Cor Caroli

The International Astronomical Union uses the name "Cor Caroli" specifically for the brighter star of the binary.

[17] Alpha Canum Venaticorum is the brightest point of light in the northern constellation of Canes Venatici.

[19] However, Robert Burnham Jr. notes that "the attribution of the name to Halley appears in a report published by J. E. Bode at Berlin in 1801, but seems to have no other verification".

[24] Consequently, the Chinese name for Alpha Canum Venaticorum itself is 常陳一 (Cháng Chén yī, English: the First Star of Imperial Guards).

α2 Canum Venaticorum has a spectral type of A0, and has an apparent visual magnitude which varies between 2.84 and 2.98, with a period of 5.47 days.

This is thought to be due to some elements sinking down into the star under the force of gravity while others are elevated by radiation pressure.

Cor Caroli seen from northern England on March 1, 2011
A light curve for α 2 Canum Venaticorum, plotted from TESS data [ 27 ]