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53 Arietis

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Star in the constellation Aries
53 Arietis
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 03 07 25.67315
Declination +17° 52′ 47.9696″
Apparent magnitude (V) 6.10
Characteristics
Spectral type B1.5 V
U−B color index 0.80
B−V color index −0.12
Variable type β Cep
Astrometry
Radial velocity (Rv)+21.2 km/s
Proper motion (μ) RA: −23.733 mas/yr
Dec.: +8.080 mas/yr
Parallax (π)3.1874 ± 0.0630 mas
Distance1,020 ± 20 ly
(314 ± 6 pc)
Details
Mass7.5±0.2 M
Radius4.2 R
Luminosity1,962 L
Surface gravity (log g)3.99 cgs
Temperature19,065 K
Metallicity −0.18 dex
Rotational velocity (v sin i)5 km/s
Other designations
UW Arietis, BD+17°493, HD 19374, HIP 14514, HR 938, SAO 93284.
Database references
SIMBADdata

53 Arietis (abbreviated 53 Ari) is a variable star in the northern constellation of Aries. 53 Arietis is the Flamsteed designation; it also bears the variable star designation UW Arietis. It is a B-type main sequence star with a stellar classification of B1.5 V and mean apparent magnitude of 6.10, which is near the lower limit for naked eye visibility. Based upon an annual parallax shift of 3.2 mas, the estimated distance to this star is roughly 1,020 light-years (314 parsecs).

The claimed variability of 53 Arietis has not been confirmed. It is a runaway star with a peculiar velocity of 48.1 km/s relative to its neighbors. The star was ejected from the Orion nebula some 4–5 million years ago, possibly when an orbiting companion exploded as a supernova.

References

  1. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ Crawford, D. L.; Barnes, J. V.; Golson, J. C. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere", The Astronomical Journal, 76: 1058, Bibcode:1971AJ.....76.1058C, doi:10.1086/111220.
  3. ^ Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode:1968ApJS...17..371L, doi:10.1086/190179.
  4. ^ Stankov, Anamarija; Handler, Gerald (June 2005), "Catalog of Galactic β Cephei Stars", The Astrophysical Journal Supplement Series, 158 (2): 193–216, arXiv:astro-ph/0506495, Bibcode:2005ApJS..158..193S, doi:10.1086/429408, S2CID 119526948.
  5. Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.), Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto: International Astronomical Union, p. 57, Bibcode:1967IAUS...30...57E.
  6. ^ Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
  7. Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode:2002ApJ...573..359A, doi:10.1086/340590.
  8. "53 Ari", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2012-08-17.
  9. "UW Ari". The International Variable Star Index. AAVSO. Retrieved 28 August 2024.
  10. "UW Ari". General Catalog of Variable Stars. Lomonosov Moscow State University. Retrieved 28 August 2024.
  11. Hoogerwerf, R.; de Bruijne, J. H. J.; de Zeeuw, P. T. (January 2001), "On the origin of the O and B-type stars with high velocities. II. Runaway stars and pulsars ejected from the nearby young stellar groups", Astronomy and Astrophysics, 365 (2): 49–77, arXiv:astro-ph/0010057, Bibcode:2001A&A...365...49H, doi:10.1051/0004-6361:20000014, S2CID 18970167.

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