Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Iota Ophiuchi

From Wikipedia, the free encyclopedia
Star in the constellation Ophiuchus
Iota Ophiuchi
Location of ι Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationOphiuchus
Right ascension16h 54m 00.47151s[1]
Declination+10° 09′ 55.2982″[1]
Apparent magnitude (V)4.39[2]
Characteristics
Evolutionary stagemain sequence[3]
Spectral typeB8V[4]
U−Bcolor index−0.32[5]
B−Vcolor index−0.08[5]
Astrometry
Radial velocity (Rv)−19.0±1.6[6] km/s
Proper motion (μ)RA: −53.80[1]mas/yr
Dec.: −34.04[1]mas/yr
Parallax (π)13.30±0.22 mas[1]
Distance245 ± 4 ly
(75 ± 1 pc)
Absolute magnitude (MV)0.01[2]
Details
Mass3.14±0.03[3] M
Radius2.8[7] R
Luminosity141+6
−5
[3] L
Surface gravity (log g)4.03[8] cgs
Temperature11,220±78[3] K
Metallicity[Fe/H]+0.09[8] dex
Rotational velocity (v sin i)124[3] km/s
Age217[9] Myr
Other designations
ι Oph,25 Oph,BD+10°3092,FK5 1442,GC 22775,HD 152614,HIP 82673,HR 6281,SAO 102458[10]
Database references
SIMBADdata

ι Ophiuchi,Latinized asIota Ophiuchi, is a single[11]star in theequatorialconstellation ofOphiuchus, positioned near the constellation border withHercules. It makes a naked-eye double with nearbyKappa Ophiuchi,[12] appearing as a faint, blue-white hued star with anapparent visual magnitude of 4.39.[2] The star is approximately 245 light years from the Sun based on parallax,[1] but is drifting closer with aradial velocity of −19 km/s.[6]

This object is aB-type main-sequence star with astellar classification of B8V.[4] It is an estimated 217[9] million years old with a moderately high rate of spin, showing aprojected rotational velocity of 124 km/s.[3] The star has 3.1[3] times themass of the Sun and around 2.8[7] times theSun's radius. Iota Ophiuchi is radiating 141[3] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 11,220 K.[3] It displays aninfrared excess, suggesting the presence of circumstellar material.[13]

References

[edit]
  1. ^abcdefVan 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
  2. ^abcAnderson, 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. ^abcdefghiZorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars".Astronomy & Astrophysics.537: A120.arXiv:1201.2052.Bibcode:2012A&A...537A.120Z.doi:10.1051/0004-6361/201117691.S2CID 55586789.Vizier catalog entry
  4. ^abCowley, A. (November 1972). "Spectral classification of the bright B8 stars".Astronomical Journal.77:750–755.Bibcode:1972AJ.....77..750C.doi:10.1086/111348.
  5. ^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
  6. ^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.
  7. ^abAllende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures".Astronomy and Astrophysics.352:555–562.arXiv:astro-ph/9911002.Bibcode:1999A&A...352..555A.Vizier catalog entry
  8. ^abWu, Yue; et al. (2010). "Coudé-feed stellar spectral library – atmospheric parameters".Astronomy & Astrophysics.525: A71.arXiv:1009.1491.Bibcode:2011A&A...525A..71W.doi:10.1051/0004-6361/201015014.S2CID 53480665.
  9. ^abGontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars".Astronomy Letters.38 (11):694–706.arXiv:1606.09028.Bibcode:2012AstL...38..694G.doi:10.1134/S1063773712110035.S2CID 119108982.
  10. ^"iot Oph".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-09-05.
  11. ^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.
  12. ^Arnold, H. J. P.; et al. (1999).The Photographic Atlas of the Stars. CRC Press. p. 156.ISBN 9780750306546.
  13. ^McDonald, I.; et al. (2012)."Fundamental parameters and infrared excesses of Hipparcos stars".Monthly Notices of the Royal Astronomical Society.427 (1):343–357.arXiv:1208.2037.Bibcode:2012MNRAS.427..343M.doi:10.1111/j.1365-2966.2012.21873.x.S2CID 118665352.
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=Iota_Ophiuchi&oldid=1286918169"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp