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Honores Friderici

From Wikipedia, the free encyclopedia
Former constellation
Gloria Frederici is seen above and to the left ofAndromeda in this 1825 star chart fromUrania's Mirror.

Honores Friderici orFrederici Honores, (Latin, "the Honours, orRegalia, of Frederic") also calledGloria Frederica orFrederici ("Glory of Frederick") was aconstellation created byJohann Bode in 1787 to honorFrederick the Great, the king ofPrussia who had died in the previous year. It was between the constellations ofCepheus,Andromeda,Cassiopeia andCygnus. Its most important stars wereIota (Rasalnaqa),Kappa (Kaffalmusalsala),Lambda (Udkadua),Omicron (Alfarasalkamil), andPsi Andromedae. The constellation is no longer in use.

History

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Johann Bode first introduced the constellation in his 1787 publicationAstronomisches Jahrbuch, calling itFriedrichs Ehre, to honourFrederick the Great, who had just died the previous year. He latinized its name to Honores Friderici in his 1801 workUranographia.[1]He illustrated it as a crown above a sword, pen and olive branch, based on his perception of Frederick as a "hero, sage and peacemaker".[2]

The constellation was taken up by some cartographers and not by others, but was increasingly ignored from the latter half of the 19th century,[2] and is no longer in use. Most of it lies within the borders of modern Andromeda, with parts in Cassiopeia, Cepheus and Pegasus.[1]

Stars

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Bode incorporated 76 stars into his new constellation, made up of 26 from Andromeda, 9 from Lacerta, 6 from Cepheus, 5 from Pegasus, and 3 from Cassiopeia.[2] The three brightest stars—all of magnitude 4—that lay within its borders are Omicron, Lambda, and Kappa Andromedae.[1] With an apparent magnitude of 3.62,Omicron Andromedae is a multiple star system, the brightest star of which is a blue-white subgiant of spectral type B6 IIIpe and its visible companion a white star of spectral type A2. Each appears to have a close companion, making it a quadruple system.[3] It is approximately 690light-years from Earth.[4]Lambda Andromedae is a yellow subgiant star of spectral type G8IVk around 1.3 times as massive as the Sun that has used up its core hydrogen and expanded to around 7 times its diameter.[5] It is a spectroscopic binary composed of two stars close together orbiting each other every 20 days, the brighter component aRS Canum Venaticorum variable.[6]Kappa Andromedae is a blue white star of apparent magnitude 4.14, that was found to have a substellar companion by direct imaging in 2012. Initially thought to be a planet, it is now thought to be abrown dwarf around 22 times as massive as Jupiter.[7]

Iota andPsi Andromedae make up theasterism. Shining at magnitude 4.29, Iota Andromedae is a blue-white main sequence star of spectral type B8V around 500 light-years distant from Earth.[4]

TheIAU Working Group on Star Names approved the name Honores for the star7 Andromedae in 2025, after the obsolete constellation. This star was chosen for the name because it was in the feather part of the constellation, in reference to the proverb "the feather is mightier than the sword". The constellation's brightest star, Omicron Andromedae, was named Alfarasalkamil after an older Arabic constellation.[8]

See also

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References

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  1. ^abcRidpath, Ian."Honores Friderici".Star Tales. self-published. Retrieved29 January 2017.
  2. ^abcBarentine, John C. (2015).The Lost Constellations: A History of Obsolete, Extinct, or Forgotten Star Lore. New York: Springer. pp. 177–98.ISBN 9783319227955.
  3. ^Olević, D.; Cvetković, Z. (March 2006)."Dynamical Masses of the Components in o Andromedae".The Astronomical Journal.131 (3):1721–1723.Bibcode:2006AJ....131.1721O.doi:10.1086/499539.
  4. ^abvan Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction".Astronomy and Astrophysics.474 (2):653–64.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.
  5. ^Drake, Jeremy J.; Ball, B.; Eldridge, John J.; Ness, J.-U.; Stancliffe, Richard J. (November 2011). "Close to the dredge: precise X-Ray C and N abundances in λ Andromeda and its precocious red giant branch mixing problem".The Astronomical Journal.142 (5): 144.arXiv:1109.3663.Bibcode:2011AJ....142..144D.doi:10.1088/0004-6256/142/5/144.S2CID 118271341.
  6. ^Frasca, A.; Biazzo, K.; Taş, G.; Evren, S.; Lanzafame, A. C. (February 2008). "Spots, plages, and flares on λ Andromedae and II Pegasi".Astronomy and Astrophysics.479 (2):557–565.arXiv:0711.3322.Bibcode:2008A&A...479..557F.doi:10.1051/0004-6361:20077915.S2CID 8049649.
  7. ^Jones, Jeremy; White, R. J.; Quinn, S.; Ireland, M.; Boyajian, T.; Schaefer, G.; Baines, E. K. (2016)."The Age of the Directly Imaged Planet Host Star κ Andromedae Determined from Interferometric Observations".The Astrophysical Journal Letters.822 (1): 7.arXiv:1604.02176.Bibcode:2016ApJ...822L...3J.doi:10.3847/2041-8205/822/1/L3.S2CID 38367518.
  8. ^"IAU Catalog of Star Names". Retrieved14 May 2025.


Constellation history
48 constellations listed byPtolemy after 150 AD
The 41 additional constellations added in the 16th, 17th and 18th centuries
Obsolete constellations (including Ptolemy's Argo Navis)
  • obsolete constellation names
Retrieved from "https://en.wikipedia.org/w/index.php?title=Honores_Friderici&oldid=1322660719"
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