|Pronunciation||//, genitive //|
|Area||334 sq. deg. (46th)|
|Stars with planets||5|
|Stars brighter than 3.00m||3|
|Stars within 10.00 pc (32.62 ly)||1|
|Brightest star||α Lup (Men) (2.30m)|
|Nearest star||LHS 397
(19.35 ly, 5.93 pc)
|Visible at latitudes between +35° and −90°.
Best visible at 21:00 (9 p.m.) during the month of June.
Lupus // is a constellation in the southern sky. Its name is Latin for wolf. Lupus was one of the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations. It lies between Centaurus and Scorpius.
Lupus has around 30 stars of 2nd and 3rd magnitude and 70 of greater than 6th, including a number of binary or multiple stars. In his book Star Names and Their Meanings, R.H. Allen gave the names Yang Mun for α Lupi, the brightest star in Lupus, and KeKwan for the blue giant β Lupi, both from Chinese. However, the first name is in error; both stars were part of a large Chinese constellation known in modern transliteration as Qíguān, the Imperial Guards.
Towards the north of the constellation are globular clusters NGC 5824 and NGC 5986, and close by the dark nebula B 228. To the south are two open clusters, NGC 5822 and NGC 5749, as well as globular cluster NGC 5927 on the eastern border with Norma. On the western border are two spiral galaxies and the Wolf-Rayet planetary nebula IC 4406, containing some of the hottest stars in existence. IC 4406, also called the Retina Nebula, is a cylindrical nebula at a distance of 5,000 light-years. It has dust lanes throughout its center. Another planetary nebula, NGC 5882, is towards the centre of the constellation. The transiting exoplanet Lupus-TR-3b lies in this constellation. The historic supernova SN 1006 is described by various sources as appearing on April 30 to May 1, 1006, in the constellation of Lupus.
ESO 274-1 is a spiral galaxy seen from edge-on that requires an amateur telescope with at least 12 inches of aperture to view. It can be found by using Lambda Lupi and Mu Lupi as markers, and can only be seen under very dark skies. It is 9 arcminutes by 0.7 arcminutes with a small, elliptical nucleus.
Mythology and history
In ancient times, the constellation was considered an asterism within Centaurus, and was considered to have been an arbitrary animal, killed, or about to be killed, on behalf of, or for, Centaurus. An alternative visualization, attested by Eratosthenes, saw this constellation as a wineskin held by Centaurus. It was not separated from Centaurus until Hipparchus of Bithynia named it Therion (meaning beast) in the 200s BC. No particular animal was associated with it until the Latin translation of Ptolemy's work identified it with the wolf.
The Greek constellation is probably based on the Babylonian figure known as the Mad Dog (UR.IDIM). This was a strange hybrid creature that combined the head and torso of a man with the legs and tail of a lion (the cuneiform sign 'UR' simply refers to a large carnivore; lions, wolves and dogs are all included). It is often found in association with the sun god and another mythical being called the Bison-man, which is supposedly related to the Greek constellation of Centaurus.
- Allen, R. H. (1899). Star-names and Their Meanings. New York: G. E. Stechart. p. 279.
- Preibisch, T., Mamajek, E.; Mamajek (2008). "The Nearest OB Association: Scorpius-Centaurus (Sco OB2)". Handbook of Star-Forming Regions 2: 0. arXiv:0809.0407. Bibcode:2008hsf2.book..235P.
- Wilkins, Jamie; Dunn, Robert (2006). 300 Astronomical Objects: A Visual Reference to the Universe (1st ed.). Buffalo, New York: Firefly Books. ISBN 978-1-55407-175-3.
- Dalrymple 2013, p. 41.
- Mark R. Chartrand III (1983) Skyguide: A Field Guide for Amateur Astronomers, p. 160 (ISBN 0-307-13667-1).
- Chartrand, p. 172.
- Babylonian Star-lore by Gavin White, Solaria Pubs, 2008, page 145 & 59ff
- Dalrymple, Les (May 2013). "Exploring the M83 Galaxy Group". Sky & Telescope.
- Ian Ridpath and Wil Tirion (2007). Stars and Planets Guide, Collins, London. ISBN 978-0-00-725120-9. Princeton University Press, Princeton. ISBN 978-0-691-13556-4.
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