67 Cancri

67 Cancri is a wide binary star[9] system in the zodiac constellation of Cancer, located 195[1] light years away from the Sun.

It is just visible to the naked eye as a faint, white-hued star with a combined apparent magnitude of 6.07.

[2] The binary nature of this system was discovered by James South and John Herschel.

[5] The primary, designated component A, is an A-type main-sequence star with a stellar classification of A8 Vn.

[11] Uesugi and Fukuda (1970) gave a projected rotational velocity estimate of 105[7] km/s for the star, although Abt et al. (1997) suggested it could be as high as 205 km/s.