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Transcript
24
Ages of Oceanic and Continental Crust
Figure 11 shows the locations and activities of both constructive and destructive place boundaries in
the Pacific Ocean.
Figure 11 — Ages of Ocean Floor Basalts
Since new oceanic crust is made at divergent boundaries (mid-ocean ridges), the ocean floor basalts
on the ridges must be very young. As new crust is continually being made at these ridges, the age of
the ocean floor basalts must increase with distance from the ridges. Their ages must also increase
symmetrically on either side of the ridges. Basalt that is (say) 100km from the eastern side of a
ridge must be the same ages as basalt that is 100km from the western side.
Oceanic crust is continually being destroyed at destructive plate boundaries (subduction zones) so
no that ocean floor basalts are very old. The oldest ocean floor basalts are only about 200 million
years old, whereas the oldest known continental crust rocks are about 3, 800 million years old.
1
On figure 11, mark and label the positions of the youngest and oldest ocean floor basalts.
Due to plate movement, oceanic crust is generally much younger than continental crust.
Earthquakes and Volcanoes
Figure 12 shows that Earthquakes and volcanic activity are generally concentrated along the Earth’s
plate boundaries.
2.
On figure 12, mark and label the locations of:
a.
One mid-ocean ridge. This is an example of a ________________ plate boundary.
b.
One subduction zone, which is an example of a ______________ plate boundary
c.
One volcano that is away from a plate boundary.
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
25
Figure 12 — Worldwide Distribution of Earthquakes, Volcanoes and Plate Boundaries
Source: Adapted from http://www.maine.gov/dacf/mgs/hazards/tsunamis/index.shtml
Volcanoes away from plate boundaries, such as the Hawaiian Islands, occur above hot spots in the
mantle.
Earthquakes away from plate boundaries are weaker than those that are actually on the boundaries.
They tend to occur because all the Earth’s plates are continually moving and exerting forces on
each other.
Movement of the Plates
Heat energy and convection currents are largely responsible for the movement of tectonic plates
The convection currents in the mantle material carry the sea floor in a conveyor belt fashion to the
deep-ocean trenches, where the sea floor descends into the mantle. Thus, the addition of new
oceanic crust forces plates away from each other, thereby separating and moving the continents.
The primary heat source driving the convection currents is thought to be from heat being generated
by decaying radioactive elements within Earth and/or heat left over from the formation of the
planet.
Figure 13 shows how convection currents in the asthenosphere move the rocky continents around.
Up‐ welling moves the continents apart and spreads the ocean floor, whilst subduction causes
continents to crumple and form mountains. Stress release from these movements results in
earthquakes, volcanoes, landslides and tsunamis.
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
26
Figure 13 — Convection Currents Moving the Earth's Plates
Source: Adapted from http://dn.redwoods.edu/coursenotes/renner/geo_images/plate_tectonics/mantle_convection.jpg
3.
4.
On figure 13, mark and label the following features:
a.
Asthenosphere, lower mantle, outer core, inner core.
b.
A convergent boundary and a divergent boundary.
Draw arrows on the convection currents to indicate the direction in which the magma is
flowing.
Plate Tectonics and Australia Though Time
1
Look carefully at Figure 1 and Figure 12, both of which show the locations of today’s plate
boundaries.
a.
How many plate boundaries lie within the Australian continent? ___________________
b.
How many plate boundaries are parallel and close to any part of the Australian
coastline?
_________________________________________________________________________
2
Suggest two features of the Australian continent that result from its location with respect to
today’s plate boundaries.
i.
______________________________________________________________________
ii.
______________________________________________________________________
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
27
The small earthquakes (less than 7 on the Richter Scale) that occur in Australia are due to friction
caused by movement of the continent as it is carried along on the Indo-Australian Plate. The
comparatively recent (starting 33 million years ago) volcanic activity that occurred in Australia was
associated hotspots in the Earth’s mantle.
Australia has not always been an island continent with its present boundaries. The oldest rocks in
Australia are found in Western Australia, and they were probably part of another continental
landmass when they were originally formed. Australia became an island continent about 34 million
years ago when it finally broke from Antarctica.
We have seen that the continents have not always occupied their present positions on the Earth’s
surface. Plate boundaries have also moved, increasing the complexity of continental wandering.
Throughout the history of the Earth landmasses have been continually in motion. At different times
they have all collected together to form supercontinents, which have eventually separated into
smaller landmasses. Rodinia was a supercontinent containing most or all of the Earth's landmass,
which existed between 1.1 billion and 750 million years ago. The most recent supercontinent,
Pangaea, formed approximately 300 million years ago and began to break apart about 200 million
years ago. Figure 14 shows how today’s continental landmasses were combined to form Pangaea.
The supercontinent split first into two continents: a northern continent of Laurasia and a southern
continent of Gondwana. These two large continents eventually divided to form the landmasses and
oceans we know today.
3
Label figure 14 to show the locations of the following continents:
Europe and Asia (parts of the same landmass), Africa and Arabia (also parts of the same
landmass), North America, South America, Indic, Australia, Antarctica.
Figure 14 — The Most Recent Supercontinent — Pangaea
Source: http://volcano.oregonstate.edu/vwdocs/vwlessons/lessons/Pangea/Pangea4.html
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
28
The landmass that now forms continental Australia grew from west to east. Rocks more than 2,500
million years old mostly occur in the west, rocks between 2, 500 and 540 million years old occur in
the centre in and the youngest rocks are found in the east.
Compared with other periods of time, Australia was relatively quiescent between 1300 Ma and 700
Ma, possibly because the landmass was largely in a long way from any plate boundaries during this
time.
The Mount Lofty and Flinders Ranges in South Australia and the Great Dividing Range in New
South Wales and Queensland are the remains of fold mountain ranges that were formed, possibly by
subduction of an oceanic plate under a continental plate hundreds of millions of years ago.
The Mount Lofty and Flinders Ranges together form a structure known as the Adelaide
Geosyncline, which stretches from the northern parts of the Flinders Ranges to Kangaroo Island.
Sediments were deposited in a depression that is believed to have formed as the crust was stretched
during the breakup of the supercontinent of Rodinia. It was in the form of an arc about 1000 km
long and several hundred km wide. At their deepest the sediments that eventually formed
limestones, shales and sandstones, as well as some volcanics, reached up to 24,000m thick. The
nature of the rocks suggests that most of the sediments were deposited marine environment. At the
time of their deposition, from about 870 million years ago to about 500 million years ago the area
was the ocean next to the existing east coast of the continent. Similar rocks are found on the west
cost of North America, leading to the suggestion that before the break-up of Rodinia, North
America was connected to eastern Gondwana.
About 500 million years ago, the sediments deposited in the Adelaide Geosyncline were folded and
uplifted to become a high mountain range. The Flinders Ranges and the Mt Lofty Ranges are highly
eroded remains of this mountain range. There were also a number of igneous intrusions, such as the
granites of Victor Harbor, and in the eastern Mt Lofty Ranges. The earliest subduction phase was to
the east, and the folding and uplifting may have been the result of collision with an island arc
complex on the Pacific Plate with the margin of Australia.
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
29
The Tasman Geosyncline was a linear trough in the Earth’s crust that formed a broad belt to the east
of the Flinders and Mt. Lofty Ranges and extending from Tasmania in the south to Cape York in the
north. Sediments that produced rocks formed about 400 million years ago were deposited in this
trough. Several folding and uplifting events occurred during the existence of the Tasman
Geosyncline, and these episodes folded and crumpled the rock strata to form what has eventually
become the Great Dividing Range.
Figure 25 — Major Tectonic Features of the Australian Continent
4
5
6
On Figure 15, Indicate and label the positions of the following tectonic features of the
Australian continent:
a.
Approximate locations of rocks more than 2,500 million years old.
b.
Rocks about 540 million years old.
c.
Rocks between 400 and 251 million years old.
Indicate the locations of two geosynclines and the eroded remnants of former mountain ranges
a.
Adelaide Geosyncline and Mt. Lofty/Flinders Ranges.
b.
Tasman Geosyncline and Great Dividing Range.
Draw possible positions of former plate bondaries.
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
30
Rocks younger than 251 million years are essentially flat, lying above the folded layers produced in
the Tasman Geosyncline, thus providing evidence for the stability of eastern Australia in the past
251 million years.
As a general rule, we can say that folded and faulted rocks, mountain ranges and some volcanic
activity indicate the locations of former plate boundaries, while flat lying rocks were formed a long
way from any plate boundaries.
Year 9 Plate Tectonics Unit
Student Booklet — April, 17
31
References:
http://www.cotf.edu/ete/modules/msese/earthsysflr/plates1.html
Moving Continen ts Puzzle — see p7
Year 9 Plate Tectonics Unit
Student Booklet — April, 17