Studies of hydrogen molecules in the Venusian atmosphere by NASA's Pioneer - Venus probe indicate that the planet
once had liquid water on its surface, perhaps even expansive oceans.
Not exact matches
NASA's twin Mars Exploration Rovers
have discovered evidence that
liquid water once flowed, at least fitfully,
on the Red Planet's
surface (ScienceNOW, 13 December 2006).
The
surface of the red planet is bone dry, but several studies
have shown
liquid water may
once have flowed
on Mars and could still exist in pockets below the
surface.
Venus may
have once been habitable; current research puts
liquid water on the
surface about 2 billion years ago.
Clues
on the Martian
surface, including features resembling dry riverbeds and minerals that only form in the presence of
water, suggest Mars
once had a denser atmosphere that supported the presence of
liquid water on the
surface.
Other factors also suggest Mars
once had a much thicker atmosphere, such as evidence of persistent presence of
liquid water on the planet's
surface long ago even though the atmosphere is too scant for
liquid water to persist
on the
surface now.