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Nu Eridani

From Wikipedia, the free encyclopedia
Variable star in the constellation Eridanus
ν Eridani
Location of ν Eridani (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationEridanus
Right ascension04h 36m 19.141s[1]
Declination−03° 21′ 08.86″[1]
Apparent magnitude (V)+3.930±0.023[2]
Characteristics
Spectral typeB1.5 IV[3]
U−Bcolor index−0.879±0.007[2]
B−Vcolor index−0.210±0.009[2]
Variable typeSPB andBeta Cephei[4]
Astrometry
Radial velocity (Rv)14.9[5] km/s
Proper motion (μ)RA: +1.53[1]mas/yr
Dec.: −5.01[1]mas/yr
Parallax (π)4.83±0.19 mas[1]
Distance680 ± 30 ly
(207 ± 8 pc)
Absolute magnitude (MV)−2.84±0.15[3]
Details[3]
Mass9.3±0.3 M
Radius6.2±0.5 R
Luminosity7,943 L
Surface gravity (log g)3.85±0.05 cgs
Temperature22,000±250 K
Rotational velocity (v sin i)26±2 km/s
Other designations
ν Eri,BD−03°834,48 Eridani,FK5 169,HD 29248,HIP 21444,HR 1463,SAO 131346[6]
Database references
SIMBADdata

Nu Eridani (ν Eri) is astar in theconstellationEridanus. It is visible to thenaked eye with anapparent visual magnitude of 3.93.[2] The distance to this star is roughly 520 light years, based upon an annualparallax shift of 0.00625 arcseconds.[1] If the star were 33 ly (10 pc) from theSun, it would be the brightest star in the night sky with an apparent magnitude of −2.84.[3] (Currently, the brightest star isSirius at magnitude −1.46.)

Alight curve for Nu Eridani, plotted fromTESS data[7]
Nu Eridani (bright star) and the galaxies:NGC 1618,NGC 1622 andNGC 1625 (from right to left)

This is aB-typesubgiant star with astellar classification of B1.5 IV.[3] In 1926, Robert H. Baker announced his discovery that the brightness of Nu Eridani is variable.[8][9] It is ahybrid pulsatorvariable, lying as it does on the overlappinginstability strips forBeta Cephei variables andslowly pulsating B-type stars.[4] The star shows at least fourteen pulsations frequencies, with nine that also display radial velocity variations.[10] It has about nine times themass of the Sun and six times theSun's radius. Nu Eridani shines with 7,943 times thesolar luminosity from itsouter atmosphere at aneffective temperature of 22,000 K.[3]

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. ^abcdNieva, M.-F. (February 2013), "Temperature, gravity, and bolometric correction scales for non-supergiant OB stars",Astronomy & Astrophysics,550: A26,arXiv:1212.0928,Bibcode:2013A&A...550A..26N,doi:10.1051/0004-6361/201219677,S2CID 119275940.
  3. ^abcdefNieva, María-Fernanda; Przybilla, Norbert (2014), "Fundamental properties of nearby single early B-type stars",Astronomy & Astrophysics,566: A7,arXiv:1412.1418,Bibcode:2014A&A...566A...7N,doi:10.1051/0004-6361/201423373,S2CID 119227033.
  4. ^abMoravveji, Ehsan (January 2016), "The impact of enhanced iron opacity on massive star pulsations: updated instability strips",Monthly Notices of the Royal Astronomical Society: Letters,455 (1):L67–L71,arXiv:1509.08652,Bibcode:2016MNRAS.455L..67M,doi:10.1093/mnrasl/slv142.
  5. ^Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities",Carnegie Institute Washington D.C. Publication,Carnegie Institute of Washington D.C.,Bibcode:1953GCRV..C......0W.
  6. ^"nu. Eri".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-11-03.
  7. ^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved19 August 2022.
  8. ^Baker, R. H. (April 1926)."Variable Stars of Small Range".Publications of the Astronomical Society of the Pacific.38 (222):86–96.Bibcode:1926PASP...38...86B.doi:10.1086/123545. Retrieved24 December 2024.
  9. ^Walker, Merle F. (September 1952)."Photoelectric Observations of nu Eridani".Astrophysical Journal.116:391–397.Bibcode:1952ApJ...116..391W.doi:10.1086/145623. Retrieved24 December 2024.
  10. ^Daszyńska-Daszkiewicz, J.; Walczak, P. (March 2010), "Complex asteroseismology of the β Cep/slowly pulsating B-type pulsator ν Eridani: constraints on opacities",Monthly Notices of the Royal Astronomical Society,403 (1):496–504,arXiv:0912.0622,Bibcode:2010MNRAS.403..496D,doi:10.1111/j.1365-2966.2009.16141.x,S2CID 118430678.
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