Stella Ludoviciana: Difference between revisions
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The name was made popular with its mention in Allen (1899)<ref name=":0" />. | The name was made popular with its mention in Allen (1899)<ref name=":0" />. | ||
The star was observed on 2 December 1722 by the German theologian and scientist Johann Georg Liebknecht ( | The star was observed on 2 December 1722 by the German theologian and scientist Johann Georg Liebknecht (1679–1749). He thought he observed relative motion (proper motion) to the neighbouring stars, Mizar and Alcor, and, therefore, mistook it for a planet. Subsequently, he named it after Louis V, Landgrave of Hesse-Darmstadt. Unknown to Liebknecht, it had been previously observed by the Italian mathematician and Benedictine monk Benedetto Castelli (1578–1643) in 1616.<ref>Siebert, Harald (2005). "The early search for stellar parallax: Galileo, Castelli, and Ramponi". [[wikipedia:Journal_for_the_History_of_Astronomy|Journal for the History of Astronomy]]. 36 (3): 251–271. Bibcode:[https://ui.adsabs.harvard.edu/abs/2005JHA....36..251S 2005JHA....36..251S]. [https://doi.org/10.1177%2F002182860503600301 doi:10.1177/002182860503600301]</ref> | ||
==Mythology== | ==Mythology== | ||
==IAU Working Group on Star Names== | ==IAU Working Group on Star Names== | ||
The name was | The name was approved by the IAU WGSN in 2026, following a suggestion by the SIMBAD team. | ||
The star [https://simbad.cds.unistra.fr/simbad/sim-id?Ident=HD+116798 HD 116798] is a white (A-type) giant star with apparent V magnitude 7.59, and lies 92 parsecs away. The star rotates rapidly (rotation period is only 8 hours) and it is a member of Latyshev 2 stellar group (also called Coma Berenices Neighbor Moving Group or [TPY2019] Group-X) ([https://ui.adsabs.harvard.edu/abs/2022AJ....164..115N/abstract Newton et al. 2022], [https://ui.adsabs.harvard.edu/search/p_=0&q=identifier%3A(2022A%26A...657L...3M) Messina et al. 2022]). | The star [https://simbad.cds.unistra.fr/simbad/sim-id?Ident=HD+116798 HD 116798] is a white (A-type) giant star with apparent V magnitude 7.59, and lies 92 parsecs away. The star rotates rapidly (rotation period is only 8 hours) and it is a member of Latyshev 2 stellar group (also called Coma Berenices Neighbor Moving Group or [TPY2019] Group-X) ([https://ui.adsabs.harvard.edu/abs/2022AJ....164..115N/abstract Newton et al. 2022], [https://ui.adsabs.harvard.edu/search/p_=0&q=identifier%3A(2022A%26A...657L...3M) Messina et al. 2022]). | ||
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== Reference == | == Reference == | ||
* [[References|References (general)]] | * [[References|References (general)]] | ||
[[Category:Star Name]] | [[Category:Star Name]] [[Category:Asterism]] | ||
[[Category:Eurasia]] | [[Category:Eurasia]] | ||
[[Category:Modern]] | [[Category:Modern]] [[Category:Latin]] [[Category:European]] [[Category:UMa]] | ||
Latest revision as of 21:05, 23 July 2026
Authors: Susanne M Hoffmann, Eric Mamajek, Youla Azkarrula
Stella Ludoviciana is a modern star name for HD 116798 (Vmag=7.58) adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is modern Latin. It is the name of a faint star between Alcor and Mizar in constellation Ursa Major.
Concordance, Etymology, History
Variants:
The name was made popular with its mention in Allen (1899)[1].
The star was observed on 2 December 1722 by the German theologian and scientist Johann Georg Liebknecht (1679–1749). He thought he observed relative motion (proper motion) to the neighbouring stars, Mizar and Alcor, and, therefore, mistook it for a planet. Subsequently, he named it after Louis V, Landgrave of Hesse-Darmstadt. Unknown to Liebknecht, it had been previously observed by the Italian mathematician and Benedictine monk Benedetto Castelli (1578–1643) in 1616.[3]
Mythology
IAU Working Group on Star Names
The name was approved by the IAU WGSN in 2026, following a suggestion by the SIMBAD team.
The star HD 116798 is a white (A-type) giant star with apparent V magnitude 7.59, and lies 92 parsecs away. The star rotates rapidly (rotation period is only 8 hours) and it is a member of Latyshev 2 stellar group (also called Coma Berenices Neighbor Moving Group or [TPY2019] Group-X) (Newton et al. 2022, Messina et al. 2022).
Weblinks
Reference
- ↑ 1.0 1.1 Allen, Richard Hinckley (1899). Star Names - Their Lore and Meaning. Dover Publications, Inc., New York
- ↑ J. Kelly Beatty (2009). "The Big Dipper Adds a Star". Sky & Telescope. 2009-12-11
- ↑ Siebert, Harald (2005). "The early search for stellar parallax: Galileo, Castelli, and Ramponi". Journal for the History of Astronomy. 36 (3): 251–271. Bibcode:2005JHA....36..251S. doi:10.1177/002182860503600301
