Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 30479

From Wikipedia, the free encyclopedia
Star in the constellation Mensa
HD 30479
Observation data
Epoch J2000      Equinox J2000
ConstellationMensa
Right ascension04h 38m 21.7254s[1]
Declination−77° 39′ 21.6185″[1]
Apparent magnitude (V)6.04 ± 0.01[2]
Characteristics
Spectral typeK2 III[3]
U−Bcolor index+0.95[4]
B−Vcolor index+1.10[4]
Astrometry
Radial velocity (Rv)10.3 ± 0.1[5] km/s
Proper motion (μ)RA: −6.975[1]mas/yr
Dec.: −11.166[1]mas/yr
Parallax (π)6.0377±0.0223 mas[1]
Distance540 ± 2 ly
(165.6 ± 0.6 pc)
Absolute magnitude (MV)−0.05
Details
Mass1.28[6] M
Radius17.99[7] R
Luminosity116[8] L
Surface gravity (log g)2[9] cgs
Temperature4,390[9] K
Metallicity [Fe/H]−0.15[10] dex
Rotational velocity (v sin i)<1[11] km/s
Other designations
13 G. Mensae,CPD−77°181,FK5 2350,GC 5750,HD 30479,HIP 21611,HR 1531,SAO 256116
Database references
SIMBADdata

HD 30479 (HR 1531) is a solitary star in the southerncircumpolar constellationMensa. It has anapparent magnitude of 6.04,[2] making it barely visible to thenaked eye even under ideal conditions. It is located at a distance of 540light years[1] but is receding with a heliocentricradial velocity of10.3 km/s.[5]

HD 30479 has astellar classification of K2 III,[3] indicating that it is an earlyK-typegiant star and has anangular diameter of1.01±0.07 mas[9] (afterlimb darkening correction). This yields a radius 17.99[7] times that of theSun at its estimated distance. At present it has 1.28[6] times themass of the Sun and radiates at 116[8] times theluminosity of the Sun at aneffective temperature of 4,390[9]K from its enlarged photosphere, which gives it an orange glow. HD 30479 is believed to be one of the metal-deficient members of the young disk population[10] with an iron abundance of 71%[10] that of theSun. Currently, it spins leisurely with aprojected rotational velocity less thankm/s,[11] common for giants.

References

[edit]
  1. ^abcdefBrown, 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. ^abHøg, 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. ^abHouk, N.; Cowley, A. P. (1975).University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0.Bibcode:1975mcts.book.....H.
  4. ^abJohnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4:99–110.Bibcode:1966CoLPL...4...99J.
  5. ^abBrown, 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 atVizieR.
  6. ^abAnders, F.; et al. (1 August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18".Astronomy and Astrophysics.628: A94.arXiv:1904.11302.Bibcode:2019A&A...628A..94A.doi:10.1051/0004-6361/201935765.ISSN 0004-6361.S2CID 131780028.
  7. ^abLang, Kenneth R. (2006).Astrophysical formulae. Astronomy and astrophysics library. Vol. 1 (3 ed.).Birkhäuser.ISBN 3-540-29692-1.. The radius (R*) is given by:
    2R=(165.61.01103) AU0.0046491 AU/R35.98R{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(165.6\cdot 1.01\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 35.98\cdot R_{\bigodot }\end{aligned}}}
  8. ^abMcDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017)."Fundamental parameters and infrared excesses of Tycho-Gaia stars".Monthly Notices of the Royal Astronomical Society.471 (1): 770.arXiv:1706.02208.Bibcode:2017MNRAS.471..770M.doi:10.1093/mnras/stx1433.
  9. ^abcdLafrasse, Sylvain; Mella, Guillaume; Bonneau, Daniel; Duvert, Gilles; Delfosse, Xavier; Chesneau, Olivier; Chelli, Alain (16 July 2010). "Building the 'JMMC Stellar Diameters Catalog' using SearchCal".Optical and Infrared Interferometry II. Vol. 7734. pp. 77344E.arXiv:1009.0137.Bibcode:2010SPIE.7734E..4EL.doi:10.1117/12.857024.S2CID 32097037.
  10. ^abcEggen, O. J. (February 1994)."Evolved GK stars near the Sun. 2: The young disk population".The Astronomical Journal.107: 594.Bibcode:1994AJ....107..594E.doi:10.1086/116879.ISSN 0004-6256.
  11. ^abDe Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014)."A catalog of rotational and radial velocities for evolved stars: V. Southern stars⋆⋆⋆".Astronomy & Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.ISSN 0004-6361.
Stars
Bayer
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
NGC
Other
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_30479&oldid=1183280993"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp