Gamma Cephei is accompanied by a low mass companion (a red dwarf with a mass around 0.3 or 0.4 solar masses) that orbits with a period between 57 and 66 years at a distance of about 19 AU.

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Jim Kaler

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Gamma Cephei

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In other words, since he is starting from a point much “higher up”, to use an analogy from the time-space context, that part of his consciousness involved in “clicking out” will have that much more time to interact in dimensions beyond time-space because less time is required to traverse the intervening layers.

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Errai (Gamma Cephei) (stars.astro.illinois.edu) Errai (Gamma Cephei) is the among the visually brightest stars to host a planet, and also has a low mass companion with a relatively small orbit.

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