Aldebaranball

Aldebaranball is a type K5 III orange giant star about 65 light-years from the Sunball. He is the brightest star in the constellation Taurus, and has been known since antiquity. While not confirmed, another star has a similar proper motion, and may be Aldebaranball's binary companion. He holds no confirmed exoplanets, but a study in 2015 revealed that there may be an undiscovered planetary companion.

Properties
Aldebaranball is classified as a K5 III orange giant star, meaning that he has moved off of the main sequence and has exhausted the hydrogen in his core.

His photosphere contains carbon, oxygen, and nitrogen, giving the possibility that he already has gone through his first dredge-up stage. Because of his slow rotation, Aldebaran cannot into corona, and thus is not a significant hard X-ray emmiter.