Some volcanoes can produce eruptions so powerful they release oceans of dust
and toxic gases into the air, blocking out sunlight and changing a planet's
climate for decades. By studying the topography and mineral composition of a
portion of the Arabia Terra region in northern Mars, scientists recently
found evidence for thousands of such eruptions, or "super eruptions," which
are the most violent volcanic explosions known.
Spewing water vapor, carbon dioxide, and sulfur dioxide into the air, these
explosions tore through the Martian surface over a 500-million-year period
about 4 billion years ago. Scientists reported this estimate in a paper
published in the journal Geophysical Research Letters in July 2021.
"Each one of these eruptions would have had a significant climate
impact—maybe the released gas made the atmosphere thicker or blocked the Sun
and made the atmosphere colder," said Patrick Whelley, a geologist at NASA's
Goddard Space Flight Center in Greenbelt, Maryland, who led the Arabia Terra
analysis. "Modelers of the Martian climate will have some work to do to try
to understand the impact of the volcanoes."After blasting the equivalent of
400 million Olympic-size swimming pools of molten rock and gas through the
surface and spreading a thick blanket of ash up to thousands of miles from
the eruption site, a volcano of this magnitude collapses into a giant hole
called a caldera. Calderas, which also exist on Earth, can be dozens of
miles wide. Seven calderas in Arabia Terra were the first giveaways that the
region may once have hosted volcanoes capable of super eruptions.
Once thought to be depressions left by asteroid impacts to the Martian
surface billions of years ago, scientists first proposed in a 2013 study
that these basins were volcanic calderas. They noticed that they weren't
perfectly round like craters, and they had some signs of collapse, such as
very deep floors and benches of rock near the walls.
"We read that paper and were interested in following up, but instead of
looking for volcanoes themselves, we looked for the ash, because you can't
hide that evidence," Whelley said.
Whelley and his colleagues got the idea to look for evidence of ash after
meeting Alexandra Matiella Novak, a volcanologist at the Johns Hopkins
Applied Physics Laboratory in Laurel, Maryland. Matiella Novak already had
been using data from NASA's Mars Reconnaissance Orbiter to find ash
elsewhere on Mars, so she partnered with Whelley and his team to look
specifically in Arabia Terra.
The team's analysis followed up on the work of other scientists who earlier
suggested that the minerals on the surface of Arabia Terra were volcanic in
origin. Another research group, upon learning that the Arabia Terra basins
could be calderas, had calculated where ash from possible super eruptions in
that region would have settled: traveling downwind, to the east, it would
thin out away from the center of the volcanoes, or in this case, what's left
of them—the calderas.
"So we picked it up at that point and said, "OK, well, these are minerals
that are associated with altered volcanic ash, which has already been
documented, so now we're going to look at how the minerals are distributed
to see if they follow the pattern we would expect to see from super
eruptions," Matiella Novak said.
The team used images from MRO's Compact Reconnaissance Imaging Spectrometer
for Mars to identify the minerals in the surface. Looking in the walls of
canyons and craters from hundreds to thousands of miles from the calderas,
where the ash would have been carried by wind, they identified volcanic
minerals turned to clay by water, including montmorillonite, imogolite, and
allophane. Then, using images from MRO cameras, the team made
three-dimensional topographic maps of Arabia Terra. By laying the mineral
data over the topographic maps of the canyons and craters analyzed, the
researchers could see in the mineral-rich deposits that the layers of ash
were very well preserved—instead of getting jumbled by winds and water, the
ash was layered in the same way it would have been when it was fresh.
"That's when I realized this isn't a fluke, this is a real signal," said
Jacob Richardson, a geologist at NASA Goddard who worked with Whelley and
Novak. "We're actually seeing what was predicted and that was the most
exciting moment for me."
The same scientists who originally identified the calderas in 2013 also
calculated how much material would have exploded from the volcanoes, based
on the volume of each caldera. This information allowed Whelley and his
colleagues to calculate the number of eruptions needed to produce the
thickness of ash they found. It turned out there were thousands of
eruptions, Whelley said.
One remaining question is how a planet can have only one type of volcano
littering a region. On Earth, volcanoes capable of super eruptions—the most
recent erupted 76,000 years ago in Sumatra, Indonesia—are dispersed around
the globe and exist in the same areas as other volcano types. Mars, too, has
many other types of volcanoes, including the biggest volcano in the solar
system, called Olympus Mons. Olympus Mons is 100 times larger by volume than
Earth's largest volcano of Mauna Loa in Hawaii, and is known as a "shield
volcano," which drains lava down a gently sloping mountain. Arabia Terra so
far has the only evidence of explosive volcanoes on Mars.
It's possible that super-eruptive volcanoes were concentrated in regions on
Earth but have been eroded physically and chemically or moved around the
globe as continents shifted due to plate tectonics. These types of explosive
volcanoes also could exist in regions of Jupiter's moon Io or could have
been clustered on Venus. Whatever the case may be, Richardson hopes Arabia
Terra will teach scientists something new about geological processes that
help shape planets and moons.
"People are going to read our paper and go, "How? How could Mars do that?
How can such a tiny planet melt enough rock to power thousands of super
eruptions in one location?'" he said. "I hope these questions bring about a
lot of other research.
Reference:
Patrick Whelley et al, Stratigraphic Evidence for Early Martian Explosive
Volcanism in Arabia Terra, Geophysical Research Letters (2021).
DOI: 10.1029/2021GL094109
Tags:
Space & Astrophysics