7 Ceti

7 Ceti

A light curve for AE Ceti, plotted from data presented by Tabur, et al. (2009)
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 00h 14m 38.41655s
Declination −18° 55 58.3145
Apparent magnitude (V) 4.44 (4.26–4.46)
Characteristics
Evolutionary stage AGB
Spectral type M1 III
B−V color index 1.640±0.044
Variable type LB:
Astrometry
Radial velocity (Rv)−22.9±1.0 km/s
Proper motion (μ) RA: −26.15 mas/yr
Dec.: −73.58 mas/yr
Parallax (π)7.29±0.28 mas
Distance450 ± 20 ly
(137 ± 5 pc)
Absolute magnitude (MV)–1.24
Details
Radius54 R
Luminosity1019.14 L
Temperature3,800 K
Other designations
3 Cet, AE Ceti, BD−19°21, HD 1038, HIP 1170, HR 48, SAO 147169
Database references
SIMBADdata

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

This is an aging red giant star with a stellar classification of M1 III, currently on the asymptotic giant branch. In 1959, Alan William James Cousins announced the detection of variability in the brightness of 7 Ceti. It was given its variable star designation in 1973. 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. Tabur et al. (2009) list it as a semiregular variable with four known periods ranging in frequency from 19.2 to 41.7 days. The stellar atmosphere of 7 Ceti has expanded to an estimated 54 times the Sun's radius. It is radiating around 1,019 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,800 K.

Luminosity variation
Period
(Days)
Amplitude
(Mag.)
19.20.018
19.60.020
27.10.018
41.70.017