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Tau Piscium

From Wikipedia, the free encyclopedia
Orange-hued star in the constellation Pisces
Tau Piscium
Location of τ Piscium (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationPisces
Right ascension01h 11m 39.63647s[1]
Declination+30° 05′ 22.6909″[1]
Apparent magnitude (V)+4.518[2]
Characteristics
Evolutionary stagered clump[3]
Spectral typeK0.5 IIIb[4]
U−Bcolor index+1.016[2]
B−Vcolor index+1.094[2]
Astrometry
Radial velocity (Rv)36.36±0.34[5] km/s
Proper motion (μ)RA: +73.88[1]mas/yr
Dec.: −38.30[1]mas/yr
Parallax (π)19.32±0.24 mas[1]
Distance169 ± 2 ly
(51.8 ± 0.6 pc)
Absolute magnitude (MV)+1.033[6]
Details[5]
Mass1.69[7] M
Radius10 R
Luminosity44.7 L
Surface gravity (log g)2.6 cgs
Temperature4,624±5 K
Metallicity[Fe/H]−0.04 dex
Rotational velocity (v sin i)2.2 km/s
Age2.27[5] Gyr
Other designations
τ Psc,83 Piscium,BD+29°190,FK5 43,HD 7106,HIP 5586,HR 352,SAO 74546[8]
Database references
SIMBADdata

Tau Piscium (τ Piscium) is an orange-huedstar in thezodiacconstellation ofPisces. With anapparent visual magnitude of +4.52,[2] it is a dim star but visible to the naked eye. Based upon an annualparallax shift of 19.32 mas as seen from Earth,[1] it is located around 169 light years from theSun. It is most likely (96% chance) a member of thethin disk population.[6]

This is anevolvedK-typegiant star with astellar classification of K0.5 IIIb.[4] It is about 2.27[5] billion years and is ared clump star on thehorizontal branch, which indicates it is generating energy throughhelium fusion at itscore.[3] The star has 1.7[7] times themass of the Sun and has expanded to about 10 times theSun's radius.[5] It is radiating 45 times theSun's luminosity from itsphotosphere at aneffective temperature of 4,624 K.[5]

Naming

[edit]

InChinese,奎宿 (Kuí Sù), meaningLegs, refers to an asterism consisting of τ Piscium,η Andromedae,65 Piscium,ζ Andromedae,ε Andromedae,δ Andromedae,π Andromedae,ν Andromedae,μ Andromedae,β Andromedae,σ Piscium,91 Piscium,υ Piscium,φ Piscium,χ Piscium andψ¹ Piscium. Consequently, theChinese name for τ Piscium itself is奎宿十一 (Kuí Sù shíyī, English:the Eleventh Star of Legs.)[9]

References

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  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. ^abcdJennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants",Monthly Notices of the Royal Astronomical Society,172 (3):667–679,Bibcode:1975MNRAS.172..667J,doi:10.1093/mnras/172.3.667.
  3. ^abMishenina, T. V.; et al. (September 2006), "Elemental abundances in the atmosphere of clump giants",Astronomy and Astrophysics,456 (3):1109–1120,arXiv:astro-ph/0605615,Bibcode:2006A&A...456.1109M,doi:10.1051/0004-6361:20065141,S2CID 18764566.
  4. ^abKeenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars",Astrophysical Journal Supplement Series,71: 245,Bibcode:1989ApJS...71..245K,doi:10.1086/191373.
  5. ^abcdefMassarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209.
  6. ^abSoubiran, C.; et al. (2008), "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants",Astronomy and Astrophysics,480 (1):91–101,arXiv:0712.1370,Bibcode:2008A&A...480...91S,doi:10.1051/0004-6361:20078788,S2CID 16602121.
  7. ^abLuck, R. Earle (September 2015), "Abundances in the Local Region. I. G and K Giants",The Astronomical Journal,150 (3): 23,arXiv:1507.01466,Bibcode:2015AJ....150...88L,doi:10.1088/0004-6256/150/3/88,S2CID 118505114, 88.
  8. ^"tau Psc".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-07-24.{{cite web}}: CS1 maint: postscript (link)
  9. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 19 日Archived 2016-03-03 at theWayback Machine
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