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Continental crust
• Rocks as old as 4000my have been traced in
some localities in the continents whereas the
oceanic crust is no older then 200my .
• The crust predating the limit has been
subducted in the oceanic trenches as a
consequence of sea floor spreading.
• The heterogeneous character of the
continental crust is evident if the rocks formed
in the archean, proterozoic and phanerozoic
are compared.
2
• Archean rocks are traced in continental Nuclei
and shields and are of high grade tonalitic
gnesiss of metamorphic origin, surrounded by
greenstone belts, which are low grade volcano
sedimentary sequences.
• The Archean geological setup is characterized
by sodium rich granite, granodiorite and
tonalite complexes
3
• Development of extensive shield areas took place
in the early Paleozoic
• Extensive limestone sandstone ironstone
characterize the proterozoic sequences.
• Global dynamic processes since the beginning of
the phanerozoic have been attributed to late
movements
• Phanerozoic sutures and arcs like the Urals in
siberia and variscan mountains in Europe came
into being.
• Continental flood basalts covered large tracts of
the land as in western India, Karoo in south Africa
and Parana in south America.
4
Characterizing the composition of Earth’s lower crust and
understanding the physical and chemical processes that
produced its characteristics are relevant to geodynamics,
geochemistry, and seismology.
For example, in geodynamics, we seek to understand where,
why, and at what timescales and lengthscales body forces evolve.
In geochemistry, we investigate how physical and chemical
processes have shaped the differentiation of Earth’s crust—for
example, how radiogenic is lower crust? In seismology, we
evaluate the constraints that wavespeeds provide about the
composition of Earth’s lower crust.
This manuscript builds on earlier reviews concerning continental
crust (e.g., McLennan et al. 2005; Rudnick&Gao 2003, 2014),
focusing on three questions specific to continental lower crust:
THICKNESS, LAYERING, AND COMPOSITION
OF CONTINENTAL CRUST
Earth’s continental crust is widely believed to be andesitic
to dacitic, with 57 to 66 wt% SiO2 (e.g.,Rudnick & Gao
2003, 2014), distinct from mafic oceanic crust, with 48 to
52 wt% SiO2, and from upper mantle residual peridotites,
with <46 wt% SiO2.
Compared with oceanic crust and upper mantle,
continental crust has slower seismic wavespeeds and is
less dense (Holbrook et al. 1992, Rudnick & Fountain
1995).
There are also differences in the thickness of
continental crust— and the nature of theMohoroviˇci´c
(Moho) discontinuity—in different tectonic settings.
Whether these downward changes in physical and
chemical properties occur gradually or in distinct layers
of regional significance is not well known.
Crustal Thickness
The release of considerable new seismic-refraction data from Russia and
China in the early 1990s prompted reexamination of the thicknesses and
wavespeeds of continental crust (e.g., Mooney et al. 1998).
Crustal thickness varies considerably with tectonic setting, but the average
crust
was determined to be ∼40 km thick (Figure 1a) (Christensen & Mooney 1995,
Rudnick & Fountain 1995).
Recently, Huang et al. (2013) calculated a thinner average crustal thickness
from the 2◦ × 2◦ CRUST2.0 wavespeed–thickness model (Bassin et al.
2000)—principally because CRUST2.0 includes substantially more submerged
continental crust.
They then merged that with global gravity data (suggesting 32.7 km) and
surface-wave dispersion data (34.8 km) to yield an average crustal thickness
of 34.4 ± 4.1 km (Figure 1b).
Composition and Formation of Earth's Continental Crust
Composition and Formation of Earth's Continental Crust
Composition and Formation of Earth's Continental Crust
Composition and Formation of Earth's Continental Crust
Composition and Formation of Earth's Continental Crust
Composition and Formation of Earth's Continental Crust

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Composition and Formation of Earth's Continental Crust

  • 2. • Rocks as old as 4000my have been traced in some localities in the continents whereas the oceanic crust is no older then 200my . • The crust predating the limit has been subducted in the oceanic trenches as a consequence of sea floor spreading. • The heterogeneous character of the continental crust is evident if the rocks formed in the archean, proterozoic and phanerozoic are compared. 2
  • 3. • Archean rocks are traced in continental Nuclei and shields and are of high grade tonalitic gnesiss of metamorphic origin, surrounded by greenstone belts, which are low grade volcano sedimentary sequences. • The Archean geological setup is characterized by sodium rich granite, granodiorite and tonalite complexes 3
  • 4. • Development of extensive shield areas took place in the early Paleozoic • Extensive limestone sandstone ironstone characterize the proterozoic sequences. • Global dynamic processes since the beginning of the phanerozoic have been attributed to late movements • Phanerozoic sutures and arcs like the Urals in siberia and variscan mountains in Europe came into being. • Continental flood basalts covered large tracts of the land as in western India, Karoo in south Africa and Parana in south America. 4
  • 5. Characterizing the composition of Earth’s lower crust and understanding the physical and chemical processes that produced its characteristics are relevant to geodynamics, geochemistry, and seismology. For example, in geodynamics, we seek to understand where, why, and at what timescales and lengthscales body forces evolve. In geochemistry, we investigate how physical and chemical processes have shaped the differentiation of Earth’s crust—for example, how radiogenic is lower crust? In seismology, we evaluate the constraints that wavespeeds provide about the composition of Earth’s lower crust. This manuscript builds on earlier reviews concerning continental crust (e.g., McLennan et al. 2005; Rudnick&Gao 2003, 2014), focusing on three questions specific to continental lower crust:
  • 6. THICKNESS, LAYERING, AND COMPOSITION OF CONTINENTAL CRUST Earth’s continental crust is widely believed to be andesitic to dacitic, with 57 to 66 wt% SiO2 (e.g.,Rudnick & Gao 2003, 2014), distinct from mafic oceanic crust, with 48 to 52 wt% SiO2, and from upper mantle residual peridotites, with <46 wt% SiO2. Compared with oceanic crust and upper mantle, continental crust has slower seismic wavespeeds and is less dense (Holbrook et al. 1992, Rudnick & Fountain 1995).
  • 7. There are also differences in the thickness of continental crust— and the nature of theMohoroviˇci´c (Moho) discontinuity—in different tectonic settings. Whether these downward changes in physical and chemical properties occur gradually or in distinct layers of regional significance is not well known.
  • 8. Crustal Thickness The release of considerable new seismic-refraction data from Russia and China in the early 1990s prompted reexamination of the thicknesses and wavespeeds of continental crust (e.g., Mooney et al. 1998). Crustal thickness varies considerably with tectonic setting, but the average crust was determined to be ∼40 km thick (Figure 1a) (Christensen & Mooney 1995, Rudnick & Fountain 1995). Recently, Huang et al. (2013) calculated a thinner average crustal thickness from the 2◦ × 2◦ CRUST2.0 wavespeed–thickness model (Bassin et al. 2000)—principally because CRUST2.0 includes substantially more submerged continental crust. They then merged that with global gravity data (suggesting 32.7 km) and surface-wave dispersion data (34.8 km) to yield an average crustal thickness of 34.4 ± 4.1 km (Figure 1b).