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zodiacal light

 
Dictionary: zodiacal light

n.
A faint hazy cone of light, often visible in the west just after sunset or in the east just before sunrise, apparently caused by the reflection of sunlight from meteoric particles in the plane of the ecliptic.


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Band of very faint light in the night sky. It is thought to be sunlight reflected from interplanetary dust grains lying mostly in the plane of the zodiac, or ecliptic. Seen in the west after twilight and in the east before dawn, it is most clearly visible in the tropics, where the ecliptic is approximately perpendicular to the horizon. In midnorthern latitudes it is best seen evenings in February and March and mornings in September and October (vice versa in midsouthern latitudes). The light can be followed visually to a point about 90° from the Sun. It continues to the region opposite the Sun, where a slight enhancement, the gegenschein, is visible.

For more information on zodiacal light, visit Britannica.com.

Sci-Tech Encyclopedia: Zodiacal light
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A diffuse, night-sky luminosity easily seen at low to middle geographic latitudes in the absence of moonlight. It is caused by sunlight scattered and absorbed by interplanetary (solar system) dust particles. Zodiacal light extends over the entire sky, but it is brightest toward the Sun and in the zodiacal band. It is best seen in the west after evening twilight and in the east before morning twilight when the ecliptic is close to the vertical. In the Northern Hemisphere this corresponds to spring evenings and autumn mornings. See also Ecliptic; Interplanetary matter.

The density of particles responsible for the zodiacal light falls off somewhat faster than 1/R, where R is heliocentric distance. The particles are primarily in the size range of tens to hundreds of micrometers in diameter, and are believed to originate primarily from comets. See also Comet.

The visual zodiacal light brightness decreases monotonically with elongation (angular distance from the Sun) to a relatively flat minimum in the ecliptic at 120 to 140°, after which it gradually increases out to the antisolar point at 180°. The enhanced brightness near the antisolar point is called the Gegenschein or counterglow. It is barely above the visible threshold and is described by visual observers as being oval in appearance, 6 by 10° or larger, with the long axis in the ecliptic. Space observations have shown the Gegenschein to be an intrinsic part of the zodiacal light; that is, the zodiacal dust particles have an increased scattering efficiency near backscattering.

Although the Earth's atmosphere complicates attempts to observe zodiacal light closer than approximately 30° to the Sun, eclipse and space observations have shown the brightness to increase smoothly all the way in to the F-corona. The F-corona or inner zodiacal light and the “primary” zodiacal light seen at larger elongations come primarily from dust particles located relatively close to the Sun. See also Solar corona; Sun.


 
Columbia Encyclopedia: zodiacal light
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zodiacal light or zodiacal band, a faint band of light sometimes seen in the western sky just after sunset in the spring, extending up from the horizon at the point where the sun has just set, or in the eastern sky just before sunrise in the autumn. The light is so faint as to be obscured by moonlight. It is caused by the reflection and scattering of sunlight by a sparse band of tiny dust particles that appears to be an extension of the solar corona, stretching out beyond the orbit of Jupiter. Concentrated in the plane of the ecliptic, the faint light is best seen in the region of the sky called the zodiac. Near the equator the zodiacal light sometimes seems to stretch completely across the sky. It was first investigated and explained by the astronomer Gian Domenico Cassini about 1690.

See also gegenschein.


Wikipedia: Zodiacal light
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The zodiacal light in the eastern sky before the beginning of morning twilight. The planet Venus and the open cluster M44 are also visible in this photograph.

The zodiacal light is a faint, roughly triangular, whitish glow seen in the night sky which appears to extend up from the vicinity of the sun along the ecliptic or zodiac. It is so faint that it is completely masked by either moonlight or light pollution. The zodiacal light decreases in intensity with distance from the Sun, but on very dark nights it has been observed in a band completely around the ecliptic. In fact, the zodiacal light covers the entire sky, being responsible for 60% of the total skylight on a moonless night. There is also a very faint, but still slightly increased, oval glow directly opposite the Sun which is known as the gegenschein.

This phenomenon was first investigated by the astronomer Giovanni Domenico Cassini in 1683 and first explained by Nicolas Fatio de Duillier in 1684.

Contents

Viewing

A green and red Orionid meteor striking the sky below Milky Way and to the right of Venus. Zodiacal light is also seen in this image

In mid-latitudes, the zodiacal light is best observed in the western sky in the spring after the evening twilight has completely disappeared, or in the eastern sky in the autumn just before the morning twilight appears. The zodiacal light appears as a column, brighter at the horizon, tilted at the angle of the ecliptic. Since the light scattered from extremely small dust particles is strongly forward scattering, although the zodiacal light actually extends all the way around the sky, it's brightest when you're looking in the direction toward the sun, because the scattered light is scattered most strongly in the nearly-forward directions. This is why it is most clearly visible near sunrise or sunset, when the sun is blocked, but the dust particles nearest the line of sight to the sun are not. The dust band that makes up the zodiacal light is actually uniform across the whole ecliptic, but the dust furthest from the ecliptic is almost indetectable, except when viewed looking nearly into the sun. Thus you can see of the width the closer to the sun you look, and it seems wider near the horizon.


Formation

Zodiacal Light Seen from Paranal.

The zodiacal light is produced by sunlight reflecting off dust particles in the solar system known as cosmic dust. Consequently, its spectrum is the same as the solar spectrum. The material producing the zodiacal light is located in a lens-shaped volume of space centered on the sun and extending well out beyond the orbit of Earth. This material is known as the interplanetary dust cloud. Since most of the material is located near the plane of the solar system, the zodiacal light is seen along the ecliptic. The amount of material needed to produce the observed zodiacal light is amazingly small. If it were in the form of 1 mm particles, each with the same albedo (reflecting power) as Earth's moon, each particle would be 8 km from its neighbors. The gegenschein may be because particles directly opposite the sun as seen from Earth would be in full phase.

The Poynting-Robertson effect causes the particles to spiral slowly into the Sun, thus requiring a continuous source of new particles to maintain the zodiacal cloud. Cometary dust and dust generated by collisions among the asteroids are believed to be mostly responsible for the maintenance of the dust cloud producing the zodiacal light and the gegenschein. In recent years, observations by a variety of spacecraft have shown significant structure in the zodiacal light including dust bands associated with debris from particular asteroid families and several cometary trails.


Historical explanations

Previously, it was believed that zodiacal light was just the atmosphere of the sun. According to the 1728 Cyclopaedia:

"The zodiacal light is nothing but the solar atmosphere, a rare and subtile fluid, either luminous by itself, or made so by the rays of the sun surrounding its globe; but in a greater quantity, and more extensively, about its equator, than any other."

Importance to Islam

The Islamic Prophet Muhammed is known to have described zodiacal light in reference to the timing of the five daily prayers, calling it the "false dawn," (Arabic: al-fajr al-kaadhib‎ الفجر الكاذب). Muslim oral tradition preserves numerous sayings, or hadith, in which Muhammed describes the difference between the light of false dawn, appearing in the sky long after sunset, and the light of the first band of horizontal light at sunrise, the true dawn. Practitioners of Islam use Muhammed's descriptions of zodiacal light to avoid errors in determining the timing of daily prayers.

Such practical descriptions and applications of astronomical observations were vital to the golden age of Islamic astronomy.

See also

References

External links


 
 
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Dictionary. The American Heritage® Dictionary of the English Language, Fourth Edition Copyright © 2007, 2000 by Houghton Mifflin Company. Updated in 2009. Published by Houghton Mifflin Company. All rights reserved.  Read more
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Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2003, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/ Read more
Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Zodiacal light" Read more