Lambda Aurigae

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λ Aurigae A
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension 05h 19m 08.47s [1]
Declination +40° 05′ 56.6″ [1]
Apparent magnitude (V) 4.69
Characteristics
Spectral type G1.5 IV-VFe-1
U−B color index 0.12
B−V color index 0.63
R−I color index 0.32
Variable type ?
Astrometry
Radial velocity (Rv)66.4 km/s
Proper motion (μ) RA: 518.99 ± 0.26 [1] mas/yr
Dec.: -665.06 ± 0.13 [1] mas/yr
Parallax (π)79.17 ± 0.28 mas[1]
Distance41.2 ± 0.1 ly
(12.63 ± 0.04 pc)
Absolute magnitude (MV)4.18
Details
Temperature5890 ± 4.3[2] K
Age5.0–7.9 × 109[3] years
Other designations
LHS 1753, FK5 1145, JP11 1022, ROT 755, 15 Aur, GC 6494, LFT 403, SAO 40233, GCRV 3155, LSPM J0519+4005, ADS 3886, LTT 11625, SPOCS 256, AG+40° 608, GJ 197, 2MASS J05190848+4005565, TD1 4327, ASCC 394559, HD 34411, N30 1135, UBV M 10785, BD+39° 1248, HIC 24813, NLTT 14837, UBV 5041, CCDM J05192+4007, HIP 24813, PLX 1199, USNO-B1.0 1301-00122816, Ci 20 326, HR 1729, PMC 90-93 767, uvby98 100034411, CSI+39 1248 1, IDS 05121+4001, PPM Star Catalogue 47977.
Database references
SIMBADdata
Database references
SIMBADdata

Lambda Aurigae (λ Aur, λ Aurigae) is a binary star in the constellation Auriga. It is approximately 41.2 light-years from Earth.

The primary component, λ Aurigae A, is a yellow G-type subgiant with an apparent magnitude of +4.69. Its companion, λ Aurigae B, is 29 arcseconds away and has an apparent magnitude of +13.4. The binary star also has two optical companions, the 12th magnitude λ Aurigae C at 42 arcseconds and the magnitude +8.6 λ Aurigae D, 146 arcseconds from the primary.

Name

Sometimes, this star is called by the name Al Hurr, meaning the fawn in Arabic[4].

This star, along with μ Aur and ρ Aur, were Kazwini's Al Ḣibāʽ, the Tent.[5]. According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Ḣibāʽ were the title for three stars : λ Aur as Al Ḣibāʽ I, μ Aur as Al Ḣibāʽ II and ρ Aur as Al Ḣibāʽ III[6]

In Chinese, 咸池 (Xián Chí), meaning Pool of Harmony, refers to an asterism consisting of λ Aurigae, ρ Aurigae and HD 36041.[7] Consequently, λ Aurigae itself is known as 咸池三 (Xián Chí sān, English: the Third Star of Pool of Harmony.)[8]

References

  1. ^ a b c d e van Leeuwen, F. (2007). "HIP 24813". Hipparcos, the New Reduction. Retrieved 2009-12-16.
  2. ^ Kovtyukh; et al. (2003). "High precision effective temperatures for 181 F-K dwarfs from line-depth ratios". Astronomy and Astrophysics. 411 (3): 559–564. doi:10.1051/0004-6361:20031378. {{cite journal}}: Explicit use of et al. in: |author= (help)
  3. ^ Mamajek, Eric E.; Hillenbrand, Lynne A. (2008). "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics". The Astrophysical Journal. 687 (2): 1264–1293. Bibcode:2008ApJ...687.1264M. doi:10.1086/591785. {{cite journal}}: Unknown parameter |month= ignored (help)CS1 maint: multiple names: authors list (link)
  4. ^ Star Name - R.H.Allen p.92
  5. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York, NY: Dover Publications Inc. p. 91. ISBN 0486210790. Retrieved 2010-12-12.
  6. ^ Jack W. Rhoads - Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propultion Laboratory, California Institue of Technology; November 15, 1971
  7. ^ Template:Zh icon 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 9789867332257.
  8. ^ Template:Zh icon AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 13 日

Components

NAME Right ascension Declination Apparent magnitude (V) Spectral type Database references
ADS 3886 B (BD+39 1248B ) 05h 19m 03.6s +40° 06' 32 13.4 Simbad
ADS 3886 C (BD+39 1248C) 05h 19m 02.5s +40° 06' 28 12.1 Simbad
ADS 3886 D (BD+39 1248D) 05h 19m 06.3s +40° 07' 15 8.6 Simbad
ADS 3886 E (BD+39 1248E) 05h 19m30s +40° 09' 00 Simbad
Auriga Constellation

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