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53 Arietis
Star in the constellation Aries
Star in the constellation Aries
| r-i = | v-r = | b-v = −0.12 | u-b = +0.80
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 , the estimated distance to this star is roughly 314 pc.
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.
References
References
- "The Internet Encyclopedia of Science: Barnard's Loop (Sh 2-276)". David Darling.
- {{cite Gaia DR3. 58850711337487616
- "UW Ari". AAVSO.
- "UW Ari". Lomonosov Moscow State University.
- Lesh, Janet Rountree. (December 1968). "The Kinematics of the Gould Belt: an Expanding Group?". Astrophysical Journal Supplement.
- Evans, D. S.. (June 20–24, 1966). "Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30". [[International Astronomical Union]].
- (July 2002). "Rotational Velocities of B Stars". The Astrophysical Journal.
- (1971). "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere". The Astronomical Journal.
- (January 2011). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". [[Monthly Notices of the Royal Astronomical Society]].
- (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.
- (June 2005). "Catalog of Galactic β Cephei Stars". The Astrophysical Journal Supplement Series.
- "53 Ari".
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