GIANT ANCIENT VOLCANO DISCOVERED ON MARS

 From - Sky & Telescope

By- Javer Barbuzano

Edited by Amal Udawatta

The newly discovered giant volcano on Mars is located just south of the planet’s equator, in eastern Noctis Labyrinthus, west of the Valles Marineris canyone system. The volcano sits on the eastern edge of a broad regional topographic rise called Tharsis, home to three other well-known giant volcanoes: Ascraeus Mons, Pavonis Mons, and Arsia Mons. Although more eroded and lower than these giants, the newly discovered volcano rivals the others in diameter (red dashed circle).
Background: NASA / USGS; interpretation and annotations by Pascal Lee and Sourabh Shubham

It's not every day that a giant volcano is discovered hiding in plain sight. By reviewing satellite imagery from many missions, scientists have spotted the remains of a colossal volcano on Mars. The volcano, provisionally named “Noctis Mons,” had been imaged repeatedly since the early 1970s, but extensive erosion had concealed it from view. Researchers have also spotted hints at an adjacent glacier buried underneath the volcanic slopes.

Noctis Mons is located near the Martian equator, in the eastern part of the Tharsis volcanic province, sandwiched between the vast canyons of Valles Marineris and the fractured maze-like terrain of Noctis Labyrinthus. “In fact, it is eastern Noctis Labyrinthus that is the volcano,” says planetary scientist Pascal Lee (SETI Institute and the Mars Institute) who announced the finding during the 55th Lunar and Planetary Science Conference in The Woodlands, Texas. The discovery adds yet another landmark to this intriguing region.

A LARGE VOLCANO WITH A COMPLEX STORY

The newfound giant volcano is located in the middle of the action on Mars: This topographic map shows the location of the Noctis Volcano, which lies in the middle of the largest volcanic and canyon provinces on Mars.
Background: NASA Mars Global Surveyor / Mars Orbiter Laser Altimeter digital elevation model; interpretation & annotations: Pascal Lee & Sourabh Shubham

The newfound volcano is 450 kilometers (280 miles) wide and, even eroded as it is, reaches elevations of more than 9 kilometers (close to 30,000 feet). It dwarfs Earth’s largest volcano, Mauna Loa, which is 8 km tall from seafloor to summit, and spans 120 kilometers on its largest side. Mars, however, tends to have larger volcanos, with the record-bearing Olympus Mons reaching a height more than 22 kilometers.

While it has been imaged repeatedly since Mariner 9, which orbited the Red Planet in 1971, the volcano’s heavily deteriorated form prevented its detection. “It's deeply eroded and doesn't look like a beautiful cone-shaped shield [volcano], but that’s pretty much what it is,” Lee says. A combination of fracturing, thermal erosion, and glacial erosion has produced a jumbled landscape, with a few elevated mesas — sandwiches of lava, pyroclastics, and water ice — cut through by a network of valleys and collapsed areas.

Still, scientists pieced together several clues to reveal the formations’ volcanic origin. The elevated mesas form a curved ridge that gently slopes outwards from a central summit. A caldera remnant — a collapsed volcanic crater once filled with lava — is also visible near the center of the structure. Additionally, lava flows, deposits of volcanic ash and pumice, and accumulations of hydrated minerals are scattered throughout the structure.

While some of these volcanic deposits had been spotted before, connecting all the evidence to find a giant, long-lost volcano took the scientists by surprise. “When we saw that that arc of high points reaching 9,000 meters and sloping away, that's when we thought: Could this possibly be a volcano?” Lee says. “Now that we know that is there, it’s very difficult to unsee it.”

It’s possible other mechanisms could have formed the newfound eroded dome, such as uplift caused by raising magma underneath the region, says Alexis Rodriguez (NASA’s Marshall Space Flight Center), who wasn’t involved with the present study. However, Lee says that, putting together all the evidence, the giant volcano scenario is very promising. The researchers are already writing a paper detailing their findings.

The study also revealed a vast region of volcanic deposits surrounding Noctis Mons. This area is dominated by numerous, low, rounded mounds resembling blisters, referred to as rootless cones. These are believed to have formed where hot volcanic material came to rest on top of ice- or water-rich ground, causing explosive bursts of steam to pierce the surface.

Evidence for the newfound Noctis Volcano comes in the form of well-preserved volcanic lava flow and erupted rocks. Those volcanic rocks, thrown out during eruption, resulted in steam vents (labeled "rootless cones"), produced when the hot materials came in contact with water ice. Breaks in the volcanic deposits reveal light-toned sulfate salts, which are a result of chemical reactions between the volcanic rocks and existing water ice. The discovery team had previously described the largest sulfate deposits as appearing glacier-like (labeled "relict glacier"). Glacier ice might still be preserved there, protected under a thin layer of sulfate salts. By extension, the rootless cones and other sulfate deposits in this area may be blanketing even more glacier ice.
Background: NASA Mars Reconnaissance Orbiter / High Resolution Imaging Science Experiment / Context Imager / Compact Reconnaissance Imaging Spectrometer for Mars; interpretation and annotations: Pascal Lee & Sourabh Shubham

This finding connects with the team’s previous discovery of a nearby sulfate-salt deposit, which has shapes and features resembling those of a glacier. Lee and his collaborator, graduate student Sourabh Shubham (University of Maryland, College Park), think that this glacier-like feature formed when a layer of volcanic ash landed on top of a glacier. The ash reacted with the acidic water and turned into a salty mineral called jarosite, forming deposits that mimicked the shapes of the glacier underneath it, like plaster in a mold. Later on, some sort of erosive process removed the upper layers of ash, revealing the glacier-like salt layers.

“The ice is probably still there, but it’s protected from disappearing by salt,” Lee says.

Similarly, the researchers think that the giant Noctis Mons volcano was built like a layered cake, alternating deposits of ice and volcanic material. The slopes of the mesas show evidence of this, because there salt deposits alternate with layers of volcanic material and now-solid lava flows.

Taken together, the eroded volcano and the remnant of the glacier suggest that the volcanic blanket in this large region may be concealing a vast sheet of glacier ice beneath its surface.

“Finding this interaction between buried glaciers and magmatism is very positive, and it’s connected with topics such as habitability and the likelihood of finding biosignatures,” Rodriguez says. “If it’s really true, it would be a very important discovery.”

NEW TARGET FOR EXPLORATION

Many questions remain open about Noctis Mons.  The available evidence suggests that it became active early in Mars’ history, but the exact timeframe and whether it’s currently active remain a mystery. The likely presence of volcanic heat and underground water, maybe continuously over billions of years, makes the location a prime candidate in the search for Martian life. From a purely geological standpoint, it also provides a cross-section view at the interior of a giant Martian volcano.

The possible presence of shallow, near-equatorial ice is also potentially useful, since it could provide a readily accessible source of water for human exploration. The proximity to Valles Marineris and Noctis Labyrinthus is likewise attractive for future crewed exploration, since these are great places to look for signs of Martian life.