Alphard lies somewhat westward of Sirius, and approximately southward of the Sickle in Leo. This is a binary system, in whicb the highly luminousorangegiant Alphard A is accompanied by the dwarf Alphard B, probably also of the K-typeclassification, in an extremely distant orbit that takes nearly a million years to complete.
The brightest of the long string of stars that form the vast but generally rather faint constellation of Hydra, the Water Snake, Alphard forms an approximate equilateral triangle with two more prominent stars to its north: Regulus in Leo and Procyon in Canis Minor. Though only second magnitude, it stands out as the brighteststar in its own region of the sky, and this is the reason behind its name: Alphard (often transliterated Alfard) comes from the Arabic for the 'lone' star.
Alphard is notable as being one of the most intrinsically luminousstars known, generating nearly seven hundred times as much energy as the Sun. A giantstar of the orangeK-typeclassification, it has a dwarfstar, designated Alphard B, in a distant orbit. The outer shell of this immense star (Alphard's diameter is some forty to fifty times greater than the Sun's) shows pulsating patterns that oscillate over periods ranging up to days in length.