Astronomy:64 Ceti

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Short description: Subgiant in the constellation Cetus

Coordinates: Sky map 02h 11m 21.08s, +08° 34′ 11.31″

64 Ceti
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cetus
Right ascension  02h 11m 21.079s[1]
Declination +08° 34′ 11.31″[1]
Apparent magnitude (V) 5.623±0.01[1]
Characteristics
Evolutionary stage Subgiant[1]
Spectral type G0IV[1]
Apparent magnitude (B) 6.189[1]
Apparent magnitude (R) 6.81[1]
Apparent magnitude (G) 5.497[1]
Apparent magnitude (J) 4.763[1]
Apparent magnitude (H) 4.373[1]
Apparent magnitude (K) 4.308[1]
B−V color index 0.52[2]
Astrometry
Radial velocity (Rv)-19.01±0.22[3] km/s
Proper motion (μ) RA: -141.042[3] mas/yr
Dec.: -113.463[3] mas/yr
Parallax (π)23.7901 ± 0.066[3] mas
Distance136.97 ly
(42.016 pc)
Absolute magnitude (MV)2.49[4]
Details[2]
Mass1.53±0.04 M
Radius2.56±0.56 R
Luminosity8.13[lower-alpha 1] L
Surface gravity (log g)3.81±0.09 cgs
Temperature6066±42 K
Metallicity [Fe/H]0.14±0.04 dex
Rotation15 days[lower-alpha 2]
Rotational velocity (v sin i)8.96±1.52 km/s
Age2.63[lower-alpha 3] Gyr
Other designations
64 Ceti, Gaia DR2 2521857809546128896, HD 13421, HIP 10212, HR 635, SAO 110390, PPM 145360, LSPM J0211+0834, GSC 00630-01238, IRAS 02087+0820, WISE J021120.97+083410.1
Database references
SIMBADdata

64 Ceti is a star located located in the constellation Cetus. Based on its spectral type of G0IV, it is a G-type star that has left the main sequence and evolved into a subgiant.[1] It is located 42.02 parsecs (137.1 light-years) away, based on a parallax measured by Gaia DR3, and it is moving towards Earth at a velocity of 19 km/s.[3] The apparent magnitude of 64 Ceti is 5.62,[1] which makes it visible to the naked eye only in dark skies, far away from light pollution.[4]

Characteristics

64 Ceti is a G-type star that has left the main sequence and now evolved into a subgiant, based on its spectral type of G0IV.[1] It has about 1.53 times the Sun's mass and has expanded to 2.53 times the Sun's diameter.[2] It is emitting 8.13 times the solar luminosity from its photosphere at an effective temperature of 6,066 K.[2] The age of 64 Ceti is estimated at 2.63 billion years, about 58% of the Solar System's age,[lower-alpha 4] and it rotates under its axis at a speed of 8.96 km/s, translating into a rotation period of 15 days.[lower-alpha 2][2] The B-V index of the star is 0.52, corresponding to a yellow-white hue of a late G/early F star.[2][lower-alpha 5]

It is located in the constellation Cetus, based on its celestial coordinates. Gaia DR3 measured a parallax of 23.8 milliarcseconds for this star, translating into a distance of 42.02 parsecs (137.1 light-years).[3] The apparent magnitude of 64 Ceti is 5.62,[1] which means that it is a faint star, visible to the naked eye only from locations with dark skies.[4] The absolute magnitude, i.e. its brightness if it was seen at a distance of 10 pc (32.6 ly), is 2.49.[4] The star is moving towards Earth at a velocity of 19 km/s.[3] It has a high proper motion across the sky[1] and belongs to the thin disk population, being located 31.03 parsecs (101.2 ly) above the galactic plane.[2]

Notes

  1. from a logarithm of 0.91
  2. 2.0 2.1 The rotational period is calculated using the star's circumference (π*diameter (km)) and later divided by the rotational period. The value will be divided by 86400 to convert from seconds to days.
  3. From a logarithm of 9.42.
  4. The Solar System has an age of 4.532 billion years.
  5. See the Color index article

References