This is a widely separated system of at least two stars, and possibly three. The primaryyellowgiant, Iota Cancri A, shows indirect signs of possessing a white dwarf companion, though that companion has yet to be directly detected. Meanwhile Iota Cancri B, far from the giantprimary, is a much lower-masswhitestar, rotating rapidly enough to have expelled belts of material into its surrounding space.
The brightstar in the centre of this image is the yellowgiant Iota Cancri A, with the fainter Iota Cancri B discernable to its immediate northwest. Based on their individual parallax measurements, these two stars lie as far as ten light years apart, but their shared motion through space suggests that they are nonetheless gravitationally related to one another. Imagery provided by Aladin sky atlas
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