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70 Aquarii

70 Aquarii is a variable star located 425[2] light years away from the Sun in the equatorial constellation of Aquarius. It has the variable star designation FM Aquarii;[7] 70 Aquarii is the Flamsteed designation. It is near the lower limit of visibility to the naked eye, appearing as a dim, yellow-white hued star with a baseline apparent visual magnitude of 6.19.[3] This star is moving closer to the Earth with a heliocentric radial velocity of –5.8 km/s.[6]

70 Aquarii

The visual band light curve of 70 Aquarii, adapted from Weiss (1977)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 48m 30.21043s[2]
Declination –10° 33′ 19.7143″[2]
Apparent magnitude (V) 6.19[3]
Characteristics
Evolutionary stage main sequencec
Spectral type F0 V[4]
B−V color index +0.28[3]
Variable type δ Sct[5]
Astrometry
Radial velocity (Rv)–5.8[6] km/s
Proper motion (μ) RA: +31.535[2] mas/yr
Dec.: +7.915[2] mas/yr
Parallax (π)7.6654 ± 0.0704 mas[2]
Distance425 ± 4 ly
(130 ± 1 pc)
Absolute magnitude (MV)+0.88[7]
Details
Radius4.17+0.17
−0.23
[2] R
Luminosity44.8±0.5[2] L
Surface gravity (log g)3.48[7] cgs
Temperature7,314+187
−144
[2] K
Metallicity [Fe/H]0.02±0.15[8] dex
Rotational velocity (v sin i)110[9] km/s
Other designations
70 Aqr, BD−11°5923, FK5 3825, HD 215874, HIP 112615, HR 8676, SAO 165308[10]
Database references
SIMBADdata

This is an F-type main-sequence star with a stellar classification of F0 V.[4] Located in the lower part of the instability strip, it is a Delta Scuti-type variable that ranges in brightness from magnitude 6.16 down to 6.19 with a period of 125 minutes (0.087 days).[5] The star has a high rate of spin, showing a projected rotational velocity of 110 km/s.[9] It has four[2] times the Sun's radius and is radiating 45[2] times the luminosity of the Sun from its photosphere at an effective temperature of around 7,314 K.[2]

References edit

  1. ^ Weiss, W. W. (November 1977). "HR 239 and HR 8676: Two delta Scuti-Type Variables". Information Bulletin on Variable Stars. 1364: 1. Bibcode:1977IBVS.1364....1W. Retrieved 16 October 2021.
  2. ^ a b c d e f g h i j k l 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.
  3. ^ a b c Corben, P. M.; Stoy, R. H. (1968), "Photoelectric Magnitudes and Colours for Bright Southern Stars", Monthly Notes of the Astronomical Society of Southern Africa, 27: 11, Bibcode:1968MNSSA..27...11C.
  4. ^ a b Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, 5, Bibcode:1999MSS...C05....0H.
  5. ^ a b Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
  6. ^ a b Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Carnegie Institute of Washington, D.C., Bibcode:1953GCRV..C......0W.
  7. ^ a b c Paunzen, E.; et al. (September 2002), "On the Period-Luminosity-Colour-Metallicity relation and the pulsational characteristics of lambda Bootis type stars", Astronomy and Astrophysics, 392 (2): 515–528, arXiv:astro-ph/0207494, Bibcode:2002A&A...392..515P, doi:10.1051/0004-6361:20020854, S2CID 54666586
  8. ^ Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 171, arXiv:1604.07403, Bibcode:2016ApJ...826..171G, doi:10.3847/0004-637X/826/2/171, S2CID 119241004.
  9. ^ a b Royer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy and Astrophysics, 393: 897–911, arXiv:astro-ph/0205255, Bibcode:2002A&A...393..897R, doi:10.1051/0004-6361:20020943, S2CID 14070763.
  10. ^ "70 Aqr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-05-19.

External links edit

  • Image 70 Aquarii

aquarii, variable, star, located, light, years, away, from, equatorial, constellation, aquarius, variable, star, designation, aquarii, flamsteed, designation, near, lower, limit, visibility, naked, appearing, yellow, white, hued, star, with, baseline, apparent. 70 Aquarii is a variable star located 425 2 light years away from the Sun in the equatorial constellation of Aquarius It has the variable star designation FM Aquarii 7 70 Aquarii is the Flamsteed designation It is near the lower limit of visibility to the naked eye appearing as a dim yellow white hued star with a baseline apparent visual magnitude of 6 19 3 This star is moving closer to the Earth with a heliocentric radial velocity of 5 8 km s 6 70 AquariiThe visual band light curve of 70 Aquarii adapted from Weiss 1977 1 Observation dataEpoch J2000 Equinox J2000 Constellation Aquarius Right ascension 22h 48m 30 21043s 2 Declination 10 33 19 7143 2 Apparent magnitude V 6 19 3 Characteristics Evolutionary stage main sequencec Spectral type F0 V 4 B V color index 0 28 3 Variable type d Sct 5 AstrometryRadial velocity Rv 5 8 6 km sProper motion m RA 31 535 2 mas yr Dec 7 915 2 mas yrParallax p 7 6654 0 0704 mas 2 Distance425 4 ly 130 1 pc Absolute magnitude MV 0 88 7 DetailsRadius4 17 0 17 0 23 2 R Luminosity44 8 0 5 2 L Surface gravity log g 3 48 7 cgsTemperature7 314 187 144 2 KMetallicity Fe H 0 02 0 15 8 dexRotational velocity v sin i 110 9 km s Other designations70 Aqr BD 11 5923 FK5 3825 HD 215874 HIP 112615 HR 8676 SAO 165308 10 Database referencesSIMBADdata This is an F type main sequence star with a stellar classification of F0 V 4 Located in the lower part of the instability strip it is a Delta Scuti type variable that ranges in brightness from magnitude 6 16 down to 6 19 with a period of 125 minutes 0 087 days 5 The star has a high rate of spin showing a projected rotational velocity of 110 km s 9 It has four 2 times the Sun s radius and is radiating 45 2 times the luminosity of the Sun from its photosphere at an effective temperature of around 7 314 K 2 References edit Weiss W W November 1977 HR 239 and HR 8676 Two delta Scuti Type Variables Information Bulletin on Variable Stars 1364 1 Bibcode 1977IBVS 1364 1W Retrieved 16 October 2021 a b c d e f g h i j k l 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 Corben P M Stoy R H 1968 Photoelectric Magnitudes and Colours for Bright Southern Stars Monthly Notes of the Astronomical Society of Southern Africa 27 11 Bibcode 1968MNSSA 27 11C a b Houk N Swift C 1999 Michigan catalogue of two dimensional spectral types for the HD Stars Michigan Spectral Survey 5 Bibcode 1999MSS C05 0H a b Samus N N et al 2017 General Catalogue of Variable Stars Astronomy Reports 5 1 61 1 80 88 Bibcode 2017ARep 61 80S doi 10 1134 S1063772917010085 S2CID 125853869 a b Wilson R E 1953 General Catalogue of Stellar Radial Velocities Carnegie Institute Washington D C Publication Carnegie Institute of Washington D C Bibcode 1953GCRV C 0W a b c Paunzen E et al September 2002 On the Period Luminosity Colour Metallicity relation and the pulsational characteristics of lambda Bootis type stars Astronomy and Astrophysics 392 2 515 528 arXiv astro ph 0207494 Bibcode 2002A amp A 392 515P doi 10 1051 0004 6361 20020854 S2CID 54666586 Gaspar Andras et al 2016 The Correlation between Metallicity and Debris Disk Mass The Astrophysical Journal 826 2 171 arXiv 1604 07403 Bibcode 2016ApJ 826 171G doi 10 3847 0004 637X 826 2 171 S2CID 119241004 a b Royer F et al October 2002 Rotational velocities of A type stars in the northern hemisphere II Measurement of v sin i Astronomy and Astrophysics 393 897 911 arXiv astro ph 0205255 Bibcode 2002A amp A 393 897R doi 10 1051 0004 6361 20020943 S2CID 14070763 70 Aqr SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2019 05 19 External links editImage 70 Aquarii Retrieved from https en wikipedia org w index php title 70 Aquarii amp oldid 1186931961, wikipedia, wiki, book, books, library,

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