θ Cassiopeiae (theta Cassiopeiae)
θ Cassiopeiae is a variable and double main-sequence star in the constellation of Cassiopeia.
θ Cassiopeiae visual magnitude is 4.33. Because of its moderate brightness, θ Cassiopeiae should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.
The proper motion of θ Cassiopeiae is 0.229 arcsec per year in Right Ascension and -0.022 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Key facts about θ Cassiopeiae
Celestial coordinates and finder chart of θ Cassiopeiae
θ Cassiopeiae is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of θ Cassiopeiae are provided in the following table:
The simplified sky map below shows the position of θ Cassiopeiae in the sky:
Visibility of θ Cassiopeiae from your location
θ Cassiopeiae (theta Cassiopeiae) is circumpolar and transits at 14:39 UTC (altitude: 86.3°)
Distance of θ Cassiopeiae from the Sun and relative movement
θ Cassiopeiae is distant 137.38 light years from the Sun and it is moving far from the Sun at the speed of 9 kilometers per second.
Spectral properties of θ Cassiopeiae
θ Cassiopeiae belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where θ Cassiopeiae is situated in the Hertzsprung–Russell diagram.
θ Cassiopeiae star system properties
θ Cassiopeiae is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the θ Cassiopeiae double sysyem: