in the autumn and winter; these seasons are reversed for the Southern Hemisphere.

<span class="mw-page-title-main">Sky</span> View upward from the surface of the Earth

The sky is an unobstructed view upward from the surface of the Earth. It includes the atmosphere and outer space. It may also be considered a place between the ground and outer space, thus distinct from outer space.

<span class="mw-page-title-main">Diffuse sky radiation</span> Solar radiation reaching the Earths surface

Diffuse sky radiation is solar radiation reaching the Earth's surface after having been scattered from the direct solar beam by molecules or particulates in the atmosphere. It is also called sky radiation, the determinative process for changing the colors of the sky. Approximately 23% of direct incident radiation of total sunlight is removed from the direct solar beam by scattering into the atmosphere; of this amount about two-thirds ultimately reaches the earth as photon diffused skylight radiation.

<span class="mw-page-title-main">Sunbeam</span> Rays of sunlight that appear to radiate from the point in the sky where the sun is located

A sunbeam, in meteorological optics, is a beam of sunlight that appears to radiate from the position of the Sun. Shining through openings in clouds or between other objects such as mountains and buildings, these beams of particle-scattered sunlight are essentially parallel shafts separated by darker shadowed volumes. Their apparent convergence in the sky is a visual illusion from linear perspective. The same illusion causes the apparent convergence of parallel lines on a long straight road or hallway at a distant vanishing point. The scattering particles that make sunlight visible may be air molecules or particulates.

<span class="mw-page-title-main">Tan (color)</span> Pale tone of brown

Tan is a pale tone of brown. The name is derived from tannum used in the tanning of leather.

<span class="mw-page-title-main">Tyndall effect</span> Scattering of light by particles in a colloid such as a fine suspension

The Tyndall effect is light scattering by particles in a colloid such as a very fine suspension. Also known as Tyndall scattering, it is similar to Rayleigh scattering, in that the intensity of the scattered light is inversely proportional to the fourth power of the wavelength, so blue light is scattered much more strongly than red light. An example in everyday life is the blue colour sometimes seen in the smoke emitted by motorcycles, in particular two-stroke machines where the burnt engine oil provides these particles.

<span class="mw-page-title-main">Blue hour</span> Period of twilight in the morning or evening

The blue hour is the period of twilight when the Sun is at a significant depth below the horizon. During this time, the remaining sunlight takes on a mostly blue shade. This shade differs from the colour of the sky on a clear day, which is caused by Rayleigh scattering.

<span class="mw-page-title-main">Belt of Venus</span> Atmospheric phenomenon

The Belt of Venus is an atmospheric phenomenon visible shortly before sunrise or after sunset, during civil twilight. It is a pinkish glow that surrounds the observer, extending roughly 10–20° above the horizon. It appears opposite to the afterglow, which it also reflects.

<span class="mw-page-title-main">Shades of orange</span> Varieties of the color orange

In optics, orange has a wavelength between approximately 585 and 620 nm and a hue of 30° in HSV color space. In the RGB color space it is a secondary color numerically halfway between gamma-compressed red and yellow, as can be seen in the RGB color wheel. The complementary color of orange is azure. Orange pigments are largely in the ochre or cadmium families, and absorb mostly blue light.

<span class="mw-page-title-main">Ruby (color)</span> Color that represents the ruby gemstone

Ruby is a color that is a representation of the color of the cut and polished ruby gemstone and is a shade of red or pink.

<span class="mw-page-title-main">Shades of red</span> Varieties of the color red

Varieties of the color red may differ in hue, chroma or lightness, or in two or three of these qualities. Variations in value are also called tints and shades, a tint being a red or other hue mixed with white, a shade being mixed with black. A large selection of these various colors are shown below.

<span class="mw-page-title-main">Shades of magenta</span> Varieties of the color magenta

The color magenta has notable tints and shades. These various colors are shown below.

Livid is a medium bluish-gray color. This color name comes from the Latin color term lividus meaning "'a dull leaden-blue color', and also used to describe the color of contused flesh, leading to the English expression 'black and blue'". The first recorded use of livid as a color name in English was in 1622.

<span class="mw-page-title-main">Atmospheric optics</span> Study of the optical characteristics of the atmosphere or products of atmospheric processes

Atmospheric optics is "the study of the optical characteristics of the atmosphere or products of atmospheric processes .... [including] temporal and spatial resolutions beyond those discernible with the naked eye". Meteorological optics is "that part of atmospheric optics concerned with the study of patterns observable with the naked eye". Nevertheless, the two terms are sometimes used interchangeably.

<span class="mw-page-title-main">Earth's shadow</span> Shadow that Earth itself casts through its atmosphere and into outer space

Earth's shadow is the shadow that Earth itself casts through its atmosphere and into outer space, toward the antisolar point. During the twilight period, the shadow's visible fringe – sometimes called the dark segment or twilight wedge – appears as a dark and diffuse band just above the horizon, most distinct when the sky is clear.

<span class="mw-page-title-main">Crepuscular rays</span> Sunbeams that originate when the Sun is just below the horizon

Crepuscular rays are sunbeams that originate when the Sun is just above a layer of clouds, during the twilight period. Crepuscular rays are noticeable when the contrast between light and dark is most obvious. Crepuscular comes from the Latin word crepusculum, meaning "twilight". Crepuscular rays usually appear orange because the path through the atmosphere at sunrise and sunset passes through up to 40 times as much air as rays from a high Sun at midday. Particles in the air scatter short-wavelength light through Rayleigh scattering much more strongly than longer-wavelength yellow and red light.

<span class="mw-page-title-main">Shades of rose</span> Varieties of the color rose

Rose is the color halfway between red and magenta on the HSV color wheel, also known as the RGB color wheel.

References

  1. Maerz and Paul A Dictionary of Color New York:1930 McGraw-Hill Page 205; Color Sample of Sunset: Page 43 Plate 10 Color Sample C4
  2. 1 2 K. Saha (2008). The Earth's Atmosphere – Its Physics and Dynamics . Springer. p.  107. ISBN   978-3-540-78426-5.
  3. 1 2 B. Guenther, ed. (2005). Encyclopedia of Modern Optics. Vol. 1. Elsevier. p. 186.
  4. "Hyperphysics, Georgia State University". Hyperphysics.phy-astr.gsu.edu. Retrieved 2012-04-07.
  5. 1 2 Craig Bohren (ed.), Selected Papers on Scattering in the Atmosphere, SPIE Optical Engineering Press, Bellingham, WA, 1989
  6. Corfidi, Stephen F. (February 2009). "The Colors of Twilight and Sunset". Norman, OK: NOAA/NWS Storm Prediction Center.
  7. "Atmospheric Aerosols: What Are They, and Why Are They So Important?". nasa.gov. August 1996.
  8. 1 2 E. Hecht (2002). Optics (4th ed.). Addison Wesley. p.  88. ISBN   0-321-18878-0.
  9. "Red Sunset, Green Flash".
  10. Maerz and Paul A Dictionary of Color New York:1930 McGraw-Hill Page 205
  11. Maerz and Paul A Dictionary of Color New York:1930 McGraw-Hill Page 205; Color Sample of Sunset: Page 43 Plate 10 Color Sample J6

See also