30 Ophiuchi
Star in the constellation Ophiuchus
30 Ophiuchi
Location of 30 Ophiuchi (circled)
Observation dataEpoch J2000 Equinox ICRS
Constellation
Ophiuchus
Right ascension
17h 01m 03.60142s
Declination
−04° 13′ 21.5308″
Apparent magnitude (V)
4.82
Characteristics
Spectral type
K4III
U−B color index
+1.80
B−V color index
+1.48
Variable type
none
Astrometry Radial velocity (Rv )−6.70 km/s Proper motion (μ) RA: −39.13 mas /yr Dec.: −78.09 mas /yr Parallax (π)9.3138± 0.1676 mas Distance 350 ± 6 ly (107 ± 2 pc ) Absolute magnitude (MV )−0.65
Details Radius 35.89+0.54 −2.12 R ☉ Luminosity 299.8± 6.2 L ☉ Surface gravity (log g )1.73 cgs Temperature 4,009.00+126.67 −29.67 K Metallicity [Fe/H] −0.03 dex Rotational velocity (v sin i )1.4 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
Database references SIMBAD data
30 Ophiuchi is a single star in the equatorial constellation of Ophiuchus , and figures 0.99° east (specifically E½S ) of the heart of cluster Messier 10 . It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 4.82. The distance to this star is approximately 350 light years based on parallax . Its present motion is, net, one of approaching rather than parting, at − 6.7 km/s, its "radial velocity ".
This is an aging giant star with a stellar classification of K4III, having exhausted the supply of hydrogen at its core and expanded to 36 times the Sun's radius . The star is radiating 300 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,009 K. It is emitting a far infrared excess due to circumstellar dust, which extends out to a diameter of 240 AU and has a mass of 62× 1025 g .
The primary presents with two visual companions : B, at magnitude 9.71 and separation 99.8″, and C, at magnitude 8.75 and separation 220.9″ (3′ 40.9″) .
References
1 2 3 4 5 6 7 8 9 Brown, 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 at VizieR .
1 2 3 4 Anderson, 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
1 2 Hoffleit, 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 .
1 2 Mallama, 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
↑ 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 .
1 2 Gontcharov, 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 .
1 2 3 Van 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
↑ 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 .
↑ 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
↑ "30 Oph" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-06-19 .
↑ 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 .
↑ O'Meara, Stephen James (1998). Deep-Sky Companions: The Messier Objects . Cambridge University Press. p. 63. ISBN 9780521553322 .
↑ 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 .
↑ 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 .
↑ 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