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7 Boötis

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Star in the constellation Boötes
7 Boötis
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 13 53 12.93033
Declination +17° 55′ 58.3282″
Apparent magnitude (V) 5.71
Characteristics
Evolutionary stage Hertzsprung gap
Spectral type G5 III
B−V color index 0.845
Astrometry
Radial velocity (Rv)−11.00±0.18 km/s
Proper motion (μ) RA: −34.842 mas/yr
Dec.: +5.092 mas/yr
Parallax (π)5.5236 ± 0.0776 mas
Distance590 ± 8 ly
(181 ± 3 pc)
Details
Mass4.0±0.7 M
Radius19.0 R
Luminosity229 L
Temperature4,600 K
Metallicity +0.08 dex
Rotational velocity (v sin i)14.5 km/s
Other designations
7 Boo, BD+18°2795, HD 121107, HIP 67787, HR 5225, SAO 100751
Database references
SIMBADdata

7 Boötis is a single star in the northern constellation of Boötes, located 590 light-years away from the Sun. It is barely visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 5.71. 7 Boötis is moving closer to the Earth with a heliocentric radial velocity of −11 km/s.

This is an evolved giant star with a stellar classification of G5 III, currently at the end of the Hertzsprung gap. It has a weak level of magnetic activity but a fairly strong X-ray luminosity of 3.72×10 erg s. The rotation rate is moderate, with a projected rotational velocity of 14.5 km/s. It has four times the mass of the Sun and has expanded to 19 times the Sun's radius. The star is radiating 229 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,600 K.

References

  1. ^ 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.
  2. ^ Aurière, M.; et al. (February 2015), "The magnetic fields at the surface of active single G-K giants", Astronomy & Astrophysics, 574: 30, arXiv:1411.6230, Bibcode:2015A&A...574A..90A, doi:10.1051/0004-6361/201424579, S2CID 118504829, A90.
  3. 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.
  4. ^ "7 Boo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved September 13, 2018.
  5. 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.
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