Corona Australis
Constellation | |
Abbreviation | CrA |
---|---|
Genitive |
|
Pronunciation | Corona Australids |
Bordering constellations | |
Visible at latitudes between +40° and −90°. Best visible at 21:00 (9 p.m.) during the month of August. |
Corona Australis is a
Although fainter than its northern counterpart, the oval- or horseshoe-shaped pattern of its brighter stars renders it distinctive.
Name
The name of the constellation was entered as "Corona Australis" when the International Astronomical Union (IAU) established the 88 modern constellations in 1922.[5][6] In 1932, the name was instead recorded as "Corona Austrina" when the IAU's commission on notation approved a list of four-letter abbreviations for the constellations.[7] The four-letter abbreviations were repealed in 1955.[8] The IAU presently uses "Corona Australis" exclusively.[4]
Characteristics
Corona Australis is a small constellation bordered by Sagittarius to the north, Scorpius to the west, Telescopium to the south, and Ara to the southwest. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is "CrA".[9] The official constellation boundaries, as set by Belgian astronomer Eugène Delporte in 1930, are defined by a polygon of four segments (illustrated in infobox). In the equatorial coordinate system, the right ascension coordinates of these borders lie between 17h 58.3m and 19h 19.0m , while the declination coordinates are between −36.77° and −45.52°.[4] Covering 128 square degrees, Corona Australis culminates at midnight around the 30th of June[10] and ranks 80th in area.[11] Only visible at latitudes south of 53° north,[11] Corona Australis cannot be seen from the British Isles as it lies too far south,[12] but it can be seen from southern Europe[13] and readily from the southern United States.[14]
Features
While not a bright constellation, Corona Australis is nonetheless distinctive due to its easily identifiable pattern of stars,
Stars
The only star in the constellation to have received a name is
Some of the more prominent double stars include
Corona Australis Molecular Cloud
The Corona Australis Molecular Cloud is a dark molecular cloud just north of Beta Coronae Australis. Illuminated by a number of embedded reflection nebulae[25] the cloud fans out from Epsilon Coronae Australis eastward along the constellation border with Sagittarius. It contains 7000 M☉,[25] Herbig–Haro objects (protostars) and some very young stars,[41] being one of the closest star-forming regions, 430 light years (130 parsecs) to the Solar System,[42] at the surface of the Local Bubble. The first nebulae of the cloud were recorded in 1865 by Johann Friedrich Julius Schmidt.[43]
Between Epsilon and
Nearby north, another young variable star, TY Coronae Australis, illuminates another nebula: reflection nebula NGC 6726/NGC 6727. TY Coronae Australis ranges irregularly between magnitudes 8.7 and 12.4, and the brightness of the nebula varies with it.[46] Blue-white, it is of spectral type B8e.[49] The largest young stars in the region, R, S, T, TY and VV Coronae Australis, are all ejecting jets of material which cause surrounding dust and gas to coalesce and form Herbig–Haro objects, many of which have been identified nearby.[50]
Not part of it is the globular cluster known as NGC 6723, which can be seen adjacent to the nebulosity in the neighbouring constellation of Sagittarius, but is much much further away.[51]
Deep sky objects
IC 1297 is a planetary nebula of apparent magnitude 10.7, which appears as a green-hued roundish object in higher-powered amateur instruments.[52] The nebula surrounds the variable star RU Coronae Australis, which has an average apparent magnitude of 12.9[53] and is a WC class Wolf–Rayet star.[54] IC 1297 is small, at only 7 arcseconds in diameter; it has been described as "a square with rounded edges" in the eyepiece, elongated in the north–south direction.[55] Descriptions of its color encompass blue, blue-tinged green, and green-tinged blue.[55]
Corona Australis' location near the Milky Way means that galaxies are uncommonly seen. NGC 6768 is a magnitude 11.2 object 35′ south of IC 1297. It is made up of two galaxies merging,[33] one of which is an elongated elliptical galaxy of classification E4 and the other a lenticular galaxy of classification S0.[56] IC 4808 is a galaxy of apparent magnitude 12.9 located on the border of Corona Australis with the neighbouring constellation of Telescopium and 3.9 degrees west-southwest of Beta Sagittarii. However, amateur telescopes will only show a suggestion of its spiral structure. It is 1.9 arcminutes by 0.8 arcminutes. The central area of the galaxy does appear brighter in an amateur instrument, which shows it to be tilted northeast–southwest.[57]
Southeast of Theta and southwest of Eta lies the open cluster ESO 281-SC24, which is composed of the yellow 9th magnitude star GSC 7914 178 1 and five 10th to 11th magnitude stars.[33] Halfway between Theta Coronae Australis and Theta Scorpii is the dense globular cluster NGC 6541. Described as between magnitude 6.3[46] and magnitude 6.6,[26] it is visible in binoculars and small telescopes. Around 22000 light years away, it is around 100 light years in diameter.[46] It is estimated to be around 14 billion years old.[58] NGC 6541 appears 13.1 arcminutes in diameter and is somewhat resolvable in large amateur instruments; a 12-inch telescope reveals approximately 100 stars but the core remains unresolved.[59]
Meteor showers
The
History
Corona Australis may have been recorded by ancient
In the 3rd century BC, the Greek didactic poet Aratus wrote of, but did not name the constellation,[68] instead calling the two crowns Στεφάνοι (Stephanoi). The Greek astronomer Ptolemy described the constellation in the 2nd century AD, though with the inclusion of Alpha Telescopii, since transferred to Telescopium.[69] Ascribing 13 stars to the constellation,[10] he named it Στεφάνος νοτιος (Stephanos notios), "Southern Wreath", while other authors associated it with either Sagittarius (having fallen off his head) or Centaurus; with the former, it was called Corona Sagittarii.[70] Similarly, the Romans called Corona Australis the "Golden Crown of Sagittarius".[71] It was known as Parvum Coelum ("Canopy", "Little Sky") in the 5th century.[72] The 18th-century French astronomer Jérôme Lalande gave it the names Sertum Australe ("Southern Garland")[70][72] and Orbiculus Capitis, while German poet and author Philippus Caesius called it Corolla ("Little Crown") or Spira Australis ("Southern Coil"), and linked it with the Crown of Eternal Life from the New Testament. Seventeenth-century celestial cartographer Julius Schiller linked it to the Diadem of Solomon.[70] Sometimes, Corona Australis was not the wreath of Sagittarius but arrows held in his hand.[72]
Corona Australis has been associated with the myth of
In
The ǀXam speaking San people of South Africa knew the constellation as ≠nabbe ta !nu "house of branches"—owned originally by the Dassie (rock hyrax), and the star pattern depicting people sitting in a semicircle around a fire.[76]
The indigenous
See also
- Corona Australis (Chinese astronomy)
- Chamaeleon complex
References
Citations
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- ^ "Corona". Merriam-Webster.com Dictionary., "Australis". Merriam-Webster.com Dictionary..
- ^ "Corona Australis". Dictionary.com Unabridged (Online). n.d.
- ^ a b c d IAU, The Constellations, Corona Australis.
- ^ Proceedings of the 1st General Assembly. Transactions of the International Astronomical Union. Vol. 1. Rome. 1922. p. 158.
- ^ Ridpath, Ian. "IAU constellation list 1". Retrieved 2017-01-06.
- .
- ^ Ridpath, Ian. "IAU constellation list 2". Retrieved 2017-01-06.
- ^ Russell 1922, p. 469.
- ^ a b c Malin & Frew 1995, p. 218
- ^ a b Ridpath, Constellations.
- ^ Moore & Tirion 1997, p. 164
- ^ Moore 2005, p. 202
- ^ Moore, Stargazing 2000, p. 86
- ^ a b c d e Ridpath & Tirion 2017, pp. 126–127.
- ^ Falkner 2011, p. 100
- ^ Bakich 1995, p. 130.
- ^ SIMBAD Mu Coronae Australis.
- ^ Wagman 2003, pp. 114–115.
- ^ Allen 1963, pp. 172–173.
- ^ a b c Kaler, Alfecca Meridiana.
- ^ SIMBAD Alpha Coronae Australis.
- ^ Royer, Zorec & Gómez 2007, p. 463.
- ^ SIMBAD Beta Coronae Australis.
- ^ a b c d Kaler, Beta Coronae Australis.
- ^ a b c d Moore & Rees 2011, p. 413.
- ^ SIMBAD LTT 7565.
- ^ SIMBAD HR 7226.
- ^ SIMBAD HR 7227.
- ^ Kaler, Epsilon Coronae Australis.
- ^ SIMBAD Epsilon Coronae Australis.
- ^ a b c Motz & Nathanson 1991, pp. 254–255.
- ^ a b c d Streicher 2008, pp. 135–139.
- ^ SIMBAD HR 6953.
- ^ SIMBAD HR 6952.
- ^ SIMBAD Lambda Coronae Australis.
- ^ SIMBAD Zeta Coronae Australis.
- ^ SIMBAD Theta Coronae Australis.
- ^ a b Ho Wynn C. G. et al. 2007.
- ^ Drake, Jeremy J. et al. 2002.
- ^ a b Malin 2010.
- ^ Reipurth 2008, p. 735.
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- ^ a b c d e O'Meara 2002, pp. 164–165, 271–273, 311
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- ^ SIMBAD RU Coronae Australis.
- ^ a b Bakich 2010, p. 270.
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- ^ Bakich Podcast & 18 August 2011.
- ^ O'Meara 2011, p. 322
- ^ Bakich Podcast & 5 July 2012.
- ^ Sherrod & Koed 2003, p. 50
- ^ Weiss 1957, p. 300.
- ^ a b Rogers & Keay 1993, p. 274.
- ^ Weiss 1957, p. 302.
- ^ a b Ellyett & Keay 1956, p. 479.
- ^ Jenniskens 1994, p. 1007.
- ^ Jopek et al. 2010, p. 871–872.
- ^ Rogers 1998, p. 19.
- ^ Bakich 1995, p. 83.
- ^ Ridpath, Star Tales Corona Australis.
- ^ a b c d e Allen 1963, pp. 172–174.
- ^ Simpson 2012, p. 148.
- ^ a b c d Motz & Nathanson 1988, p. 254.
- ^ Staal 1988, pp. 232–233.
- ^ AEEA 2006.
- ^ Porter1996, pp. 35–36
- ^ Lloyd 1873.
- ^ Hamacher & Frew 2010.
- ^ Hamacher & 28 March 2011.
- ^ Staal 1988, pp. 223–224.
- ^ Makemson 1941, p. 281.
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- "Alpha Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 3 July 2012.
- "Beta Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 3 July 2012.
- "LTT 7565 (Gamma Coronae Australis)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 3 July 2012.
- "HR 7226 (Gamma Coronae Australis A)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 3 July 2012.
- "HR 7227 (Gamma Coronae Australis B)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 3 July 2012.
- "Epsilon Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 5 July 2012.
- "HR 6953 (Kappa² Coronae Australis)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 17 August 2012.
- "HR 6952 (Kappa¹ Coronae Australis)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 17 August 2012.
- "Lambda Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 21 July 2012.
- "HR 7050 (Mu Coronae Australis)". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 8 September 2012.
- "Zeta Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 9 July 2012.
- "Theta Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 15 August 2012.
- "R Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 4 July 2012.
- "TY Coronae Australis". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 6 July 2012.
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External links
- The Deep Photographic Guide to the Constellations: Corona Australis
- Warburg Institute Iconographic Database (medieval and early modern images of Corona Australis)