[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] 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.
[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.
[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.