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Alpha Scuti

Today, Alpha Scuti has become a topic of great relevance and interest to a wide spectrum of society. From its impact on the economy to its influence on political decisions, Alpha Scuti has positioned itself as a central topic in current conversations and discussions. In order to better understand this phenomenon, it is important to analyze its different dimensions and consequences. In this article, we will explore in depth the various facets of Alpha Scuti and how they have shaped and impacted our environment.

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α Scuti
Location of α Scuti (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Scutum[1]
Right ascension 18h 35m 12.42776s[2]
Declination −08° 14′ 38.6529″[2]
Apparent magnitude (V) 3.83[3]
Characteristics
Spectral type K3III[4]
U−B color index +1.53[3]
B−V color index +1.34[3]
Astrometry
Radial velocity (Rv)+36.50[5] km/s
Proper motion (μ) RA: −17.00[2] mas/yr
Dec.: −313.52[2] mas/yr
Parallax (π)16.38±0.22 mas[2]
Distance199 ± 3 ly
(61.1 ± 0.8 pc)
Absolute magnitude (MV)−0.08[1]
Details
Mass1.33[6] M☉
Radius20[6] R☉
Luminosity186[1] L☉
Surface gravity (log g)1.96[6] cgs
Temperature4,315[7] K
Metallicity −0.04[1] dex
Rotational velocity (v sin i)1.7[8] km/s
Other designations
α Sct, BD−08°4638, FK5 1482, GC 25385, HD 171443, HIP 91117, HR 6973, LTT 7377, NSV 11056, SAO 142408
Database references
SIMBADdata

Alpha Scuti, Latinized from α Scuti, is an orange-hued star in the southern constellation of Scutum. Originally part of the Aquila constellation, Alpha Scuti was a latter designation of 1 Aquilae.[9] It is faintly visible to the naked eye with an apparent visual magnitude of 3.83.[3] Based upon an annual parallax shift of 16.38 mas as seen from the Earth,[2] it is located around 199 light years from the Sun. It is moving away from the Sun with a radial velocity of +36.5 km/s.[5]

Properties

With a stellar classification of K3 III,[4] the spectrum indicates it is an evolved giant star of type K. Alpha Scuti is a suspected variable star with magnitude range reported as 3.81 to 3.87.[10] The star has an estimated 1.33 times the mass of the Sun, but the outer envelope has expanded to 20 times the Sun's radius.[6] It is radiating 186[1] times the Sun's luminosity from its inflated photosphere at an effective temperature of 4,315 K.[7]

References

  1. ^ a b c d e 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. XHIP record for this object at VizieR.
  2. ^ a b c d e f Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  3. ^ 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.
  4. ^ a b 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. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
  5. ^ 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.
  6. ^ a b c d 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
  7. ^ a b Martínez, M. Isabel Pérez; Schröder, K.-P.; Cuntz, M. (2011). "The basal chromospheric Mg ii h+k flux of evolved stars: Probing the energy dissipation of giant chromospheres". Monthly Notices of the Royal Astronomical Society. 414 (1): 418–427. arXiv:1102.4832. Bibcode:2011MNRAS.414..418P. doi:10.1111/j.1365-2966.2011.18421.x. S2CID 59268230. Vizier catalog entry
  8. ^ De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics. 561: A126. arXiv:1312.3474. Bibcode:2014A&A...561A.126D. doi:10.1051/0004-6361/201220762. S2CID 54046583. Vizier catalog entry
  9. ^ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy. 18 (3): 212. Bibcode:1987JHA....18..209W. doi:10.1177/002182868701800305. S2CID 118445625.
  10. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
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