54 Ceti

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54 Ceti
Local 54 cet.png
Location of 54 Ceti (HD 11257) near the constellation boundary of Aries (pink). Nearby are the constellations of Pisces (blue) and Cetus (green).
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 01h 50m 51.97276s[1]
Declination +11° 02′ 36.1563″[1]
Apparent magnitude (V) 5.94[2]
Characteristics
Spectral type F2 Vw[3]
U−B color index –0.03[2]
B−V color index +0.30[2]
R−I color index 0.17
Astrometry
Radial velocity (Rv) +11.1[4] km/s
Proper motion (μ) RA: –69.39[1] mas/yr
Dec.: –28.45[1] mas/yr
Parallax (π) 23.80 ± 0.44[1] mas
Distance 137 ± 3 ly
(42.0 ± 0.8 pc)
Details
Radius 1.2–1.8[5] R
Surface gravity (log g) 4.50[3] cgs
Temperature 7,099[3] K
Metallicity [Fe/H] –0.20[3] dex
Rotational velocity (v sin i) 29[6] km/s
Other designations
BD+10° 252, HD 11257, NSV 635, HIP 8588, HR 534, SAO 92659.[7]

54 Ceti is an older Flamsteed designation[8] for a star that is now located within the constellation boundaries of Aries,[9] the Ram. In the present day it is known by star catalogue identifiers like HD 11257 or HR 534.[7] At an apparent visual magnitude of 5.94,[2] it can be seen with the naked eye. The distance to this star, as determined using parallax measurements made during the Hipparcos mission, is approximately 139 light-years (43 parsecs), give or take a 6 light-year margin of error.[1] It is located near the ecliptic and hence is subject to occasional occultations by the Moon and planets.[7]

This is an F-type main sequence star with a stellar classification of F2 Vw,[3] where the 'w' indicates weak absorption lines in the spectrum. It is a candidate member of the Ursa Major Moving Group, which has an estimated age of 500 ± 100 million years.[10]

References

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  3. 3.0 3.1 3.2 3.3 3.4 Lua error in package.lua at line 80: module 'strict' not found.
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External links