Southern celestial hemisphere

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A star chart of the entire Southern Sky, centered on the south celestial pole South Hemisphere.png
A star chart of the entire Southern Sky, centered on the south celestial pole

The southern celestial hemisphere, also called the Southern Sky, is the southern half of the celestial sphere; that is, it lies south of the celestial equator. This arbitrary sphere, on which seemingly fixed stars form constellations, appears to rotate westward around a polar axis as the Earth rotates.

Contents

At all times, the entire Southern Sky is visible from the geographic South Pole; less of the Southern Sky is visible the further north the observer is located. The northern counterpart is the northern celestial hemisphere.

Astronomy

Earth rotating within the celestial sphere. In this view, the southern celestial hemisphere is below the celestial equator, the middle parallel (in cyan). Earth within celestial sphere.gif
Earth rotating within the celestial sphere. In this view, the southern celestial hemisphere is below the celestial equator, the middle parallel (in cyan).

In the context of astronomical discussions or writing about celestial mapping, it may also simply then be referred to as the Southern Hemisphere.

For the purpose of celestial mapping, the sky is considered by astronomers as the inside of a sphere divided in two halves by the celestial equator.[ according to whom? ] The Southern Sky or Southern Hemisphere is, therefore, that half of the celestial sphere that is south of the celestial equator. Even if this one is the ideal projection of the terrestrial equatorial onto the imaginary celestial sphere, the Northern and Southern celestial hemispheres should not be confused with descriptions of the terrestrial hemispheres of Earth itself.[ according to whom? ]

Observation

Chart of the southern constellations from declination -40deg to the south celestial pole by the Jesuit missionary Francois Noel published in Acta Eruditorum, 1711. Acta Eruditorum - V astronomia, 1711 - BEIC 13378880.jpg
Chart of the southern constellations from declination –40° to the south celestial pole by the Jesuit missionary François Noël published in Acta Eruditorum , 1711.

From the South Pole, in good visibility conditions, the Southern Sky features over 2,000 fixed stars that are easily visible to the naked eye, while about 20,000 to 40,000 with the aided eye.[ citation needed ][ dubious ] In large cities, about 300 to 500 stars can be seen depending on the extent of light and air pollution.[ citation needed ] The farther north, the fewer are visible to the observer.[ citation needed ]

The brightest star in the night sky is located in the southern celestial hemisphere and is larger than the Sun. Sirius in the constellation of Canis Major has the brightest apparent magnitude of −1.46; it has a radius twice that of the Sun and is 8.6 light-years away. Canopus and the next fixed star α Centauri, 4.2 light-years away, are also located in the Southern Sky, having declinations around −60°; too close to the south celestial pole for either to be visible from Central Europe. [1]

Of the 88 modern constellations, 45 are only visible from the Southern celestial hemisphere. The southern constellations are:[ citation needed ]

History

The first telescopic chart of the Southern Sky was made by the English astronomer Edmond Halley, [2] [3] from the island of St Helena in the South Atlantic Ocean and published by him in 1678. [4]

See also

Related Research Articles

<span class="mw-page-title-main">Carina (constellation)</span> Constellation in the southern celestial hemisphere

Carina is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was the southern foundation of the larger constellation of Argo Navis until it was divided into three pieces, the other two being Puppis, and Vela.

<span class="mw-page-title-main">Declination</span> Astronomical coordinate analogous to latitude

In astronomy, declination is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle. The declination angle is measured north (positive) or south (negative) of the celestial equator, along the hour circle passing through the point in question.

<span class="mw-page-title-main">Lepus (constellation)</span> Constellation in the southern celestial hemisphere

Lepus is a constellation lying just south of the celestial equator. Its name is Latin for hare. It is located below—immediately south—of Orion, and is sometimes represented as a hare being chased by Orion or by Orion's hunting dogs.

<span class="mw-page-title-main">Octans</span> Constellation in the southern celestial hemisphere, containing the south celestial pole

Octans is a faint constellation located in the deep Southern Sky. Its name is Latin for the eighth part of a circle, but it is named after the octant, a navigational instrument. Devised by French astronomer Nicolas Louis de Lacaille in 1752, Octans remains one of the 88 modern constellations. The southern celestial pole is located within the boundaries of Octans.

<span class="mw-page-title-main">Right ascension</span> Astronomical equivalent of longitude

Right ascension is the angular distance of a particular point measured eastward along the celestial equator from the Sun at the March equinox to the point in question above the Earth. When paired with declination, these astronomical coordinates specify the location of a point on the celestial sphere in the equatorial coordinate system.

<span class="mw-page-title-main">Taurus (constellation)</span> Zodiac constellation straddling the celestial equator

Taurus is one of the constellations of the zodiac and is located in the northern celestial hemisphere. Taurus is a large and prominent constellation in the Northern Hemisphere's winter sky. It is one of the oldest constellations, dating back to the Early Bronze Age at least, when it marked the location of the Sun during the spring equinox. Its importance to the agricultural calendar influenced various bull figures in the mythologies of Ancient Sumer, Akkad, Assyria, Babylon, Egypt, Greece, and Rome. Its old astronomical symbol is (♉︎), which resembles a bull's head.

<span class="mw-page-title-main">Celestial sphere</span> Imaginary sphere of arbitrarily large radius, concentric with the observer

In astronomy and navigation, the celestial sphere is an abstract sphere that has an arbitrarily large radius and is concentric to Earth. All objects in the sky can be conceived as being projected upon the inner surface of the celestial sphere, which may be centered on Earth or the observer. If centered on the observer, half of the sphere would resemble a hemispherical screen over the observing location.

<span class="mw-page-title-main">Celestial pole</span> Imaginary sky rotation points

The north and south celestial poles are the two points in the sky where Earth's axis of rotation, indefinitely extended, intersects the celestial sphere. The north and south celestial poles appear permanently directly overhead to observers at Earth's North Pole and South Pole, respectively. As Earth spins on its axis, the two celestial poles remain fixed in the sky, and all other celestial points appear to rotate around them, completing one circuit per day.

<span class="mw-page-title-main">Cancer (constellation)</span> Zodiac constellation in the northern hemisphere

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<span class="mw-page-title-main">Circumpolar star</span> Star that never sets due to its apparent proximity to a celestial pole

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<span class="mw-page-title-main">Celestial equator</span> Projection of Earths equator out into space

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<span class="mw-page-title-main">Orion (constellation)</span> Constellation straddling the celestial equator

Orion is a prominent set of stars visible during winter in the northern celestial hemisphere. It is one of the 88 modern constellations; it was among the 48 constellations listed by the 2nd-century astronomer Ptolemy. It is named for a hunter in Greek mythology.

<span class="mw-page-title-main">Planisphere</span> Class of star chart

In astronomy, a planisphere is a star chart analog computing instrument in the form of two adjustable disks that rotate on a common pivot. It can be adjusted to display the visible stars for any time and date. It is an instrument to assist in learning how to recognize stars and constellations. The astrolabe, an instrument that has its origins in Hellenistic astronomy, is a predecessor of the modern planisphere. The term planisphere contrasts with armillary sphere, where the celestial sphere is represented by a three-dimensional framework of rings.

<span class="mw-page-title-main">Pole star</span> Visible star that is nearly aligned with Earths axis of rotation

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<span class="mw-page-title-main">Spherical astronomy</span> Branch of astronomy about the celestial sphere

Spherical astronomy, or positional astronomy, is a branch of observational astronomy used to locate astronomical objects on the celestial sphere, as seen at a particular date, time, and location on Earth. It relies on the mathematical methods of spherical trigonometry and the measurements of astrometry.

<span class="mw-page-title-main">Winter Hexagon</span> Evening sky asterism with vertices at Rigel, Aldebaran, Capella, Pollux, Procyon, and Sirius

The Winter Hexagon or Winter Circle/Oval is an asterism appearing to be in the form of a hexagon with vertices at Rigel, Aldebaran, Capella, Pollux, Procyon, and Sirius. It is mostly upon the Northern Hemisphere's celestial sphere. On most locations on Earth, this asterism is visible in the evening sky at the equator from approximately December to June, and in the morning sky from July to the end of November, while in the evenings on the northern hemisphere it is less months visible between December and June, and on the southern hemisphere less months between July and November. In the tropics and southern hemisphere, this can be extended with the bright star Canopus in the south.

<span class="mw-page-title-main">Daytime</span> Period of a day in which a location experiences natural illumination

Daytime as observed on Earth is the period of the day during which a given location experiences natural illumination from direct sunlight. Daytime occurs when the Sun appears above the local horizon, that is, anywhere on the globe's hemisphere facing the Sun. In direct sunlight the movement of the sun can be recorded and observed using a sundial that casts a shadow that slowly moves during the day. Other planets and natural satellites that rotate relative to a luminous primary body, such as a local star, also experience daytime, but this article primarily discusses daytime on Earth.

<span class="mw-page-title-main">Constellation family</span> Designated common star constellations

Constellation families are collections of constellations sharing some defining characteristic, such as proximity on the celestial sphere, common historical origin, or common mythological theme. In the Western tradition, most of the northern constellations stem from Ptolemy's list in the Almagest, and most of the far southern constellations were introduced by sailors and astronomers who traveled to the south in the 16th to 18th centuries. Separate traditions arose in India and China.

<span class="mw-page-title-main">Northern celestial hemisphere</span> Northern half of the celestial sphere

The northern celestial hemisphere, also called the Northern Sky, is the northern half of the celestial sphere; that is, it lies north of the celestial equator. This arbitrary sphere appears to rotate westward around a polar axis due to Earth's rotation.

References

  1. David Ellyard, Wil Tirion: The Southern Sky Guide. Cambridge Univ. Press, Cambridge 2009, ISBN   978-0-521-71405-1
  2. "Edmond Halley (1656–1742)". BBC. 2014. Retrieved 2021-07-11.
  3. "Edmond Halley's southern star catalogue" . Retrieved 2023-07-26.
  4. Kanas, Nick (2012). Star Maps: History, Artistry, and Cartography (2nd ed.). Chichester, UK: Springer. p. 123. ISBN   978-1-4614-0917-5.