Astronomy:Beta Scuti

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Short description: Star in the constellation Scutum
β Scuti
Location of β Scuti (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Scutum[1]
Right ascension  18h 47m 10.474s[2]
Declination −04° 44′ 52.34″[2]
Apparent magnitude (V) 4.22[3]
Characteristics
Evolutionary stage Giant star
Spectral type G4IIa[4]
U−B color index +0.84[5]
B−V color index +1.09[5]
Astrometry
Radial velocity (Rv)−28.75±4.88[2] km/s
Proper motion (μ) RA: −7.972[2] mas/yr
Dec.: −16.398[2] mas/yr
Parallax (π)4.8549 ± 0.3403[2] mas
Distance670 ± 50 ly
(210 ± 10 pc)
Absolute magnitude (MV)−2.99[1]
Orbit[6]
Period (P)834 days
Semi-major axis (a)2.8 mas
Eccentricity (e)0.350
Inclination (i)105.9°
Longitude of the node (Ω)288.1°
Periastron epoch (T)2422480.9
Argument of periastron (ω)
(secondary)		33.9°
Details
Radius49.26+3.24
−3.72[7] R☉
Luminosity1,315±186[7] L☉
Surface gravity (log g)0.94[8] cgs
Temperature4,951±25[7] K
Metallicity [Fe/H]-0.16[1] dex
Rotational velocity (v sin i)7.8[9] km/s
Other designations
β Sct, BD−04°4582, FK5 1489, GC 25730, GSC 05122-01426, HIP 92175, HR 7063, HD 173764, SAO 142618, CCDM 18472-0445
Database references
SIMBADdata

Beta Scuti, Latinized from β Scuti, is a binary star system in the southern constellation Scutum. Based upon an annual parallax shift of 4.85 mas as seen from Earth,[2] it is located approximately 670 light years from the Sun.

Characteristics

This is a spectroscopic binary with an orbital period of 2.3 years and eccentricity around 0.35.[10] The secondary is about 3.3 magnitudes dimmer than the primary and estimated as type B9 based on the flux of far-ultraviolet radiation.[11]

The primary component has an apparent visual magnitude of +4.22 and is radiating about 1,315 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 4,951 K.[7] This yellow-hued star is a G-type bright giant with a stellar classification of G4 IIa.[4] Its angular diameter was measured at 2.121 milliarcseconds by the Navy Precision Optical Interferometer, which gives it a physical radius of approximately 49 R☉ at the estimated distance.[7]

The secondary was directly detected with a magnitude difference of 3.6 at a separation of about 17 milli-arcseconds using observations from the Navy Precision Optical Interferometer.[12] This detection was significant as observations with the Hubble Space Telescope which indicated a companion star was present were not definitive.[13] With an orbit and a parallax the sum of the masses of the two stars can be determined via a dynamical parallax.[14] This eventually can yield a precise mass for the evolved giant primary star.

Beta Scuti was a latter designation of 6 Aquilae.[15]

References

  1. ↑ 1.0 1.1 1.2 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 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.
  3. ↑ Mallik, Sushma V. (December 1999), "Lithium abundance and mass", Astronomy and Astrophysics 352: 495–507, Bibcode: 1999A&A...352..495M 
  4. ↑ 4.0 4.1 Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". The Astrophysical Journal Supplement Series 71: 245. doi:10.1086/191373. Bibcode: 1989ApJS...71..245K. 
  5. ↑ 5.0 5.1 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. 
  6. ↑ Ren, Shulin (2013). "Hipparcos Photocentric Orbits of 72 Single-lined Spectroscopic Binaries". The Astronomical Journal 145 (3): 81. doi:10.1088/0004-6256/145/3/81. Bibcode: 2013AJ....145...81R. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 Baines, Ellyn K.; Clark, James H., III; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01). "33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble". The Astronomical Journal 166 (6): 268. doi:10.3847/1538-3881/ad08be. ISSN 0004-6256. Bibcode: 2023AJ....166..268B. 
  8. ↑ Soubiran, Caroline; Le Campion, Jean-François; Brouillet, Nathalie; Chemin, Laurent (2016). "The PASTEL catalogue: 2016 version". Astronomy & Astrophysics 591: A118. doi:10.1051/0004-6361/201628497. Bibcode: 2016A&A...591A.118S. 
  9. ↑ De Medeiros, J. R.; Mayor, M. (1999). "A catalog of rotational and radial velocities for evolved stars". Astronomy and Astrophysics Supplement Series 139 (3): 433. doi:10.1051/aas:1999401. Bibcode: 1999A&AS..139..433D.  Vizier catalog entry
  10. ↑ Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G. et al. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics 424 (2): 727–732. doi:10.1051/0004-6361:20041213. Bibcode: 2004A&A...424..727P. 
  11. ↑ Parsons, Sidney B.; Ake, Thomas B. (1998). "Ultraviolet and Optical Studies of Binaries with Luminous Cool Primaries and Hot Companions. V. The Entire IUE Sample". The Astrophysical Journal Supplement Series 119 (1): 83. doi:10.1086/313152. Bibcode: 1998ApJS..119...83P. 
  12. ↑ Hutter, D. J.; Zavala, R. T.; Tycner, C.; Benson, J. A.; Hummel, C. A.; Sanborn, J.; Franz, O. G.; Johnston, K. J. (2016). "Surveying the Bright Stars by Optical Interferometry. I. A Search for Multiplicity among Stars of Spectral Types F-K". Astrophysical Journal Supplement Series 227 (1): 4. doi:10.3847/0067-0049/227/1/4. Bibcode: 2016ApJS..227....4H. 
  13. ↑ Parsons, S. B.; Franz, O. G.; Wassermann, L. H. (2005). "The Fine Guidance Sensor Orbit of the G4 Bright Giant HD 173764". Astronomical Journal 129 (3): 1700. doi:10.1086/427853. Bibcode: 2005AJ....129.1700P. 
  14. ↑ Heintz, Wulff D. (1978) (in en). Double Stars - Springer. 15. doi:10.1007/978-94-009-9836-0. ISBN 978-90-277-0886-1. Bibcode: 1978GAM....15.....H. 
  15. ↑ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy 18 (3): 212. doi:10.1177/002182868701800305. Bibcode: 1987JHA....18..209W. 



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