Tamu Massif, is a massive shield volcano that rises over 20 kilometers into the air
and covers an area the size of California or Japan.
Photo credit: Will Sager.
From SchmidtOcean
Tamu Massif, located about 1000 miles east of Japan, is the largest known single volcano on Earth, but the process that created it remains a mystery.
With an area equivalent to Japan or California, the undersea volcanic mountain - a part of the western
Pacific Shatsky Rise oceanic plateau - is believed to have formed during the late Jurassic period. Exactly how it formed in the age when dinosaurs still ruled is unknown, but scientists on this 32-day expedition aboard Falkor hope to reveal its origins.
Tamu Massif is located within the Shatsky rise.
Credit: Will Sager.
Tamu Massif in the GeoGarage platform
Principal Investigator William Sager from the University of Houston Department of Earth and Atmospheric Sciences, and Geophysicist Masao Nakanishi from Chiba University, along with their science team, will transit over the western Pacific Ocean to Shatsky Rise, an undersea oceanic plateau where Tamu Massif is located.
As one of the few oceanic plateau volcanoes formed during a time of geomagnetic reversals, Tamu Massif holds a unique record of undersea geographic formation: magnetic anomalies in the oceanic crust.
This makes it easier to understand the underwater volcano’s history and the key interactions it has with the mid-ocean ridges.
Reversing poles
To appreciate geomagnetic reversals, one needs to know some aspects
of Earth’s magnetic field.
Our planet has a magnetic field with North
and South Poles, just like a bar magnet.
Geophysicists reason that the
Earth’s magnetic field is created by the motion of the fluid iron outer
core, which creates electric currents that in turn produce the magnetic
field.
At certain times in the past, core flow changed, causing the
poles to flip - what was once the North Pole is now the South, and vice
versa.
Lava becomes magnetized as it solidifies to rock on the ocean
floor, creating a record of the magnetic pole direction at the time.
The
magnetic lava rock perturbs the Earth’s magnetic field, causing a
negative or positive “magnetic anomaly” depending on whether it adds to
or subtracts from the Earth’s field.
In the ocean basins, the mid-ocean spreading ridges, divergent plate
boundaries where oceanic crust is formed, record linear magnetic
anomalies that parallel the spreading ridge crest.
Correlating the
magnetic reversal pattern to time, scientists have used these magnetic
anomalies to determine the age of the oceanic crust and the pattern of
its development.
Because Tamu Massif formed during a time of
geomagnetic reversals, its lavas also preserve magnetic anomalies that
can be interpreted by scientists to show the construction of the
volcano.
Using multibeam sonar systems and a marine magnetometer, the science
team and Falkor crew plan on collecting seafloor and magnetic data in
October and November of this year, to build a well-constrained magnetic
anomaly map.
This map will allow for a better understanding of both Tamu
Massif formation and its internal structure.
While it will not be
possible to completely cover all of Tamu Massif with multibeam sonar
bathymetry data, new underwater depth information collected on the
cruise will substantially improve the knowledge of Tamu Massif
topography and structure, all of which will help in understanding the
monster volcano hidden beneath the sea.
Cruise survey plan. Heavy lines show proposed cruise tracks.
Ingress and
egress transit tracks are not shown.
Credit: Will Sager.
The Birth of a Giant
Shatsky Rise is one of the largest oceanic plateaus and is believed to
have formed at the triple junction of three tectonic plates: the
Pacific, the Farallon, and the Izanagi.
Like most oceanic plateaus, it
is a huge volcanic mountain range consisting mainly of basalt rock
covered with a generally thin veneer of sediments.
How such a massive
volcano as Tamu Massif formed in this area is unknown.
Did it erupt as a
huge boil on top of the mid-ocean ridges?
Did it disrupt and reorganize
the seafloor, spreading the ground wide at the triple junction?
The
answer to these fundamental questions will help scientists understand
how oceanic plateaus form and how such volcanic eruptions interact with
mid-ocean ridges and their underlying magma convection system.
Model of hotspot volcanism. A. Rising mantle plume. B. Outpourings of
basalt generate the oceanic plateau. C. Less voluminous activity
produces a volcanic chain. Image from Tasa Graphics.
Plume Head versus Fertile Mantle
There are two main, competing models that are debated about Tamu
Massif’s formation.
The “plume head” hypothesis proposes that hot mantle
under the ocean floor, begins to rise, forming a growing column of
slowly flowing material.
When this “plume head” reaches the base of the
outermost shell of the Earth, it bursts through, causing a massive
eruption and intrusion of igneous material, as well as forming large
oceanic plateaus (if undersea, as the case would be here).
This model gained acceptance mainly because geochronology data from
several other geographic features appear consistent with short-lived and
massive outpourings of lava.
This hypothesis excites Earth scientists
because it implies periods of massive flux of mantle material to the
surface.
Moreover, such massive eruptions also imply the release of
large quantities of heat and gasses, which could have far-ranging
environmental effects.
An alternative idea - the “fertile mantle” hypothesis - suggests
eruptions occur because plate boundaries and cracks are releasing
pressure above areas of upper mantle with lower melting temperatures.
This hypothesis implies that the source of plateau magma is shallow, and
that the massive vertical mantle movement of the “plume head”
hypothesis does not occur.
Simply, a “plume head” creates a large volcano in a huge, short,
gushing eruption.
At a much slower pace, and a “fertile mantle” fosters
extended surges of molten core, releasing stress at plate boundaries and
forming a series of merging volcanoes over a longer period of time.
Oceanic plateau structure is key to figuring out whether this dichotomy
is true, but plateau structure is poorly understood because these
features are so large in size, as well as hidden and inaccessible
beneath the sea.
Today, earth scientists still debate which of these two mechanisms
provide a better explanation for large areas of volcanic rocks, known as
igneous provinces.
Many oceanic plateaus contain significant
complexities – unexpected ingredients or evidence - that do not lend
themselves to clear origin certainty.
Depending on whom you talk to, the
“plume head” model either needs amendments or should be dismissed.
As
is often the case in science, neither hypothesis may be entirely
correct, but these two concepts provide a framework for debate that will
ultimately help geoscientists understand this important flux of
material to the Earth’s surface.
Translating Evidence into Fact
The linear magnetic anomalies in the mid-ocean ridges are key to
understanding how Tamu Massif formed.
One side (north) of Tamu Massif
seems to have magnetic lineations, but the other (south) seems to have a
broad, coherent anomaly caused by the whole volcano.
On this side,
massive lava flows have been cored and imaged by acoustic profiling.
Magnetic lineations imply well-behaved, limited magmatic eruptions
whereas the coherent anomaly implies a massive eruption.
Thus, it
appears that Tamu Massif may have a Jekyll and Hyde personality.
To
date, the magnetic data has been collected sparsely, and the science
team hopes this cruise will fill the existing gaps with precise mapping
of undersea geography and magnetic charting.
The goal is to combine the
newly collected data with existing data to construct both magnetic and
bathymetric contour maps of Tamu Massif.
Perhaps a revelation from tiny
magnetically charged particles will explain the creation of one of
Earth’s largest physical features.
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