Astronomy:4 Camelopardalis

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Short description: Probable multiple star system in the constellation Camelopardalis
4 Camelopardalis
Observation data
Equinox J2000.0]] (ICRS)
Constellation Camelopardalis
Right ascension  04h 48m 00.2729s[1]
Declination +56° 45′ 25.837″[1]
Apparent magnitude (V) 5.29[2]
Characteristics
Spectral type A3m[3]
U−B color index 0.12[4]
B−V color index 0.246±0.003[2]
Astrometry
Radial velocity (Rv)+22.50±0.9[5] km/s
Proper motion (μ) RA: +52.892[1] mas/yr
Dec.: −140.618[1] mas/yr
Parallax (π)18.4464 ± 0.1109[1] mas
Distance177 ± 1 ly
(54.2 ± 0.3 pc)
Absolute magnitude (MV)1.68[2]
Orbit[6]
PrimaryAa
CompanionAb
Period (P)90 yr
Semi-major axis (a)0.503″
Eccentricity (e)0.87
Inclination (i)120.0°
Longitude of the node (Ω)54.5°
Argument of periastron (ω)
(secondary)
235.9°
Details
Mass2.01[7] M
Radius2.57+0.05
−0.17
[8] R
Luminosity17.64[2] L
Surface gravity (log g)3.98[9] cgs
Temperature7,700[9] K
Metallicity [Fe/H]+0.27[9] dex
Rotational velocity (v sin i)75[10] km/s
Age560[7] Myr
Other designations
4 Cam, BD+56°973, FK5 175, HD 30121, HIP 22287, HR 1511, SAO 24829[11]
Database references
SIMBADdata

4 Camelopardalis is a probable multiple star in the northern constellation of Camelopardalis,[11] located 177 light years away from the Sun, based upon parallax.[1] With a combined apparent visual magnitude of 5.29,[2] it is visible to the naked eye as a faint, white-hued star. The pair have a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.158 per year.[12] The system's proper motion makes it a candidate for membership in the IC 2391 supercluster.[13] They are moving away from the Earth with a heliocentric radial velocity of 22.5 km/s.[5]

The brighter member, designated component A, is classified as an Am star, which indicates that the spectrum shows abnormalities of certain elements.[14] It is an estimated 560[7] million years old and is spinning with a projected rotational velocity of 75[10] The star has 2.01[7] times the mass of the Sun and 2.57[8] times the Sun's radius. It is radiating 18[2] times the Sun's luminosity from its photosphere at an effective temperature of 7,700 K.[9]

There is a faint, magnitude 9.49 companion at an angular separation of 0.610″ – component B; the pair most likely form a binary systemwith a period of about 90 years.[6] There is also a 13th-magnitude visual companion 13 away which shares a common proper motion and parallax.[15][6] Another listed companion, a 12th-magnitude star nearly 2 away, is probably unrelated.[16]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  3. Cowley, A. et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal 74: 375–406, doi:10.1086/110819, Bibcode1969AJ.....74..375C 
  4. Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD, Bibcode1986EgUBV........0M 
  5. 5.0 5.1 Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters 32 (11): 759–771, doi:10.1134/S1063773706110065, Bibcode2006AstL...32..759G. 
  6. 6.0 6.1 6.2 Tokovinin, Andrei; Everett, Mark E.; Horch, Elliott P.; Torres, Guillermo; Latham, David W. (2019), "Speckle Observations and Orbits of Multiple Stars", The Astronomical Journal 158 (4): 167, doi:10.3847/1538-3881/ab4137, Bibcode2019AJ....158..167T. 
  7. 7.0 7.1 7.2 7.3 De Rosa, R. J. et al. (2014), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc", Monthly Notices of the Royal Astronomical Society 437 (2): 1216–1240, doi:10.1093/mnras/stt1932, Bibcode2014MNRAS.437.1216D. 
  8. 8.0 8.1 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  9. 9.0 9.1 9.2 9.3 Takeda, Yoichi et al. (October 2018), "Photospheric carbon, nitrogen, and oxygen abundances of A-type main-sequence stars*", Publications of the Astronomical Society of Japan 70 (5): 91, doi:10.1093/pasj/psy091, 91, Bibcode2018PASJ...70...91T. 
  10. 10.0 10.1 Royer, F. et al. (2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i in the northern hemisphere", Astronomy and Astrophysics 393 (3): 897–911, doi:10.1051/0004-6361:20020943, Bibcode2002A&A...393..897R 
  11. 11.0 11.1 "4 Cam". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=4+Cam. 
  12. Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal 129 (3): 1483–1522, doi:10.1086/427854, Bibcode2005AJ....129.1483L. 
  13. Eggen, Olin J. (December 1995), "Reality Tests of Superclusters in the Young Disk Population", Astronomical Journal 110: 2862, doi:10.1086/117734, Bibcode1995AJ....110.2862E. 
  14. Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars", Astronomy and Astrophysics 498 (3): 961–966, doi:10.1051/0004-6361/200810788, Bibcode2009A&A...498..961R 
  15. Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  16. Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.

External links