Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 126053

From Wikipedia, the free encyclopedia
Star in the constellation Virgo
HD 126053

HD 126053 and brown dwarf companion (blue circle)
Credit:unWISE & Meli_thev
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationVirgo[1]
Right ascension14h 23m 15.285s[2]
Declination+01° 14′ 29.64″[2]
Apparent magnitude (V)6.25[3]
Characteristics
HD 126053 A
Evolutionary stageMain sequence[2]
Spectral typeG1 V[4]
U−Bcolor index+0.09[5]
B−Vcolor index0.639[3]
HD 126053 B
Evolutionary stageBrown dwarf
Spectral typesdT7.5[6]
Astrometry
Radial velocity (Rv)−19.17±0.06[3] km/s
Proper motion (μ)RA: 223.531mas/yr[2]
Dec.: −478.275mas/yr[2]
Parallax (π)57.2706±0.0375 mas[2]
Distance56.95 ± 0.04 ly
(17.46 ± 0.01 pc)
Absolute magnitude (MV)+5.07[1]
Details
HD 126053 A
Mass0.89[7] M
Radius0.93[8] R
Luminosity0.83[7] L
Luminosity (bolometric)0.812[9] L
Surface gravity (log g)4.57[10] cgs
Temperature5,722[10] K
Metallicity[Fe/H]−0.28[10] dex
Rotation22 d[11]
Rotational velocity (v sin i)3.08[4] km/s
Age5.490[12] Gyr
HD 126053 B
Mass0.019-0.047[13] M
Radius0.080-0.099[13] R
Temperature680±55[13] K
Metallicity−0.35[6]
Other designations
BD+01°2920,GJ 547,HD 126053,HIP 70319,HR 5384,SAO 120424[14]
Database references
SIMBADdata

HD 126053 is theHenry Draper Catalogue designation for a star in the equatorialconstellation ofVirgo. It has anapparent magnitude of 6.25,[3] which means it is faintly visible to the naked eye. According to theBortle scale, it requires dark suburban or rural skies to view.Parallax measurements made by theHipparcos spacecraft provide an estimated distance of 57 light years to this star.[2] It is drifting closer with a heliocentricradial velocity of −19.2 km/s.[3]

This star is considered asolar analog—meaning that it isphotometrically analogous to the Sun.[7] The physical properties of this star are similar to the Sun, although it ismetal poor.[13] Like the Sun, it has amagnetic activity cycle. It shares acommon proper motion through space with thespectroscopic binary star systemHD 122742, and in the past the three may have formed a triple star system. In theBright Star Catalogue, it was noted as having aninfrared excess. This may have been accreted from the HD 122742 system when the three stars were closer to each other.[15]

In 2012, abrown dwarf was discovered orbiting this star at a distance of 2630AU. This brown dwarf has a low temperature and is a T dwarf, with an estimated spectral type of T8p in the discovery paper. Discrepancies in the Y andK bands, likely due to lowmetallicity.[13] Later the spectral types of low metallicity brown dwarfs, calledsubdwarfs, were revisited. This led to a re-classification of sdT7.5 and a metallicity of [M/H]= −0.35.[6]

References

[edit]
  1. ^abAnderson, 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.
  2. ^abcdefVallenari, 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 atVizieR.
  3. ^abcdeSoubiran, C.; et al. (April 2013), "The catalogue of radial velocity standard stars for Gaia. I. Pre-launch release",Astronomy & Astrophysics,552: 11,arXiv:1302.1905,Bibcode:2013A&A...552A..64S,doi:10.1051/0004-6361/201220927,S2CID 56094559, A64.
  4. ^abMartínez-Arnáiz, R.; et al. (September 2010),"Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter"(PDF),Astronomy and Astrophysics,520: A79,arXiv:1002.4391,Bibcode:2010A&A...520A..79M,doi:10.1051/0004-6361/200913725,S2CID 43455849, archived fromthe original(PDF) on 2017-09-22, retrieved2018-11-04.
  5. ^Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  6. ^abcBurgasser, Adam J.; Schneider, Adam C.; Meisner, Aaron M.; Caselden, Dan; Hsu, Chih-Chun; Gerasimov, Roman; Aganze, Christian; Softich, Emma; Karpoor, Preethi (2024-11-08)."New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs".The Astrophysical Journal.982 (2): 79.arXiv:2411.01378.Bibcode:2025ApJ...982...79B.doi:10.3847/1538-4357/adb39f.
  7. ^abcDo Nascimento, J. D.; et al. (September 2010), "Rotation and lithium abundance of solar-analog stars. Theoretical analysis of observations",Astronomy and Astrophysics,519: 9,arXiv:1006.3861,Bibcode:2010A&A...519A.101D,doi:10.1051/0004-6361/200811026,S2CID 56098215, A101.
  8. ^Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics",Astronomy & Astrophysics,367 (2):521–24,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  9. ^Eiroa, C.; et al. (July 2013), "DUst around NEarby Stars. The survey observational results",Astronomy & Astrophysics,555: A11,arXiv:1305.0155,Bibcode:2013A&A...555A..11E,doi:10.1051/0004-6361/201321050,S2CID 377244.
  10. ^abcGray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–170,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637,S2CID 119476992.
  11. ^Baliunas, S.; Sokoloff, D.; Soon, W. (1996), "Magnetic Field and Rotation in Lower Main-Sequence Stars: an Empirical Time-dependent Magnetic Bode's Relation?",Astrophysical Journal Letters,457 (2): L99,Bibcode:1996ApJ...457L..99B,doi:10.1086/309891.
  12. ^Vican, Laura (June 2012), "Age Determination for 346 Nearby Stars in the Herschel DEBRIS Survey",The Astronomical Journal,143 (6): 135,arXiv:1203.1966,Bibcode:2012AJ....143..135V,doi:10.1088/0004-6256/143/6/135,S2CID 118539505.
  13. ^abcdePinfield, D. J.; et al. (May 2012), "Discovery of the benchmark metal-poor T8 dwarf BD +01° 2920B",Monthly Notices of the Royal Astronomical Society,422 (3):1922–1932,arXiv:1201.3243,Bibcode:2012MNRAS.422.1922P,doi:10.1111/j.1365-2966.2012.20549.x,S2CID 6257539.
  14. ^"HD 126053".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2015-11-13.{{cite web}}: CS1 maint: postscript (link)
  15. ^Frisch, P. C. (April 1993), "G-star astropauses - A test for interstellar pressure",Astrophysical Journal, Part 1,407 (1):198–206,Bibcode:1993ApJ...407..198F,doi:10.1086/172505.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
Messier
NGC
Numbered
Other
Galaxy clusters
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_126053&oldid=1328035203"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp