Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 References  














HD 224635 and HD 224636






فارسی
Français
Italiano
Slovenščina
Svenska

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


HD 224635/HD 224636
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
HD 224635
Right ascension 23h59m 29.2915s[1]
Declination +33° 43′ 25.8773″[1]
Apparent magnitude (V) 6.46[2]
HD 224636
Right ascension 23h59m 29.2054s[3]
Declination +33° 43′ 27.6539″[3]
Apparent magnitude (V) 6.72[2]
Characteristics
HD 224635
Spectral type F8[4]
B−V color index 0.51[5]
HD 224636
Spectral type G1[4]
B−V color index 0.55[5]
Astrometry
Radial velocity (Rv)−7.90±0.2[6] km/s
Proper motion (μ) RA: −59.68±0.65[7] mas/yr
Dec.: −113.19±0.35[7] mas/yr
Parallax (π)34.57 ± 0.51 mas[7]
Distance94 ± 1 ly
(28.9 ± 0.4 pc)
Details
Mass1.19 + 1.13 [8] M
Luminosity3.47[9] L
Temperature6,072[10] K
Metallicity-0.070[10]
Other designations

BD+32 4747, HIP 118281, SAO 73656, ADS 17149, WDS J23595+3343

HD 224635: HR 9074
HD 224636: HR 9075
Database references
SIMBADdata
Database references
SIMBADdata

HD 224635 and HD 224636 is a pair of stars comprising a binary star system in the constellation Andromeda. They are located approximately 94 light years away[7] and they orbit each other every 717 years.[2]

The primary star is HD 224635, a magnitude 6.46[2] star (making it visible by the naked eye under very favourable conditions) with a spectral type F8[4] that is 1.19 times more massive than the Sun.[8]

The secondary star is the slightly fainter HD 224636, with an apparent visual magnitude of 6.72,[2] a spectral type G1,[4] and 1.13 times more massive than the Sun.[8]

References

[edit]
  1. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this sourceatVizieR.
  • ^ a b c d e Malkov, O. Yu.; et al. (2012), "Dynamical Masses of a Selected Sample of Orbital Binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69
  • ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this sourceatVizieR.
  • ^ a b c d Struve, Otto; Franklin, K. L. (1955). "Spectrographic Observations of Visual Double Stars". The Astrophysical Journal. 121: 337. Bibcode:1955ApJ...121..337S. doi:10.1086/145993.
  • ^ a b Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (2002). "The Tycho double star catalogue". Astronomy and Astrophysics. 384: 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822.
  • ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
  • ^ a b c d van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  • ^ a b c Tokovinin, Andrei (2014). "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs". The Astronomical Journal. 147 (4): 14. arXiv:1401.6827. Bibcode:2014AJ....147...87T. doi:10.1088/0004-6256/147/4/87. S2CID 56066740. 87.
  • ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
  • ^ a b Soubiran, Caroline; et al. (2016), "The PASTEL catalogue: 2016 version", Astronomy & Astrophysics, 591: A118, arXiv:1605.07384, Bibcode:2016A&A...591A.118S, doi:10.1051/0004-6361/201628497, S2CID 119258214.

  • t
  • e

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_224635_and_HD_224636&oldid=1185400181"

    Categories: 
    Andromeda (constellation)
    Henry Draper Catalogue objects
    Double stars
    Bright Star Catalogue objects
    Hipparcos objects
    Durchmusterung objects
    Multiple star stubs
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
    All stub articles
     



    This page was last edited on 16 November 2023, at 14:00 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki