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==References==
==References==
{{reflist|refs=
{{reflist|refs=

<ref name="van Leeuwen2007">{{citation
| last1=van Leeuwen | first1=F.
| title=Validation of the new Hipparcos reduction
| journal=Astronomy and Astrophysics
| volume=474 | issue=2 | pages=653–664 | date=2007
| arxiv=0708.1752 | bibcode=2007A&A...474..653V
| doi=10.1051/0004-6361:20078357 | s2cid=18759600
| postscript=. }}</ref>

<ref name=luck2015>{{citation
| title=Abundances in the Local Region. I. G and K Giants
| journal=The Astronomical Journal
| last1=Luck | first1=R. Earle | postscript=.
| volume=150 | issue=3 | pages=88 | year=2015
| bibcode=2015AJ....150...88L | doi=10.1088/0004-6256/150/3/88
| arxiv=1507.01466 | s2cid=118505114
}}</ref>


<ref name=houk1979>{{citation
<ref name=houk1979>{{citation
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| year=1979 | volume=1
| year=1979 | volume=1
| bibcode=1978mcts.book.....H | postscript=. }}</ref>
| bibcode=1978mcts.book.....H | postscript=. }}</ref>

<ref name="Gontcharov2006">{{citation
| last1=Gontcharov | first1=G. A.
| 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 | date=November 2006
| doi=10.1134/S1063773706110065 | bibcode=2006AstL...32..759G
| postscript=. |arxiv = 1606.08053 | s2cid=119231169
}}</ref>


<ref name=Cousins1977>{{citation
<ref name=Cousins1977>{{citation
Line 122: Line 95:
| doi=10.1051/0004-6361/201425221 | bibcode=2015A&A...575A..35B
| doi=10.1051/0004-6361/201425221 | bibcode=2015A&A...575A..35B
| arxiv=1412.3648 | s2cid=59039482 | postscript=. }}</ref>
| arxiv=1412.3648 | s2cid=59039482 | postscript=. }}</ref>

<ref name=Alves2015>{{citation
| display-authors=1 | last1=Alves | first1=S.
| last2=Benamati | first2=L. | last3=Santos | first3=N. C.
| last4=Adibekyan | first4=V. Zh. | last5=Sousa | first5=S. G.
| last6=Israelian | first6=G. | last7=De Medeiros | first7=J. R.
| last8=Lovis | first8=C. | last9=Udry | first9=S.
| title=Determination of the spectroscopic stellar parameters for 257 field giant stars
| journal=Monthly Notices of the Royal Astronomical Society
| volume=448 | issue=3 | pages=2749–2765 | date=April 2015
| doi=10.1093/mnras/stv189 | bibcode=2015MNRAS.448.2749A
| arxiv=1503.02556 | postscript=. }}</ref>

<ref name=Mcdonald2012>{{citation
| display-authors=1 | last1=McDonald | first1=I.
| last2=Zijlstra | first2=A. A. | last3=Boyer | first3=M. L.
| title=Fundamental Parameters and Infrared Excesses of Hipparcos Stars
| journal=Monthly Notices of the Royal Astronomical Society
| volume=427 | issue=1 | pages=343–57 | date=2012
| bibcode=2012MNRAS.427..343M | arxiv=1208.2037
| doi = 10.1111/j.1365-2966.2012.21873.x | s2cid=118665352 | postscript=. }}</ref>

<ref name=aaa431_773>{{citation
| display-authors=1 | last1=Richichi | first1=A.
| last2=Percheron | first2=I. | last3=Khristoforova | first3=M.
| title=CHARM2: An updated Catalog of High Angular Resolution Measurements
| journal=Astronomy and Astrophysics
| volume=431 | pages=773–777 |date=February 2005
| issue=2 | doi=10.1051/0004-6361:20042039 | bibcode=2005A&A...431..773R
| postscript=. | doi-access=free }}</ref>

<ref name=lang2006>{{citation
| first1=Kenneth R. | last1=Lang
| title=Astrophysical formulae | volume=1
| series=Astronomy and astrophysics library | edition=3rd
| publisher=[[Birkhäuser]] | date=2006 | isbn=3-540-29692-1
| url=https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 | postscript=. }}. The radius (R<sub>*</sub>) is given by:
:<math>\begin{align} 2\cdot R_*
& = \frac{(43.2\cdot 2.32\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\
& \approx 21.6\cdot R_{\bigodot}
\end{align}</math></ref>


<ref name=csiro>{{citation
<ref name=csiro>{{citation

Revision as of 15:53, 30 May 2024

ζ Volantis
Location of ζ Volantis
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Volans
Right ascension 07h 41m 49.259s[1]
Declination −72° 36′ 21.957″[1]
Apparent magnitude (V) 3.918±0.003 [2]
Characteristics
Spectral type K0 III[3]
B−V color index 1.029±0.004 [2]
Astrometry
Radial velocity (Rv)48.5±0.14[1] km/s
Proper motion (μ) RA: +36.179 mas/yr[1]
Dec.: +14.816 mas/yr[1]
Parallax (π)22.4377 ± 0.0947 mas[1]
Distance147.09+0.68
−0.75
 ly
(45.12+0.21
−0.23
 pc)[1]
Absolute magnitude (MV)+0.75[4]
Details[2]
Mass1.224±0.155 M
Radius10.677±0.255 R
Luminosity60[1] L
Surface gravity (log g)2.82±0.09 cgs
Temperature4788±37 K
Metallicity [Fe/H]−0.17±0.03 dex
Age5.1±1.515 Gyr
Other designations
ζ Vol, CPD−72°627, FK5 297, HD 63295, HIP 37504, HR 3024, SAO 256438[5]
Database references
SIMBADdata

Zeta Volantis, Latinized from ζ Volantis, is a binary star[6] system in the southern constellation of Volans. It has an apparent visual magnitude of 3.91,[2] which is bright enough to be seen with the naked eye. Based upon measurements by the Gaia spacecraft, it is approximately 141 light-years (43 parsecs) from the Sun.[1] The companion is a magnitude 9.7 star at an angular separation of 16.7.[6] Based upon their motion through space, this system made its perihelion passage some 858,000 years ago when it came within 22 ly (6.6 pc) of the Sun.[7] It is currently moving away with a radial velocity of 48 km/s.[1]

The primary component is K-type giant star with a stellar classification of K0 III.[3] It has a derived luminosity of around 60 times that of the Sun,[1] 1.2 times the Sun's mass and is about 5.1 billion years old. At this age, it has expanded to 10.7 times the Sun's size.[2] The expanded outer envelope has an effective temperature of 4,788 K,[2] giving it the orange glow of a K-type star.[8]

References

  1. ^ a b c d e f g h i j Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ a b c d e f Gomes da Silva, J.; Santos, N. C.; Adibekyan, V.; Sousa, S. G.; Campante, T. L.; Figueira, P.; Bossini, D.; Delgado-Mena, E.; Monteiro, M. J. P. F. G.; de Laverny, P.; Recio-Blanco, A.; Lovis, C. (2021-02-01). "Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample. I. A catalogue of homogeneous chromospheric activity". Astronomy and Astrophysics. 646: A77. doi:10.1051/0004-6361/202039765. ISSN 0004-6361. Zeta Volantis' database entry at VizieR.
  3. ^ a b Houk, Nancy; Cowley, A. P. (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
  4. ^ 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.
  5. ^ "zet Vol -- High proper-motion Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2016-09-05.
  6. ^ a b 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.
  7. ^ Bailer-Jones, C. A. L. (March 2015), "Close encounters of the stellar kind", Astronomy & Astrophysics, 575: 13, arXiv:1412.3648, Bibcode:2015A&A...575A..35B, doi:10.1051/0004-6361/201425221, S2CID 59039482, A35.
  8. ^ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on 2013-12-03, retrieved 2012-01-16.
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