Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Nu Virginis

Coordinates:Sky map11h 45m 52s, +06° 31′ 46″
From Wikipedia, the free encyclopedia
Variable star in the constellation Virgo
ν Virginis
Location of ν Virginis (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationVirgo
Right ascension11h 45m 51.5596s[1]
Declination+06° 31′ 45.749″[1]
Apparent magnitude (V)4.04[2]
Characteristics
Evolutionary stageasymptotic giant branch[3]
Spectral typeM1 III[4]
U−Bcolor index+1.80[2]
B−Vcolor index+1.52[2]
Astrometry
Radial velocity (Rv)50.19±0.30[5] km/s
Proper motion (μ)RA: −21.1mas/yr[1]
Dec.: −182.9mas/yr[1]
Parallax (π)9.8446±0.2744 mas[1]
Distance331 ± 9 ly
(102 ± 3 pc)
Absolute magnitude (MV)−0.87[6]
Details[7]
Mass0.92±0.00 M
Radius54.8±0.9 R
Luminosity523±31 L
Surface gravity (log g)1.0[5] cgs
Temperature3,728±47 K
Metallicity[Fe/H]−0.41 dex
Rotational velocity (v sin i)3.8[5] km/s
Age11.69±0.13 Gyr
Other designations
ν Vir,3 Virginis,BD+07°2479,FK5 1302,HD 102212,HIP 57380,HR 4517,SAO 119035[8]
Database references
SIMBADdata

ν Virginis,Latinized asNu Virginis, is a single[9]star in thezodiacconstellation ofVirgo, located at the western tip of the classic constellation and nearly due south of the prominent starDenebola.[10] It is a red-hued star with anapparent visual magnitude of 4.04[2] and can be seen with thenaked eye. Because the star lies near theecliptic it is subject tooccultations by theMoon.[11]Parallax measurements provide an estimated distance of around 331 light years from theSun,[1] and it is drifting further away with aradial velocity of +50 km/s.[5]

Alight curve for Nu Virginis, plotted fromHipparcos data[12]

This object is anM-typered giant, currently on theasymptotic giant branch,[3] with astellar classification of M1 III.[4] The star was discovered to be avariable star when theHipparcos data was analyzed.[13] It is an SRB-type[14]semiregularvariable star with its brightness varying by 0.0125 in magnitude.[15] These variations have four periods lasting 11.1, 12.3, 16.8, and 23.7 days.[16] This star has 90% themass of the sun, but it has expanded to 54 times theSun's radius and shines 520 times asbrightly as the Sun. Theeffective temperature of itsouter atmosphere is 3,728 K.[7]

References

[edit]
  1. ^abcdeVallenari, 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.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abEggen, Olin J. (July 1992), "Asymptotic giant branch stars near the sun",Astronomical Journal,104 (1):275–313,Bibcode:1992AJ....104..275E,doi:10.1086/116239.
  4. ^abMorgan, W. W.; Keenan, P. C. (1973), "Spectral Classification",Annual Review of Astronomy and Astrophysics,11:29–50,Bibcode:1973ARA&A..11...29M,doi:10.1146/annurev.aa.11.090173.000333.
  5. ^abcdMassarotti, Alessandro; et al. (January 2008), "Rotational and radial velocities for a sample of 761 HIPPARCOS giants and the role of binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209,S2CID 121883397.
  6. ^Pace, G.; et al. (April 2003), "The Wilson-Bappu effect: A tool to determine stellar distances",Astronomy and Astrophysics,401 (3):997–1007,arXiv:astro-ph/0301637,Bibcode:2003A&A...401..997P,doi:10.1051/0004-6361:20030163,S2CID 17029463.
  7. ^abBaines, Ellyn K.; Armstrong, J. Thomas; Schmitt, Henrique R.; Zavala, R. T.; Benson, James A.; Hutter, Donald J.; Tycner, Christopher; van Belle, Gerard T. (2017)."Fundamental parameters of 87 stars from the Navy Precision Optical Interferometer".The Astronomical Journal.155 (1): 16.arXiv:1712.08109.Bibcode:2018AJ....155...30B.doi:10.3847/1538-3881/aa9d8b.S2CID 119427037.
  8. ^"* nu. Vir".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2016-09-08.{{cite web}}: CS1 maint: postscript (link)
  9. ^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.
  10. ^Kaler, James B.,"Nu Virginis",STARS, retrieved2019-10-06.
  11. ^White, Nathaniel M.; Feierman, Barry H. (September 1987), "A Catalog of Stellar Angular Diameters Measured by Lunar Occultation",Astronomical Journal,94: 751,Bibcode:1987AJ.....94..751W,doi:10.1086/114513.
  12. ^"/ftp/cats/more/HIP/cdroms/cats".Centre de Données astronomiques de Strasbourg. Strasbourg astronomical Data Center. Retrieved15 October 2022.
  13. ^Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (January 1999)."The 74th Special Name-list of Variable Stars"(PDF).Information Bulletin on Variable Stars.4659:1–27.Bibcode:1999IBVS.4659....1K. Retrieved14 December 2024.
  14. ^Kazarovets, E. V.; et al. (1999), "The 74th Special Name-list of Variable Stars",Information Bulletin on Variable Stars,4659 (4659): 1,Bibcode:1999IBVS.4659....1K.
  15. ^Koen, Chris; Eyer, Laurent (March 2002)."New periodic variables from the Hipparcos epoch photometry".Monthly Notices of the Royal Astronomical Society.331 (1):45–59.arXiv:astro-ph/0112194.Bibcode:2002MNRAS.331...45K.doi:10.1046/j.1365-8711.2002.05150.x.S2CID 10505995.
  16. ^Tabur, V.; et al. (December 2009), "Long-term photometry and periods for 261 nearby pulsating M giants",Monthly Notices of the Royal Astronomical Society,400 (4):1945–1961,arXiv:0908.3228,Bibcode:2009MNRAS.400.1945T,doi:10.1111/j.1365-2966.2009.15588.x,S2CID 15358380.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
Messier
NGC
Other
Galaxy clusters
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=Nu_Virginis&oldid=1266665291"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp