Astronomy:Upsilon Boötis

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Short description: Star in the constellation Boötes
Upsilon Boötis
Location of υ Boötis (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Boötes
Right ascension  13h 49m 28.641s[1]
Declination +15° 47′ 52.46″[1]
Apparent magnitude (V) 4.023[2]
Characteristics
Spectral type K5.5 III[3]
U−B color index +1.893[2]
B−V color index +1.518[2]
Astrometry
Radial velocity (Rv)−5.94±0.26[4] km/s
Proper motion (μ) RA: −93.269[1] mas/yr
Dec.: +40.166[1] mas/yr
Parallax (π)13.4228 ± 0.1380[1] mas
Distance243 ± 2 ly
(74.5 ± 0.8 pc)
Absolute bolometric
magnitude
 (Mbol)
−1.44±0.14[5]
Details
Mass1.11±0.33[6] M
Radius40.72+0.77
−0.79
[7] R
Luminosity332±54[6] L
Surface gravity (log g)1.5[4] cgs
Temperature3,920[6] K
Metallicity [Fe/H]−0.23[4] dex
Rotational velocity (v sin i)5.1[4] km/s
Age10.08±1.41[7] Gyr
Other designations
υ Boo, 5 Boötis, BD+16°2564, GC 18674, HD 120477, HIP 67459, HR 5200, SAO 100725, PPM 130100[8]
Database references
SIMBADdata

Upsilon Boötis is a single,[9] orange-hued star in the northern constellation of Boötes. Its name is a Bayer designation that is Latinized from υ Boötis, and abbreviated Upsilon Boo or υ Boo. This is a fourth[2] magnitude star that is visible to the naked eye. Based upon an annual parallax shift of 12.38 mas as seen from the Earth,[1] it is located about 243 light-years (75 pc) distant. The star is moving closer to the Sun with a radial velocity of −6 km/s.[4]

This is an evolved K-type giant star with a stellar classification of K5.5 III.[3] Astroseismology was used to obtain a mass estimate of 1.11 times the mass of the Sun,[6] while interferometric measurements give a size of about 38[5] times the Sun's radius. It is radiating about 332[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,920 K.[6] The star is roughly 10[7] billion years old and is spinning with a projected rotational velocity of 5.1 km/s.[4]

References

  1. 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940.  Gaia DR3 record for this source at VizieR.
  2. 2.0 2.1 2.2 2.3 Gutierrez-Moreno, Adelina et al. (1966), "A System of photometric standards", Publications of the Department of Astronomy University of Chile (Publicaciones Universidad de Chile, Department de Astronomy) 1: 1–17, Bibcode1966PDAUC...1....1G. 
  3. 3.0 3.1 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series 71: 245, doi:10.1086/191373, Bibcode1989ApJS...71..245K. 
  4. 4.0 4.1 4.2 4.3 4.4 4.5 Massarotti, Alessandro et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal 135 (1): 209–231, doi:10.1088/0004-6256/135/1/209, Bibcode2008AJ....135..209M. 
  5. 5.0 5.1 Piau, L. et al. (2010), "Surface convection and red giants radii measurements", Astronomy and Astrophysics 526: 12, doi:10.1051/0004-6361/201014442, A100, Bibcode2011A&A...526A.100P. 
  6. 6.0 6.1 6.2 6.3 6.4 6.5 Stello, D. et al. (2008), "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses", The Astrophysical Journal Letters 674 (1): L53–L56, doi:10.1086/528936, Bibcode2008ApJ...674L..53S. 
  7. 7.0 7.1 7.2 Baines, Ellyn K. et al. (2018), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer", The Astronomical Journal 155 (1): 30, doi:10.3847/1538-3881/aa9d8b, Bibcode2018AJ....155...30B .
  8. "ups Boo". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ups+Boo. 
  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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode2008MNRAS.389..869E.