Did Ancient Mars Have a Runaway Greenhouse?
The southern rim of Argyre Planitia. Image Credit: NASA
Cosmic impacts that once bombed Mars might have sent temperatures skyrocketing upward on the Red Planet in ancient times, enough to set warming of the surface on a runaway course, researchers say.
According to scientists, these findings could potentially help explain how this cold, dry world might have once sustained liquid water, conditions potentially friendly for life.
The largest craters still visible on Mars were created about 3.7 billion to 4.1 billion years ago. For instance, the Argyre basin is thought to be 3.8 billion to 3.9 billion years old, a crater about 710 miles (1,140 kilometers) wide potentially generated by a comet or asteroid 60 to 120 miles (100 to 200 kilometers) in diameter.
The origin of these immense craters roughly coincides with when many branching Martian river valley networks apparently formed. The impact that created Argyre basin would have released an extraordinary amount of energy, far more than any bomb made by humanity, or even the meteor suspected of ending the Age of Dinosaurs — it would have been an explosion with an energy on the order of 10^26 joules, or 100 billion megatons of TNT. Altogether, scientists had calculated these giant collisions would have raised surface temperatures on Mars by hundreds of degrees.
The planet Venus has a greenhouse atmosphere. Could Mars also have experienced a similar effect early in its history? Image Credit: NASA
Now these researchers find this heating might not have been fleeting. Instead, this warming might have gone on a runaway course, pushing Mars into a long-term stable warm state.
The idea of runaway warming is most commonly associated with Venus. Scientists think that planet’s close proximity to the Sun heated its water, causing it to build up in its atmosphere as steam. Water is a greenhouse gas, trapping heat from the Sun that would have vaporized still more water, leading to a runaway greenhouse effect that apparently boiled all the oceans off Venus. Ultraviolet light would have then eventually split this atmospheric water into hydrogen and oxygen — the hydrogen escaped into space, the oxygen became trapped in the rocks of the planet, and the end-result was a bone-dry Venus.
The researchers note the many giant impacts Mars experienced might have heated the planet enough to send vast amounts of the the greenhouse gases water and carbon dioxide into the air. Their computer models suggest that there might have been enough of these gas in the Martian atmosphere to trigger a long-lasting runaway greenhouse effect. The impact that created the Argyre basin might have by itself been large enough to trigger such a chain reaction. Other impacts that might have pushed Mars toward a runaway greenhouse include the ones that created the Isidis and Hellas basins.
"Any terrestrial planet, including Venus, the Earth, or even exoplanets, may have experienced a temporary or permanent runaway greenhouse climate caused by impacts," researcher Teresa Segura, a planetary scientist at the commercial satellite firm Space Systems/Loral in Palo Alto, Calif., told Astrobiology Magazine.
False color image of gully channels in a crater in the southern highlands of Mars, taken by the High Resolution Image Science Experiment (HiRISE) camera on the Mars Reconnaissance Orbiter. The gullies emanating from the rocky cliffs near the crater’s rim (upper left) show meandering and braided patterns typical of water-carved channels. North is approximately up and illumination is from the left. The scale is 26 centimeters per pixel. Image Credit: NASA/JPL/University of Arizona
It is possible that any impacting comets might have delivered even more greenhouses gases into the atmosphere once they vaporized. Still, "the kinetic energy is of most importance," Segura said.
The researchers do note that during the runaway greenhouse phase, Mars would actually have been too warm for liquid water to last on its surface. Still, this heat would eventually subside — ultraviolet light would have caused the Martian atmosphere to lose its water just as Venus did, forcing the Red Planet to cool.
After runaway greenhouse conditions collapsed but before Mars became too cold for liquid water on its surface, the planet might have remained wet for a long time, possessing "a prolonged hydrological cycle with rainfall and valley networks as well as surface lakes," Segura said. It remains uncertain just how long either this runaway state or any wet period afterward might have lasted, but previous research suggests the warm climate may have lasted for at least centuries, she noted.
Future research could analyze the effects cosmic impacts might have on the climates of Venus, exoplanets and even Earth. Although impacts might very well be capable of causing a runaway greenhouse effect now, "the size of the impact required is much larger than that we need to worry about today," Segura said. That is to say, if our planet was hit by an impact large enough to create the Argyre basin, there probably wouldn’t be anyone on Earth left to worry about any of the collision’s potential effects on climate.
Segura and her colleagues Christopher McKay and Owen Toon detailed their findings online May 2 in the journal Icarus.