...By studying the tides caused by low-mass stars on their potential earth-like companions, Heller and his colleagues have concluded that tidal effects modify the traditional concept of the habitable zone.
Heller deduced this from three different effects. Firstly, tides can cause the axis of a planet`s rotation to become perpendicular to its orbit in just a few million years. In comparison, Earth's axis of rotation is inclined by 23.5 degrees -- an effect which causes our seasons. Owing to this effect, there would be no seasonal variation on such Earth-like planets in the habitable zone of low-mass stars. These planets would have huge temperature differences between their poles, which would be in perpetual deep freeze, and their hot equators which in the long run would evaporate any atmosphere. This temperature difference would cause extreme winds and storms.
The second effect of these tides would be to heat up the exoplanet, similar to the tidal heating of Io, a moon of Jupiter that shows global vulcanism.
Finally, tides can cause the rotational period of the planet (the planet's "day") to synchronize with the orbital period (the planet's "year"). This situation is identical to the Earth-moon setup: the moon only shows Earth one face, the other side being known as "the dark side of the moon." As a result one half of the exoplanet receives extreme radiation from the star while the other half freezes in eternal darkness.
The habitable zone around low-mass stars is therefore not very comfortable -- it may even be uninhabitable. From an observer's point of view, low-mass stars have so far been the most promising candidates for habitable exoplanets. Now, due to Heller's findings, Earth-like exoplanets that have already been found in the conventional habitable zone of low-mass stars, have to be re-examined to consider tidal effects. ...
via New conditions for life on other planets: Tidal effects change 'habitable zone' concept.