Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

60 Aurigae

From Wikipedia, the free encyclopedia
Binary star system in the constellation Auriga
60 Aurigae
Observation data
Epoch J2000      Equinox J2000
ConstellationAuriga
Right ascension06h 53m 13.40058s[1]
Declination+38° 26′ 16.8476″[1]
Apparent magnitude (V)6.319[2] (6.47/8.96)[3]
Characteristics
Spectral typeF5 V[4] (A8/G0)[3]
B−Vcolor index+0.328[2]
Astrometry
Radial velocity (Rv)+32.4[5] km/s
Proper motion (μ)RA: +42.40[1]mas/yr
Dec.: -179.12[1]mas/yr
Parallax (π)15.21±1.03 mas[1]
Distance210 ± 10 ly
(66 ± 4 pc)
Absolute magnitude (MV)2.11[2]
Orbit[6]
Period (P)271.10±61.00yr
Semi-major axis (a)0.793±0.073
Eccentricity (e)0.487±0.090
Inclination (i)58.4±5.4°
Longitude of the node (Ω)156.4±7.0°
Periastronepoch (T)2002.72±6.07
Argument of periastron (ω)
(secondary)
59.7±19.9°
Details
Temperature6,223[2] K
Metallicity [Fe/H]+0.04[2] dex
Age1.7[2] Gyr
Other designations
60 Aurigae,BD+38° 1636,HD 50037,HIP 33064,HR 2541,SAO 59576.[4]
Database references
SIMBADdata

60 Aurigae is abinary star[3] system in the northernconstellation ofAuriga. The pair have a combinedapparent visual magnitude of 6.319[2] and, based uponparallax measurements, they are approximately 210light-years (64parsecs) distant from the Earth.[1]

The combinedspectrum of the pair match astellar classification of F5 V.[4] The primary component may be anA-type star with an apparent magnitude of 6.47,[3] while the fainter, 8.96 magnitude secondary is possibly aG-type star. The pair orbit each other with a period of 271.1 years at anangular separation of 0.793 arcseconds.[6]

Nomenclature

[edit]

60 Aurigae is theFlamsteed designation of this star, also catalogued asHR 2541 andHD 50037. The designation60 Aurigae has sometimes been identified withPsi8 Aurigae however Simbad lists Psi8 Aurigae as61 Aurigae.[7]

References

[edit]
  1. ^abcdefvan Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752v1,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.Note: see VizieR catalogueI/311.
  2. ^abcdefgHolmberg, J.; Nordström, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics",Astronomy and Astrophysics,501 (3):941–947,arXiv:0811.3982,Bibcode:2009A&A...501..941H,doi:10.1051/0004-6361/200811191.
  3. ^abcdCvetkovic, Z.; Ninkovic, S. (June 2010), "On the Component Masses of Visual Binaries",Serbian Astronomical Journal,180 (180):71–80,Bibcode:2010SerAJ.180...71C,doi:10.2298/SAJ1080071C.
  4. ^abc"60 Aur -- Star",SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved2012-08-24.
  5. ^Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto: International Astronomical Union, p. 57,Bibcode:1967IAUS...30...57E.
  6. ^abHartkopf, William I.; Mason, Brian D. (2009)."Speckle Interferometry at Mount Wilson Observatory: Observations Obtained in 2006-2007 and 35 New Orbits"(PDF).The Astronomical Journal.138 (3):813–826.Bibcode:2009AJ....138..813H.doi:10.1088/0004-6256/138/3/813.Archived from the original on September 25, 2017.
  7. ^Kostjuk, N. D. (2004). "VizieR Online Data Catalog: HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index (Kostjuk, 2002)".VizieR On-line Data Catalog: IV/27A. Originally Published in: Institute of Astronomy of Russian Academy of Sciences (2002).4027.Bibcode:2004yCat.4027....0K.

External links

[edit]
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Other
Galaxies
Galaxy clusters
Retrieved from "https://en.wikipedia.org/w/index.php?title=60_Aurigae&oldid=1235796311"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp