Mars Megatsunami May Have Been Caused by Chicxulub-Like Asteroid Impact
A Martian megatsunami could have been attributable to an asteroid collision much like the Chicxulub affect – which contributed to the mass extinction of all non-avian dinosaurs on Earth 66 million years in the past – in a shallow ocean area. This is in keeping with a research revealed immediately (December 1) within the journal Scientific Reports.
Previous analysis has proposed that an asteroid or comet affect inside an ocean within the Martian northern lowlands could have triggered a megatsunami roughly 3.four billion years in the past. However, previous to this research, the placement of the ensuing affect crater was unclear.
Alexis Rodriguez and colleagues analyzed maps of Mars’ surface, created by combining images from previous missions to the planet, and identified an impact crater that could have resulted from the asteroid collision that caused the megatsunami. The crater – which they have named Pohl – has a diameter of about 70 miles (110 kilometers) and is located within an area of the northern lowlands that previous studies have suggested may have been covered by an ocean, in a region around 400 feet (120 meters) below its proposed sea level. The authors suggest that Pohl may have formed around 3.4 billion years ago based on its position above and below rocks previously dated to this time.
The authors simulated asteroid and comet collisions with this region to test what type of impact that could have created Pohl and whether this could have led to a megatsunami. They found that the simulations that formed craters with similar dimensions to Pohl were caused by either a nine-kilometer asteroid encountering strong ground resistance – releasing 13 million megatons of TNT energy – or a three-kilometer asteroid encountering weak ground resistance – releasing 0.5 million megatons of TNT energy. The amount of energy released by Tsar Bomba, the most powerful nuclear bomb ever tested, was approximately 57 megatons of TNT energy.
Both simulated impacts formed craters measuring 70 miles (110 kilometers) in diameter and generated megatsunamis that reached as far as 900 miles (1,500 kilometers) from the center of the impact site. Analysis of the megatsunami caused by the two-mile (three-kilometer) asteroid impact indicated that this tsunami may have measured up to approximately 820 feet (250 meters) tall on land.
The authors suggest that the aftermath of the proposed Pohl impact may have had similarities with the Chicxulub impact on Earth, which previous research has suggested occurred within a region 650 feet (200 meters) below sea level, generated a crater with a temporary diameter of 60 miles (100 kilometers), and led to a megatsunami that was 650 feet (200 meters high) on land.
Reference: “Evidence of an oceanic impact and megatsunami sedimentation in Chryse Planitia, Mars” 1 December 2022, Scientific Reports.