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Eta Scuti

Eta Scuti, Latinized from η Scuti, is a single[10] star in the southern constellation of Scutum, near the constellation border with Aquila. Eta Scuti was a latter designation of 9 Aquilae before the official constellation borders were set in 1922.[11] It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of +4.83.[2] This object is located approximately 213 light-years from the Sun based on parallax, and is drifting further away with a radial velocity of −92.[1]

η Scuti
Location of η Scuti (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Scutum
Right ascension 18h 57m 03.67027s[1]
Declination −5° 50′ 46.7305″[1]
Apparent magnitude (V) 4.83[2]
Characteristics
Evolutionary stage horizontal branch[3]
Spectral type K1-III[4]
U−B color index +1.02[5]
B−V color index +1.08[5]
Astrometry
Radial velocity (Rv)−92.22±0.16[1] km/s
Proper motion (μ) RA: +61.545[1] mas/yr
Dec.: −41.429[1] mas/yr
Parallax (π)15.2960 ± 0.1740 mas[1]
Distance213 ± 2 ly
(65.4 ± 0.7 pc)
Absolute magnitude (MV)0.87[2]
Details
Mass1.50[6] M
Radius11.97+0.18
−0.13
[1] R
Luminosity62.7±0.8[1] L
Surface gravity (log g)2.54[6] cgs
Temperature4,693+27
−266
[1] K
Metallicity [Fe/H]−0.03[6] dex
Rotational velocity (v sin i)< 1.0[7] km/s
Age2.8[8] Gyr
Other designations
η Sct, BD−06°4976, FK5 3821, GC 26013, HD 175751, HIP 93026, HR 7149, SAO 142838, GSC 05127-07358[9]
Database references
SIMBADdata

This is an aging giant star with a stellar classification of K1-III.[4] After exhausting the supply of hydrogen at its core, the star cooled and expanded until currently it has 12[1] times the girth of the Sun. It is a red clump giant, which indicates it is presently on the horizontal branch and is generating energy through core helium fusion.[3] The star is about 2.8 billion years old[8] with 1.5 times the mass of the Sun.[6] It is radiating 63[1] times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,693 K.[1]

References

  1. ^ a b c d e f g h i j k l m 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.
  2. ^ a b c 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. Vizier catalog entry
  3. ^ a b Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal, 539 (2): 732–741, arXiv:astro-ph/0003329, Bibcode:2000ApJ...539..732A, doi:10.1086/309278, S2CID 16673121.
  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 Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 42 (2): 443. Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  6. ^ a b c d Reffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas (2015). "Precise radial velocities of giant stars". Astronomy & Astrophysics. 574: A116. arXiv:1412.4634. Bibcode:2015A&A...574A.116R. doi:10.1051/0004-6361/201322360. hdl:10722/215277. S2CID 59334290. Vizier catalog entry
  7. ^ 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
  8. ^ a b da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy and Astrophysics, 458 (2): 609–623, arXiv:astro-ph/0608160, Bibcode:2006A&A...458..609D, doi:10.1051/0004-6361:20065105, S2CID 9341088
  9. ^ "eta Sct". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-23.
  10. ^ 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.
  11. ^ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy. 18 (3): 213. Bibcode:1987JHA....18..209W. doi:10.1177/002182868701800305. S2CID 118445625.

scuti, latinized, from, scuti, single, star, southern, constellation, scutum, near, constellation, border, with, aquila, latter, designation, aquilae, before, official, constellation, borders, were, 1922, visible, naked, faint, orange, hued, star, with, appare. Eta Scuti Latinized from h Scuti is a single 10 star in the southern constellation of Scutum near the constellation border with Aquila Eta Scuti was a latter designation of 9 Aquilae before the official constellation borders were set in 1922 11 It is visible to the naked eye as a faint orange hued star with an apparent visual magnitude of 4 83 2 This object is located approximately 213 light years from the Sun based on parallax and is drifting further away with a radial velocity of 92 1 h ScutiLocation of h Scuti circled Observation dataEpoch J2000 Equinox J2000Constellation ScutumRight ascension 18h 57m 03 67027s 1 Declination 5 50 46 7305 1 Apparent magnitude V 4 83 2 CharacteristicsEvolutionary stage horizontal branch 3 Spectral type K1 III 4 U B color index 1 02 5 B V color index 1 08 5 AstrometryRadial velocity Rv 92 22 0 16 1 km sProper motion m RA 61 545 1 mas yr Dec 41 429 1 mas yrParallax p 15 2960 0 1740 mas 1 Distance213 2 ly 65 4 0 7 pc Absolute magnitude MV 0 87 2 DetailsMass1 50 6 M Radius11 97 0 18 0 13 1 R Luminosity62 7 0 8 1 L Surface gravity log g 2 54 6 cgsTemperature4 693 27 266 1 KMetallicity Fe H 0 03 6 dexRotational velocity v sin i lt 1 0 7 km sAge2 8 8 GyrOther designationsh Sct BD 06 4976 FK5 3821 GC 26013 HD 175751 HIP 93026 HR 7149 SAO 142838 GSC 05127 07358 9 Database referencesSIMBADdataThis is an aging giant star with a stellar classification of K1 III 4 After exhausting the supply of hydrogen at its core the star cooled and expanded until currently it has 12 1 times the girth of the Sun It is a red clump giant which indicates it is presently on the horizontal branch and is generating energy through core helium fusion 3 The star is about 2 8 billion years old 8 with 1 5 times the mass of the Sun 6 It is radiating 63 1 times the Sun s luminosity from its swollen photosphere at an effective temperature of 4 693 K 1 References Edit a b c d e f g h i j k l m Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c 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 Vizier catalog entry a b Alves David R August 2000 K Band Calibration of the Red Clump Luminosity The Astrophysical Journal 539 2 732 741 arXiv astro ph 0003329 Bibcode 2000ApJ 539 732A doi 10 1086 309278 S2CID 16673121 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 a b Mallama A 2014 Sloan Magnitudes for the Brightest Stars The Journal of the American Association of Variable Star Observers 42 2 443 Bibcode 2014JAVSO 42 443M Vizier catalog entry a b c d Reffert Sabine Bergmann Christoph Quirrenbach Andreas Trifonov Trifon Kunstler Andreas 2015 Precise radial velocities of giant stars Astronomy amp Astrophysics 574 A116 arXiv 1412 4634 Bibcode 2015A amp A 574A 116R doi 10 1051 0004 6361 201322360 hdl 10722 215277 S2CID 59334290 Vizier catalog entry De Medeiros J R Alves S Udry S Andersen J Nordstrom B Mayor M 2014 A catalog of rotational and radial velocities for evolved stars Astronomy amp Astrophysics 561 A126 arXiv 1312 3474 Bibcode 2014A amp A 561A 126D doi 10 1051 0004 6361 201220762 S2CID 54046583 Vizier catalog entry a b da Silva L et al November 2006 Basic physical parameters of a selected sample of evolved stars Astronomy and Astrophysics 458 2 609 623 arXiv astro ph 0608160 Bibcode 2006A amp A 458 609D doi 10 1051 0004 6361 20065105 S2CID 9341088 eta Sct SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2019 08 23 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 Wagman M August 1987 Flamsteed s Missing Stars Journal for the History of Astronomy 18 3 213 Bibcode 1987JHA 18 209W doi 10 1177 002182868701800305 S2CID 118445625 Retrieved from https en wikipedia org w index php title Eta Scuti amp oldid 1125089079, wikipedia, wiki, book, books, library,

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