Delta Crateris

Delta Crateris is a solitary star in the southern constellation of Crater. With an apparent [visual magnitude] of 3.56, it is the brightest star in this rather dim constellation. It has an annual parallax shift of as measured from Earth, indicating Delta Crateris lies at a distance of from the Sun.

Characteristics

This is an evolved orange-hued giant star belonging to the spectral class K0 III. Delta Crateris is a member of the so-called red clump, indicating that it is generating energy through the thermonuclear fusion of helium at its core. The star has an estimated 1.47 times the mass of the Sun but has expanded to 20 times the Sun's radius.
It is around 2.89 billion years old with a rotation rate that is too small to measure; the projected rotational velocity is 0.0 km/s. Delta Crateris is radiating as much luminosity as the Sun from its outer envelope at an effective temperature of K.
This star is occasionally called by the name Labrum, usually in an astrological context.