Astronomy:29 Camelopardalis

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Short description: Double star in the constellation Camelopardalis
29 Camelopardalis
Observation data
Equinox J2000.0]] (ICRS)
Constellation Camelopardalis
Right ascension  05h 50m 33.8729s[1]
Declination +56° 55′ 08.1822″[1]
Apparent magnitude (V) 6.590±0.009[2]
Characteristics
29 Cam A
Spectral type A4 IV-V
U−B color index +0.13[2]
B−V color index +0.09[2]
29 Cam B
Spectral type A3 V
Astrometry
29 Cam A
Radial velocity (Rv)3.9±2[3] km/s
Proper motion (μ) RA: –19.460[1] mas/yr
Dec.: –4.249[1] mas/yr
Parallax (π)6.7370 ± 0.0607[1] mas
Distance484 ± 4 ly
(148 ± 1 pc)
Absolute magnitude (MV)+0.71[4]
29 Cam B
Proper motion (μ) RA: +2.585[5] mas/yr
Dec.: –0.570[5] mas/yr
Parallax (π)1.6375 ± 0.0483[5] mas
Distance1,990 ± 60 ly
(610 ± 20 pc)
Details
29 Cam A
Mass2.47 ± 0.08[6] M
Radius3.49+0.14
−0.12
[7] R
Luminosity58.9+8.9
−7.6
[6] L
Surface gravity (log g)3.77[8] cgs
Temperature8,337 ± 96[6] K
Rotational velocity (v sin i)123[9] km/s
Age380 ± 14[6] Myr
29 Cam B
Mass2.12[10] M
Radius2.06[11] R
Luminosity15.043[11] L
Temperature7911[11] K
Rotational velocity (v sin i)110±8[12] km/s
Other designations
Database references
SIMBADdata

29 Camelopardalis (29 Cam) is a double star in the circumpolar constellation Camelopardalis. With an apparent magnitude of 6.59,[2] it's right below the max visibility to the naked eye, and can only be viewed under phenomenal conditions. The star is located 484 light years[1] away based on parallax, but is drifting further away with a radial velocity of 3.9 km/s.[3]

29 Cam A

29 Cam A has a classification of A4IV-V, which suggests that this star is beginning to evolve off the main sequence. Zorec et al. models it as a star that has completed 90.6% of the main sequence, which correlates to an age of 380 million years.[6] At present, 29 Cam has 2.47 the mass of the Sun,[6] and 3.49 times its radius. [7] It radiates at 58.9 times the luminosity of the Sun from an effective temperature of 8,337 K,[6] which gives it a white hue of an A-type star. 29 Cam spins rapidly at a projected rotational velocity of 123 km/s despite its evolved state.

29 Cam B

29 Cam has a companion designated BD+56 1065B, which is a 10 magnitude star. According to the proper motion, this star is unrelated to the primary, and is 4 times farther than the primary.[13] The companion is relatively cooler and less luminous than the primary.

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 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.
  2. 2.0 2.1 2.2 2.3 Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series 89: 415–419. ISSN 0365-0138. Bibcode1991A&AS...89..415O. 
  3. 3.0 3.1 Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities.". Carnegie Institute Washington D.C. Publication. Bibcode1953GCRV..C......0W. 
  4. Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331–346. doi:10.1134/S1063773712050015. ISSN 1063-7737. Bibcode2012AstL...38..331A. 
  5. 5.0 5.1 5.2 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.
  6. 6.0 6.1 6.2 6.3 6.4 6.5 6.6 Zorec, J.; Royer, F. (1 January 2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics 537: A120. doi:10.1051/0004-6361/201117691. ISSN 0004-6361. Bibcode2012A&A...537A.120Z. 
  7. 7.0 7.1 Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W. et al. (October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256. Bibcode2019AJ....158..138S. 
  8. Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A. et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics 628: A94. doi:10.1051/0004-6361/201935765. ISSN 0004-6361. Bibcode2019A&A...628A..94A. 
  9. Royer, F.; Grenier, S.; Baylac, M.-O.; Gómez, A. E.; Zorec, J. (October 2002). "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i". Astronomy and Astrophysics 393: 897–911. doi:10.1051/0004-6361:20020943. ISSN 0004-6361. Bibcode2002A&A...393..897R. 
  10. Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W. et al. (2019-10-01). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256. Bibcode2019AJ....158..138S. 
  11. 11.0 11.1 11.2 Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; Babusiaux, C.; Bailer-Jones, C. A. L.; Biermann, M. et al. (2018-08-01). "Gaia Data Release 2. Summary of the contents and survey properties". Astronomy and Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. ISSN 0004-6361. Bibcode2018A&A...616A...1G. 
  12. Glebocki, R.; Gnacinski, P. (2005-03-01). "Systematic errors in the determination of stellar rotational velocities". 13th Cambridge Workshop on Cool Stars 560: 571. Bibcode2005ESASP.560..571G. 
  13. Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001-12-01). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal 122 (6): 3466–3471. doi:10.1086/323920. ISSN 0004-6256. Bibcode2001AJ....122.3466M.