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Tau6 Eridani

Tau6 Eridani, Latinized from τ6 Eridani, is a single[9] star in the equatorial constellation of Eridanus, located near the constellation border with Fornax. It has a yellow-white hue with an apparent visual magnitude of 4.22,[2] which is bright enough to be seen with the naked eye. Based upon parallax measurements, the distance to this star is around 57.5 light years.[1] It is drifting further away with a radial velocity of +8 km/s.[4]

τ6 Eridani
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Eridanus
Right ascension 03h 46m 50.88819s[1]
Declination −23° 14′ 59.0046″[1]
Apparent magnitude (V) 4.22[2]
Characteristics
Spectral type F5IV-V[3]
U−B color index −0.03[2]
B−V color index +0.43[2]
Astrometry
Radial velocity (Rv)8.0±0.8[4] km/s
Proper motion (μ) RA: −158.84[1] mas/yr
Dec.: −528.95[1] mas/yr
Parallax (π)56.73 ± 0.19 mas[1]
Distance57.5 ± 0.2 ly
(17.63 ± 0.06 pc)
Absolute magnitude (MV)2.98[5]
Details
Mass1.35[4] M
Radius1.80+0.08
−0.03
[6] R
Luminosity5.47±0.06[6] L
Surface gravity (log g)4.21±0.13[4] cgs
Temperature6,584+47
−144
[6] K
Metallicity [Fe/H]−0.03±0.11[4] dex
Rotational velocity (v sin i)16.25[7] km/s
Age2.0[4] Gyr
Other designations
τ6 Eri, 27 Eridani, CD−23°1565, FK5 140, GC 168827, HD 23754, HIP 17651, HR 1173, SAO 101600[8]
Database references
SIMBADdata

The spectrum of Tau6 Eridani matches a stellar classification of F5IV-V,[3] indicating it is an F-type star that shows traits of both a main sequence star and a subgiant. It has an estimated 135%[4] of the Sun's mass and about 1.8 time the radius of the Sun.[6] The star is radiating 5.5[6] times the luminosity of the Sun at an effective temperature of 6,508 K,[4] and it does not display any surface magnetic activity.[7] The star has been examined for infrared excess emission that could indicate the presence of circumstellar matter, but none has been detected.[10]

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 ^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode:1986EgUBV........0M.
  3. ^ a b Gray, 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.
  4. ^ a b c d e f g h Kordopatis, G.; Gilmore, G.; Steinmetz, M.; Boeche, C.; Seabroke, G. M.; Siebert, A.; Zwitter, T.; Binney, J.; et al. (November 2013), "The Radial Velocity Experiment (RAVE): Fourth Data Release", The Astronomical Journal, 146 (5): 36, arXiv:1309.4284, Bibcode:2013AJ....146..134K, doi:10.1088/0004-6256/146/5/134, S2CID 119221010, 134.
  5. ^ Reiners, Ansgar (January 2006), "Rotation- and temperature-dependence of stellar latitudinal differential rotation", Astronomy and Astrophysics, 446 (1): 267–277, arXiv:astro-ph/0509399, Bibcode:2006A&A...446..267R, doi:10.1051/0004-6361:20053911, S2CID 8642707
  6. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  7. ^ a b Martínez-Arnáiz, R.; et al. (September 2010), (PDF), Astronomy and Astrophysics, 520: A79, arXiv:1002.4391, Bibcode:2010A&A...520A..79M, doi:10.1051/0004-6361/200913725, S2CID 43455849, archived from the original (PDF) on 2017-09-22, retrieved 2018-11-04.
  8. ^ "* tau06 Eri". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-10-13.
  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. ^ Weinberger, Alycia J.; Bryden, Geoff; Kennedy, Grant M.; Roberge, Aki; Defrère, Denis; Hinz, Philip M.; Millan-Gabet, Rafael; Rieke, George; et al. (February 2015), "Target Selection for the LBTI Exozodi Key Science Program", The Astrophysical Journal Supplement Series, 216 (2): 8, arXiv:1501.01319, Bibcode:2015ApJS..216...24W, doi:10.1088/0067-0049/216/2/24, S2CID 38713562, 24.

tau6, eridani, other, star, systems, with, this, bayer, designation, eridani, latinized, from, eridani, single, star, equatorial, constellation, eridanus, located, near, constellation, border, with, fornax, yellow, white, with, apparent, visual, magnitude, whi. For other star systems with this Bayer designation see Tau Eridani Tau6 Eridani Latinized from t6 Eridani is a single 9 star in the equatorial constellation of Eridanus located near the constellation border with Fornax It has a yellow white hue with an apparent visual magnitude of 4 22 2 which is bright enough to be seen with the naked eye Based upon parallax measurements the distance to this star is around 57 5 light years 1 It is drifting further away with a radial velocity of 8 km s 4 t6 Eridani Observation dataEpoch J2000 0 Equinox J2000 0 ICRS Constellation EridanusRight ascension 03h 46m 50 88819s 1 Declination 23 14 59 0046 1 Apparent magnitude V 4 22 2 CharacteristicsSpectral type F5IV V 3 U B color index 0 03 2 B V color index 0 43 2 AstrometryRadial velocity Rv 8 0 0 8 4 km sProper motion m RA 158 84 1 mas yr Dec 528 95 1 mas yrParallax p 56 73 0 19 mas 1 Distance57 5 0 2 ly 17 63 0 06 pc Absolute magnitude MV 2 98 5 DetailsMass1 35 4 M Radius1 80 0 08 0 03 6 R Luminosity5 47 0 06 6 L Surface gravity log g 4 21 0 13 4 cgsTemperature6 584 47 144 6 KMetallicity Fe H 0 03 0 11 4 dexRotational velocity v sin i 16 25 7 km sAge2 0 4 GyrOther designationst6 Eri 27 Eridani CD 23 1565 FK5 140 GC 168827 HD 23754 HIP 17651 HR 1173 SAO 101600 8 Database referencesSIMBADdataThe spectrum of Tau6 Eridani matches a stellar classification of F5IV V 3 indicating it is an F type star that shows traits of both a main sequence star and a subgiant It has an estimated 135 4 of the Sun s mass and about 1 8 time the radius of the Sun 6 The star is radiating 5 5 6 times the luminosity of the Sun at an effective temperature of 6 508 K 4 and it does not display any surface magnetic activity 7 The star has been examined for infrared excess emission that could indicate the presence of circumstellar matter but none has been detected 10 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 Mermilliod J C 1986 Compilation of Eggen s UBV data transformed to UBV unpublished Catalogue of Eggen s UBV Data SIMBAD Bibcode 1986EgUBV 0M a b Gray 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 a b c d e f g h Kordopatis G Gilmore G Steinmetz M Boeche C Seabroke G M Siebert A Zwitter T Binney J et al November 2013 The Radial Velocity Experiment RAVE Fourth Data Release The Astronomical Journal 146 5 36 arXiv 1309 4284 Bibcode 2013AJ 146 134K doi 10 1088 0004 6256 146 5 134 S2CID 119221010 134 Reiners Ansgar January 2006 Rotation and temperature dependence of stellar latitudinal differential rotation Astronomy and Astrophysics 446 1 267 277 arXiv astro ph 0509399 Bibcode 2006A amp A 446 267R doi 10 1051 0004 6361 20053911 S2CID 8642707 a b c d e Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b Martinez Arnaiz R et al September 2010 Chromospheric activity and rotation of FGK stars in the solar vicinity An estimation of the radial velocity jitter PDF Astronomy and Astrophysics 520 A79 arXiv 1002 4391 Bibcode 2010A amp A 520A 79M doi 10 1051 0004 6361 200913725 S2CID 43455849 archived from the original PDF on 2017 09 22 retrieved 2018 11 04 tau06 Eri SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2016 10 13 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 Weinberger Alycia J Bryden Geoff Kennedy Grant M Roberge Aki Defrere Denis Hinz Philip M Millan Gabet Rafael Rieke George et al February 2015 Target Selection for the LBTI Exozodi Key Science Program The Astrophysical Journal Supplement Series 216 2 8 arXiv 1501 01319 Bibcode 2015ApJS 216 24W doi 10 1088 0067 0049 216 2 24 S2CID 38713562 24 Retrieved from https en wikipedia org w index php title Tau6 Eridani amp oldid 1176937022, wikipedia, wiki, book, books, library,

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