v1 foley-geoHW3
pdf
keyboard_arrow_up
School
Worcester Polytechnic Institute *
*We aren’t endorsed by this school
Course
2341
Subject
Geology
Date
Jan 9, 2024
Type
Pages
9
Uploaded by ChiefSquirrelPerson783
1
Geology 2341, A Term 2023
Worcester Polytechnic Institute
Homework Assignment 3, Due by Sep. 14
PART A: OBJECTIVE: TO DISCOVER SOME OF THE ASPECTS OF
PLATE TECTONICS BY EXAMINING REAL DATA.
Background:
The Hawaiian-Emperor seamount chain stretches for 6,000 km across the Pacific Ocean. This
string of more than 100 volcanoes was formed as the Pacific plate slid across a hot spot (or
mantle plume) in the asthenosphere below. Some of these volcanoes extend above sea level to
form islands while others are submerged seamounts. Over time the volcanoes erode, cool and
subside below sea level often forming flat-topped guyots.
Procedure:
Step 1: Plot the age-distance data
To better understand this process you will plot the age-distance relationship of 30 volcanoes
listed in Table 1 on the graph provided. Mark a “
+
“ at each volcano’s age-distance point. Give
the plot a descriptive title and label each axis so that someone seeing the graph for the first time
could understand what it represents. (Use Microsoft Excel to plot the data; and don’t forget units
of the axes).
Step 2: Interpret the data
1)
Draw a straight line that best fits (is closest to) all the data points. The slope of this line
represents the average rate at which the plate is moving (in km/Ma). Note that the points do not
all lie on the line. Give some reasons why all the points don’t lie exactly on the line.
2
The points may not all fall exactly on the line because the Pacific Plate has changed its rate of
movement throughtout the years. The line of best fit (trendline) shows the overall average speed
over millions of years. Its rate of speed is constantly changing.
2)
Calculate the rate (distance/time) at which the Pacific plate is sliding across the hot spot.
a. First determine the slope of the line. If you don’t know how to do this see page 4.
Plate rate = _______75.39__________ km/Ma
b. The answer above is in units of km/Ma. Geologists typically measure plate motions in units of
cm/year. Convert the value above to cm/yr. See page 4.
Plate rate = ___________7.539____________ cm/yr
In what direction is the Pacific plate moving? _____west-southest____________
3)
Try fitting the data better by putting a bend in your line thus drawing two lines with different
slopes. How long ago would
the bend (see the above figure)
have happened?____________
What caused the bend?_____________________________________________________
4)
Examine the map on the first page of the exercise. Note that there is a bend in the seamount
chain on the map.
How do you explain this? ___The bend indicates that the plate was changing direction. The hot
spot stayed in place while the volcanoes moved with the plate.____________
When did this happen? _______~43 million years ago (around when the plates direction
changed).______________
5)
How old is the oldest volcano in the chain? ___(Meiji) 85 million_____ yrs
The creation of the Hawaiian-Emperor seamount chain represents what percentage of the
earth’s whole history? ____1.88____% (Take 4.5 billion years as the earth’s history)
6)
Questions to ponder (
for bonus points
):
•
Are there other island chains similar to this one?
Yes, the Cosgrove Track.
3
•
Why does the chain stop at Meiji?
The chain stops at Meiji because, due to subduction, the other volcanoes in this chain were
destroyed.
•
How long does an island in the chain last?
Based on what we know, it seems an island in the chain lasts around 90 million years before it
will get subducted.
•
Where will the next island be?
The next island will most likely be near Kilauea, the youngest island, which would also be at the
hotspot. We can assume it is already under contruction as magma from the Earth begins to rise.
Table 1. Volcano age and distance from Hawaii hot spot
Volcano
number
Volcano name
Age
(Ma)
Distance
(Km)
Age
error
(Ma)
Distance
error (Km)
1
Kilauea
0.2
0
0.2
1.5
3
Mauna Kea
0.38
54
0.05
1.8
5
Kohala
0.43
100
0.02
2
6
East Maui
0.75
182
0.04
2.5
8
West Maui
1.32
221
0.04
2.7
10
East Molokai
1.76
256
0.07
2.9
11
West Molokai
1.9
280
0.06
3
13
Waianae
3.7
374
0.1
3.5
14
Kauai
5.1
519
0.2
4.2
15
Niihau
4.89
565
0.11
4.5
17
Nihoa
7.2
780
0.3
5.6
20
unnamed 1
9.6
913
0.8
6.3
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help
4
23
Necker
10.3
1058
0.4
7.1
26
La Perouse
12
1209
0.4
7.9
30
Gardner
12.3
1435
1
9.1
36
Laysan
19.9
1818
0.3
11.1
37
Northampton
26.6
1841
2.7
11.3
50
Pearl & Hermes
20.6
2291
0.5
13.6
52
Midway
27.7
2432
0.6
14.4
57
unnamed 2
28
2600
0.4
15.3
63
unnamed 3
27.4
2825
0.5
16.5
65
Colahan
38.6
3128
0.3
18.1
67
Daikakuji
42.4
3493
2.3
20
72
Kimmei
39.9
3668
1.2
20.9
74
Koko
48.1
3758
0.8
21.4
81
Ojin
55.2
4102
0.7
23.2
83
Jingu
55.4
4175
0.9
23.6
86
Nintoku
56.2
4452
0.6
25.1
90
Suiko 1
59.6
4794
0.6
26.9
91
Suiko 2
64.7
4860
1.1
27.2
Note: Ma = Mega annum (million years ago)
Volcano Number is the volcano’s number in the chain counting NW from the hot spot. Not all
volcanoes are on this list. The last two columns are estimates of the errors in the first two
columns.
Hints
How to draw a “best fit” line
Here is a website that illustrates how to draw graphics and a best-fit line in excel.
http://phoenix.phys.clemson.edu/tutorials/excel/graph.html
.
How to calculate slope
By definition, slope is the ratio of the vertical change in a line to the horizontal change.
In the figure below the sloping line is defined by two points (a,b) and (x,y). The vertical change
is equal to
y - b
and the horizontal change is equal to
x - a
. The slope,
m,
is therefore equal to:
m=(y-b)/(x-a)
5
How to convert from km/Ma to cm/yr
The rate you calculated from the raw data will be in the units of kilometers (km) per million
years (Ma). However, geologists routinely report the rate of plate motions in centimeters (cm)
per year. So you must convert the rate to cm/yr with the following conversion:
Km/Ma * 1000 m/Km * 100 cm/m * 1Ma/10
6
years = cm/year
PART B: THE BEHAVIOR OF MELTS
Basalts (and Gabbros) are igneous rocks rich in Ca-Plagioclase, Olivine and
Pyroxene. Andesites (and Diorites) are igneous rocks with Na-Plagioclase and
Pyroxene. Rhyolites (and Granites) are igneous rocks with Quartz and Alkali Feldspar
(rich in potassium and sodium).
In general, the viscosity of a melt (a measure of its resistance to flow) is inversely
proportional to its temperature. At high temperatures the melt tends to flow more
readily than at low temperatures. Water can drastically modify the viscosity of a melt;
the higher the water content, the lower the viscosity.
Questions
1.
Relate the type (quiet versus explosive) of eruption to the viscosity of a melt.
2.
In your own words, compare and contrast the viscosities of rhyolites, andesites
and basalts. Which, other things being equal, tend to have the highest viscosity?
Rhyolites have the highest viscosity (650-800 degrees Celcius), Andesites have the
middle/intermediate viscosity (800-1000 degrees Celcius), and Basalts have the
lowest (1000-1200 degrees Celcius). Rhyolites contain the highest silica content,
which explains the higher viscosity.
3.
At what types of plate tectonic settings do you tend to find these three lava
types?
Ocean-ocean faults result in Basaltic, low viscosity settings due to the ocean. These
are divergent plates. Ocean-lithosphere faults result in Andesite. It is intermediate
viscosity due to the partial ocean involvement. Subduction is involved here and they
are convergent plates. Continent-continent faults result in Rhyolite. As mentioned
above, Rhyolite is the most viscious. Contient-continent faults are land-on-land and
can provide high silica levels to produce these high-viscocity settings.
6
PART C Igneous Rock Identification
Composition
Composition
of igneous rocks is properly identified by determination of the rock's chemical
composition. Color is often an indicator of the composition of a rock or mineral and can be
effectively used to identify the composition of most igneous rocks. Light colors, including white,
light gray, tan and pink, indicate a
felsic composition
.
Felsic
compositions are rich in silica
(SiO2). Dark colors, such as black and dark brown, indicate a
mafic or ultramafic composition
.
Mafic
compositions are poor in silica, but rich in iron (Fe) and magnesium (Mg).
Intermediate
compositions have an intermediate color, often gray or consisting of equal parts of dark and light
mineral. Beware that even though an igneous rock may have a
felsic
composition (light color),
the rock can contain dark colored minerals.
Mafic
rocks may contain light colored minerals as
well. As mentioned above, the composition of most igneous rocks can be identified using this
system, formally known as the
Color Index
. However, there are exceptions. The two most
notable are
obsidian
and
dunite
.
Obsidian
is volcanic glass which erupts as a lava flow. Most
obsidian
is
felsic
in composition, yet typically it will have a very dark color (dark brown to
black).
Dunite
has an
ultramafic
composition yet is apple green to yellowish green in color.
Dunite
is composed almost entirely of the mineral olivine which usually contains both iron and
magnesium.
The
texture
of an igneous rock
does not refer to the roughness or smoothness of the surface.
Textures are based primarily on crystal size.
Pegmatitic
texture
is composed of very large
crystals (larger than 2-3 cm).
Phaneritic
texture
is composed of crystals which are large
enough to see but smaller than
pegmatitic
texture, and the entire rock is composed of crystals.
Aphanitic
texture
is a fine grained texture but the crystals are too small to see.
Porphyritic
texture
is composed of crystals of two different sizes. Typically the large crystals
(phenocrysts) are visible while the smaller crystal are not (referred to as groundmass).
Glassy
texture
is the most readily recognized. The rock is composed entirely of glass. Few, if any,
crystals will be visible.
Vesicular
texture
is formed when lava solidifies before gases are able
to escape. The result is a "bubbly" appearance. Lastly,
pyroclastic
texture
is composed of
volcanic fragments. These fragments or clasts can be very fine (ash) or coarse (lapilli) or very
coarse (bombs and blocks).
Please identify the Texture, Composition and Rock Name of the following igneous rock
samples:
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help
7
Texture: Mafic;
Composition: Aphanitic;
Rock name: Basalt.
Texture: Glassy;
Composition: Felsic;
Rock name: Obsidian.
8
Texture: Phaneritic;
Composition: Felsic;
Rock name: Granite.
Texture: Phaneritic;
Composition: Intermediate;
Rock name: Diorite.
9
PART D: Google Earth virtual tours and characterization of volcanoic mountains
D1. Using the search panel in Google Earth, nagivate to Mt. St. Helens and add it to your “My
Places”.
Using the line/path function, create an east-west trending path across Mt. St. Helens (start and
stop your path on each side of the mountain at the boundary between the vegetated and non-
vegetated area). Make sure your path pass through the crater.Then, righ-click on the path you
created and select “Show Elevation Profile” from the menu.
D1-1. Before the 1980 eruption, the summit of Mt. St. Helens was at an elevation of 2,950
meters (9,677 feet), using the elevation profile, estimate the elevation of the current summit.
D1-2. Using the elevation profile, approximate the radius of the Mt. St. Helens (The radius of the
volcano is a measure of how wide a volcano is. It is the distance from the middle of the volcano,
marked by the summit, to the lower flanks of the volcano, or where the volcano’s slope flattens
out).
D1-3. Using the elevation profile, approximate the average slope of the eastern and the western
flanks of the crater as an angle.
D1-4. Using the polygon tool to draw a polygon that is approximate the same dimesnions as the
Mt. St. Helens crater. Using the measurements tabl on the Polygon pop-up box, determine the the
perimeter and area of the carter, respectively.
D2. Repeat parts D1-2 and D1-3
for Volcano Etna.
Texture: Aphanitic;
Composition: Felsic;
Rock name: Rhyolite.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help