Origin of Igneous Rocks
Summary
TLDRThis script delves into the formation of rocks, focusing on igneous rocks and their crystallization from magma. It explains two primary melting mechanisms: decompression and flux melting, which are key to volcanic activity. The crystallization sequence, as outlined by Bowen's Reaction Series, reveals how the chemistry of magma influences the mineral composition of igneous rocks. The process of differentiation is highlighted, showing how magma evolves as it cools, with examples of how it affects volcanic eruptions in different geological settings.
Takeaways
- š Minerals and rocks are formed in response to environmental factors such as pressure, temperature, and the chemical composition of the starting material.
- š„ Igneous rocks are the first type of rocks to appear on Earth and are formed from the crystallization of melted rock, known as magma when underground and lava when erupted.
- š Magma originates from the mantle, which can melt and move towards the surface under certain conditions, such as decompression melting and flux melting.
- š Decompression melting occurs when mantle rock ascends and experiences lower pressure, leading to melting, which is responsible for volcanism at mid-ocean ridges and hotspots.
- š§ Flux melting is induced by the addition of water to mantle rock, lowering its melting point and causing melting, which is common at subduction zones.
- š Bowen's Reaction Series explains the crystallization sequence in a cooling magma, starting with olivine and ending with quartz, muscovite, and alkali feldspar.
- š¬ The crystallization process in magma leads to a change in the composition of the remaining melt, enriching it in silica, calcium, alkalis, and aluminum as it cools.
- š Differentiation describes how magma changes as it cools, with the amount of differentiation related to the thickness of the crust it moves through.
- š The location of volcanic eruptions and the type of magma they produce are influenced by the thickness of the crust, with thicker continental crust leading to more differentiated, felsic magmas.
- šļø The comparison between Hawaii and Yellowstone illustrates the impact of crust thickness on volcanic activity, with Hawaii's thinner oceanic crust producing less viscous, mafic lava.
- š The crystallization of minerals from magma is influenced by the relative melting points and chemical compositions of the minerals, with magnesium-rich endmembers crystallizing before iron-rich ones.
Q & A
What are the three types of rocks mentioned in the script?
-The three types of rocks mentioned are igneous, sedimentary, and metamorphic, which differ in their mechanism of formation.
What is the difference between magma and lava according to the script?
-Magma is molten rock when it is underground, while lava is the term used for molten rock when it reaches the surface of the Earth.
Why doesn't lava erupt everywhere on Earth?
-Lava doesn't erupt everywhere because under normal conditions, the mantle is solid and cannot melt; volcanoes are an exception due to specific melting processes.
What are the two processes that can cause the mantle to melt in large quantities?
-The two processes are decompression melting and flux melting.
How does decompression melting occur?
-Decompression melting occurs when mantle rock moves upward due to convection and experiences lower pressure, which leads to melting, especially above mid-ocean ridges and hotspots.
What is the equation used to calculate pressure in the context of the script?
-The equation used to calculate pressure is P = Ļgz, where Ļ is density, g is acceleration due to gravity, and z is the depth below Earth's surface.
What is Bowen's Reaction Series and why is it significant?
-Bowen's Reaction Series is a model that describes the crystallization order of minerals in a cooling magma. It's significant because it explains the sequence in which minerals crystallize and how the composition of the remaining melt changes.
How does the crystallization of olivine affect the composition of the remaining magma?
-As olivine crystallizes, it depletes the magma of MgO and enriches it in silica, calcium, alkalis, and aluminum because olivine has a smaller fraction of silica compared to the original melt.
What is the role of solid solution in the crystallization process?
-Solid solution complicates the crystallization process by causing minerals to crystallize in a sequence where magnesium-rich endmembers form before iron-rich ones, and calcium-rich before sodium-rich ones.
Why do some volcanoes erupt with more differentiated magmas?
-Volcanoes erupt with more differentiated magmas if the magma has moved through a thicker crust, which allows for more extensive cooling and crystallization, as seen in the comparison between Hawaii and Yellowstone.
What is the difference between the magma erupted at the Hawaii hotspot and Yellowstone hotspot?
-The Hawaii hotspot erupts basaltic, mafic lava at higher temperatures, while Yellowstone erupts cooler, more viscous, felsic magma due to its location beneath thick continental crust.
Outlines
š Formation of Igneous Rocks and Mantle Melting
This paragraph introduces the concept of rocks and their formation from minerals influenced by environmental factors such as pressure, temperature, and chemistry. It delves into the specifics of igneous rocks, which are the first to appear on Earth and are formed from the crystallization of magma. The text explains the distinction between magma and lava and explores the processes of decompression melting and flux melting that cause the mantle to melt, leading to volcanic activity. Decompression melting is described as occurring above mid-ocean ridges and hotspots due to the upward movement of less dense, hot mantle material, which encounters lower pressure and melts. Flux melting, on the other hand, is induced by the addition of water to the mantle rock, particularly at subduction zones, where water released from the subducting lithosphere lowers the melting point of the mantle.
š¬ Bowen's Reaction Series and Igneous Rock Differentiation
The second paragraph discusses the diversity of igneous rocks despite their common origin from the chemically homogeneous mantle. It introduces Bowen's Reaction Series, developed by geologist N. L. Bowen in 1928, which outlines the sequence of mineral crystallization in a cooling magma. The sequence begins with olivine and ends with quartz and muscovite, with plagioclase present throughout. The crystallization process leads to the enrichment of silica and other elements in the remaining melt as denser minerals like olivine sink. This results in a differentiation of the magma, with the last minerals to crystallize being rich in silica and alkalis. The differentiation process is influenced by the thickness of the crust the magma must pass through, with more differentiated magmas found in areas of thick crust, such as continents. The paragraph contrasts the eruptions of Hawaii, which produces less differentiated, mafic lava, with Yellowstone, where more differentiated, felsic magma leads to explosive eruptions due to its high viscosity.
Mindmap
Keywords
š”Minerals
š”Rocks
š”Igneous Rocks
š”Magma
š”Decompression Melting
š”Flux Melting
š”Bowen's Reaction Series
š”Differentiation
š”Mafic Lava
š”Felsic Magma
Highlights
Minerals and rocks are formed in response to environmental factors such as pressure, temperature, and starting material chemistry.
Crystallization of magma and its chemistry are key in determining a rock's mineralogy.
There are three main types of rocks: igneous, sedimentary, and metamorphic, each with a distinct formation mechanism.
Igneous rocks were the first to appear on Earth, formed from the crystallization of melted rock.
Magma and lava are terms used for molten rock underground and on the surface, respectively.
Most igneous rocks originate from the mantle, which melts and moves toward the surface under certain conditions.
Decompression melting and flux melting are two processes that cause the mantle to melt in large quantities.
Decompression melting occurs as mantle rock ascends and experiences lower pressure, leading to melting.
Flux melting is induced by the addition of water to mantle rock, lowering its melting point and causing melting at subduction zones.
The crystallization sequence in cooling magma is influenced by the magma's chemistry and mineral melting points.
Bowen's Reaction Series outlines the crystallization order of minerals from a standard magma as it cools.
Differentiation describes the changes in magma composition as it cools, leading to the formation of various minerals.
The amount of differentiation is related to the thickness of the crust the magma moves through to reach the surface.
Cool, felsic magma from Yellowstone and mafic lava from Hawaii demonstrate the impact of crust thickness on volcanic eruptions.
Solid solution and the crystallization of magnesium-rich endmembers before iron-rich ones contribute to the complexity of rock formation.
The crystallization process and the resulting rock types are essential for understanding Earth's geological history and dynamics.
Transcripts
Now that we have a better understanding ofĀ minerals, we are ready to discuss rocks.Ā Ā
Minerals and rocks form in response toĀ environmental forcing, with importantĀ Ā
variables being pressure, temperature,Ā and chemistry of the starting material.Ā Ā
Here, we will discuss the crystallization of magmaĀ and the importance of its chemistry in determiningĀ Ā
a rockās mineralogy. There are three types ofĀ rocks: igneous, sedimentary, and metamorphic,Ā Ā
and these differ in their mechanism of formation.Ā We will begin our discussion with igneous rocks,Ā Ā
which were the first type of rocks to appear onĀ Earth after its formation and subsequent cooling.Ā
Igneous rocks are formed when a mass of meltedĀ rock crystallizes. There are two terms geologistsĀ Ā
use for molten rock. When it is underground, itĀ is called magma, up here it is called lava. So,Ā Ā
where does this magma come from? Most igneousĀ rocks were once mantle rock that, at some point,Ā Ā
melted and moved toward the surface, where itĀ cooled and solidified. You may now be wonderingĀ Ā
why lava isnāt erupting everywhere on Earth. ItĀ turns out that under normal conditions, the mantleĀ Ā
is perfectly happy as a solid and cannot melt;Ā and volcanoes are an exception to the rule. So,Ā Ā
what sort of process is going on here that allowsĀ the mantle to melt? In fact, there are two waysĀ Ā
to melt the mantle in large quantities:Ā decompression melting and flux melting.Ā Ā
Letās start with decompression melting. This isĀ exactly what it sounds like, melting the mantleĀ Ā
by lowering its pressure. Decompression melting isĀ responsible for the volcanism above both mid-oceanĀ Ā
ridges and hotspots. Beneath these environments,Ā hot mantle rock is moving upward due to mantleĀ Ā
convection. Since hot material is less denseĀ than cold material, the weight of a column of hotĀ Ā
material will be less than that of cold material.Ā Therefore, at a given depth, the pressure is lowerĀ Ā
beneath a mid-ocean ridge or hotspot thanĀ it is beneath a regular piece of crust.Ā
Letās follow an ascending piece of mantle rock asĀ it rises beneath a mid-ocean ridge. At a depth ofĀ Ā
about 30 kilometers, our piece of mantle hasĀ a temperature of 1400Ā°C. Its pressure can beĀ Ā
calculated using the following equation: P = Ļgz,Ā where Ļ is its density, g is acceleration due toĀ Ā
gravity, and z is the depth below Earth's surface.Ā Since Ļ and g are more or less constant for thisĀ Ā
example, the main variable affecting the pressureĀ is the depth, which should be fairly intuitive:Ā Ā
the more mass above a given area, the higherĀ the pressure will be. The two black arrowsĀ Ā
are representative of the downward pressure.Ā The upper right section shows a phase diagramĀ Ā
corresponding to the state of our piece of mantleĀ in pressure-depth space. The green dashed curve isĀ Ā
the average geotherm, which shows how temperatureĀ changes with depth. The red solid line is theĀ Ā
melting point of mantle rock. Notice how the twoĀ curves are nearly parallel, this illustrates theĀ Ā
requirement for abnormal conditions to get theĀ mantle to melt. As our mantle rock ascends,Ā Ā
it experiences lower pressure, since there isĀ now less mass above it. But notice that theĀ Ā
temperature did not change, it is still 1400Ā°C.Ā This is an example of an adiabatic process,Ā Ā
meaning heat has not been added or removed fromĀ the system. Essentially, the rising motion ofĀ Ā
the mantle occurs at sufficient speed that we canĀ assume that heat is not lost to its surroundingsĀ Ā
during ascent. Therefore, the key to decompressionĀ melting is the advection of hot material upward,Ā Ā
to a lower-pressure environment. Finally, at aĀ pressure of 2 kilobars, the mantle is melting,Ā Ā
with the purple dashed line signaling the onset ofĀ melting. So long as there is upward-moving mantle,Ā Ā
our magma factory will persist - this isĀ decompression melting. The vast majority ofĀ Ā
volcanism on Earth, both past and present,Ā is due to decompression partial melting.Ā
Flux melting involves the addition of waterĀ to mantle rock, which lowers its meltingĀ Ā
point. This is responsible for the volcanism atĀ subduction zones. Here, the subducting oceanicĀ Ā
lithosphere releases water into the mantleĀ above it, which induces melting. It is notĀ Ā
actual liquid water that is transported to theĀ mantle, but hydroxide anions that are releasedĀ Ā
from the high-pressure breakdown of hydrousĀ minerals, like serpentine, or Mg3Si2O5(OH)4.Ā Ā
This chemically bound water is releasedĀ around the same depth everywhere on Earth,Ā Ā
about 100 kilometers, which explains why volcanoesĀ occur in a line, or arc at subduction zones.Ā
Since most igneous rocks are derived fromĀ the mantle, which is relatively chemicallyĀ Ā
homogeneous, we might expect igneous rocks to alsoĀ be this way, but they arenāt. To understand this,Ā Ā
we must first discuss the crystallization process,Ā and more importantly, crystallization sequence. InĀ Ā
a cooling magma, crystallization order isĀ dependent upon the chemistry of the magmaĀ Ā
and the relative melting points of the stableĀ minerals. Since most magmas are derived fromĀ Ā
melting the same stuff, the mantle, we can ignoreĀ the influence of chemistry for these purposes.Ā Ā
In 1928, pioneering geologist N. L.Ā Bowen created an experimental modelĀ Ā
for the crystallization order of a standardĀ magma as it cools and chemically evolves. InĀ Ā
Bowenās Reaction Series, the first mineral toĀ crystallize is olivine, followed by pyroxene,Ā Ā
then amphibole, then biotite, and finallyĀ potassium feldspar, muscovite, and quartz.Ā Ā
Plagioclase can exist at all stages of BowenāsĀ Reaction Series, as it is the most abundantĀ Ā
mineral in the crust. We may recall that the firstĀ mineral to crystallize, olivine, an orthosilicate,Ā Ā
has the smallest amount of silica of all theĀ silicate minerals, while the last group containsĀ Ā
potassium feldspar and quartz, which are frameworkĀ silicates, the minerals with the most silica. ThisĀ Ā
has important implications for the composition ofĀ a cooling melt. Letās consider an average basalt,Ā Ā
having 50% SiO2, 15% Al2O3, 20% MgO, 10% CaO, andĀ 5% alkalis. Now, letās start to crystallize outĀ Ā
forsterite, the magnesium endmember of olivine,Ā which is composed of 57% MgO and 43% SiO2. WhatĀ Ā
is going to happen? Well, the olivine crystals,Ā which are more dense, will sink to the bottomĀ Ā
of the magma chamber, becoming isolated fromĀ the upward-moving magma. Since olivine has aĀ Ā
smaller fraction of silica in comparison to theĀ melt, the melt will become enriched in silicaĀ Ā
as olivine crystallizes. In fact, the meltĀ will become enriched in everything but MgO,Ā Ā
which gets depleted making olivine, since olivineĀ has a higher fraction of MgO than the melt. TheĀ Ā
result is a melt that becomes enriched in silica,Ā calcium, alkalis, and aluminum as it cools andĀ Ā
moves upward. This process is then repeated forĀ pyroxene, amphibole, and biotite, which depletesĀ Ā
the melt in everything but silica, aluminum, andĀ the alkalis, which become concentrated in theĀ Ā
cooling melt. This results in the last minerals toĀ form being those with silicon, aluminum, sodium,Ā Ā
and potassium in their chemistry, such asĀ quartz, muscovite, and alkali feldspar.Ā
Solid solution further complicates things. For aĀ general rule of thumb, magnesium-rich endmembersĀ Ā
crystallize before iron-rich endmembers,Ā and calcium-rich endmembers form beforeĀ Ā
sodium-rich endmembers. This explains theĀ right side of Bowenās Reaction Series;Ā Ā
since anorthite has a higher melting point thanĀ albite, the first plagioclase that crystallizesĀ Ā
will be calcium-rich and the last will be moreĀ sodium-rich. The same thing happens with olivine,Ā Ā
pyroxene, and amphibole; the first mineralsĀ to form will be magnesium-rich, with crystalsĀ Ā
becoming progressively iron-enriched duringĀ cooling. These processes are together referredĀ Ā
to as differentiation, which describes how aĀ magma changes, or becomes different, as it cools.Ā
The amount of differentiation a magmaĀ undergoes is generally related to theĀ Ā
amount of crust that it had to move through toĀ make it near the surface. Therefore, the coolestĀ Ā
and most differentiated magmas commonly eruptĀ in areas where the crust is relatively thick,Ā Ā
such as on continents. This is easy to see whenĀ comparing Hawaii and Yellowstone, as they are bothĀ Ā
hotspots. The volcanoes of Hawaii erupt basaltic,Ā or mafic lava at around 1300 degrees Celsius,Ā Ā
whereas Yellowstone erupts cool, felsic magmaĀ that is so thick and viscous, that it clogs up theĀ Ā
volcano, causing extremely explosive eruptions.Ā What is the difference? The Yellowstone hotspotĀ Ā
is beneath thick continental crust, while theĀ Hawaii hotspot is beneath thin, oceanic crust. WeĀ Ā
have more to discuss regarding igneous rocks, soĀ letās move forward and learn more about them now.
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