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Night sky

From Wikipedia, the free encyclopedia
Appearance of the sky in a clear night
For other uses, seeNight sky (disambiguation).
Stars in the night sky

Thenight sky is thenighttime appearance ofcelestial objects likestars,planets, and theMoon, which are visible in a clearsky betweensunset andsunrise, when theSun is below thehorizon.

Natural light sources in a night sky includemoonlight,starlight, andairglow, depending on location and timing.Aurorae light up the skies above thepolar circles. Occasionally, a largecoronal mass ejection from the Sun or simply high levels ofsolar wind may extend the phenomenon toward theEquator.[1]

The night sky and studies of it have a historical place in both ancient and modern cultures. In the past, for instance, farmers have used the status of the night sky as acalendar to determine when to plant crops. Many cultures have drawnconstellations between stars in the sky, using them in association withlegends andmythology about theirdeities.

Thehistory of astrology has generally been based on the belief that relationships between heavenly bodies influence or explain events on Earth. The scientific study of objects in the night sky takes place in the context ofobservational astronomy.

Visibility of celestial objects in the night sky is affected bylight pollution. The presence of the Moon in the night sky has historically hindered astronomical observation by increasing the amount ofsky brightness. With the advent of artificial light sources, however, light pollution has been a growing problem for viewing the night sky.Optical filters and modifications to light fixtures can help to alleviate this problem, but for optimal views, both professional andamateur astronomers seek locations far from urbanskyglow.

Brightness

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Main article:Sky brightness
TheMilky Way is brighter in the Southern Hemisphere than in the North. (Photo taken atLa Silla Observatory)[2]

The fact that the sky is not completely dark at night, even in the absence of moonlight and city lights, can be easily observed, since if the sky were absolutely dark, one would not be able to see the silhouette of an object against the sky.

The intensity of the sky brightness varies greatly over the day and the primary cause differs as well. During daytime when the Sun is above the horizon direct scattering of sunlight (Rayleigh scattering) is the overwhelmingly dominant source of light. In twilight, the period of time between sunset and sunrise, the situation is more complicated and a further differentiation is required. Twilight is divided in three segments according to how far the Sun is below the horizon in segments of 6°.

After sunset,civil twilight sets in and ends when the Sun drops more than 6° below the horizon. This is then followed bynautical twilight, when the Sun reaches heights of −6° and −12°, after which comesastronomical twilight defined as the period from −12° to −18°. When the Sun drops more than 18° below the horizon, the sky generally attains its minimum brightness.

Several sources can be identified as the source of the intrinsic brightness of the sky, namelyairglow, indirect scattering of sunlight, scattering of starlight, and artificiallight pollution.

Visual presentation

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Paranal Observatory nights.[3] The concept ofnoctcaelador tackles the aesthetic perception of the night sky.[4]

Depending on local sky cloud cover, pollution, humidity, and light pollution levels, the stars visible to the unaided naked eye appear as hundreds, thousands or tens of thousands of white pinpoints of light in an otherwise near black sky together with some faint nebulae or clouds of light.[5] In ancient times the stars were often assumed to be equidistant on a dome above the Earth because they are much too far away forstereopsis to offer any depth cues. Visible stars range in color from blue (hot) to red (cold), but with such small points of faint light, most look white because they stimulate therod cells without triggering thecone cells. If it is particularly dark and a particularly faint celestial object is of interest,averted vision may be helpful.

The stars of the night sky cannot be counted unaided because they are so numerous and there is no way to track which have been counted and which have not. Further complicating the count, fainter stars may appear and disappear depending on exactly where the observer is looking. The result is an impression of an extraordinarily vast star field.

Becausestargazing is best done from a dark place away from city lights, darkadaptation is important to achieve and maintain. It takes several minutes for eyes to adjust to the darkness necessary for seeing the most stars, and surroundings on the ground are hard to discern. A redflashlight can be used to illuminate star charts and telescope parts without undoing the dark adaptation.

Video of the night sky taken withDSLR cameras in Japan

Constellations

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Star charts are produced to aid stargazers in identifying constellations and other celestial objects. Constellations are prominent because their stars tend to be brighter than other nearby stars in the sky. Different cultures have created different groupings of constellations based on differing interpretations of the more-or-less random patterns of dots in the sky. Constellations were identified without regard to distance to each star, but instead as if they were all dots on a dome.

Orion is among the most prominent and recognizable constellations.[6] TheBig Dipper (which has a wide variety of other names) is helpful for navigation in the northern hemisphere because it points toPolaris, the north star.

Thepole stars are special because they are approximately in line with the Earth's axis of rotation so they appear to stay in one place while the other stars rotate around them through the course of a night (or a year).

Planets

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Planets, named for theGreek word for 'wanderer', process through the starfield a little each day, executing loops with time scales dependent on the length of the planet's year or orbital period around the Sun. Planets, to the naked eye, appear as points of light in the sky with variable brightness. Planets shine due to sunlight reflecting or scattering from the planets' surface or atmosphere. Thus, the relative Sun-planet-Earth positions determine the planet's brightness. With a telescope or good binoculars, the planets appear as discs demonstrating finite size, and it is possible to observe orbiting moons which cast shadows onto the host planet's surface.Venus is the most prominent planet, often called the "morning star" or "evening star" because it is brighter than the stars and often the only "star" visible near sunrise or sunset, depending on its location in its orbit. Because of its brightness, Venus can sometimes be seen after sunrise.Mercury,Mars,Jupiter andSaturn are also visible to the naked eye in the night sky.

The Moon

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TheMoon appears as a grey disc in the sky with cratering visible to the naked eye. It spans, depending on its exact location, 29–33arcminutes – which is about the size of a thumbnail at arm's length, and is readily identified. Over 29.53 days on average, the moon goes through a full cycle oflunar phases. People can generally identify phases within a few days by looking at the Moon. Unlike stars and most planets, the light reflected from the Moon is bright enough to be seen during the day.

Some of the most spectacular moons come during the full moon phase near sunset or sunrise. The Moon on the horizon benefits from theMoon illusion which makes it appear larger. The Sun's light reflected from the Moon traveling through the atmosphere also appears to color the Moon orange and/or red.

Comets

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Comets come to the night sky only rarely. Comets are illuminated by the Sun, and their tails extend away from the Sun. A comet with a visible tail is quite unusual – agreat comet appears about once a decade. They tend to be visible only shortly before sunrise or after sunset because those are the times they are close enough to the Sun to show a tail.

Clouds

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Clouds obscure the view of other objects in the sky, though varying thicknesses of cloud cover have differing effects. A very thincirrus cloud in front of the moon might produce arainbow-colored ring around the moon. Stars and planets are too small or dim to take on this effect and are instead only dimmed (often to the point of invisibility). Thicker cloud cover obscures celestial objects entirely, making the sky black or reflecting city lights back down. Clouds are often close enough to afford some depth perception, though they are hard to see without moonlight or light pollution.

Other objects

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TheMilky Way contains billions of stars, arranged in two strikingly different structures:halo anddisc.[7]

On clear dark nights in unpolluted areas, when the Moon appears thin or below the horizon, the Milky Way, a band of what looks like white dust, can be seen.

TheMagellanic Clouds of the southern sky are easily mistaken to be Earth-based clouds (hence the name) but are in fact collections of stars found outside the Milky Way known asdwarf galaxies.

Zodiacal light is a glow that appears near the points where the Sun rises and sets, and is caused by sunlight interacting withinterplanetary dust.

Gegenschein is a faint bright spot in the night sky centered at theantisolar point, caused by thebackscatter of sunlight byinterplanetary dust.

Shortly after sunset and before sunrise, artificial satellites often look like stars – similar in brightness and size – but move relatively quickly. Those that fly inlow Earth orbit cross the sky in a couple of minutes. Some satellites, includingspace debris, appear to blink or have a periodic fluctuation in brightness because they are rotating.Satellite flares can appear brighter than Venus, with notable examples including theInternational Space Station (ISS) andIridium Satellites.

Meteors streak across the sky infrequently. During ameteor shower, they may average one a minute at irregular intervals, but otherwise their appearance is a random surprise. The occasional meteor will make a bright, fleeting streak across the sky, and they can be very bright in comparison to the night sky.

Aircraft are also visible at night, distinguishable at a distance from other objects because their navigation lights blink.

Sky map

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Main article:Starchart

Future and past

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Main articles:Fixed star § "Fixed stars" not fixed,Variable star, andAstronomical chronology

Beside the Solar System objects changing in the course of them and Earth orbiting and changing orbits over time around the Sun and in the case of the Moon around Earth, appearing over time smaller by expanding its orbit, the night sky also changes over the course of the years with stars having aproper motion and changing brightness because of beingvariable stars, by the distance to them getting larger or other celestial events likesupernovas.

Overa timescale of tens of billions of years the night sky in theLocal Group will significantly change when thecoalescence of the Andromeda Galaxy and the Milky Way merge into a single elliptical galaxy.

This series of photo illustrations shows the predicted merger between the Milky Way and the neighboringAndromeda Galaxy.

See also

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References

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  1. ^Yukon, Northwestel."Aurora Borealis Explained". Northern Lights Centre. Archived fromthe original on 2019-09-27. Retrieved2015-02-28.
  2. ^"Starry Night at La Silla".ESO Picture of the Week. Retrieved20 August 2013.
  3. ^"Paranal Nights".ESO Picture of the Week. Retrieved7 January 2014.
  4. ^Kelly, William E.; Daughtry, Don (22 December 2007)."Academic Orientation, Academic Achievement, and Noctcaelador: Does Interest in Night-Sky Watching Correlate with Students' Approach to the Academic Environment?".Education.128 (2): 274. Archived fromthe original on 12 August 2014.
  5. ^Hawley."Number of Stars in the Sky".Newton Ask A Scientist. US Department of Energy. RetrievedOctober 23, 2010.
  6. ^Dolan, Chris."Orion". Archived fromthe original on 2011-12-07. Retrieved2007-10-05.
  7. ^"Where Heaven and Earth Collide".www.eso.org. Retrieved29 August 2016.

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