The third brightest of the Hyades (after Chamukuy and Ain), Prima Hyadum is the westernmost of the brightstars in the cluster, and thus leads the entire group through the skies of Earth. This is the source of its name, Prima Hyadum or Hyadum I (the following brightstar in the cluster, Delta1Tauri, is named Secunda Hyadum (or Hyadum II) on the same system, but the sequence does not continue). Though apparently on the leading edge of the cluster to an observer on Earth, Prima Hyadum is actually close to its centre, at a distance of about 151 light years from the Sun.
Prima Hyadum has completed its development along the main sequence and has depleted its reserves of hydrogen. Its fusion processes are now consuming helium, and the star is therefore swelling and evolving from a yellow to an orangestar, towards ultimately becoming a redgiant. It is physically far larger than the Sun (about thirteen times larger, in terms of diameter) and much more inherently luminous. The pattern of variations in the brightness of Prima Hyadum raise the possibility that, as it has expanded, it may have consumed one or more inner members of its own planetary system.