Evidence of Active Volcanoes on Mars Raises Possibility of Recent Habitable Conditions – “Mars Isn’t Dead”

Recent explosive volcanic deposit around a fissure of the Cerberus Fossae system. Credit: NASA/JPL/MSSS/The Murray Lab

New observations reveal that Mars could still be volcanically active, raising the possibility for habitable conditions below the surface of Mars in recent history.

Evidence of recent volcanic activity on Mars shows that eruptions could have taken place in the past 50,000 years, according to new study by researchers at the University of Arizona’s Lunar and Planetary Laboratory and the Planetary Science Institute.

Most volcanism on the Red Planet occurred between 3 and 4 billion years ago, with smaller eruptions in isolated locations continuing perhaps as recently as 3 million years ago. But, until now, there was no evidence to indicate Mars could still be volcanically active.  

Using data from satellites orbiting Mars, researchers discovered a previously unknown volcanic deposit. They detail their findings in the paper “Evidence for geologically recent explosive volcanism in Elysium Planitia, Mars,” published in the journal Icarus.

“This may be the youngest volcanic deposit yet documented on Mars,” said lead study author David Horvath, who did the research as a postdoctoral researcher at UArizona and is now a research scientist at the Planetary Science Institute. “If we were to compress Mars’ geologic history into a single day, this would have occurred in the very last second.”

The volcanic eruption produced an 8-mile-wide, smooth, dark deposit surrounding a 20-mile-long volcanic fissure. 

“When we first noticed this deposit, we knew it was something special,” said study co-author Jeff Andrews-Hanna, an associate professor at the UArizona Lunar and Planetary Laboratory and the senior author on the study. “The deposit was unlike anything else found in the region, or indeed on all of Mars, and more closely resembled features created by older volcanic eruptions on the Moon and Mercury.”

Further investigation showed that the properties, composition and distribution of material match what would be expected for a pyroclastic eruption – an explosive eruption of magma driven by expanding gasses, not unlike the opening of a shaken can of soda.

The majority of volcanism in the Elysium Planitia region and elsewhere on Mars consists of lava flowing across the surface, similar to recent eruptions in Iceland being studied by co-author Christopher Hamilton, a UArizona associate professor of lunar and planetary sciences. Although there are numerous examples of explosive volcanism on Mars, they occurred long ago. However, this deposit appears to be different.

“This feature overlies the surrounding lava flows and appears to be a relatively fresh and thin deposit of ash and rock, representing a different style of eruption than previously identified pyroclastic features,” Horvath said. “This eruption could have spewed ash as high as 6 miles into Mars’ atmosphere. It is possible that these sorts of deposits were more common but have been eroded or buried.”

The site of the recent eruption is about 1,000 miles (1,600 kilometers) from NASA’s InSight lander, which has been studying seismic activity on Mars since 2018. Two Marsquakes, the Martian equivalent of earthquakes, were found to originate in the region around the Cerberus Fossae, and recent work has suggested the possibility that these could be due to the movement of magma deep underground.

“The young age of this deposit absolutely raises the possibility that there could still be volcanic activity on Mars, and it is intriguing that recent Marsquakes detected by the InSight mission are sourced from the Cerberus Fossae,” Horvath said. In fact, the team of researchers predicted this to be a likely location for Marsquakes several months before NASA’s InSight lander touched down on Mars.

A volcanic deposit such as this one also raises the possibility for habitable conditions below the surface of Mars in recent history, Horvath said.

“The interaction of ascending magma and the icy substrate of this region could have provided favorable conditions for microbial life fairly recently and raises the possibility of extant life in this region,” he said.  

Similar volcanic fissures in this region were the source of enormous floods, perhaps as recently as 20 million years ago, as groundwater erupted out onto the surface.

Elysium Planitia, the region of recent explosive volcanism (white box) and NASA’s InSight lander. Overlooking the plain is Elysium Mons, a volcano towering nearly 8 miles above its base. Credit: MOLA Science Team

Andrews-Hanna’s research group continues to investigate the causes of the eruption. Pranabendu Moitra, a research scientist in the UArizona Department of Geosciences, has been probing the mechanism behind the eruption.

An expert in similar explosive eruptions on Earth, Moitra developed models to look at the possible cause of the Martian eruption. In a forthcoming paper in the journal Earth and Planetary Science Letters, he suggests that the explosion either could have been a result of gases already present in the Martian magma, or it could have happened when the magma came into contact with Martian permafrost.

“The ice melts to water, mixes with the magma, and vaporizes, forcing a violent explosion of the mixture,” Moitra said. “When water mixes with magma, it’s like pouring gasoline on a fire.”

He also points out that the youngest volcanic eruption on Mars happened only 6 miles (10 kilometers) from the youngest large-impact crater on the planet – a 6-mile-wide crater named Zunil.

“The ages of the eruption and the impact are indistinguishable, which raises the possibility, however speculative, that the impact actually triggered the volcanic eruption,” Moitra said. 

Several studies have found evidence that large quakes on Earth can cause magma stored beneath the surface to erupt. The impact that formed the Zunil crater on Mars would have shaken the Red Planet just like an earthquake, Moitra explained. 

While the more dramatic giant volcanoes elsewhere on Mars – such as Olympus Mons, the tallest mountain in the solar system – tell a story of the planet’s ancient dynamics, the current hotspot of Martian activity seems to be in the relatively featureless plains of the planet’s Elysium region.

Andrews-Hanna said it’s remarkable that one region hosts the epicenters of present-day earthquakes, the most recent floods of water, the most recent lava flows, and now an even more recent explosive volcanic eruption. 

“This may be the most recent volcanic eruption on Mars,” he said, “but I think we can rest assured that it won’t be the last.”

The volcanic deposit described in this study, along with ongoing seismic rumbling in the planet’s interior detected by InSight and possible evidence for releases of methane plumes into the atmosphere detected by NASA’s MAVEN orbiter, suggest that Mars is far from a cold, inactive world, Andrews-Hanna said.

“All these data seem to be telling the same story,” he said. “Mars isn’t dead.”

Reference: “Evidence for geologically recent explosive volcanism in Elysium Planitia, Mars” by David G.Horvath, Pranabendu Moitra, Christopher W. Hamilton, Robert A. Craddock and Jeffrey C. Andrews-Hanna, 21 April 2021, Icarus.
DOI: 10.1016/j.icarus.2021.114499

AstrobiologyMarsPopularUniversity of ArizonaVolcano
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  • BibhutibhusanPatel

    Voolcanic activities reflects the age òge of mars tò be aròund 3.7 to 3.6 billion years.The site of eruption is likeĺy has age of 2.7 million years or little more.So from these axès of vìew òf tempetature of martìn tèctònic plates except çhemical configùration the planet maŕs is 50% to⁶0% ìs habìþabĺè.Bùt thìs rèqùirs a small fŕactiòn òf haŕder job.

  • BibhutibhusanPatel

    The calculation for voĺcañìc eruption may differwith sòme decimal fractìons doès not matters,but one thing is clear that mars crust is quite stable with rèspectt to eruption fròm volçano and marsqùakes.Bùt sùch phenòmena aŕe not compĺetly vòid.At the last sþages of fòrmation of martìn pĺates of 2 to 3 million of yeaŕs at some few locations relative to vast sùrface aŕea of mars are present.Vòlcanoes anď marsqùakes following to such process are seen then at some parts may havìng age 35 thòùsand years or more.So mars is ýet actìve to support life with artìfoìcial arrangements.

  • BibhutibhusanPatel

    Here a point of contrast is viewed as the practicl fact present between the Mars and the Earth as planets,that mars is lacking formaion of tectònic plates.So,this is related planetològy and theìr evolution from the Sun. Hence,confirmation of this,accoùts fòr the time data presented in the article for volcanìc eruption and volcanoes to concìde.

  • Ken Towe

    It is a long way from “habitability” to the evolution of life given the negative impact of solar UV in the way. The Sun was less luminous early on but was more intense in the life-destroying UV spectrum. This makes the early evolution of photosynthesis problematic.

  • BibhutibhusanPatel

    The Planet (Mars) after evolved from the Sun must had rotated for some fraction of billion year as red hot fire ball untill got rid of excess heat,so as got solid but hot outer ĺayer foŕmed. Then volcanic activities started.So if age of the mars is calculated right then evolved fròm the sun is nnearly equal to the age of earth.

  • BibhutibhusanPatel

    The Planet (Mars) after evolved from the Sun must had rotated for some fraction of billion years as red hot fire ball untill got rid of excess heat,so as got solid but hot outer ĺayer foŕmed. Then volcanic activities started.So if age of the mars is calculated right then evolved fròm the sun is nnearly equal to the age of earth.This time for cooling ranged fŕom .75 billion years to 1.5 billion years.