This section is divided into 2 parts; Hydrothermal Systems and Oceanic volcanism


Oceanic Volcanism

Journey to the centre of the earth


In the section on plate tectonics we have looked at some aspects of ocean volcanism eg the formation of spreading ridges and island arcs – in this section we will discuss in more detail the various oceanic environments where magmatic activity occurs and investigate the kind of rocks produced. Volcanic eruptions on the surface of the earth are driven by melting at depth - to produce magma. Magma types are termed mafic, intermediate, or felsic depending on their silica (SiO2) content.

There are three types of volcanism or volcanic settings in the ocean basins:
1. Ocean spreading ridge volcanism
2. Trench related volcanism; island arcs and mountain chains
3. Mantle Plume (hot spot) volcanism

Ocean spreading ridge volcanism


Oceanic spreading ridges are the most active volcanic zones on earth, continually producing new oceanic lithosphere. Our understanding of the composition of the oceanic lithosphere comes from:

1. Collecting samples from the sea floor,
2. seismic studies that show layers of different velocity. These layers have been subdivided into 4 – the seismic velocity increases from layer 1 (sediments) at the top to layer 4 (mantle) at the base.
3. cores collected by the Ocean Drilling Program and
4. sections of the oceanic lithosphere that have been pushed up onto the continents. These sections are termed ophiolites. One of the most famous and best studies ophiolite complexes is the Semail ophiolite, which comprises the Oman Mountains in northern Oman (virtual tour at http://www.bris.ac.uk/Depts/Geol/vft/oman.htm). But ophiolites can also be found closer to home in Papua New Guinea, New Caledonia and New Zealand and on Australias' own MacQuarie Island.

< Schematic representation of ocean crust at a mid-ocean ridge. In an active ridge, magma rises out of the mantle and into the overlying crust where it feeds a magmatic system comprised of a crystal mush zone (85 percent crystals and 15 percent melt) and a magma lens at the base of sheeted dikes. Magma is also channeled through dikes to the seafloor. On both sides of the crystal mush zone are gabbroic cumulates, the fossil remains of earlier magmatic systems. The gabbros are divided into upper gabbros where there is no significant crystal layering, and layered gabbros, where crystal layering (dashed lines in the figure) is well developed. The upper gabbros are further characterized by shear zones oriented parallel to the high-angle normal faults. These provide channels for the migration of late, evolved melts. The sheeted dikes and pillow lavas are composed of basaltic rocks formed, respectively, by the rapid cooling of magma near the seafloor and the quenching of magma on the seafloor (from http://www.oceandrilling.org/Documents/Oceanus/Lith/Lith3HR.html)



The top of the idealized ophiolite sequence consists of ocean sediments (eg chert, limestone etc). Below this are pillow basalts - tholeiite, which form when hot magma is extruded onto the ocean floor. Pillow lavas are the most abundant volcanic rock on earth. They are often altered to serpentinite by interaction with hot seawater. Sheeted or intruded dikes occur below the pillow basalts. These dikes represent the feeders to the subaqueous pillow basalts. Underlying the basalts is a layer of intrusive rock called gabbro. Gabbro is similar in composition to basalt but because it cools more slowly it has bigger crystals. The upper part of the gabbro is generally massive, but the basal part of the gabbro commonly contains layers. The layers (called cumulates) are composed of the crystals that form first and sink to the bottom of the magma. The contact between the gabbro layer and an ultramafic rock called peridotite, marks the geophysical base of the crust known as the Moho. Here the density contrast causes a marked attenuation in seismic velocity.


< Pillow lava on the sea floor (photo USGS)

< Late magmatic liquid (white) intrudes a foliated gabbro. This core was retrieved during ODP Leg 118 on the Southwest Indian Ridge

< On ODP Leg 147 (Hess Deep Rift Valley in the Pacific Ocean). Core reveals black peridotite impregnated with white magmatic liquid.


Trench related volcanism; island arcs and mountain chains


As we noted in the section on convergent boundaries, in the process known as subduction, one plate descends beneath another. Subduction zones are characterised by the formation of deep ocean trenches and the growth of chains of volcanoes on the overriding plate, parallel to the trench. The so called Ring of Fire, a region of subduction zone volcanism surrounds the Pacific Ocean.

In the past people thought that volcanoes were caused by water seeping into underground caverns, We now know this is not the case, but water does play an essential part in the formation of trench related volcanoes. The subducting lithosphere contains a lot of water – in a layer of waterlogged sediment and also in hydrated minerals within the seafloor basalt. As the subducting slab descends it encounters greater temperatures and greater pressures which cause the release of water into the overlying mantle wedge. This water has the effect of lowering the melting temperature of the mantle and generating water -rich viscous magmas that produce explosive eruptions. The rock type commonly formed contains more silica than basalt and is called andesite (named after the Andes).

< Andesite lava flow Brokeoff Volcano, California (USGS photo gallery)
The linear belt of volcanoes parallel to the oceanic trench is called an island arc (see the Bismark volcanic arc that has formed behind the New Britain Trench north of Australia). If the oceanic lithosphere subducts beneath an adjacent plate of continental lithosphere, then a similar belt of volcanoes will be generated on the continental crust. This belt is referred to as a volcanic arc, and examples include the Andes volcanic arc of South America.


Australia’s own ancient volcanic arc

The east coast of Australia is also thought to have been an active convergent margin and the site of a volcanic arc 350 to 450 million years ago. Remnants of the volcanoes can be found from Nowra to Eden
(ref http://www.mq.edu.au/scienceresearch/dadd.htm)



The Wadati-Benioff Zone (WBZ to his friends)

There are lots of earthquakes around convergent margins. Scientists measuring these earthquakes noted that they are generated from an area that gets progressively deeper as you move away from the trench. At most convergent margins, these earthquake foci define a dipping plane - the Wadati-Benioff zone, or WBZ. The WBZ corresponds to a fault zone between the subducting oceanic lithosphere and the overriding plate ie.the dip of the WBZ coincides with the dip of the subducting plate. The WBZ extends to a depth of about 700 km from the Earth's surface.

Mantle Plume (hot spot) volcanism

While most volcanism coincides with the location of plate boundaries there are many well know regions of volcanism that occur no where near a plate boundary –like the Hawaiian volcanoes and Australia’s only active volcano on Heard Island. These are examples of hot spot volcanism (also sometimes referred to as intraplate volcanism).

Hot spots are caused by a rising plume that is thought to originate near the core-mantle boundary. The formation of mantle plumes is not fully understood, but they appear to be part of the Earth’s mantle convection system. Volcanoes form on the plate above the hot spot. Because the plates are moving over the hot spot, new volcanoes form and the old ones, which no longer overlie the hot spot, become extinct. In this way hot spot trails are formed.

< The Hawaiian Island – Emperor Seamount chain have formed above a hot spot. The hot spot has remained stationary for the last 70 million years. However during this time the Pacific Plate has moved over it, carrying with it the old volcanoes that formed above the hot spot. You can calculate the history of plate movement by determining the age of the rocks in the hot spot chain.

In some cases hot spot volcanism can produce huge amounts of magma and form what are termed large igneous provinces (LIP). One such LIP, Kerguelen Plateau – Broken Ridge, was recently studied by the Ocean Drilling Program (Leg 183). They discovered that the earliest volcanism associated with the Kerguelen hot spot began about 130 million years ago when Africa, Antarctica, Australia, India and Madagascar were just beginning to break apart, leading to the formation of the Indian Ocean. Northward movement of the Indian plate over the hot spot plume formed a 5000-km-long hot spot track known as the Ninetyeast Ridge. Changing tectonic plate motions about 40 million years ago resulted in the Antarctic Plate moving over the hot spot. Since then the Kerguelen Archipelago, Heard and McDonald Islands, and a chain of submarine volcanoes between these islands have been constructed The Kerguelen hot spot continues to erupt today at Heard and McDonald islands.

Basalts formed at hot spots are similar to those formed at mid ocean ridges but they tend to have less silica higher concentrations of Na and K. Consequently they are often called alkali basalts.

Hydrothermal Systems


Exercises

Oceanic Volcanism Terminology

This exercise is simply designed to test you understanding of the terminology required to describe and explain Mid-Ocean Ridges, the oceanic crust and several common sea-floor features.

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Hydrothermal Hunt.

Ever wondered, "The ocean is a pretty big place - How do you find anything down there?". In this exericse we'll have a look at methodology involved in the search for mineral systems associated with hydrothermal vents by following the goings-on aboard the RV Baruna Jaya VIII, an Indonesian Research Vessel. Read the text - there's not too much, and answer the questions.

Planning the expedition, a journey of some 2 weeks, required 3 years preparation time! Outside of logistics, the best area to explore had to be decided, a tricky and complicated task. The problem to be addressed was...

Test whether modern sediment-hosted hydrothermal activity occurs in Tomini Bay, an unexplored Neogene sedimentary basin surrounded by the northern, western and southeastern arms of Sulawesi. Modern analogue for black shale hosted metals?

To make the decision process easier, geologists (or any scientist) relies on models - simplified 'stereotypical' examples derived from previously discovered, similar targets. The model for hydrothermal mineral deposits is roughly this:

  • Some sort of vent system is required to produce the metals (read all about it in this chapters notes).
  • quiescent (low energy) environments concentrate minerals (it may take millions of years for enough sulphide to accumulate to be economic).
  • Anoxic water is required (or rapid burial) if the suphides are to be preserved (Sulphides are highly reactive and 'rust' in the presence of oxygen).

Here is the geological and tectonic map of northern Suawesi, The area was deemed to be highly prospective based on:

  • Bathymetry defines an enclosed basin some 2000 m deep, separated from Gorontalo Bay to the east by a sill more than 300 m high.
  • Magmatic heat sources to drive hydrothermal circulation: Single active volcano, Colo, on Una Una island in Tomini Bay.
  • Inflow of organic debris from rivers draining the encircling heavily vegetated, high rainfall landmass of Sulawesi.
  • High sedimentation rate from erosion of 2,000 m high mountains near coast.
  • Possible anoxic, saline conditions on the sea floor.
  • Possible presence of faults to act as conduits

Now, how do we prove if it's there or not....

Lets go!


Hotspots

Hotspots occur beneath the oceanic plates and act independantly from them. Largely believed to remain stationary, the plate slowly moves over the top of them. Resulting volcanism generally occurs as linear chains, producing seamounts, islands and atolls. Active volcanism is restricted to the proximity of the hotspot, but dates of now-extinct volcanism show a distinct increase in age away from the hotspot. Two good examples of hotspot activity are 1) Lord Howe Island Chain and 2) The Hawaiian Island Chain.

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Additional Exercises

Download these exercises to further test your understanding

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Helping Hints

We realise that not everyone has had experience with the intrinsic concepts of Marine Science. This 'computer' has numerous examples which will help you understand these fundamental facets! Very helpful, very colourful!

Lets go!


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Marine Sediments
Pelagic Sed. Distribution
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Calcareous Seds
The Carbon Cycle
The CCD
Carbonate Sed. Examples
Forams
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Pteropods
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Gas Hydrates
Man and Hydrocarbon
The nature of Gas Hydrate
Finding Gas Hydrate
Formation of Gas Hydrates
Hazards
Underwater landslides and tsunamis
Archimedes and the Bermuda Triangle
Gas Hydrates and the Greenhouse
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Authigenic Deposits
Phosphorites
Glauconite
Volcanogenic Sediments
Cosmogenous Sediments


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Exercises
Hydrotherml Systems; Vents
Life at Vents
Hydrothermal Mineral Deposits
Mining the Ocean
How to Find a Vent
Why Locate Vents

Oceanic Volcanism
Journey to the Centre of the Earth
Ocean Spreading Ridge Volcanism
Trench Related Volcanism
Australias Volcanic Arc
Wadati-Benioff Zone
Mantle Plume Volcanism
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Basin Topography
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Our very own Shelf
Deformation - Californian active continental margin
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Salt and What Else

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