Water ice buried at Mars’ equator is over 2 miles thick

The Mars Express orbiter has detected enough water ice buried beneath the Red Planet’s equator to cover the entire planet in a shallow ocean if melted.

a black-and-white map of mars with blue sections denoting where water ice has been detected

This map shows the estimated amount of ice within the mounds that form the Medusae Fossae Formation (MFF) consists of a series of wind-sculpted deposits measuring hundreds of kilometers across and several kilometers high, indicating that the ice-rich deposits are up to 3000m thick. (Image credit: Planetary Science Institute/Smithsonian Institution)

A European Space Agency (ESA) probe has found enough water to cover Mars in an ocean between 4.9 and 8.9 feet (1.5 and 2.7 meters) deep, buried in the form of dusty ice beneath the planet’s equator.

The finding was made by ESA’s Mars Express mission, a veteran spacecraft that has been engaged in science operations around Mars for 20 years now. While it’s not the first time that evidence for ice has been found near the Red Planet’s equator, this new discovery is by far the largest amount of water ice detected there so far and appears to match previous discoveries of frozen water on Mars.

“Excitingly, the radar signals match what we expect to see from layered ice and are similar to the signals we see from Mars’ polar caps, which we know to be very ice rich,” said lead researcher Thomas Watters of the Smithsonian Institution in the United States in an ESA statement.

The deposits are thick, extended 3.7km (2.3) miles underground, and topped by a crust of hardened ash and dry dust hundreds of meters thick. The ice is not a pure block but is heavily contaminated by dust. While its presence near the equator is a location more easily accessible to future crewed missions, being buried so deep means that accessing the water-ice would be difficult.

Some 15 years ago, Mars Express detected deposits beneath a geological formation called the Medusae Fossae Formation (MFF), but scientists were not sure what those deposits consisted of. Mars’ geography is split between northern highlands and southern lowlands, and the huge 5,000-km-long MMF is situated near the boundary between the two.

It is suspected that the MMF itself formed within the past 3 billion years from lava flows and was covered in volcanic ash during an era long ago when Mars was volcanically active. Today, the MMF is covered in heaps of dust towering several kilometers high — it’s actually the most plentiful source of dust on the entire planet, fuel for the giant dust storms that can engulf Mars on a seasonal basis. Were the deposits just dust, perhaps filling a deep valley?

This perspective view shows Eumenides Dorsum, part of Mars’s Medusae Fossae Formation (MFF). The MFF consists of a series of wind-sculpted deposits measuring hundreds of kilometers across and several kilometers high. Found at the boundary between Mars’ highlands and lowlands, the deposits are possibly the biggest single source of dust on Mars, and one of the most extensive deposits on the planet. (Image credit: Caltech/JPL Global CTX Mosaic of Mars/Smithsonian Institution)

New observations by MARSIS, which is a subsurface radar on board Mars Express, now have the answer — and it’s not dust.

“Given how deep it is, if the MFF was simply a giant pile of dust, we’d expect it to become compacted under its own weight,” said Andrea Cicchetti of the National Institute for Astrophysics in Italy in a press statement. “This would create something far denser than what we actually see with MARSIS.”

Instead, the deposits are low in density and fairly transparent to MARSIS’ radar, which is exactly how one would expect water ice to appear in the data.

In this image, the white line on Mars’ surface (top) shows a stretch of land that was scanned by MARSIS. The graph below shows the shape of the land and the structure of the subsurface, with the layer of dry sediments (likely dust or volcanic ash) in brown and the layer of suspected ice-rich deposits in blue. The graph shows that the ice deposit is thousands of meters high and hundreds of kilometers wide. (Image credit: CReSIS/KU/Smithsonian Institution)

More pertinent is the question of how the water ice ended up buried at the equator. Sub-surface ice has been found in plentiful quantities on Mars before; NASA’s Phoenix mission dug up ice just beneath the dusty surface at the lander’s polar landing site in 2008. Meanwhile, early in its mission, Mars Express detected abundant water-ice extending down into the mid-latitudes, and NASA’s Mars Odyssey even found clues to the presence of water in the MMF in 2009.

More recently, ESA’s Trace Gas Orbiter detected hydrogen from water ice just beneath the surface of Candor Chaos, which is a segment of the immense rip in the surface of Mars that we call Vallis Marineris. Additionally, the remains of ancient glaciers, called relict glaciers, have been spotted in Eastern Noctis Labyrinthus, which is just 7.3 degrees south of the equator.

The presence of subsurface water-ice at low and equatorial latitudes hints at how Mars’ climate was very different in the distant past.

“This latest analysis challenges our understanding of the MFF and raises as many questions as answers,” said Colin Wilson, who is an ESA Project Scientist for Mars Express and the Trace Gas Orbiter, in the statement. “How long did these ice deposits form, and what was Mars like at the time?”

The ice’s existence could be the result of Mars’ wandering axis. Across the Red Planet’s history, the axial tilt of the planet’s poles is understood to have varied quite chaotically. Currently Mars’ poles are tilted to the ecliptic by 25 degrees (compared to Earth, which has a tilt of 23 degrees) but in the past this could have ranged from as shallow an angle as 10 degrees, to as extreme an angle as 60 degrees.

During the periods of high obliquity, when the poles are pointing closer to the sun than the equator, water-ice could form in large quantities on the surface at the equator. That ice could then be buried by ash and dust falls, to remain covered to this day.

The changing obliquity could also explain 400,000-year-old features discovered on Mars by the Chinese Zhurong rover, as well as the existence of gullies formed by liquid water where no such water should have existed.

The new discovery is described in a paper published in Geophysical Research Letters.

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