Iota Cancri, a binary star system, has a surface temperature of approximately 5,400 Kelvin for its primary component, which is a G-type main-sequence star. This temperature is comparable to that of our Sun, which has a surface temperature of about 5,800 Kelvin. The secondary component, a smaller star, has a lower temperature. Together, they form a visually appealing binary system located roughly 50 light-years away from Earth.
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