Astronomy:Theta Cephei

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Short description: Star in the constellation Cepheus
Theta Cephei
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cepheus
Right ascension  20h 29m 34.86518s[1]
Declination +62° 59′ 38.6216″[1]
Apparent magnitude (V) 4.22[2]
Characteristics
Spectral type A7 III[3] or kA7hF1mF2[4][5]
U−B color index +0.16[2]
B−V color index +0.20[2]
Astrometry
Radial velocity (Rv)−6.8[6] km/s
Proper motion (μ) RA: 52.416[1] mas/yr
Dec.: −2.544[1] mas/yr
Parallax (π)25.7611 ± 0.5808[1] mas
Distance127 ± 3 ly
(38.8 ± 0.9 pc)
Absolute magnitude (MV)+1.12[7]
Orbit[8]
Period (P)914.3±7.0 d
Eccentricity (e)0.377±0.006
Periastron epoch (T)2456991.3±8.5 JD
Argument of periapsis (ω)
(primary)		48.8±1.1°
Semi-amplitude (K1)
(primary)		7.72±0.06 km/s
Details
primary
Mass2.75[9] M☉
Radius3.09+0.36
−0.25[1] R☉
Luminosity46.5[9] L☉
Surface gravity (log g)3.74[3] cgs
Temperature7,375+307
−404[1] K
Metallicity [Fe/H]+0.27±0.04[7] dex
Rotational velocity (v sin i)52.0[3] km/s
Age55[9] Myr
companion
Mass>0.62[8] M☉
Radius0.654+0.044
−0.102[8] R☉
Temperature4,070+340
−130[8] K
Other designations
θ Cep, 2 Cep, BD+62°1821, FK5 767, HD 195725, HIP 101093, HR 7850, SAO 18897[10]
Database references
SIMBADdata

Theta Cephei, Latinized from θ Cephei, is a stellar class A7, fourth-magnitude star in the constellation Cepheus. This displays at a metallic-line Am star.[4] It is a white-hued, single-lined spectroscopic binary system, located about 127 light-years from Earth. The pair have an orbital period of 2.5 years;[8] the eccentricity was long thought to be low, at 0.03,[11] but recent calculations have put it at a much higher 0.377.[8] They are separated by 4.16 astronomical unit|AU.[12] The companion star is calculated to be about 400 times fainter than the primary. It is completely invisible in the spectrum, but is estimated to be a K7 main sequence star.[9]

Shared with η Cep, this star system has the title Al Kidr.[13] In Chinese, 天鈎 (Tiān Gōu), meaning Celestial Hook, refers to an asterism consisting of 4 Cephei, HD 194298, η Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei.[14] Consequently, the Chinese name for θ Cephei itself is 天鈎三 (Tiān Gōu sān, English: the Third Star of Celestial Hook.).[15]

References

  1. ↑ Jump up to: 1.0 1.1 1.2 1.3 1.4 1.5 1.6 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. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. ↑ Jump up to: 2.0 2.1 2.2 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J. 
  3. ↑ Jump up to: 3.0 3.1 3.2 Takeda, Yoichi et al. (April 2012), "Lithium, Sodium, and Potassium Abundances in Sharp-Lined A-Type Stars", Publications of the Astronomical Society of Japan 64 (2): 15, doi:10.1093/pasj/64.2.38, 38, Bibcode: 2012PASJ...64...38T 
  4. ↑ Jump up to: 4.0 4.1 Abt, Helmut A.; Morrell, Nidia I. (1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars", The Astrophysical Journal Supplement Series 99: 135, doi:10.1086/192182, Bibcode: 1995ApJS...99..135A. 
  5. ↑ Skiff, B. A (2014), "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016)", VizieR On-line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014) 1, Bibcode: 2014yCat....1.2023S. 
  6. ↑ Evans, D. S. (1967), "The Revision of the General Catalogue of Radial Velocities", Determination of Radial Velocities and Their Applications 30: 57, Bibcode: 1967IAUS...30...57E. 
  7. ↑ Jump up to: 7.0 7.1 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  8. ↑ Jump up to: 8.0 8.1 8.2 8.3 8.4 8.5 Bischoff, Richard; Mugrauer, Markus; Lux, Oliver; Zehe, Tamara; Heyne, Therese; Wagner, Daniel; Geymeier, Michael (2020), "Spectroscopic orbit determination of the long periodic binary system θ Cep", Astronomische Nachrichten 341 (10): 989, doi:10.1002/asna.202013850, Bibcode: 2020AN....341..989B. 
  9. ↑ Jump up to: 9.0 9.1 9.2 9.3 Fouesneau, M.; Andrae, R.; Dharmawardena, T.; Rybizki, J.; Bailer-Jones, C. A. L.; Demleitner, M. (2022), "Astrophysical parameters from Gaia DR2, 2MASS, and AllWISE", Astronomy and Astrophysics 662: A125, doi:10.1051/0004-6361/202141828, Bibcode: 2022A&A...662A.125F. 
  10. ↑ "tet Cep". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=tet+Cep. 
  11. ↑ Abt, Helmut A. (March 1961), "The Frequency of Binaries among Metallic-Line Stars", Astrophysical Journal Supplement 6: 37, doi:10.1086/190060, Bibcode: 1961ApJS....6...37A. 
  12. ↑ Trilling, D. E. et al. (April 2007), "Debris disks in main-sequence binary systems", The Astrophysical Journal 658 (2): 1264–1288, doi:10.1086/511668, Bibcode: 2007ApJ...658.1289T. 
  13. ↑ Allen, Richard Hinckley (1963-06-01), Star Names: Their Lore and Meaning, Dover Publications, p. 155, ISBN 978-0486210797, https://archive.org/details/starnamestheirlo00alle/page/155 
  14. ↑ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN:978-986-7332-25-7.
  15. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 6 日



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