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Pi Tauri

Pi Tauri (π Tauri) is a solitary,[9] yellow-hued star in the zodiac constellation of Taurus. With an apparent visual magnitude of +4.69,[2] it is bright enough to be visible to the naked eye. Although it appears to lie among the stars of the Hyades cluster, it is not itself a member, being three times farther from Earth than the cluster. The distance to this star, as determined using an annual parallax shift of 7.83 mas as seen from the Earth,[1] is around 420 light years. At that range, the visual magnitude of the star is diminished by an extinction factor of 0.24 due to interstellar dust.[5]

Pi Tauri
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Taurus
Right ascension 04h 26m 36.37093s[1]
Declination +14° 42′ 49.6126″[1]
Apparent magnitude (V) +4.69[2]
Characteristics
Spectral type G7 IIIa Fe-1[3]
U−B color index +0.72[2]
B−V color index +0.98[2]
Astrometry
Radial velocity (Rv)+31.4±0.3[4] km/s
Proper motion (μ) RA: −9.52[1] mas/yr
Dec.: −31.44[1] mas/yr
Parallax (π)7.83 ± 0.22 mas[1]
Distance420 ± 10 ly
(128 ± 4 pc)
Absolute magnitude (MV)−1.27[5]
Details
Mass3.94[5] M
Radius21[6] R
Luminosity229[7] L
Surface gravity (log g)2.54[5] cgs
Temperature5,086[7] K
Metallicity [Fe/H]−0.08[5] dex
Age17[5] Myr
Other designations
π Tau, 73 Tau, BD+14° 697, HD 28100, HIP 20732, HR 1396, SAO 93935[8]
Database references
SIMBADdata

This is an evolved G-type giant star with a stellar classification of G7 IIIa Fe-1,[3] where the suffix notation indicates an underabundance of iron in the spectrum. The measured angular diameter is 1.55±0.06 mas.[10] At the estimated distance of Pi Tauri, this yields a physical size of about 21 times the radius of the Sun.[6] It possesses nearly four[5] times the mass of the Sun and is radiating 229 times the Sun's luminosity at an effective temperature of 5,086 K.[7]

References Edit

  1. ^ a b c d e f van 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. ^ a b c d Argue, A. N. (1966), "UBV photometry of 550 F, G and K type stars", Monthly Notices of the Royal Astronomical Society, 133 (4): 475–493, Bibcode:1966MNRAS.133..475A, doi:10.1093/mnras/133.4.475.
  3. ^ a b Keenan, 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.
  4. ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
  5. ^ a b c d e f g Takeda, Yoichi; et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants", Publications of the Astronomical Society of Japan, 60 (4): 781–802, arXiv:0805.2434, Bibcode:2008PASJ...60..781T, doi:10.1093/pasj/60.4.781.
  6. ^ a b Lang, 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:
     
  7. ^ a b c McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
  8. ^ "pi Tau". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-30.
  9. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  10. ^ 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.

tauri, tauri, solitary, yellow, hued, star, zodiac, constellation, taurus, with, apparent, visual, magnitude, bright, enough, visible, naked, although, appears, among, stars, hyades, cluster, itself, member, being, three, times, farther, from, earth, than, clu. Pi Tauri p Tauri is a solitary 9 yellow hued star in the zodiac constellation of Taurus With an apparent visual magnitude of 4 69 2 it is bright enough to be visible to the naked eye Although it appears to lie among the stars of the Hyades cluster it is not itself a member being three times farther from Earth than the cluster The distance to this star as determined using an annual parallax shift of 7 83 mas as seen from the Earth 1 is around 420 light years At that range the visual magnitude of the star is diminished by an extinction factor of 0 24 due to interstellar dust 5 Pi Tauri Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation TaurusRight ascension 04h 26m 36 37093s 1 Declination 14 42 49 6126 1 Apparent magnitude V 4 69 2 CharacteristicsSpectral type G7 IIIa Fe 1 3 U B color index 0 72 2 B V color index 0 98 2 AstrometryRadial velocity Rv 31 4 0 3 4 km sProper motion m RA 9 52 1 mas yr Dec 31 44 1 mas yrParallax p 7 83 0 22 mas 1 Distance420 10 ly 128 4 pc Absolute magnitude MV 1 27 5 DetailsMass3 94 5 M Radius21 6 R Luminosity229 7 L Surface gravity log g 2 54 5 cgsTemperature5 086 7 KMetallicity Fe H 0 08 5 dexAge17 5 MyrOther designationsp Tau 73 Tau BD 14 697 HD 28100 HIP 20732 HR 1396 SAO 93935 8 Database referencesSIMBADdataThis is an evolved G type giant star with a stellar classification of G7 IIIa Fe 1 3 where the suffix notation indicates an underabundance of iron in the spectrum The measured angular diameter is 1 55 0 06 mas 10 At the estimated distance of Pi Tauri this yields a physical size of about 21 times the radius of the Sun 6 It possesses nearly four 5 times the mass of the Sun and is radiating 229 times the Sun s luminosity at an effective temperature of 5 086 K 7 References Edit a b c d e f van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 a b c d Argue A N 1966 UBV photometry of 550 F G and K type stars Monthly Notices of the Royal Astronomical Society 133 4 475 493 Bibcode 1966MNRAS 133 475A doi 10 1093 mnras 133 4 475 a b Keenan 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 de Bruijne J H J Eilers A C October 2012 Radial velocities for the HIPPARCOS Gaia Hundred Thousand Proper Motion project Astronomy amp Astrophysics 546 14 arXiv 1208 3048 Bibcode 2012A amp A 546A 61D doi 10 1051 0004 6361 201219219 S2CID 59451347 A61 a b c d e f g Takeda Yoichi et al August 2008 Stellar Parameters and Elemental Abundances of Late G Giants Publications of the Astronomical Society of Japan 60 4 781 802 arXiv 0805 2434 Bibcode 2008PASJ 60 781T doi 10 1093 pasj 60 4 781 a b Lang Kenneth R 2006 Astrophysical formulae Astronomy and astrophysics library vol 1 3rd ed Birkhauser ISBN 3 540 29692 1 The radius R is given by 2 R 127 7 1 55 10 3 AU 0 0046491 AU R 42 6 R displaystyle begin aligned 2 cdot R amp frac 127 7 cdot 1 55 cdot 10 3 text AU 0 0046491 text AU R bigodot amp approx 42 6 cdot R bigodot end aligned nbsp a b c McDonald I et al 2012 Fundamental Parameters and Infrared Excesses of Hipparcos Stars Monthly Notices of the Royal Astronomical Society 427 1 343 57 arXiv 1208 2037 Bibcode 2012MNRAS 427 343M doi 10 1111 j 1365 2966 2012 21873 x S2CID 118665352 pi Tau SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2017 06 30 Eggleton P P Tokovinin A A September 2008 A catalogue of multiplicity among bright stellar systems Monthly Notices of the Royal Astronomical Society 389 2 869 879 arXiv 0806 2878 Bibcode 2008MNRAS 389 869E doi 10 1111 j 1365 2966 2008 13596 x S2CID 14878976 Richichi A et al February 2005 CHARM2 An updated Catalog of High Angular Resolution Measurements Astronomy and Astrophysics 431 2 773 777 Bibcode 2005A amp A 431 773R doi 10 1051 0004 6361 20042039 Retrieved from https en wikipedia org w index php title Pi Tauri amp oldid 1170345108, wikipedia, wiki, book, books, library,

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