Multiple lines of evidence point to past flows of water across the Martian surface, but conditions on the planet now preclude
the existence of liquid water.
Studies of anomalies in water's behavior have indicated
the existence of liquid water with both lower and higher densities than this standard.
«We have 54 planets in the habitable zone of their stars,» Borucki says, referring to the temperate orbital zone around a star that would allow for
the existence of liquid water on a planet.
Both coexisted with the massive volcanic province Tharsis, located on the unseen side of the planet, which may have helped support
the existence of liquid water.
Previous scientific findings point to
the existence of a liquid water ocean located under the moon's icy crust.
Earlier this week, Kepler scientists announced the discovery of Kepler - 22b, a relatively large planet (2.4 Earth diameters) in the habitable zone of its parent star, where temperatures allow
the existence of liquid water.
All of the planet candidates are within the habitable zone, the orbital area that can support
the existence of liquid water on the surface, and are considered Super-Earths.
One of the big revelations from the study is that the «habitable zones» around stars aren't the only places conditions for life can arise because it turns out that close proximity to the sun isn't essential for
the existence of liquid water.
The planet boasts a «balmy temperature» of 72 degrees, which «would support
the existence of liquid water,» says BBC News.
Another major discovery is that planets don't need plate tectonics to keep control of their temperature and ensure
the existence of liquid water — volcanic activity and other forms of tectonics can accomplish the same thing.