Quadrans Muralis
Topic: Astronomy
From HandWiki - Reading time: 3 min
Quadrans Muralis (Latin for mural quadrant) was a constellation created by the French astronomer Jérôme Lalande in 1795. It depicted a wall-mounted quadrant with which he and his nephew Michel Lefrançois de Lalande had charted the celestial sphere, and was named Le Mural in the French atlas.[1] It was between the constellations of Boötes and Draco, near the tail of Ursa Major,[2] containing stars between β Bootis (Nekkar) and η Ursae Majoris (Alkaid).[3]
Johann Elert Bode converted its name to Latin as Quadrans Muralis and shrank the constellation a little in his 1801 Uranographia star atlas, to avoid it clashing with neighboring constellations.[1]
In 1922, Quadrans Muralis was omitted when the International Astronomical Union (IAU) formalised its list of officially recognized constellations.[4]
Notable features
- The variable star BP Boötis was a member of the constellation.
- 39 Boötis is a double star that was transferred by Lalande into Quadrans.[5]
- The Quadrantid meteor shower is still named after the obsolete constellation.
References
- ↑ 1.0 1.1 Ridpath, Ian. "Quadrans Muralis". Star Tales. Self-published. http://www.ianridpath.com/startales/quadrans.html.
- ↑ Ridpath, Ian. "Lalande's Quadrans Muralis". Star Tales. Self-published. http://www.ianridpath.com/startales/quadranslalande.html.
- ↑ Inglis, Mike; Moore, Patrick (2015). The Observer's Year: 366 Nights of the Universe: 2015 – 2020. New York, New York: Springer. p. 178. ISBN 978-3-31918-678-8. https://books.google.com/books?id=23uBCgAAQBAJ&pg=PA178.
- ↑ "The Constellations". International Astronomical Union. https://www.iau.org/public/themes/constellations/.
- ↑ Smyth, William Henry (1844). A Cycle of Celestial Objects: For the Use of Naval, Military, and Private Astronomers. 2. London, United Kingdom: John W. Parker. p. 329. https://books.google.com/books?id=HnHvAAAAMAAJ&pg=PA329.
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