A new model suggests volcanic activity in Mars’ distant past spewed enough greenhouse gases to melt ice and warm the atmosphere
Why does the cold, barren surface of Mars contain geological features that appear to have been formed by flowing water: river valleys, lake basins, and deltas? A new model, published online in Nature Geoscience, suggests that sulfur spewed into the Martian atmosphere by ancient volcanoes could have periodically warmed the surface enough for the ice to melt and water to flow.
Weizmann Institute of Science
Satellite image of Olympus Mons on Mars, the largest volcano in the solar system at about three times the height of Mount Everest. Around 3.5 to 4 billion years ago, the release of volcanic gases, especially the greenhouse gas sulfur dioxide, may have warmed the surface of Mars episodically, melting the ice and thereby explaining the presence of geomorphological features indicative of the flow of water on the planet’s ancient surface.
Indeed, the signs of flowing water have been a puzzle, as the latest generation of climate models portrays Mars as an eternally ice-cold planet with all of its water frozen solid, especially early in its history, when the Sun was weaker than it is today.
Today, most of that water is locked in polar caps. Dr. Itay Halevy of the Weizmann Institute of Science’s Department of Earth and Planetary Sciences and Dr. James Head III of Brown University thought the answer might lie in the now dormant volcanoes on the planet’s surface, which could have played a larger role than previously thought in shaping its climate.
On Earth, volcanic emissions – sulfur compounds and ash – tend to cool the climate. But in the presumably dusty early atmosphere of Mars, the net effects might have been different. To understand their impact, Drs. Halevy and Head first calculated the size of ancient volcanic eruptions, based on the volcanic rock formations observed on the planetary surface today.
Their estimations show that the eruptions were violent – hundreds of times the force of the average eruption on Earth – and may have lasted up to a decade. This means that the amounts of gases spewed from the mouths of these volcanoes, from what we know of Earth’s eruptions, must have been enormous.
The team’s simulations showed large amounts of the greenhouse gas sulfur dioxide mixing into the atmosphere. But warming caused by the sulfur dioxide was thought to be outweighed by cooling due to the creation of sun-blocking sulfuric acid particles, which form as sulfur dioxide reacts in the atmosphere.
Drs. Halevy and Head showed that, in an atmosphere already as dusty as that of Mars, the sulfuric acid mostly forms thin coatings around particles of mineral dust and volcanic ash, subduing the added cooling. The net effect, according to the model the scientists created, was modest warming – just enough to allow water to flow at low latitudes on either side of the planet’s equator.
Liquid water may have flowed in these regions for tens to hundreds of years during and immediately after volcanic eruptions. The model suggests that during these brief, but intense, wet periods, the surface of the planet could have been carved by flowing rivers and streams.
Dr. Itay Halevy’s research is supported by the Sir Charles Clore Research Prize; the Carolito Stiftung; the estate of Olga Klein Astrachan; and the European Research Council.
The Weizmann Institute of Science in Rehovot, Israel, is one of the world’s top-ranking multidisciplinary research institutions. The Institute’s 3,800-strong scientific community engages in research addressing crucial problems in medicine and health, energy, technology, agriculture, and the environment. Outstanding young scientists from around the world pursue advanced degrees at the Weizmann Institute’s Feinberg Graduate School. The discoveries and theories of Weizmann Institute scientists have had a major impact on the wider scientific community, as well as on the quality of life of millions of people worldwide.
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