75 Ceti

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75 Ceti
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 02h 32m 09.42241s[1]
Declination −01° 02′ 05.6166″[1]
Apparent magnitude (V) +5.36[2]
Characteristics
Spectral type K1 III[3]
B−V color index +1.004±0.002[2]
Distance
268 ± 2 ly
(82.2 ± 0.6 pc)
Absolute magnitude (MV)0.808[4]
Details
Gyr
HR 739, SAO 129959[8]
Database references
Exoplanet Archive
data

75 Ceti is a single

apparent visual magnitude of +5.36.[2] The star is located 268 light-years (82 parsecs) distant from the Sun, based on parallax, but is drifting closer with a radial velocity of −6 km/s.[1]

In

66 Ceti. Consequently, 75 Ceti itself is known as the Tenth Star of Circular Celestial Granary.[10]

This is an aging

luminosity of the Sun from its swollen photosphere at an effective temperature of 4,846 K.[7]

Planetary system

A planetary companion was discovered by

insolation than does Jupiter and, indeed, Earth.[12]

There may be additional periodic factors in the data, corresponding to m sin i of around 0.4 MJ and 1 MJ, at distances of ~0.9 AU and ~4 AU, where i is the orbital inclination and m is the planet's actual mass.[11] In 2023, the presence of a second, Jupiter-mass planet orbiting at 4 AU (75 Ceti c) was confirmed, which is more irradiated than Earth as well. The shorter period signal corresponding to a possible planet at 0.9 AU was found to be an alias of the true period of planet c.[6]

The 75 Ceti planetary system[6]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥2.479+0.074
−0.090
 MJ
1.912+0.002
−0.003
696.62+1.33
−1.69
0.093+0.026
−0.042
c ≥0.912+0.088
−0.143
 MJ
3.929+0.058
−0.052
2051.62+45.98
−40.47
0.023+0.191
−0.003

References