Abstract
There is continued interest in the study of habitability for the Gliese 581 system. Previously, for Gliese 581c, a quasi-consensus has been reached that this planet, a super-Earth, is interior to the stellar habitable zone, akin to Venus in the solar system. In this work, I revisit this view considering detailed results about the orbital planetary parameters (including their uncertainties) and previous studies on habitability.
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