Iota Tauri: Difference between revisions
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{{Short description|Double star in the constellation Taurus}} |
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{{unreferenced|date=December 2009}} |
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{{Starbox |
{{Starbox begin |
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| name = ι Tauri |
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epoch=[[J2000.0]] | |
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ra=05<sup>h</sup> 03<sup>m</sup> 05.7<sup>s</sup> | |
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dec=+21° 35' 24" | |
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spectral=A7V | |
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appmag_v=+4.62 | |
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dist_ly=163 ± 7 | |
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dist_pc=50 ± 2 | |
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names=102 Tauri, [[Star catalogue#BS, BSC, HR|HR]] 1620, [[Henry Draper Catalogue|HD]] 32301, [[Star catalogue#BD/CD/CPD|BD]]+21 751, FK5 184, [[Hipparcos catalogue|HIP]] 23497, [[Star catalogue#SAO|SAO]] 76920. |
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}} |
}} |
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{{Starbox image |
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'''Iota Tauri''' (ι Tau, ι Tauri) is a [[star]] in the [[constellation]] [[Taurus (constellation)|Taurus]] and an outlying member of the [[Hyades (star cluster)|Hyades]] [[open cluster|star cluster]]. |
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|image= |
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{{Location mark |
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|image=Taurus constellation map.svg|alt=|float=center|width=280 |
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|label=|position=right |
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|mark=Red circle.svg|mark_width=10|mark_link=Iota Tauri |
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|x=325|y=397 |
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}} |
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|caption=Location of ι Tauri (circled) |
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}} |
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{{Starbox observe |
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| epoch = J2000 |
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⚫ | |||
| ra = {{RA|05|03|05.74725}}<ref name=vanLeeuwen2007>{{cite journal | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | year=2007 | last1=Van Leeuwen | first1=F. | s2cid=18759600 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2023497 Vizier catalog entry]</ref> |
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| dec = {{DEC|21|35|23.8627}}<ref name=vanLeeuwen2007/> |
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| appmag_v = 4.62<ref name=XHIP>{{cite journal | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | title=XHIP: An extended hipparcos compilation | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | s2cid=119257644 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V/137D/XHIP&HIP=23497 Vizier catalog entry]</ref> |
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}} |
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{{Starbox character |
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| class = A7 V<ref name=Abt1995>{{cite journal | bibcode=1995ApJS...99..135A | title=The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars | journal=Astrophysical Journal Supplement | volume=99 | pages=135 | last1=Abt | first1=Helmut A. | last2=Morrell | first2=Nidia I. | year=1995 | doi=10.1086/192182 | doi-access=free }}</ref> |
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| b-v = +0.16<ref name=Mallama2014>{{cite journal | bibcode=2014JAVSO..42..443M | title=Sloan Magnitudes for the Brightest Stars | journal=The Journal of the American Association of Variable Star Observers | volume=42 | pages=443 | last1=Mallama | first1=A. | year=2014 | issue=2 }}[http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/other/JAVSO/42.443/ugriz&HD=032301 Vizier catalog entry]</ref> |
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| u-b = +0.15<ref name=Mallama2014/> |
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}} |
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{{Starbox astrometry |
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| radial_v = +38.30<ref name=Gontcharov2006>{{Cite journal | doi=10.1134/S1063773706110065 | bibcode=2006AstL...32..759G| title=Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system| journal=Astronomy Letters| volume=32| issue=11| pages=759–771| year=2006| last1=Gontcharov| first1=G. A.|arxiv = 1606.08053 | s2cid=119231169}}</ref> |
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| prop_mo_ra = +68.88<ref name=vanLeeuwen2007/> |
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| prop_mo_dec = -41.06<ref name=vanLeeuwen2007/> |
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| parallax = 18.88 |
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| p_error = 0.30 |
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| parallax_footnote = <ref name=vanLeeuwen2007/> |
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| absmag_v = 1.00<ref name=XHIP/> |
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}} |
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{{Starbox detail |
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| mass = 2.22<ref name=Zorec2012>{{cite journal | arxiv=1201.2052 | bibcode=2012A&A...537A.120Z | doi=10.1051/0004-6361/201117691 | title=Rotational velocities of A-type stars | journal=Astronomy & Astrophysics | volume=537 | pages=A120 | year=2012 | last1=Zorec | first1=J. | last2=Royer | first2=F. | s2cid=55586789 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/A%2bA/537/A120/table1&HD=32301 Vizier catalog entry]</ref> |
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| radius = 2.6<ref name=AllendePrieto>{{cite journal | bibcode=1999A&A...352..555A | arxiv=astro-ph/9911002 | title=Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures | journal=Astronomy and Astrophysics | volume=352 | pages=555–562 | last1=Allende Prieto | first1=C. | last2=Lambert | first2=D. L. | year=1999 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/A%2bA/352/555/table1&Name=HIP23497 Vizier catalog entry]</ref> |
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| temperature = 8,054<ref name=Zorec2012/> |
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| luminosity = 36<ref name=Zorec2012/> |
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| rotational_velocity = 131<ref name=Zorec2012/> |
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| gravity = 3.97<ref name=David2015>{{cite journal | bibcode=2015ApJ...804..146D | doi=10.1088/0004-637X/804/2/146 | arxiv=1501.03154 | title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets | journal=The Astrophysical Journal | volume=804 | issue=2 | pages=146 | year=2015 | last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A. | s2cid=33401607 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/ApJ/804/146/table5&HIP=23497 Vizier catalog entry]</ref> |
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| metal_fe = +0.15<ref name=XHIP/> |
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| age_myr = 717<ref name=David2015/> |
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}} |
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{{Starbox catalog |
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| names = {{odlist | B=ι Tau | F=102 Tauri | BD=+21° 751 | FK5=184 | HD=32301 | HIP=23497 | HR=1620 | SAO=76920 | GC=6158 | GSC=01293-02747 | WDS=J05031+2135AB }} |
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}} |
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{{Starbox reference |
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| Simbad = Iota+Tauri |
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}} |
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{{Starbox end}} |
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'''Iota Tauri''', [[Latinisation of names|Latinized]] from ι Tauri, is a white-hued [[star]] in the [[zodiac]] [[constellation]] [[Taurus (constellation)|Taurus]] and an outlying member of the [[Hyades (star cluster)|Hyades]] [[open cluster|star cluster]].<ref name=Varenne1999>{{citation | title=Chemical abundances of A and F-type stars: the Hyades open cluster | last1=Varenne | first1=O. | last2=Monier | first2=R. | journal=Astronomy and Astrophysics | volume=351 | pages=247–266 | date=November 1999 | bibcode=1999A&A...351..247V | postscript=. }}</ref> It is visible to the naked eye with an [[apparent visual magnitude]] of 4.62,<ref name=XHIP/> and is located at an estimated distance of about 173 [[light year]]s based upon [[stellar parallax|parallax measurements]].<ref name=vanLeeuwen2007/> The star is moving away from the Sun with a [[radial velocity]] of +38 km/s.<ref name=Gontcharov2006/> |
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Iota Tauri is a white [[stellar classification|A-type]] [[main sequence|main sequence dwarf]] with an [[apparent magnitude]] of +4.62. It is approximately 163 [[light years]] from [[Earth]]. |
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This has been reported as a double star with two components at separation 0.1", both of type A7V and magnitude 5.4.<ref name=WDS>{{cite journal | bibcode=2001AJ....122.3466M | doi=10.1086/323920 | title=The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog | journal=The Astronomical Journal | volume=122 | issue=6 | pages=3466 | year=2001 | last1=Mason | first1=Brian D. | last2=Wycoff | first2=Gary L. | last3=Hartkopf | first3=William I. | last4=Douglass | first4=Geoffrey G. | last5=Worley | first5=Charles E. | doi-access=free }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=B/wds/wds&WDS=05031%2B2135 Vizier catalog entry]</ref><ref name=Eggleton2008>{{cite journal | bibcode=2008MNRAS.389..869E | doi=10.1111/j.1365-2966.2008.13596.x | arxiv = 0806.2878 | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869 | year=2008 | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | doi-access=free | s2cid=14878976 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/MNRAS/389/869/table1&mHR=1620 Vizier catalog entry]</ref> The combined [[stellar spectrum|spectrum]] matches a [[stellar classification]] of A7 V,<ref name=Abt1995/> which would normally indicate an [[A-type main-sequence star]] that is generating energy through [[hydrogen fusion]] at its [[stellar core|core]]. It has an estimated age of 717<ref name=David2015/> million years. |
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==References== |
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{{reflist}} |
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{{Stars of Taurus}} |
{{Stars of Taurus}} |
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{{DEFAULTSORT:Iota Tauri}} |
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[[Category:A-type main-sequence stars]] |
[[Category:A-type main-sequence stars]] |
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[[Category:Hyades (star cluster)]] |
[[Category:Hyades (star cluster)]] |
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[[Category:Durchmusterung objects|BD+21 0751]] |
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[[Category:Flamsteed objects|Tauri, 102]] |
[[Category:Flamsteed objects|Tauri, 102]] |
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[[Category:Henry Draper Catalogue objects|032301]] |
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[[Category:Hipparcos objects|023497]] |
[[Category:Hipparcos objects|023497]] |
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[[Category:Bright Star Catalogue objects|1620]] |
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{{Main-star-stub}} |
Latest revision as of 05:16, 21 August 2024
Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Taurus |
Right ascension | 05h 03m 05.74725s[1] |
Declination | 21° 35′ 23.8627″[1] |
Apparent magnitude (V) | 4.62[2] |
Characteristics | |
Spectral type | A7 V[3] |
U−B color index | +0.15[4] |
B−V color index | +0.16[4] |
Astrometry | |
Radial velocity (Rv) | +38.30[5] km/s |
Proper motion (μ) | RA: +68.88[1] mas/yr Dec.: -41.06[1] mas/yr |
Parallax (π) | 18.88 ± 0.30 mas[1] |
Distance | 173 ± 3 ly (53.0 ± 0.8 pc) |
Absolute magnitude (MV) | 1.00[2] |
Details | |
Mass | 2.22[6] M☉ |
Radius | 2.6[7] R☉ |
Luminosity | 36[6] L☉ |
Surface gravity (log g) | 3.97[8] cgs |
Temperature | 8,054[6] K |
Metallicity [Fe/H] | +0.15[2] dex |
Rotational velocity (v sin i) | 131[6] km/s |
Age | 717[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Iota Tauri, Latinized from ι Tauri, is a white-hued star in the zodiac constellation Taurus and an outlying member of the Hyades star cluster.[9] It is visible to the naked eye with an apparent visual magnitude of 4.62,[2] and is located at an estimated distance of about 173 light years based upon parallax measurements.[1] The star is moving away from the Sun with a radial velocity of +38 km/s.[5]
This has been reported as a double star with two components at separation 0.1", both of type A7V and magnitude 5.4.[10][11] The combined spectrum matches a stellar classification of A7 V,[3] which would normally indicate an A-type main-sequence star that is generating energy through hydrogen fusion at its core. It has an estimated age of 717[8] million years.
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&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
- ^ a b c d Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644. Vizier catalog entry
- ^ a b Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". Astrophysical Journal Supplement. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182.
- ^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42 (2): 443. Bibcode:2014JAVSO..42..443M.Vizier catalog entry
- ^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
- ^ a b c d Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars". Astronomy & Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. S2CID 55586789. Vizier catalog entry
- ^ Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv:astro-ph/9911002. Bibcode:1999A&A...352..555A. Vizier catalog entry
- ^ a b c David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv:1501.03154. Bibcode:2015ApJ...804..146D. doi:10.1088/0004-637X/804/2/146. S2CID 33401607. Vizier catalog entry
- ^ Varenne, O.; Monier, R. (November 1999), "Chemical abundances of A and F-type stars: the Hyades open cluster", Astronomy and Astrophysics, 351: 247–266, Bibcode:1999A&A...351..247V.
- ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920. Vizier catalog entry
- ^ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976. Vizier catalog entry