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Composition of the Earth: a more volatile elements perspective Cider 2010 Bill McDonough Geology, University of Maryland Support from:

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Presentation on theme: "Composition of the Earth: a more volatile elements perspective Cider 2010 Bill McDonough Geology, University of Maryland Support from:"— Presentation transcript:

1 Composition of the Earth: a more volatile elements perspective Cider 2010 Bill McDonough Geology, University of Maryland Support from:

2 Volatility trend @ 1AU from Sun Th & U

3 Allegre et al (1995) EPSL

4 McDonough & Sun (1995) Chem G the volatile budget?

5 Earth’s D/H ratio Do we really know comets D/H ratio of the oceans What do chondrites tell us? Source of water and other volatiles vs the sources of noble gases? Ref: Owen and Bar-Nun, in R. M. Canup and K. Righter, eds., Origin of the Earth and Moon (2000), p. 463

6 Progress Report Conclusions: Approximate concentrations Depleted Mantle H 2 O 50 ppm; CO 2 20 ppm; Cl 1 ppm; F 7 ppm Enriched Mantle H 2 O 500 ppm; CO 2 420 ppm; Cl 10 ppm; F 18 ppm Total Mantle H 2 O 366 ppm; CO 2 301 ppm; Cl 7 ppm; F 15 ppm Last CIDER report on volatiles in the Earth - Saal et al 2009 Earth: 6  10 24 kgOceans: 1.4  10 21 kg Ordinary chondritic planet -- 4 oceans Carbonaceous chondritic planet -- 600 oceans Enstatite chondritic planet -- ~2-4 oceans

7 H/C ratio of the bulk silicate Earth is superchondritic, owing chiefly to the high H/C ratio of the exosphere. H/C ratio of the mantle is lower than that of the exosphere, requiring significant H/C fractionation during ingassing or outgassing at some point in Earth history. Hirschmann and Dasgupta (2009) Volatile Budget!

8 Earth’s volatiles from chondrites? Let’s hear from what Sujoy has to say!…

9 Mantle Siderophile elements Lithophile elements Fe, Ni, P, Os Core Atmophilie elements N 2, O 2, Ar “my Earth”

10 First observations -- got it right at the 1-sigma level

11 SCIENCE Accepted as the fundamental reference and set the bar at K/U = 10 4 Th/U = 3.5 to 4.0

12 MORB (i.e., the Depleted Mantle ~ Upper Mantle) K/U ~ 10 4 and slightly sub-chondritic Th/U DM & Continental Crust – complementary reservoirs DM + Cc = BSE ahh, but the assumptions and samples…

13 Earth is “like” an Enstatite Chondrite! 1) Mg/Si -- is very different 2) shared isotopic X i -- O, Cr, Mo,Ru, Nd, 3) shared origins -- unlikely 4) core composition -- no K, U in core.. S+ 5) “Chondritic Earth” -- lost meaning… 6) Javoy’s model? -- needs to be modified

14 Volatility trend @ 1AU from Sun Th & U

15 Core Mantle Siderophile elements Lithophile elements Ca, Al, REE, K, Th & U Fe, Ni, P, Os Atmophilie elements

16 U in the Earth: ~13 ng/g U in the Earth Metallic sphere (core) <<<1 ng/g U Silicate sphere 20* ng/g U *Javoy et al (2010) predicts 11 ng/g Continental Crust 1000 ng/g U Mantle ~12 ng/g U “Differentiation” Chromatographic separation Mantle melting & crust formation

17 This translates to 11 ppb U

18 Allegre et al (1995), McD & Sun (’95) Palme & O’Neill (2003) Lyubetskaya & Korenaga (2007) Normalized concentration REFRACTORY ELEMENTS VOLATILE ELEMENTS Half-mass Condensation Temperature Potassium in the core Silicate Earth ?

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20 All peridotites are 2-component mixtures! From McDonough (1994) Melt-depletion Melt-”re-enrichment” (aka - metasomatism)

21 Initial results from: McDonough & Sun ‘95 - trends not pretty, but robust - trends cross chondritic pt -trends are melting products -important not to use highly-ITE Lyubetskaya & Korenaga (2007) made this mistake

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23 Log concentrations (in ppm) degree of melting Shaded symbols denote samples with MgO 40.5%

24 Based on mantle samples: MgO 35-41 wt% (n =330)

25 Mantle is depleted in some elements (e.g., Th & U) that are enriched in the continents. -- models of mantle convection and element distribution Th & U rich Th & U poor

26 4 most abundant elements in the Earth: Fe, O, Si and Mg 6 most abundance elements in the Primitive Mantle: - O, Si, Mg, and – Fe, Al, Ca This result and 1 st order physical data for the core yield a precise estimate for the planet’s Fe/Al ratio : 20 ± 2

27 What’s in the core? What would you like? Constraints: density profile, magnetic field, abundances of the elements, Insights from: cosmochemistry, geochemistry, thermodynamics, mineral physics, petrology, Hf-W isotopes (formation age) How well do we know some elements?

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30 Model 1Model 2 Core compositional models others

31 Model Core composition (wt%) % in core rel. Earth (ug/g) % in core rel. Earth Fe88.387V15050 O33Mn30010 Ni5.493Cu12565 S1.996Pd3.1>98 Cr0.960Re0.23>98 P0.293Os2.8>98 C0.291Au0.5>98

32 REFRACTORY ELEMENTS Nature 436, 499-503 (28 July 2005) Detecting Geoneutrino in the Earth Detecting Electron Antineutrinos from inverse beta -decay 2 flashes close in space and time Rejects most backgrounds  - decay

33 Geo-neutrinos at KamLAND Silicate Earth has ~20 ng/g U


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