7 Ceti

Star in the constellation Cetus From Wikipedia, the free encyclopedia

7 Ceti is a single,[10] variable star in the equatorial constellation of Cetus. It has the variable star designation AE Ceti.[11] The star is visible to the naked eye with a baseline apparent visual magnitude of 4.44.[2] Based upon an annual parallax shift of only 7.3 mas,[1] it is located roughly 450 light years away. It is moving closer to the Sun with a heliocentric radial velocity of −23 km/s.[6] Eggen (1965) listed it as a probable member of the Wolf 630 group of co-moving stars.[12]

A light curve for AE Ceti, plotted from data presented by Tabur, et al. (2009)[11]
Right ascension00h 14m 38.41655s[1]
Declination−18° 55 58.3145[1]
Apparentmagnitude(V)4.44[2] (4.26–4.46)[3]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
7 Ceti
Location of 7 Ceti (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 00h 14m 38.41655s[1]
Declination −18° 55 58.3145[1]
Apparent magnitude (V) 4.44[2] (4.26–4.46)[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M1 III[5]
B−V color index 1.640±0.044[2]
Variable type LB:[3]
Astrometry
Radial velocity (Rv)−22.9±1.0[6] km/s
Proper motion (μ) RA: −26.15[1] mas/yr
Dec.: −73.58[1] mas/yr
Parallax (π)7.29±0.28 mas[1]
Distance450 ± 20 ly
(137 ± 5 pc)
Absolute magnitude (MV)–1.24[2]
Details
Radius69[7] R
Luminosity1,011[7] L
Surface gravity (log g)0.77[8] cgs
Temperature3,909[7] K
Metallicity [Fe/H]+0.50[8] dex
Other designations
3 Cet, AE Ceti, BD−19°21, HD 1038, HIP 1170, HR 48, SAO 147169[9]
Database references
SIMBADdata
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This is an aging red giant star with a stellar classification of M1 III,[5] currently on the asymptotic giant branch.[4] In 1959, Alan William James Cousins announced the detection of variability in the brightness of 7 Ceti.[13] It was given its variable star designation in 1973.[14] Samus et al. (2017) has it classed as a slow irregular variable of type LB:, and ranges in magnitude from 4.26 down to 4.46.[3] Tabur et al. (2009) list it as a semiregular variable with four known periods ranging in frequency from 19.2 to 41.7 days.[11] The stellar atmosphere of 7 Ceti has expanded to an estimated 69 times the Sun's radius.[7] It is radiating around 1,011 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,909 K.[7]

More information Period (Days), Amplitude (Mag.) ...
Luminosity variation[11]
Period
(Days)
Amplitude
(Mag.)
19.20.018
19.60.020
27.10.018
41.70.017
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References

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