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Upsilon1 Eridani

From Wikipedia, the free encyclopedia
For other star systems with thisBayer designation, seeUpsilon Eridani.
Red clump star in the constellation Eridanus
υ1 Eridani
Location of υ1 Eridani (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationEridanus
Right ascension04h 33m 30.55236s[1]
Declination−29° 45′ 59.3725″[1]
Apparent magnitude (V)4.51[2]
Characteristics
Evolutionary stagered clump[3]
Spectral typeK0 III-IV[4]
U−Bcolor index+0.70[2]
B−Vcolor index+0.98[2]
Astrometry
Radial velocity (Rv)+20.89±0.69[5] km/s
Proper motion (μ)RA: −114.78[1]mas/yr
Dec.: −271.79[1]mas/yr
Parallax (π)25.67±0.24 mas[1]
Distance127 ± 1 ly
(39.0 ± 0.4 pc)
Absolute magnitude (MV)1.60[5]
Details
Mass1.54[5] M
Radius7.3[6] R
Luminosity24[5] L
Surface gravity (log g)3.09[5] cgs
Temperature4,941[5] K
Metallicity[Fe/H]−0.16±0.08[5] dex
Rotational velocity (v sin i)2.15[7] km/s
Other designations
υ1 Eridani, υ1 Eri,50 Eridani,CD−30°1883,HD 29085,HIP 21248,HR 1453,SAO 169570[8]
Database references
SIMBADdata

Upsilon1 Eridani (υ1 Eri) is a singlestar in theconstellationEridanus. It has anapparent visual magnitude is 4.51,[2] which is bright enough to be faintly visible to the naked eye on a clear, dark night. The distance to this star, as determined using theparallax method,[1] is around 127 light years.

This is anevolvedred clump[3]giant star with astellar classification of K0III-IV.[4] The measuredangular diameter, after correction forlimb darkening, is1.74±0.02 mas.[9] At an estimated distance of this star, this yields a physical size of about 7.3 times theradius of the Sun.[6] It has 154%[5] of theSun's mass and radiates 24 times thesolar luminosity from itsouter atmosphere at aneffective temperature of 4,941 K.[5]

References

[edit]
  1. ^abcdefvan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abAlves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity",The Astrophysical Journal,539 (2):732–741,arXiv:astro-ph/0003329,Bibcode:2000ApJ...539..732A,doi:10.1086/309278,S2CID 16673121.
  4. ^abGray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–170,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637,S2CID 119476992.
  5. ^abcdefghiLuck, R. Earle; Heiter, Ulrike (June 2007), "Giants in the Local Region",The Astronomical Journal,133 (6):2464–2486,Bibcode:2007AJ....133.2464L,doi:10.1086/513194.
  6. ^abLang, Kenneth R. (2006),Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.),Birkhäuser,ISBN 3-540-29692-1. The radius (R*) is given by:
    2R=(39.01.74103) AU0.0046491 AU/R14.6R{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(39.0\cdot 1.74\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 14.6\cdot R_{\bigodot }\end{aligned}}}
  7. ^Hekker, S.; Meléndez, J. (2007). "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters".Astronomy and Astrophysics.475 (3): 1003.arXiv:0709.1145.Bibcode:2007A&A...475.1003H.doi:10.1051/0004-6361:20078233.S2CID 10436552.
  8. ^"* ups01 Eri".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-10-13.{{cite web}}: CS1 maint: postscript (link)
  9. ^Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements",Astronomy and Astrophysics,431 (2):773–777,Bibcode:2005A&A...431..773R,doi:10.1051/0004-6361:20042039.
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