Delta Ceti shines against a backdrop rich in prominent galaxies. The object in the southeast corner of this image is the face-on spiral galaxyM77 also known as the Squid Galaxy, while to the east and slightly to the north of the star is the barred spiralNGC 1055. Imagery provided by Aladin sky atlas
As its blue colouration indicates, Delta Ceti is a great deal hotter and more luminous than the Sun, with a surface temperature of over 20,000 K. The high temperature in its core, and specifically its effect on the iron in that core, causes a periodic build-up and release of energy within the star, which in turn causes the star to swell and contract. As a result, Delta Ceti is a pulsating variable of the Beta Cephei type, and its brightness increases and decreases over a regular period of some 3.8 hours.