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HD 197027

From Wikipedia, the free encyclopedia
Star in the constellation Capricornus
HD 197027

HIP 102152
Credit:ESO/Digitized Sky Survey 2
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCapricornus
Right ascension20h 41m 54.6336s[1]
Declination−27° 12′ 57.4154″[1]
Apparent magnitude (V)9.15±0.02[2]
Characteristics
Spectral typeG3 V[3]
U−Bcolor index+0.30[4]
B−Vcolor index+0.65[2]
Astrometry
Radial velocity (Rv)−43.9±0.3[5] km/s
Proper motion (μ)RA: +175.628[1]mas/yr
Dec.: −15.593[1]mas/yr
Parallax (π)12.7715±0.0164 mas[1]
Distance255.4 ± 0.3 ly
(78.3 ± 0.1 pc)
Absolute magnitude (MV)4.74[6]
Details
Mass0.97[7] M
Radius1.08+0.07
−0.05
[8] R
Luminosity1.19[6] L
Surface gravity (log g)4.40±0.02[9] cgs
Temperature5718±5[9] K
Metallicity [Fe/H]−0.020±0.005[9] dex
Rotational velocity (v sin i)1.78±0.12[9] km/s
Age6.92±0.69[9] Gyr
Other designations
CD−27°14976,CPD−27°7079,HD 197027,HIP 102152,SAO 189585[10]
Database references
SIMBADdata

HD 197027 (HIP 102152) is astar in theconstellationCapricornus. It has anapparent magnitude of 9.15,[2] making it readily visible through atelescope but not to thenaked eye. The object is located at a distance of 255light years but is approaching theSolar System with a heliocentricradial velocity of−44 km/s.[5]

HD 197027 has astellar classification of G3 V, indicating that it is an ordinaryG-type main-sequence star like theSun. It has only 97% themass of the Sun[7] but 108% of its radius.[8] It shines at 119% theluminosity of the Sun[6] from itsphotosphere at aneffective temperature of 5,718K,[9] similar to the Sun's 5,778 K. HD 197027'smetallicity – elements heavier thanhelium – is similar to the Sun.[9] At an older age of 6.92billion years, it spins with aprojected rotational velocity of aboutkm/s.[9]

Since its measured properties of this star are very similar to those of the Sun, it has been considered a candidate oldersolar twin.[11] The abundances of 21elements overall are more similar to the Sun than any other known solar twin.[citation needed] Its Iron Abundance is -0.03 with an error value of 0.02 Fe/H. (The value comes from the Hipparcos Extended Catalog.)[12]

Age

[edit]
The age of HD 197027, here annotated as HIP 102152, shown relative to the Sun, the younger solar twin18 Scorpii and the formation of theMilky Way

References

[edit]
  1. ^abcdeBrown, 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 source atVizieR.
  2. ^abcHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^Houk, N. (1982).Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0.Bibcode:1982mcts.book.....H.
  4. ^Paunzen, E. (May 2022)."Catalogue of stars measured in the Geneva seven-colour photometric system".Astronomy & Astrophysics.661: A89.arXiv:2111.04810.Bibcode:2022A&A...661A..89P.doi:10.1051/0004-6361/202142355.eISSN 1432-0746.ISSN 0004-6361.
  5. ^abGontcharov, 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.eISSN 1562-6873.ISSN 1063-7737.S2CID 119231169.
  6. ^abcAnderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.ISSN 1063-7737.S2CID 255204555.
  7. ^abTalawanda R. Monroe; et al. (Aug 2013). "High Precision Abundances of the Old Solar Twin HIP 102152: Insights on Li Depletion from the Oldest Sun".Astrophysical Journal Letters.774 (2): L32.arXiv:1308.5744.Bibcode:2013ApJ...774L..32M.doi:10.1088/2041-8205/774/2/l32.S2CID 56111132.
  8. ^abStassun, Keivan G.; et al. (9 September 2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.ISSN 0004-6256.
  9. ^abcdefghdos Santos, Leonardo A.; et al. (August 2016), "The Solar Twin Planet Search. IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars",Astronomy & Astrophysics,592: 8,arXiv:1606.06214,Bibcode:2016A&A...592A.156D,doi:10.1051/0004-6361/201628558,S2CID 53533614, A156.
  10. ^"HD 197027".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2013-09-07.
  11. ^ESO, The life cycle of a Sun-like star (annotated), fromEuropean Southern Observatory, 28 August 2013
  12. ^"HD 197027 Star Distance, Age, Colour and other Facts - Universe Guide".universeguide.com. 10 January 2024. Retrieved2024-01-19.

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