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    CIDER 2008

    Composition of the Earth

    Stan HartWoods Hole Oceanographic Institution

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    Courtesy of NASA/JPL-Caltech

    4.56 Billion Years AgoLets begin at the beginning^

    7

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    How do we determinethe composition of the Earth??

    Best Way:- grind up the Earth.- take a representative sample.- analyze in the lab for everything.

    Or we can take a desperate guess (sometimescalled the chondrite model).

    The problem:

    - direct sampling to only ~15 km.- eruptive entrainment sampling to 200 km,and possibly to 500 km.

    - mantle plume advection from the base of themantle (2900 km). If plumes exist.

    - no bona fide samples yet from the core.

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    The Solar Connection:

    Palme and Jones 2005

    Chondrites ~ Solar Nebula, to within 20%

    Why do we think meteorites have anythingto do with the Earth?

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    The Solar Connection:

    C1 Chondrites ~ Solar Nebula, to within the uncertaintiesof the solar spectroscopic measurements.

    Allegre, Hart and Shimizu, 2008

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    The Chondritic Earth model

    All classes of Chondrites have the same Sm/Nd ratio (1%!)- maybe the Earth is also the same?

    (note: Sm/Nd weight ratio is directly proportional to 147Sm/144Nd)

    1%

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    Hutchinson, 2004

    Chondrites have variable Ca/Si and Al/Si but allclasses of chondrites have the same Ca/Al ratio -

    Maybe the Earth also has the same Ca/Al?

    The Chondritic Earth model

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    Hutchinson, 2004

    Why is Ca/Si and Al/Si variable betweenchondrite classes?

    Because Si has a lower condensation temperature than Ca and Al.

    Then what is the Earths Ca/Si and Al/Si?

    The Chondritic Earth model

    Condensationtemperatures ofthe elements, K:

    Al - 1655Ca - 1520Mg - 1340Fe - 1335Si - 1310

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    Albarede 2003

    The first fuzzy step -

    The chondritic Earth model

    Peridotites represent residuesof partial melting.

    Chondrites represent differingcondensation temperatures.

    Intersection defines thecomposition of the primitiveupper mantle (PUM) andsuggests Earth had a highercondensation temperaturethan chondrites.

    QED - we know the relativeAl, Mg and Si contents ofthe Earth.

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    The more the data, the fuzzier it gets!

    Mg/Si

    A

    l/Si

    0.81.01.21.4

    Canil 2008 Line is Canils best fit to the

    off-craton xenoliths.

    Blue pentagon is PUM fromMcDonough and Sun 1995.

    Green star is PUM from Hartand Zindler 1986 (aka HaZi).

    (PUM = primitive upper mantle)

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    Chondrite model can also be used for trace elements:

    Hart and Zindler 1986

    Like Sm/Nd, Sm/Ca appears constant in chondrites (exceptingsome cooked carbonaceous chondrites).

    Ignore the open squares (metasomatized upper mantle peridotites).

    Tic marks on melting curve are % increments of melt removal.

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    McDonough, 2005

    Refractory Element

    Condensation Temps

    Re - 1820KW - 1790Zr - 1740Th - 1660REE -1660 - 1490 (Yb)Al - 1655U - 1610

    Ti - 1580Ca - 1520

    Semi-refractory

    Mg - 1340Fe - 1335Si - 1310

    8001000120014001600

    Estimated Earth Composition relative to C1 chondrites

    Good match for Refractory Elements (Tcond. >1500K)

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    Abyssal Peridotites = Simple Residues of DMMMeltingLinearized relationshipbetween two elements, A & B, ina residue of fractional melting:

    Where slope, R

    ln Cs

    A R ln CsB ln CoA

    Co

    B R

    R DB(1 D

    A)

    DA(1 D

    B)

    -9

    -8

    -7

    -6

    -5

    -4

    -3

    -2

    -1

    -9 -8 -7 -6 -5 -4 -3 -2 -1 0

    ln(Sm)

    Primitive Upper Mantle (PUM)McDonough & Sun (1995)

    Workman and Hart, 2005

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    PUM PUM

    Some other trace element trends in abyssal peridotites:

    We know the composition of DMM is somewhere onthe regression between PUM and the least depletedabyssal peridotite - but where?

    Workman and Hart, 2005

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    We work backward from the average143Nd/144Nd of melts from thedepleted upper mantle (=0.51317).

    Given the Sm/Nd of PUM, we canmodel the evolution of a continuouslydepleting reservoir that ends at thispresent day 143Nd/144Nd of N-MORB.

    From this model, we can estimate thepresent day Sm/Nd of DMM (=0.411).

    The intersection of this line with theabyssal peridotite trend defines theSm and Nd concentration of DMM.

    Workman and Hart, 2005

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    Composing Trace Element Composition of DMM

    Abyssal Peridotite Constraints

    0.01

    0.10

    1.00

    Rb Ba Th U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    PUMN

    ormalizedCon

    centrations

    Workman and Hart, 2005

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    Composing Trace Element Composition of DMM

    Parent/Daughter Constraints

    0.01

    0.10

    1.00

    Rb Ba Th U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    PUMNormalizedCon

    centrations

    Workman and Hart, 2005

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    Hofmann 2005

    Negative slope means numerator

    element is more compatible thandenominator element.

    i.e mineral/melt partition coefficient Diis larger

    Horizontal slope means both elements

    have the same partition coefficient.

    Canonical Ratios

    DNb > DTh

    DNb < DLa

    DNb ~ DU

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    Some trace elements dont fractionate from each other!

    So ratio in melt equals ratio in residue

    Canonical rat ios

    Spreading Center Lavas

    PETDB Database

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    Composing Trace Element Composition of DMM

    Cannonical Ratios Constraints

    0.01

    0.10

    1.00

    Rb Ba Th U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    PUMN

    ormalizedCon

    centrations

    Workman and Hart, 2005

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    Composing Trace Element Composition of DMM

    Connecting the Dots

    0.01

    0.10

    1.00

    Rb Ba Th U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    PUMN

    ormalizedCon

    centrations

    Workman and Hart, 2005

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    MORB Generation from model DMM

    Workman and Hart, 2005

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    0.01

    0.10

    1.00

    10.00

    100.00

    Rb Ba Th U K Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    SumDMM

    Cont. Crust

    Crust-Mantle Mass Balance - I

    How much DMM does it take to balance JUST Continental Crust?

    CC mass = 0.6% of BSE

    Bulk Continental Crust from Rudnick and Fountain (1995)

    DMM mass = 33% of BSE

    Sum of DMM + CC

    PUMn

    ormalizedconce

    ntrations

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    Crust-Mantle Mass Balance - II

    Bulk Continental Crust from Rudnick and Fountain (1995)

    0.01

    0.10

    1.00

    10.00

    100.00

    Rb Ba Th U K Nb T a La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd T b Dy Ho Y Er Yb Lu

    Sum

    DMM

    Cont. Crust

    N-MORB

    0.6% CC

    Adding Oceanic Crust into the Balance

    Most element fit to within 8%

    43 3% DMM

    2 0.3% MORB

    Sum of MORB + DMM + CC

    PUM

    normalizedconcentrations

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    Physical properties calculated with model of Stixrude and Lithgow-Bertelloni 2005

    - produces a huge effect on isotopes, heat production and some traceelements but an insignificant effect on density and shear wave velocity!

    Deplete the primitive upper mantle to make a depleted MORB mantle:

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    So were done, right?

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    Boyet and Carlson 2006

    hmmmmmm

    142Nd is the daughter of146Sm, an extinct parent.

    142Nd in the accessible Earth is20 ppm higher than inchondrites.

    So is the chondritic modelfor the Earth wrong?

    Maybe!

    Only two simple choices:

    - the earth is not chondritic.- there is a hidden terrestriallow Sm/Nd reservoir wevenot yet seen.

    All consequences are drastic!

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    Hutchinson 2004

    PUM

    Terrestrial fractionation line

    Oxygen isotope compositions of Earth, Ordinary chondrites (H, L LL),Enstatite chondrites (EH, EL), and Carbonaceous chondrites (C1, CM, etc).

    Earth is similar onlyto the EnstatiteChondrites.

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    Hutchinson 2004

    PUM

    Terrestrial fractionation line

    Oxygen isotope compositions of Earth, Moon, Mars,Iron meteorites and differentiated meteorites

    Earth is similar onlyto the Moon, andAubrites (Enstatiteachondrites).

    This oxygen DNA testsuggests the deep Earthmay be richer in enstatitethan olivine (higherperovskite/periclase ratio).

    Seismologists andmineral physiciststo the rescue??

    Im done!

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    Staytuned -

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    0.01

    0.1

    1

    10

    Rb Ba T h U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb L u

    PUMN

    ormalizedConcentrations

    Average Upper Mantle

    Observed Oceanic Crust

    ElementConcentrations

    NormalizedtoBulkSilicateEarth

    Generation of Oceanic Crust using our Upper Mantle Composition

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    0.01

    0.1

    1

    10

    Rb Ba Th U Nb Ta La Ce Pb Pr Nd Sr Zr Hf Sm Eu Ti Gd Tb Dy Ho Y Er Yb Lu

    PUMN

    ormalizedConcentrations

    DMM

    Observed Oceanic Crust

    Model Oceanic Crust

    Average Upper Mantle

    ElementConcentrations

    NormalizedtoBulkSilicateEarth

    Generation of Oceanic Crust using our Upper Mantle Composition

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    -8

    -7

    -6

    -5

    -4

    -3

    -2

    -1

    0

    1

    -7 -6 -5 -4 -3 -2 -1 0

    ln(Sm)

    PUM

    Defining a unique position on the mantle depletion trends

    DMM