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15 Orionis

15 Orionis is a suspected astrometric binary[9] star system in the equatorial constellation of Orion, near the border with Taurus. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.82.[2] The system is approximately 340 light years away from the Sun based on parallax. It is moving further from the Earth with a heliocentric radial velocity of +29 km/s,[4] having come to within 69 light-years some three million years ago.[5]

15 Orionis
Location of 15 Orionis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 09m 41.96481s[1]
Declination 15° 35′ 49.9051″[1]
Apparent magnitude (V) 4.82[2]
Characteristics
Spectral type F2IV[3]
U−B color index +0.19[2]
B−V color index +0.32[2]
Astrometry
Radial velocity (Rv)+28.79[4] km/s
Proper motion (μ) RA: −3.105[1] mas/yr
Dec.: –3.444[1] mas/yr
Parallax (π)9.5097 ± 0.2951 mas[1]
Distance340 ± 10 ly
(105 ± 3 pc)
Absolute magnitude (MV)−0.04[5]
Details
15 Ori A
Mass3.42±0.67[6] M
Radius5.9[7] R
Luminosity300[6] L
Surface gravity (log g)3.75[8] cgs
Temperature7,161+50
−49
[6] K
Metallicity [Fe/H]+0.21[8] dex
Rotational velocity (v sin i)60[6] km/s
Other designations
15 Ori, BD+15°752, GC 6306, HD 33276, HIP 24010, HR 1676, SAO 94359, CCDM J05097+1536AB, WDS J05097+1536AB
Database references
SIMBADdata

The primary component is an early F-type subgiant star with a stellar classification of F2 IV,[3] a star that has exhausted the hydrogen at its core and has begun to evolve into a giant. It has 3.42[6] times the mass of the Sun and 5.9[7] times the Sun's radius. The star still has a relatively high rotation rate, showing a projected rotational velocity of 60 km/s.[6] It is radiating 300 times the luminosity of the Sun from its expanding photosphere at an effective temperature of 7,161 K.[6]

It has one suspected companion, component B, at a separation of 0.3".[10]

References

  1. ^ a b c d e 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.
  2. ^ a b c d Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  3. ^ a b 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.
  4. ^ a b Massarotti, Alessandro; Latham, David W.; Stefanik, Robert P.; Fogel, Jeffrey (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.
  5. ^ a b 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
  6. ^ a b c d e f g Zorec, J.; Royer, F.; Asplund, Martin; Cassisi, Santi; Ramirez, Ivan; Melendez, Jorge; Bensby, Thomas; Feltzing, Sofia (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. S2CID 55586789.
  7. ^ a b Allende 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. ^ a b Wu, Yue; Singh, H. P.; Prugniel, P.; Gupta, R.; Koleva, M. (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. ^ 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. ^ 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

orionis, suspected, astrometric, binary, star, system, equatorial, constellation, orion, near, border, with, taurus, visible, naked, faint, yellow, white, hued, star, with, apparent, visual, magnitude, system, approximately, light, years, away, from, based, pa. 15 Orionis is a suspected astrometric binary 9 star system in the equatorial constellation of Orion near the border with Taurus It is visible to the naked eye as a faint yellow white hued star with an apparent visual magnitude of 4 82 2 The system is approximately 340 light years away from the Sun based on parallax It is moving further from the Earth with a heliocentric radial velocity of 29 km s 4 having come to within 69 light years some three million years ago 5 15 OrionisLocation of 15 Orionis circled Observation dataEpoch J2000 Equinox J2000Constellation OrionRight ascension 05h 09m 41 96481s 1 Declination 15 35 49 9051 1 Apparent magnitude V 4 82 2 CharacteristicsSpectral type F2IV 3 U B color index 0 19 2 B V color index 0 32 2 AstrometryRadial velocity Rv 28 79 4 km sProper motion m RA 3 105 1 mas yr Dec 3 444 1 mas yrParallax p 9 5097 0 2951 mas 1 Distance340 10 ly 105 3 pc Absolute magnitude MV 0 04 5 Details15 Ori AMass3 42 0 67 6 M Radius5 9 7 R Luminosity300 6 L Surface gravity log g 3 75 8 cgsTemperature7 161 50 49 6 KMetallicity Fe H 0 21 8 dexRotational velocity v sin i 60 6 km sOther designations15 Ori BD 15 752 GC 6306 HD 33276 HIP 24010 HR 1676 SAO 94359 CCDM J05097 1536AB WDS J05097 1536ABDatabase referencesSIMBADdataThe primary component is an early F type subgiant star with a stellar classification of F2 IV 3 a star that has exhausted the hydrogen at its core and has begun to evolve into a giant It has 3 42 6 times the mass of the Sun and 5 9 7 times the Sun s radius The star still has a relatively high rotation rate showing a projected rotational velocity of 60 km s 6 It is radiating 300 times the luminosity of the Sun from its expanding photosphere at an effective temperature of 7 161 K 6 It has one suspected companion component B at a separation of 0 3 10 References Edit a b c d e Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c d Ducati J R 2002 VizieR Online Data Catalog Catalogue of Stellar Photometry in Johnson s 11 color system CDS ADC Collection of Electronic Catalogues 2237 Bibcode 2002yCat 2237 0D a b 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 a b Massarotti Alessandro Latham David W Stefanik Robert P Fogel Jeffrey 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 a b 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 a b c d e f g Zorec J Royer F Asplund Martin Cassisi Santi Ramirez Ivan Melendez Jorge Bensby Thomas Feltzing Sofia 2012 Rotational velocities of A type stars IV Evolution of rotational velocities Astronomy and Astrophysics 537 A120 arXiv 1201 2052 Bibcode 2012A amp A 537A 120Z doi 10 1051 0004 6361 201117691 S2CID 55586789 a b Allende 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 amp A 352 555A Vizier catalog entry a b Wu Yue Singh H P Prugniel P Gupta R Koleva M 2010 Coude feed stellar spectral library atmospheric parameters Astronomy amp Astrophysics 525 A71 arXiv 1009 1491 Bibcode 2011A amp A 525A 71W doi 10 1051 0004 6361 201015014 S2CID 53480665 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 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 Retrieved from https en wikipedia org w index php title 15 Orionis amp oldid 1135309495, wikipedia, wiki, book, books, library,

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