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70 Aquarii

From Wikipedia, the free encyclopedia
Star in the constellation Aquarius
70 Aquarii

Thevisual bandlight curve of 70 Aquarii, adapted from Weiss (1977)[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationAquarius
Right ascension22h 48m 30.21043s[2]
Declination−10° 33′ 19.7143″[2]
Apparent magnitude (V)6.19[3]
Characteristics
Evolutionary stagemain sequencec
Spectral typeF0 V[4]
B−Vcolor index+0.28[3]
Variable typeδ 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

70 Aquarii is avariable star located 425[2] light years away from the Sun in theequatorialconstellation ofAquarius. It has thevariable star designationFM Aquarii;[7]70 Aquarii is theFlamsteed designation. It is near the lower limit of visibility to the naked eye, appearing as a dim, yellow-white hued star with a baselineapparent visual magnitude of 6.19.[3] This star is moving closer to the Earth with a heliocentricradial velocity of –5.8 km/s.[6]

Werner Wolfgang Weiss discovered that 70 Aquarii was a variable star in 1977.[1] It was given its variable star designation in 1981.[11]

This is anF-type main-sequence star with astellar classification of F0 V.[4] Located in the lower part of theinstability strip, it is aDelta 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 aprojected rotational velocity of 110 km/s.[9] It has four[2] times theSun's radius and is radiating 45[2] times theluminosity of the Sun from itsphotosphere at aneffective temperature of around 7,314 K.[2]

References

[edit]
  1. ^abWeiss, 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. Retrieved16 October 2021.
  2. ^abcdefghijklBrown, 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 atVizieR.
  3. ^abcCorben, 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. ^abHouk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5,Bibcode:1999MSS...C05....0H.
  5. ^abSamus, 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. ^abWilson, 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. ^abcPaunzen, 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. ^abRoyer, 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. Retrieved2019-05-19.
  11. ^Kholopov, P. N.; Samus, N. N.; Kukarkina, N. P.; Medvedeva, G. I.; Perova, N. B. (February 1981)."65th Name-List of Variable Stars".Information Bulletin on Variable Stars.1921:1–21.Bibcode:1981IBVS.1921....1K. Retrieved18 November 2024.

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