Gienah

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Gienah was the traditional name of two stars, each marking a wing (Arabic al janāħ) of its constellation:

Arabic Central Semitic language

Arabic is a Central Semitic language that first emerged in Iron Age northwestern Arabia and is now the lingua franca of the Arab world. It is named after the Arabs, a term initially used to describe peoples living in the area bounded by Mesopotamia in the east and the Anti-Lebanon mountains in the west, in northwestern Arabia, and in the Sinai Peninsula. Arabic is classified as a macrolanguage comprising 30 modern varieties, including its standard form, Modern Standard Arabic, which is derived from Classical Arabic.

Constellation one of the 88 divisions of the celestial sphere, defined by the IAU, many of which derive from traditional asterisms

A constellation is a group of stars that forms an imaginary outline or pattern on the celestial sphere, typically representing an animal, mythological person or creature, a god, or an inanimate object.

Gamma Corvi star in the southern constellation of Corvus

Gamma Corvi is a binary star and the brightest star in the southern constellation of Corvus, having an apparent visual magnitude of 2.59. The system's two components are designated Gamma Corvi A and Gamma Corvi B. The distance to this system has been measured directly using the parallax technique, yielding an estimated 154 light-years from the Sun.

Corvus (constellation) constellation in the Southern Celestial Hemisphere

Corvus is a small constellation in the Southern Celestial Hemisphere. Its name means "raven" in Latin. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it depicts a raven, a bird associated with stories about the god Apollo, perched on the back of Hydra the water snake. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi, form a distinctive quadrilateral in the night sky.

Epsilon Cygni star in the constellation Cygnus

Epsilon Cygni is multiple star system in the constellation of Cygnus. With an apparent visual magnitude of 2.48, it is readily visible to the naked eye at night as one of the brighter members of Cygnus. Based upon parallax measurement, Epsilon Cygni is about 73 light-years from the Sun.

The International Astronomical Union approved the name Gienah for Gamma Corvi A in 2016 and Aljanah for Epsilon Cygni Aa in 2017. [1]

International Astronomical Union Association of professional astronomers

The International Astronomical Union is an international association of professional astronomers, at the PhD level and beyond, active in professional research and education in astronomy. Among other activities, it acts as the internationally recognized authority for assigning designations and names to celestial bodies and any surface features on them.

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A Bayer designation is a stellar designation in which a specific star is identified by a Greek or Latin letter followed by the genitive form of its parent constellation's Latin name. The original list of Bayer designations contained 1,564 stars.

Cygnus (constellation) constellation

Cygnus is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan. Cygnus is one of the most recognizable constellations of the northern summer and autumn, and it features a prominent asterism known as the Northern Cross. Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.

Albireo star in the constellation Cygnus

Albireo is the traditional name for the double star also designated Beta Cygni, although the International Astronomical Union now regards the name as only applying to the brightest component. Although designated 'beta', it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni and is the fifth-brightest point of light in the constellation of Cygnus. Appearing to the naked eye to be a single star of magnitude 3, viewing through even a low-magnification telescope resolves it into its two components. The brighter yellow star makes a striking colour contrast with its fainter blue companion.

Gamma Cygni star in the northern constellation Cygnus

Gamma Cygni, also named Sadr, is a star in the northern constellation of Cygnus, forming the intersection of an asterism of five stars called the Northern Cross. Based upon parallax measurements obtained during the Hipparcos mission, it is approximately 1,800 light-years (560 parsecs) from the Sun.

K-type main-sequence star stellar classification

A K-type main-sequence star, also referred to as an K dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars and yellow G-type main-sequence stars. They have masses between 0.5 and 0.8 times the mass of the Sun and surface temperatures between 3,900 and 5,200 K., Tables VII, VIII. Better known examples include Alpha Centauri B and Epsilon Indi.

Delta Corvi binary star in the southern constellation Corvus

Delta Corvi, also named Algorab, is a third magnitude star at a distance of 86.9 light-years from the Sun in the southern constellation of Corvus.

Gamma<sup>2</sup> Sagittarii star

Gamma² Sagittarii, also named Alnasl, is a 3rd-magnitude star in the zodiac constellation of Sagittarius. The location of this star forms the tip of the arrow in the bow of Sagittarius the Centaur. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 96.9 light-years from the Sun. It has an apparent visual magnitude of +2.98, making it the seventh-brightest star in the constellation.

Alpha Corvi, also named Alchiba, is an F-type main-sequence star and the fifth-brightest star in the constellation of Corvus. Based on parallax measurements made during the Hipparcos mission, it is approximately 49 light-years from the Sun.

Pi¹ Cygni is a binary star in the northern constellation of Cygnus. It is visible to the naked eye, having a combined apparent visual magnitude of 4.66. The distance to this system can be roughly gauged by its annual parallax shift of 1.89 mas, which yields a separation of around 1,700 light years from the Sun, give or take a hundred light years.

Epsilon Corvi star in the southern constellation of Corvus

Epsilon Corvi is a star in the southern constellation of Corvus. It has the traditional name Minkar, from Arabic منقارminqar meaning "beak [of the crow]" The apparent visual magnitude is +3.0 and it is located at a distance of 318 light-years from Earth.

Beta Corvi second brightest star in the southern constellation of Corvus

Beta Corvi, also named Kraz, is the second-brightest star in the southern constellation of Corvus with an apparent visual magnitude of 2.647. Based on parallax measurements obtained during the Hipparcos mission, it is about 146 light-years distant from the Sun.

Girl (Chinese constellation) Chinese constellation

The Girl mansion is one of the Twenty-eight mansions of the Chinese constellations. It is one of the northern mansions of the Black Tortoise.

Delta Cygni third-magnitude star in the constellation Cygnus

Delta Cygni is a binary star of a combined third-magnitude in the constellation of Cygnus. It is also part of the Northern Cross asterism whose brightest star is Deneb. Based upon parallax measurements obtained during the Hipparcos mission, Delta Cygni is located roughly 165 light-years distant from the Sun.

Northern Cross (asterism) astronomical asterism in the northern hemisphere celestial sphere

The Northern Cross is a prominent astronomical asterism in the northern hemisphere celestial sphere, corresponding closely with the constellation Cygnus The Swan. It is much larger than the more famous Southern Cross and consists of the brightest stars in Cygnus, Deneb, Sadr, Gienah, Delta Cygni and Albireo. The 'head' of the cross, Deneb, is also part of the Summer Triangle asterism.

This is a list of articles about astronomical locations that exist in real life that have been featured in works of science fiction and fantasy, including planets, asteroids, comets and other star systems.

Corvi may refer to:

NGC 6910 open cluster

NGC 6910 is an open cluster in the constellation Cygnus. It was discovered by William Herschel on October 17, 1786. The cluster was also observed by John Herschel on September 18, 1828. It is a poor cluster and with prominent central concentration, with Trumpler class I2p. NGC 6910 is the core cluster of the stellar association Cygnus OB9.

References

  1. "Naming Stars". IAU.org. Retrieved 16 December 2017.