Binary star in the constellation Boötes
Nu2 Boötis
ν
1 (right) and ν
2 (left) Boötis in optical light
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Boötes
Right ascension
15h 31m 46.98170s [ 1]
Declination
+40° 53′ 57.5405″[ 1]
Apparent magnitude (V)
5.02[ 2] (5.80 + 5.80) [ 3]
Characteristics
Spectral type
A5 V[ 4]
U−B color index
+0.11[ 2]
B−V color index
+0.07[ 2]
R−I color index
0.04
Astrometry Radial velocity (Rv ) −16.6± 3.7[ 5] km/sProper motion (μ) RA: -21.905[ 1] mas /yr Dec.: -7.876[ 1] mas /yr Parallax (π)7.8618 ± 0.1449 mas [ 1] Distance 415 ± 8 ly (127 ± 2 pc ) Absolute magnitude (MV )−0.59[ 6]
Orbit [ 7] Period (P) 9.026± 0.017 yr Semi-major axis (a) 0.0615± 0.0007 ″Eccentricity (e) 0.006± 0.015Inclination (i) 109.7± 1.2 °Longitude of the node (Ω) 199.4± 0.9 °Periastron epoch (T) 2000 .75± 0.24Argument of periastron (ω) (secondary) 293± 9 °
Details Mass 2.84± 0.11[ 8] M ☉ Radius 6.21+1.07 −0.81 [ 1] R ☉ Luminosity 135± 3[ 1] L ☉ Temperature 7894+574 −600 [ 1] K Rotational velocity (v sin i )217[ 8] km/s
Other designations ν2 Boo, ψ2 Her ,
53 Boötis ,
BD +41° 2611,
GC 20883,
HD 138629,
HIP 76041,
HR 5774,
SAO 45590,
ADS 9688,
CCDM 15318+4054,
WDS J15318+4054AB[ 9]
Database references SIMBAD data Data sources:
Hipparcos Catalogue ,CCDM (2002),Bright Star Catalogue (5th rev. ed.)
Nu2 Boötis is a white-hued binary star [ 10] system in the northern constellation of Boötes . It is faintly visible to the naked eye with a combined apparent visual magnitude of 5.02.[ 2] Based upon an annual parallax shift of 7.86 mas as seen from the Earth,[ 1] it is located roughly 415 light years from the Sun . The system is moving closer to the Sun with a radial velocity of −16.6 km/s.[ 5]
This stellar pair have a nearly circular orbit with a period of nine years and a semimajor axis of 0.0615 arc seconds .[ 10] They are both of visual magnitude 5.80 and display a similar spectrum , with the primary, component A, being an A-type main sequence star with a stellar classification of A5 V.[ 4] This has been identified as an A-type shell star , suggesting there is a circumstellar disk of gas orbiting one or both stars.[ 11] There are two other stars that appear close to the pair, termed C and D, but they are physically unrelated.[ 12]
Ptolemy considered Nu2 Boötis to be shared by Hercules , and Bayer assigned it a designation in both constellations: Nu2 Boötis (ν2 Boo) and Psi2 Herculis (ψ2 Her). When the modern constellation boundaries were fixed in 1930, the latter designation dropped from use.[ 13]
References
^ a b c d e f g h i 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 .
^ a b c d Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99): 99, Bibcode :1966CoLPL...4...99J .
^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal , 122 (6): 3466– 3471, Bibcode :2001AJ....122.3466M , doi :10.1086/323920
^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal , 74 : 375– 406, Bibcode :1969AJ.....74..375C , doi :10.1086/110819 .
^ a b de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14, arXiv :1208.3048 , Bibcode :2012A&A...546A..61D , doi :10.1051/0004-6361/201219219 , S2CID 59451347 , A61.
^ 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 .
^ Hartkopf, W. I.; et al. (June 30, 2006), Sixth Catalog of Orbits of Visual Binary Stars , United States Naval Observatory, archived from the original on 2017-08-01, retrieved 2017-09-13 .
^ a b Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics , 537 : A120, arXiv :1201.2052 , Bibcode :2012A&A...537A.120Z , doi :10.1051/0004-6361/201117691 , S2CID 55586789 .
^ "nu02 Boo" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-09-09 .
^ a b 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 .
^ Hauck, B.; Jaschek, C. (February 2000), "A-shell stars in the Geneva system", Astronomy and Astrophysics , 354 : 157– 162, Bibcode :2000A&A...354..157H .
^ Hutter, D. J.; Tycner, C.; Zavala, R. T.; Benson, J. A.; Hummel, C. A.; Zirm, H. (2021). "Surveying the Bright Stars by Optical Interferometry. III. A Magnitude-limited Multiplicity Survey of Classical Be Stars" . The Astrophysical Journal Supplement Series . 257 (2): 69. arXiv :2109.06839 . Bibcode :2021ApJS..257...69H . doi :10.3847/1538-4365/ac23cb . S2CID 237503492 .
^ "Bayer's Uranometria and Bayer letters" . Archived from the original on 2019-03-15. Retrieved 2012-05-18 .
External links
Hoffleit; et al. (1991), "HR 5774" , Bright Star Catalogue (5th Revised ed.), retrieved 2017-09-13 .
"Nu2 Boötis" , Aladin previewer , Centre de Données astronomiques de Strasbourg, retrieved 2017-09-12 .
Information related to Nu2 Boötis