The red planet Mars has once again intrigued scientists with a remarkable discovery. Recent research reveals that Mars conceals vast expanses of ice near its equator, extending several kilometers deep. If melted, this ice could cover Mars’s entire surface, potentially creating an ocean approximately 1.5 to 2.7 meters (about 4.9 to 8.9 feet) deep.
The ice was found in the Medusae Fossae Formation, an equatorial region of Mars first identified in 2007. At that time, the composition of the formation was unclear.
This discovery bolsters the hypothesis that life may have once existed on Mars, building on previous evidence that rivers once flowed there. This is the first instance where such a significant quantity of water has been detected at the Martian equator.
Thomas Watters, a geologist at the Smithsonian Institution, shared that re-examination of the Medusae Fossae Formation with updated data from the Mars Express’s MARSIS radar revealed even thicker deposits than initially thought, measuring up to 3.7 kilometers (approximately 2.3 miles) thick. The radar signals suggest the presence of layered ice, similar to that found in Mars’s polar caps, which are known to contain a significant amount of ice.
Scientists estimate that the quantity of water buried in this region is comparable to the volume of Earth’s Red Sea.
Regarding the Medusae Fossae Formation, scientists first noticed an unusual subsurface feature in this equatorial region in 2007, spanning about 5,000 kilometers along the equator. However, the nature of this feature, which is several kilometers high, remained a mystery, with possibilities ranging from dust and volcanic ash to remnants of Mars’s past, including water.
Researchers eventually concluded that the formation likely consists of water ice. They reasoned that if it were just dust, it would have compacted due to its depth and weight. Andrea Cicchetti, a physicist at the National Institute for Astrophysics in Italy, mentioned that the depth of the Medusae Fossae Formation (MFF) suggested something denser than dust, such as ice, as modeling with ice-free materials failed to replicate the MFF’s properties observed through MARSIS.
While there’s substantial evidence of Mars’s watery past, scientists are still unraveling the mystery of what happened to all the water on the planet. This recent discovery could provide crucial insights into this ongoing puzzle.