Originally posted by PhReAk
the planet's orbital period is 9.5 days. I don't think thats very good for water
I noticed that too. The star may be a brown dwarf though, which would mean much smaller solar radiation output and therefore a habitable zone that extends very close to the star. And that concept is far from obsolete as some have indicated; life needs a sustainable energy source to survive, while not one so intense that it destroys anything less dense than solid rock. Mercury, for example, is not a candidate for life in any form, because our sun has not only fried the surface by its proximity but quite possibly cooked much of the surface rock away over the past 5 billion years. The outer planets and moons don't recieve enough solar radiation to sustain life, and none are large enough to still have active geothermal activity either. Europa, on the other hand, is a bit of an exception; the amount of solar radiation it recieves is less than the commonly assumed requirements for life, but it is protected to a large degree by Jupiter's gravity well that serves to sweep the inner solar system of smaller debris that will have serious disruptions on life (it has also likely helped Earth avoid a constant bombardment of asteroids as well) and it does recieve some boons from Jupiter's radiation output and magnetic field as well.
EDIT: In other words, habitable zones are more about the net amount (and to a degree, the concentration) of solar radiation on a planet, not between two fixed radii out from the star.
I did read somewhere that planets could travel in a much less circular orbit and still meet the requirements for habitability, maybe that's what's happening here. It just seems a little far-fetched that something that close to a star could sustain liquid
anything, and I really don't know how life would evolve from solid rock.