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Published on: November 5, 2019
Tungsten-182 evidence for an ancient kimberlite source.
Nao Nakanishi1, Andrea Giuliani2,3, Richard W Carlson4
1Department of Geology, University of Maryland, College Park, MD 20742; nnakanis@umd.edu.
Primitive kimberlites globally show uniform tungsten-182 (¹⁸²W) and neodymium-142 (¹⁴²Nd) isotopic values, suggesting derivation from an ancient, isolated mantle reservoir. This reservoir may preserve evidence of early Earth processes, potentially linked to core-mantle interactions or early silicate differentiation.
Area of Science:
- Geochemistry
- Isotope Geology
- Planetary Science
Background:
- Globally distributed kimberlites often exhibit chondritic initial Neodymium-143/Samarium-144 (¹⁴³Nd/¹⁴⁴Nd) and Hafnium-176/Lutetium-176 (¹⁷⁶Hf/¹⁷⁷Hf) isotopic ratios.
- These isotopic signatures suggest derivation from a chemically homogeneous, primitive mantle source that remained isolated from the convecting mantle throughout much of Earth's history.
- Understanding the nature of this reservoir is key to deciphering early Earth processes and mantle evolution.
Purpose of the Study:
- To investigate whether ancient mantle reservoirs, inferred from kimberlite compositions, preserve evidence of early Earth processes.
- To analyze Tungsten-182/Tungsten-184 (¹⁸²W/¹⁸⁴W) and Neodymium-142/Neodymium-144 (¹⁴²Nd/¹⁴⁴Nd) isotopic data in primitive kimberlites.
- To constrain the origin and evolution of long-lived, isolated mantle reservoirs.
Main Methods:
- Analysis of ¹⁸²W/¹⁸⁴W and ¹⁴²Nd/¹⁴⁴Nd isotopic ratios in primitive kimberlites from 10 global localities.
- Kimberlite samples range in age from 1,153 to 89 million years ago (Ma).
- Comparison of isotopic data with chondritic values and modern upper mantle compositions.
Main Results:
- Most analyzed kimberlites (1,153–89 Ma) display homogeneous μ¹⁸²W and μ¹⁴²Nd values, averaging -5.9 ± 3.6 ppm and +2.7 ± 2.9 ppm, respectively.
- Uniform, modestly negative μ¹⁸²W values, alongside chondritic to suprachondritic initial ¹⁴³Nd/¹⁴⁴Nd and ¹⁷⁶Hf/¹⁷⁷Hf ratios, support derivation from early-formed, isolated mantle reservoirs.
- Two younger kimberlites (72 and 52 Ma) show subchondritic initial ¹⁷⁶Hf/¹⁷⁷Hf and ¹⁴³Nd/¹⁴⁴Nd, with μ¹⁸²W consistent with the modern upper mantle, potentially indicating crustal contamination.
Conclusions:
- The isotopic data provide permissive evidence for the existence of long-lived, early-formed mantle reservoirs.
- Negative μ¹⁸²W values in primitive kimberlites may result from core-to-mantle W transfer, early silicate fractionation, or late accretionary input.
- Younger kimberlites suggest potential contamination of ancient sources by recycled crustal materials.
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