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Archaean magmatism

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Archaean magmatism NB- Archean (US spelling) or Archaean (UK spelling) Why? Somehow different from modern magmas Interesting to test our understanding of petrogenetic ... – PowerPoint PPT presentation

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Title: Archaean magmatism


1
Archaean magmatism
NB- Archean (US spelling) or Archaean (UK
spelling)
2
Why?
  • Somehow different from modern magmas
  • Interesting to test our understanding of
    petrogenetic processes
  • Not that rare, and good South African examples
    (Barberton)
  • Economic interest
  • Gold (large part of worlds gold secondary
    deposits)
  • PGE bearing sulphides
  • Nickel
  • Departments research interests

3
Barberton gold fields
4
Two characteristic rock types
  • Komatiites ultra-mafic, Mg-rich lavas
  • TTGs Tonalites, Trondhejmites Granodiorites
  • Link with Archaean geodynamic style?

5
The Archaean
6
Oldest crustal remnants
7
Jack Hill (Australia) zircon 4.404 ? 0.008 Ga
8
The oceanic crust is young
9
75 of the crust was formed at ca. 2.5 Ga The
Archaean is a major crust-forming period
10
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11
The average continental crust
C.C. is roughly andesitic
12
Continental crust
Ca. 30 km
13
The continental crust
  • has the composition of magmatic rocks, and is
    largely made of magmatic rocks
  • formed mostly in the Archaean
  • ? We have to study the geology of Archaean
    continental crust.

14
Earths heat production
?A 2- to 4-fold decrease from the Archaean to now
15
Effects of higher Archaean heat production?
  • Shape of convection
  • Partitioning of heat flux
  • Effects on the continents thermal structure and
    behaviour
  • Petrogenesis?

16
Shape of convection ?
(Ra gt 105)
(Ra 103 - 104)
Ra function of many things, including DT (or
heat production)
17
Archaean dome-and-keel patterns
Vertical tectonics (sagduction)
Zimbabwe (2.7 Ga)
Pilbara (3.5 Ga)
18
Superior Province
19
Bimodal Archaean terranes
  • Greenstone belts (commonly dominated by
    greenschist facies amphibolites)
  • Mafic and ultramafic ( komatiites) lavas
  • Some intermediate lavas (andesites)
  • Detrical sediments
  • Some chemical sediments (BIFs) or biogenic
    formations (stromatholites)
  • Gneissic  basement  or plutons
  • Late plutons

20
2.9 2.7 Ga granites
3.1 Ga granites syenites
Moodies
Fig Tree
Onverwacht
Ca. 3.2 Ga TTG
Ca. 3.4 Ga TTG
 Ancient gneisses  (3.6 3.4 Ga)
21
1. Komatiites
  • Viljoen, M. J. and R. P. Viljoen (1969). "The
    geology and geochemistry of the lower ultramafic
    unit of the Onverwacht group and a proposed new
    class of igneous rocks." Geological Society of
    South Africa Special Publication 2 55-86.

A truly South-African rock type!
22
Onverwacht group, BGB
The original komatiites in Komatii formation
(1.5 km from type locality)
23
Komatiites composition
24
  • Structure of komatiites flows
  • Origin of komatiites
  • Komatiites and the Archaean mantle

25
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26
Subdivision of komatiite flows (Arndt et al. 1977)
Polysutured top
Random spinifex
Orientated spinifex
parallel blades of spinifex
solid subhedral olivine
B4
Basal chill, polysutured
27
Chilled/brecciated top
  • Subaquatic emplacement

28
Spinifex textured layer(s)
  • Random spinifex
  • Orientated spinifex
  • Plate spinifex

Spinifex grass, Western Australia (Barnes 1990)
29
Random spinifex
30
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Orientated spinifex
34
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35
Plate spinifex
36
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37
Polyedral olivine
38
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39
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43
Origin of komatiites
  • High Mg contents require high degree of mantle
    melting (40-60 )
  • This implies very high temperatures and fast rise

44
What are the implications of komatiites?
  • Probably formed in hot-spot like situations
    (difficult to arrive to gt 1600 else)
  • Even though, this is hotted than modern hotspots
  • At least some parts of the Earth were very hot
  • At least part of the GSB formed from hotspots
    (intraplate situation)

45
Komatiites and the history of the Archaean mantle
46
3 groups of komatiites, from the shape of their
HREE pattern (or Gd/Yb ratios) Role of garnet
47
  • Correlation with Al (and also Ca)
  • Al depleted (grp II) vs. Al-undepleted (grp. III)
  • Only grp I komatiites exist in the late Archaean

48
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  • Early differenciation of the Earth mantle
    (completed at 3.80 Ga)
  • Deep origin of Late-Archaean komatiites (or
    locally non-differenciated bits of mantle?)
  • Maybe due to a cooler Earth, hot temperatures
    found only very deep?

50
2. TTG
  • Archaean TTG (Tonalite, Trondhjemites and
    Granodiorites)
  • grey gneisses (although in details, some TTGs
    are not grey gneisses and some grey gneisses are
    not TTG)

51
Archaean grey gneisses
Some relatively simple orthogneisses
Stolzburg pluton (Barberton, 3.45 Ga)
52
Commonly complex, migmatitic, polydeformed
orthogneisses
53
The Sand River Gneisses Ca. 3.1 Ga TTG gneisses
in Messina area, Limpopo Belt, South Africa (R.
White, Melbourne, for scale)
54
  • However, the most common component of the grey
    gneisses is relatively constant

55
Mineralogy
56
Major elements
57
REE
58
Nb-Ta anomaly
Sr contents
Y HREE depletion
59
Experimental studies
60
  • Partial melting of amphibolites ( metabasalts)
    is appropriate to generate TTG-like sodic melts
  • Melting reactions of the form
  • Amp Plag M Opx Ilm
  • Amp Plag M Grt Ilm
  • (Incongruent melting / amphibole dehydration
    melting)

61
Conditions for making TTGs

Experimental melts
62
NB
  • Some people propose that TTGs can be formed by
    hornblende dominated FC of andesites
  • Not impossible (at least in theory) but..
  • Where are the cumulates?
  • High viscosity of felsic melts
  • Lack of andesitic plutonic terms associated with
    TTGs
  • Regarded as unlikely to impossible by maybe
    80-90 of the petrologists

63
TTG are...
  • Orthogneisses
  • Tonalites, Trondhjemites Granodiorites
  • (Na-rich series)
  • Fractionnated REE, etc.
  • Largely homogeneous throughout the Archaean
  • Originated by partial melting of amphibolites
    (hydrated basalts), in garnet stability field

64
Garnet stability in mafic rocks
  • From a dozen of experimental studies
  • Well-constrained grt-in line at about 10-12 kbar

65
From chemistry to geodynamic
  • TTGs partial melts of amphibolites in garnet
    stability field
  • Does this tell something about geodynamic
    conditions?

66
Geodynamic site ?
Gt-in
Subduction
Gt-in
  • Intermediate cases
  • Shallow subduction
  • ( underplating)
  • Stacked oceanic crust

Gt-in
Gt-in
Thick (oceanic or continental) crust (e.g.
Oceanic plateau)
Gt-in
67
TTGs in a  plate  model
68
TTGs in a  non plate  model
69
Some lines of research
  • TTG and adakites
  • Secular evolution of TTGs
  • TTGs and partial melting of amphibolites
  • Diversity and components of the  grey gneisses 
  •  Sanukitoids  etc.

Youre now entering the field of active research
and controversies!
70
TTGs and adakites
  • Are TTGs and adakites similar?

Yes !
No !
Thats the stuff active scientific research is
made of
71
Are TTGs and adakite similar?
  • If they are Adakites can be used as an indicator
    of the site of TTG formation, but
  • Are the adakites formed as slab melts
  • .. Or as melts of underplated basalts (Cordilera
    Blanca)?
  • If they are not they still are rather similar,
    so what the ?

72
Secular evolution of Mg in TTG
  • Fractional crystallization reduces Mg
  • For each period the higher Mg represents TTG
    parental magma
  • From 4.0 to 2.5 Ga Mg regularly increased in
    TTG parental magmas

73
  • MgO increases inTTG in course of time
  • SiO2 decreases inTTG in course of time
  • Adakites have exactly the same evolution pattern
    as (young) TTG
  • For the same SiO2, experimental melts are
    systematically MgO poorer than TTG

74
Our conclusions
  • Relatively young TTGs are similar to adakites
  • Both are different from melts from amphibolites
    (higher Mg etc.)
  • We propose that this corresponds to interactions
    with the mantle
  • which can be achieved only in subduction (slab
    melting) situation both for young TTGs and
    adakites

NB- This is just our interpretation it is
challenged
Martin Moyen 2002
75
INTERPRETATION
EARLY ARCHAEAN
LATE ARCHAEAN/ADAKITES
TODAY
High heat production ? High geothermal gradients
? Shallow depth slab melting Thin overlying
mantle ? No or few magma/mantle interactions ?
Low Mg-Ni-Cr TTG
Lower heat production ? Lower geothermal
gradients ? Deep slab melting Thick overlying
mantle ? important magma/mantle interactions ?
High-Mg-Ni-Cr TTG
Low heat production ? Low geothermal gradients ?
No slab but mantle wedge melting
76
Sanukitoids geographic repartition
77
Sanukitoids petrography
Diorites, monzodiorites and granodiorites
Lots of microgranular mafic enclaves
Qz Pg KF Bt Hb Cpx
Ap Ilm Sph Zn
78
Sanukitoids geochemistry
79
Making sanukitoids
80
  • Sanukitoids also suggest interactions between the
    mantle and TTG (or TTG like) melts
  • Again, this is more consistent with slab melting
  • .. At least at the end of the Archaean

81
  • As usual, the answer is certainly somewhere in
    between the extremes!
  • Some TTGs are probably slab melts maybe not all
  • Some TTGs certainly formed in subduction zones
    (and therefore subduction zones existed quite
    early) but probably not all, nor everywhere
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