The colossal Olympus Mons shield volcano located on Mars could once have been an island in an ancient ocean on the Red Planet, a new study has revealed.
A team led by geoscientist Anthony Hildenbrand of Paris-Saclay University in France wrote that their research shows that Olympus Mons - the biggest volcano in the Solar System – “shares morphological similarities with active volcanic islands on Earth where major constructional slope breaks systematically occur at the sea-air transition in response to sharp lava viscosity contrasts.”
"We propose that the upper rim of the 6-kilometer high concentric main escarpment surrounding Olympus Mons most likely formed by lava flowing into liquid water when the edifice was an active volcanic island during the late Noachian–early Hesperian," the scientists added.
The Noachian and the Hesperian are geologic systems and time periods pertaining to Mars, which approximately correspond to between 4.1 and 3.7 billion years ago.
The researchers finally discovered that the shorelines of these islands have sharp escarpments, similar to those that ring Olympus Mons. "This leads us to propose that Olympus Mons was a former volcanic island surrounded by liquid water," the scientists pointed out.
They stressed that the findings would help provide “valuable insights into the timing and fate of Martian Oceans” and the history and evolution of the Red Planet on the whole.