Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

30 Ophiuchi

From Wikipedia, the free encyclopedia
Star in the constellation Ophiuchus
30 Ophiuchi
Location of 30 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension17h 01m 03.60142s[1]
Declination−4° 13′ 21.5308″[1]
Apparent magnitude (V)4.82[2]
Characteristics
Spectral typeK4III[3]
U−Bcolor index+1.80[4]
B−Vcolor index+1.48[4]
Astrometry
Radial velocity (Rv)−6.70[5] km/s
Proper motion (μ)RA: −39.13[6]mas/yr
Dec.: −78.09[6]mas/yr
Parallax (π)9.3138±0.1676 mas[1]
Distance350 ± 6 ly
(107 ± 2 pc)
Absolute magnitude (MV)−0.65[2]
Details
Radius35.89+0.54
−2.12
[1] R
Luminosity299.8±6.2[1] L
Surface gravity (log g)1.73[7] cgs
Temperature4,009.00+126.67
−29.67
[1] K
Metallicity [Fe/H]−0.03[2] dex
Rotational velocity (v sin i)1.4[8] km/s
Other designations
30 Oph,NSV 8111,BD−04°4215,FK5 1445,GC 22937,HD 153687,HIP 83262,HR 6318,SAO 141483,CCDM J17011-0413A,WDS J17011-0413A[9]
Database references
SIMBADdata

30 Ophiuchi is a single[10]star in theequatorialconstellation ofOphiuchus, and figures 0.99° east (specificallyE½S) of the heart of clusterMessier 10.[11] It is visible to the naked eye as a faint, orange-hued point of light with anapparent visual magnitude of 4.82.[2] The distance to this star is approximately 350 light years based onparallax.[6] Its present motion is, net, one of approaching rather than parting, at −6.7 km/s, its "radial velocity".[5]

This is an aginggiant star with astellar classification of K4III,[3] having exhausted the supply of hydrogen at itscore and expanded to 36[1] times theSun's radius. It is a suspectedvariable star.[12] The star is radiating 300[1] times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of 4,009 K.[1] It is emitting a farinfrared excess due to circumstellar dust,[13] which extends out to a diameter of240 AU and has a mass of62×1025 g.[14]

The primary presents with twovisual companions: B, at magnitude 9.71 and separation 99.8″, and C, at magnitude 8.75 and separation 220.9″ (3′ 40.9″).[15]

References

[edit]
  1. ^abcdefghiBrown, 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.
  2. ^abcdAnderson, 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.Vizier catalog entry
  3. ^abHoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050.Bibcode:1995yCat.5050....0H.
  4. ^abMallama, A. (2014). "Sloan Magnitudes for the Brightest Stars".The Journal of the American Association of Variable Star Observers.42 (2): 443.Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  5. ^abGontcharov, G. A. (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.S2CID 119231169.
  6. ^abcVan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  7. ^Soubiran, Caroline; Le Campion, Jean-François; Brouillet, Nathalie; Chemin, Laurent (2016). "The PASTEL catalogue: 2016 version".Astronomy & Astrophysics.591: A118.arXiv:1605.07384.Bibcode:2016A&A...591A.118S.doi:10.1051/0004-6361/201628497.S2CID 119258214.
  8. ^De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars".Astronomy & Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.S2CID 54046583.Vizier catalog entry
  9. ^"30 Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-19.
  10. ^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.
  11. ^O'Meara, Stephen James (1998).Deep-Sky Companions: The Messier Objects. Cambridge University Press. p. 63.ISBN 9780521553322.
  12. ^Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars".Astronomy Reports. 5.1.61 (1):80–88.Bibcode:2017ARep...61...80S.doi:10.1134/S1063772917010085.S2CID 125853869.
  13. ^Zuckerman, B.; et al. (June 1995)."Luminosity Class III Stars with Excess Far-Infrared Emission".Astrophysical Journal Letters.446: L79.Bibcode:1995ApJ...446L..79Z.doi:10.1086/187935.
  14. ^Jura, M. (April 1999)."Dust around First-Ascent Red Giants".The Astrophysical Journal.515 (2):706–711.Bibcode:1999ApJ...515..706J.doi:10.1086/307064.
  15. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.Vizier catalog entry
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Other
Galaxies
NGC
Other
Galaxy clusters
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=30_Ophiuchi&oldid=1241650926"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp