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1 Naming  





2 References  





3 External links  














Tau Andromedae: Difference between revisions






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{{distinguish| text=[[T Andromedae]] }}

{{short description|Star in the constellation Andromeda}}

{{short description|Star in the constellation Andromeda}}

{{Starbox begin

{{Starbox begin}}

| name = Tau Andromedae

}}

{{Starbox image

{{Starbox image

| image =

| image =

{{Location mark

<div style="position: relative">[[File:Andromeda IAU.svg|250px|alt=Diagram showing star positions and boundaries of the Andromeda constellation and its surroundings]]

| image=Andromeda IAU.svg

<div style="position: absolute; left: 28.7%; top: 41.0%;">[[File:Cercle rouge 100%.svg|12px]]</div>

| float=center | width=240 | position=right

</div>

| mark=Red circle.svg | mark_width=10 | mark_link=τ And

| x%=31.4 | y%=44.0

}}

| caption=Location of τ Andromedae (circled)

| caption=Location of τ Andromedae (circled)

}}

}}

{{Starbox observe

{{Starbox observe

| epoch = J2000

| epoch = J2000

| ra = {{RA|01|40|34.81645}}<ref name=aaa474_2_653/>

| dec = {{DEC|+40|34|37.3742}}<ref name=aaa474_2_653/>

| appmag_v = +4.94<ref name=clpl4_99/>

| constell = [[Andromeda (constellation)|Andromeda]]

| constell = [[Andromeda (constellation)|Andromeda]]

| ra = {{RA|01|40|34.81619}}<ref name="Gaia EDR3"/>

| dec = {{DEC|+40|34|37.3397}}<ref name="Gaia EDR3"/>

| appmag_v = +4.94<ref name=clpl4_99/>

}}

}}

{{Starbox character

{{Starbox character

| class = B5&nbsp;III<ref name=apj694_2_1085/>

| class = B5&nbsp;III<ref name=apj694_2_1085/>

| b-v = -0.09<ref name=clpl4_99/>

| b-v = −0.09<ref name=clpl4_99/>

| u-b = -0.41<ref name=clpl4_99/>

| u-b = −0.41<ref name=clpl4_99/>

| variable =

| variable =

}}

}}

{{Starbox astrometry

{{Starbox astrometry

| radial_v = -14<ref name=gcsrv/>

| radial_v = {{val|−13.9|2.6}}<ref name=Gontcharov2006/>

| prop_mo_ra = +15.99<ref name=aaa474_2_653/>

| prop_mo_ra = {{val|17.889|(178)}}<ref name="Gaia EDR3"/>

| prop_mo_dec = -23.76<ref name=aaa474_2_653/>

| prop_mo_dec = {{val|−20.981|(95)}}<ref name="Gaia EDR3"/>

| parallax = 4.58

| parallax = 4.7804

| p_error = 0.25

| p_error = 0.1304

| parallax_footnote = <ref name=aaa474_2_653/>

| parallax_footnote = <ref name="Gaia EDR3"/>

| absmag_v =

| absmag_v =

}}

}}

{{Starbox detail

{{Starbox detail

| mass =

| mass =

| radius =

| radius =

| luminosity = 851<ref name=apjss176_1_276/>

| luminosity = 851<ref name=apjss176_1_276/>

| temperature = 13,026<ref name=PASTEL/>

| temperature = {{val|12680|100|fmt=commas}}<ref name=Huang_et_al_2010/>

| gravity = 3.357<ref name=PASTEL/>

| gravity = {{val|3.357|0.020}}<ref name=Huang_et_al_2010/>

| metal_fe =

| metal_fe =

| age_myr = 217<ref name=Gontcharov2012/>

| age_gyr =

| rotational_velocity = 80<ref name=apj573_1_359/>

| rotational_velocity = {{val|74|13}}<ref name=Huang_et_al_2010/>

}}

}}

{{Starbox catalog

{{Starbox catalog

| names = [[Flamsteed designation|53]]&nbsp;And, [[Star catalogue#BD.2FCD.2FCPD|BD]]+39&nbsp;378, [[Henry Draper Catalogue|HD]]&nbsp;10205, [[Hipparcos catalogue|HIP]]&nbsp;7818, [[Bright Star Catalog|HR]]&nbsp;477, [[Star catalogue#SAO|SAO]]&nbsp;37418.<ref name=SIMBAD/>

| names = {{odlist | B=τ And | F=53&nbsp;And |BD=+39&nbsp;378 |HD=10205 | HIP=7818 |HR=477 | SAO=37418 | PPM=44297 }}<ref name=SIMBAD/>

}}

}}

{{Starbox reference

{{Starbox reference

Line 50: Line 52:

{{Starbox end}}

{{Starbox end}}



'''Tau Andromedae''' And, τ Andromedae) is the [[Bayer designation]] for a [[star]] in the northern [[constellation]] of [[Andromeda (constellation)|Andromeda]]. It has an [[apparent visual magnitude]] of +4.94,<ref name=clpl4_99/> which is [[Bortle Dark-Sky Scale|bright enough]] to be viewed from dark suburban skies. From [[parallax]] measurements made during the [[Hipparcos]] mission, the distance to this star can be estimated as roughly {{Convert|710|ly|pc|abbr=off|lk=on}} from Earth. The brightness of this star is diminished by 0.24 in magnitude due to [[extinction (astronomy)|extinction]] caused by intervening gas and dust.<ref name=apj694_2_1085/>

'''Tau Andromedae''', [[Romanization of Greek|Latinized]] from τ Andromedae, is the [[Bayer designation]] for a single<ref name=Eggleton_Tokovinin_2008/> [[star]] in the northern [[constellation]] of [[Andromeda (constellation)|Andromeda]]. It has an [[apparent visual magnitude]] of +4.94,<ref name=clpl4_99/> which is [[Bortle Dark-Sky Scale|bright enough]] to be viewed from dark suburban skies. From [[parallax]] measurements made during the [[Gaia (spacecraft)|Gaia]] mission, the distance to this star can be estimated as roughly {{Convert|680|ly|pc|abbr=off|lk=on}} from Earth. The brightness of this star is diminished by 0.24 in magnitude due to [[extinction (astronomy)|extinction]] caused by intervening gas and dust.<ref name=apj694_2_1085/> It is drifting closer to the Sun with a [[radial velocity]] of −14&nbsp;km/s.<ref name=Gontcharov2006/>



The [[stellar spectrum|spectrum]] of this star matches a [[stellar classification]] of B5&nbsp;III,<ref name=apj694_2_1085/> with the [[luminosity class]] of III indicating that this is a [[giant star]]. It is radiating about 851 times the luminosity of the Sun.<ref name=apjss176_1_276/>

The [[stellar spectrum|spectrum]] of this star matches a [[stellar classification]] of B5&nbsp;III,<ref name=apj694_2_1085/> with the [[luminosity class]] of III indicating that this is a [[giant star]]. It is radiating about 851 times the luminosity of the Sun<ref name=apjss176_1_276/> from its [[photosphere]] at an [[effective temperature]] of 12,670&nbsp;K.<ref name=Huang_et_al_2010/> The star is an estimated 217<ref name=Gontcharov2012/>&nbsp;million years old and is spinning with a high [[projected rotational velocity]] of ~74&nbsp;km/s.<ref name=Huang_et_al_2010/>



==Naming==

==Naming==

Line 60: Line 62:

{{reflist|refs=

{{reflist|refs=



<ref name=Gontcharov2012>{{citation

<ref name=aaa474_2_653>{{citation | first=F. | last=van Leeuwen |date=November 2007 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | postscript=. |arxiv = 0708.1752 | s2cid=18759600 }}</ref>

| title=Spatial distribution and kinematics of OB stars

| last1=Gontcharov | first1=G. A.

| journal=Astronomy Letters

| volume=38 | issue=11 | pages=694–706 | date=November 2012

| doi=10.1134/S1063773712110035 | bibcode=2012AstL...38..694G

| arxiv=1606.09028 | s2cid=119108982 | postscript=. }}</ref>



<ref name=Gontcharov2006>{{citation

<ref name=apj694_2_1085>{{citation | last1=van Belle | first1=Gerard T. | last2=von Braun | first2=Kaspar | title=Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars | journal=The Astrophysical Journal | volume=694 | issue=2 | pages=1085–1098 |date=April 2009 | doi=10.1088/0004-637X/694/2/1085 | bibcode=2009ApJ...694.1085V | postscript=. |arxiv = 0901.1206 | s2cid=18370219 }}</ref>

| title=Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system

| last=Gontcharov | first=G. A.

| journal=Astronomy Letters | postscript=.

| volume=32 | issue=11 | pages=759–771 | date=November 2006

| doi=10.1134/S1063773706110065 | arxiv=1606.08053

| bibcode=2006AstL...32..759G | s2cid=119231169 }}</ref>



<ref name="Gaia EDR3">{{Cite Gaia EDR3|347218835681961344}}</ref>

<ref name=gcsrv>{{citation | last=Wilson | first=Ralph Elmer | year=1953 | title=General Catalogue of Stellar Radial Velocities | publisher=Carnegie Institution of Washington | location=Washington | bibcode=1953GCRV..C......0W | postscript=. }}</ref>



<ref name=apj694_2_1085>{{citation

<ref name=apj573_1_359>{{citation | last1=Abt | first1=Helmut A. | last2=Levato | first2=Hugo | last3=Grosso | first3=Monica | title=Rotational Velocities of B Stars | journal=The Astrophysical Journal | volume=573 | issue=1 | pages=359–365 |date=July 2002 | doi=10.1086/340590 | bibcode=2002ApJ...573..359A | postscript=. | doi-access=free }}</ref>

| last1=van Belle | first1=Gerard T. | last2=von Braun | first2=Kaspar

| title=Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars

| journal=The Astrophysical Journal

| volume=694 | issue=2 | pages=1085–1098 | date=April 2009

| doi=10.1088/0004-637X/694/2/1085 | bibcode=2009ApJ...694.1085V

| postscript=. | arxiv=0901.1206 | s2cid=18370219 }}</ref>



<ref name=clpl4_99>{{citation | display-authors=1 | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | bibcode=1966CoLPL...4...99J | postscript=. }}</ref>

<ref name=clpl4_99>{{citation | display-authors=1 | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | page=99 | bibcode=1966CoLPL...4...99J | postscript=. }}</ref>



<ref name=SIMBAD>{{cite simbad | title=* tau And | accessdate=2012-06-24 | postscript=. }}</ref>

<ref name=SIMBAD>{{cite simbad | title=* tau And | access-date=2012-06-24 }}</ref>



<ref name=apjss176_1_276>{{citation | display-authors=1 | last1=van Belle | first1=G. T. | last2=van Belle | first2=G. | last3=Creech-Eakman | first3=M. J. | last4=Coyne | first4=J. | last5=Boden | first5=A. F. | last6=Akeson | first6=R. L. | last7=Ciardi | first7=D. R. | last8=Rykoski | first8=K. M. | last9=Thompson | first9=R. R. | title=The Palomar Testbed Interferometer Calibrator Catalog | journal=The Astrophysical Journal Supplement Series | volume=176 | issue=1 | pages=276–292 |date=May 2008 | doi=10.1086/526548 | bibcode=2008ApJS..176..276V | postscript=. |arxiv = 0711.4194 | s2cid=10713221 }}</ref>

<ref name=apjss176_1_276>{{citation | display-authors=1 | last1=van Belle | first1=G. T. | last2=van Belle | first2=G. | last3=Creech-Eakman | first3=M. J. | last4=Coyne | first4=J. | last5=Boden | first5=A. F. | last6=Akeson | first6=R. L. | last7=Ciardi | first7=D. R. | last8=Rykoski | first8=K. M. | last9=Thompson | first9=R. R. | title=The Palomar Testbed Interferometer Calibrator Catalog | journal=The Astrophysical Journal Supplement Series | volume=176 | issue=1 | pages=276–292 |date=May 2008 | doi=10.1086/526548 | bibcode=2008ApJS..176..276V | postscript=. |arxiv = 0711.4194 | s2cid=10713221 }}</ref>



<ref name=PASTEL>{{citation

<ref name=Huang_et_al_2010>{{citation

| display-authors=1 | last1=Huang | first1=Wenjin

| last1=Soubiran | first1=Caroline | last2=Le Campion | first2=Jean-François

| last3=Brouillet | first3=Nathalie | last4=Chemin | first4=Laurent

| last2=Gies | first2=D. R. | last3=McSwain | first3=M. V.

| title=The PASTEL catalogue: 2016 version

| title=A Stellar Rotation Census of B Stars: From ZAMS to TAMS

| journal=Astronomy & Astrophysics | display-authors=1

| journal=Astrophysical Journal|language=en

| volume=591 | pages=A118 | year=2016

| volume=722 | issue=1 | pages=605–619 | date=October 2010

| bibcode=2016A&A...591A.118S | doi=10.1051/0004-6361/201628497

| doi=10.1088/0004-637X/722/1/605 | issn=0004-637X

| bibcode=2010ApJ...722..605H | arxiv=1008.1761

| arxiv=1605.07384 | s2cid=119258214 | postscript=. }}</ref>

| s2cid=118532653 | postscript=. }}</ref>


<ref name=Eggleton_Tokovinin_2008>{{citation

| last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A.

| title=A catalogue of multiplicity among bright stellar systems

| journal=[[Monthly Notices of the Royal Astronomical Society]]

| volume=389 | issue=2 | pages=869–879 |date=September 2008

| doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E

| postscript=. | arxiv=0806.2878 | s2cid=14878976 }}</ref>



}}

}}

Line 90: Line 119:

{{Stars of Andromeda}}

{{Stars of Andromeda}}



{{DEFAULTSORT:Tau Andromedae}}

[[Category:B-type giants]]

[[Category:Andromeda (constellation)]]

[[Category:Bayer objects|Andromedae, Tau]]

[[Category:Bayer objects|Andromedae, Tau]]

[[Category:Durchmusterung objects|BD+39 0378]]

[[Category:Flamsteed objects|Andromedae, 53]]

[[Category:Flamsteed objects|Andromedae, 53]]

[[Category:Andromeda (constellation)]]

[[Category:B-type giants]]

[[Category:Henry Draper Catalogue objects|010205]]

[[Category:Henry Draper Catalogue objects|010205]]

[[Category:Hipparcos objects|007818]]

[[Category:Hipparcos objects|007818]]

[[Category:HR objects|0477]]

[[Category:Bright Star Catalogue objects|0477]]

[[Category:Durchmusterung objects|BD+39 0378]]


Latest revision as of 06:08, 22 December 2023

Tau Andromedae

Location of τ Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 01h40m 34.81619s[1]
Declination +40° 34′ 37.3397″[1]
Apparent magnitude (V) +4.94[2]
Characteristics
Spectral type B5 III[3]
U−B color index −0.41[2]
B−V color index −0.09[2]
Astrometry
Radial velocity (Rv)−13.9±2.6[4] km/s
Proper motion (μ) RA: 17.889(178)[1] mas/yr
Dec.: −20.981(95)[1] mas/yr
Parallax (π)4.7804 ± 0.1304 mas[1]
Distance680 ± 20 ly
(209 ± 6 pc)
Details
Luminosity851[5] L
Surface gravity (log g)3.357±0.020[6] cgs
Temperature12,680±100[6] K
Rotational velocity (v sin i)74±13[6] km/s
Age217[7] Myr
Other designations

τ And, 53 And, BD+39 378, HD 10205, HIP 7818, HR 477, SAO 37418, PPM 44297[8]

Database references
SIMBADdata

Tau Andromedae, Latinized from τ Andromedae, is the Bayer designation for a single[9] star in the northern constellationofAndromeda. It has an apparent visual magnitude of +4.94,[2] which is bright enough to be viewed from dark suburban skies. From parallax measurements made during the Gaia mission, the distance to this star can be estimated as roughly 680 light-years (210 parsecs) from Earth. The brightness of this star is diminished by 0.24 in magnitude due to extinction caused by intervening gas and dust.[3] It is drifting closer to the Sun with a radial velocity of −14 km/s.[4]

The spectrum of this star matches a stellar classification of B5 III,[3] with the luminosity class of III indicating that this is a giant star. It is radiating about 851 times the luminosity of the Sun[5] from its photosphere at an effective temperature of 12,670 K.[6] The star is an estimated 217[7] million years old and is spinning with a high projected rotational velocity of ~74 km/s.[6]

Naming[edit]

InChinese, 天大將軍 (Tiān Dà Jiāng Jūn), meaning Heaven's Great General, refers to an asterism consisting of τ Andromedae, γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, 56 Andromedae, β Trianguli, γ Trianguli and δ Trianguli. Consequently, the Chinese name for τ Andromedae itself is 天大將軍七 (Tiān Dà Jiāng Jūn qī, English: the Seventh Star of Heaven's Great General.).[10]

References[edit]

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this sourceatVizieR.
  • ^ a b c d Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J.
  • ^ a b c van Belle, Gerard T.; von Braun, Kaspar (April 2009), "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars", The Astrophysical Journal, 694 (2): 1085–1098, arXiv:0901.1206, Bibcode:2009ApJ...694.1085V, doi:10.1088/0004-637X/694/2/1085, S2CID 18370219.
  • ^ a b Gontcharov, G. A. (November 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 van Belle, G. T.; et al. (May 2008), "The Palomar Testbed Interferometer Calibrator Catalog", The Astrophysical Journal Supplement Series, 176 (1): 276–292, arXiv:0711.4194, Bibcode:2008ApJS..176..276V, doi:10.1086/526548, S2CID 10713221.
  • ^ a b c d e Huang, Wenjin; et al. (October 2010), "A Stellar Rotation Census of B Stars: From ZAMS to TAMS", Astrophysical Journal, 722 (1): 605–619, arXiv:1008.1761, Bibcode:2010ApJ...722..605H, doi:10.1088/0004-637X/722/1/605, ISSN 0004-637X, S2CID 118532653.
  • ^ a b Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.
  • ^ "* tau And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-06-24.
  • ^ 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.
  • ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年710
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Tau_Andromedae&oldid=1191218315"

    Categories: 
    B-type giants
    Andromeda (constellation)
    Bayer objects
    Durchmusterung objects
    Flamsteed objects
    Henry Draper Catalogue objects
    Hipparcos objects
    Bright Star Catalogue objects
    Hidden categories: 
    Articles citing publications with errata
    Articles with Chinese-language sources (zh)
    Articles with short description
    Short description matches Wikidata
    Articles containing Chinese-language text
    Articles containing explicitly cited English-language text
     



    This page was last edited on 22 December 2023, at 06:08 (UTC).

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