A new NASA climate simulation suggests that extremely large volcanic eruptions called “flood basalt eruptions” might significantly warm Earth’s climate and devastate the ozone layer that shields life from the Sun’s ultraviolet radiation.
The result contradicts previous studies indicating these volcanoes cool the climate. It also suggests that while extensive flood-basalt eruptions on Mars and Venus may have helped warm their climates, they could have doomed the long-term habitability of these worlds by contributing to water loss.
A new NASA climate simulation suggests that extremely large volcanic eruptions called “flood basalt eruptions” might significantly warm Earth’s climate and devastate the ozone layer that shields life from the Sun’s ultraviolet radiation. Credits: NASA/GSFC/James Tralie Download video
Unlike brief, explosive volcanic eruptions such as Pinatubo or January’s Hunga Tonga-Hunga
Ha‘apai that occur over hours or days, flood basalts are
regions with a series of eruptive episodes lasting perhaps centuries each, and
occurring over periods of hundreds of thousands of years, sometimes even
longer. Some happened at about the same time as mass-extinction events, and
many are associated with extremely warm periods in Earth’s history. They also
appear to have been common on other terrestrial worlds in our solar system,
such as Mars and Venus.
“We expected intense cooling in our simulations,” said Scott Guzewich of
NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “However, we found
that a brief cooling period was overwhelmed by a warming effect.” Guzewich is
lead author of a paper about this
research published Feb. 1 in Geophysical Research
Letters.
Image of a flood-basalt deposit on Mars in the Marte Vallis region taken by the High Resolution Science Imaging Experiment (HiRISE) instrument on board NASA’s Mars Reconnaissance Orbiter spacecraft. Credits: NASA/University of Arizona/HiRISE
While the ozone loss was not a surprise, the simulations indicated the
potential magnitude of the destruction, “about two-thirds reduction over global
average values, roughly equivalent to the whole planet having an ozone thinning
comparable to a severe Antarctic ozone hole,” said Guzewich.
The researchers used the Goddard Earth Observing System
Chemistry-Climate Model to simulate a four-year-long phase
of the Columbia River Basalt
(CRB) eruption that occurred between 15 million and
17 million years ago in the Pacific Northwest of the United States. The model
calculated the effects of the eruption on the troposphere, the turbulent lowest
layer of the atmosphere with most of the water vapor and weather, and the
stratosphere, the next layer of the atmosphere that is mostly dry and calm. CRB
eruptions were likely a mix of explosive events that sent material high into
the upper troposphere and lower stratosphere (about 8 to 10.5 miles or 13 to 17
kilometers altitude) and effusive eruptions that did not extend above 1.9 miles
(about 3 kilometers) altitude. The simulation assumed that explosive events
happened four times per year and released about 80% of the eruption’s sulfur
dioxide gas. They found that globally, there was a net cooling for about two
years before the warming overwhelms the cooling effect. “The warming
persists for about 15 years (the last two years of the eruption and then
another 13 years or so),” said Guzewich.
The new simulation is the most comprehensive yet done for flood basalt
eruptions and integrates the effects of atmospheric chemistry and climate
dynamics on each other, revealing an important feedback mechanism that earlier
simulations missed.
“Eruptions like the one we simulated would emit massive amounts of sulfur
dioxide gas,” said Guzewich. “Chemistry in the atmosphere quickly converts
these gas molecules to solid sulfate aerosols. These aerosols reflect visible
sunlight, which causes the initial cooling effect, but also absorb infrared
radiation, which warms the atmosphere aloft in the upper troposphere and lower
stratosphere. Warming this region of the atmosphere allows water vapor (that’s
normally confined near the surface) to get mixed into the stratosphere (which
is normally very dry). We see a 10,000% increase in stratospheric water vapor.
Water vapor is a very effective greenhouse gas, and it emits infrared radiation that warms the planet’s surface.”
The predicted surge of water vapor into the stratosphere also helps explain
the severity of the ozone layer depletion. “Ozone layer depletion happens in a
couple different ways,” said Guzewich. “Following the eruption, the circulation
of the stratosphere changes in ways that discourage ozone
formation. Second, all that water in the stratosphere also helps destroy
ozone with the hydroxyl (OH) radical.”
Flood basalts also release carbon dioxide, a greenhouse gas as well, but
they don’t appear to emit enough to cause the extreme warming associated with
some eruptions. The excess heating from stratospheric water vapor could provide
an explanation.
Although Mars and Venus may have had oceans of water in the distant past,
both are currently very dry. Scientists are investigating how these worlds lost
most of their water to became inhospitable for life. If the surge of water
vapor into the upper atmosphere predicted by the simulation is realistic,
extensive flood volcanism could have contributed to their arid fates. When
water vapor is lofted high in the atmosphere, it becomes susceptible to being
broken apart by sunlight, and the lightweight hydrogen atoms from the water
molecules can escape to space (water is two hydrogen atoms bound to an oxygen
atom). If sustained over long periods, this could deplete oceans.
The research was funded by the NASA Goddard Sellers Exoplanet Environments
Collaboration and NASA’s Center for Research and Exploration in Space Science
and Technology, NASA Cooperative Agreement Award #80GSFC17M0002.
Bill Steigerwald NASA Goddard Space Flight Center, Greenbelt, Maryland
Source: NASA
Simulation Suggests Some Volcanoes Might Warm Climate, Destroy Ozone Layer
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