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Thermal conductivity of iron and nickel during melting - Implication to the planetary liquid outer core

MetadataDetails
Publication Date2022-12-13
JournalPramana
AuthorsPinku Saha, Goutam Dev Mukherjee
InstitutionsIndian Institute of Science Education and Research Kolkata
Citations4
AnalysisFull AI Review Included
  • Core Achievement: Direct measurements of the thermal conductivity ($\kappa$) of pure iron (Fe) and nickel (Ni) were successfully performed across their melting transitions at high pressures (up to 22 GPa) and high temperatures (up to 2250 K).
  • Methodology: The study utilized a Laser Heated Diamond Anvil Cell (LHDAC) combined with finite-element simulations (COMSOL) to accurately model and measure the temperature gradient across the sample surface.
  • Melting Signature: A sharp, significant drop (25-40%) in $\kappa$ was consistently observed at the melting temperature for both Fe and Ni, providing a robust method for determining the high-pressure melting curve.
  • Liquid Core Constraint: The thermal conductivity of the molten metals was found to be low (Fe: 60-70 W/mK; Ni: 65-70 W/mK) and, critically, remained constant (invariant) along the melting boundary across the tested pressure range.
  • Geophysical Implication: These low, constant $\kappa$ values provide essential constraints for geodynamo models, suggesting a lower heat flux from planetary cores (like Mercury and Mars) than previously estimated by some high-end theoretical calculations (160-200 W/mK).
  • Material Physics: The constant $\kappa$ in the liquid state is attributed to the loss of long-range order while maintaining a local closed-packed hard-sphere structure, a phenomenon linked to the unfilled d-band transition metals.
ParameterValueUnitContext
Fe Thermal Conductivity (Liquid)60-70 ± 20W/m-1K-1At melting, 5-8 GPa (Mercury core conditions)
Ni Thermal Conductivity (Liquid)65-70 ± 20W/m-1K-1At melting, 4-22 GPa
Observed $\kappa$ Drop upon Melting25-30% (Fe); 30-35% (Ni)%Sharp transition from solid to liquid phase
Maximum Pressure Tested (Ni)22GPaHighest pressure point for Ni $\kappa$ measurement
Fe Melting Temperature Range1975 to 2098KObserved melting points at 5 to 8.5 GPa
Ni Specific Heat (Cp)420JKg-1K-1Used in heat energy calculation (Eqn. 3)
Fe Specific Heat (Cp)450JKg-1K-1Used in heat energy calculation (Eqn. 3)
Sample Thickness (Fe/Ni)~15”mInitial thickness of compacted metal plates
PTM MaterialNaCl-Used for pressure transmission and thermal insulation
NaCl Thermal Conductivity6W/m-1K-1Used in COMSOL simulation [49]
Laser Wavelength1.070”mDiode-pumped Ytterbium fiber optic laser
Total $\kappa$ Uncertainty~30%Estimated total error due to propagation of errors
  1. Sample Preparation and Loading: Thin plates (~15 ”m) of polycrystalline Fe and Ni were compacted. These metal plates were sandwiched between NaCl discs (~12 ”m thick), which served as both the Pressure Transmitting Medium (PTM) and thermal insulation.
  2. High-Pressure Apparatus: A single-sided Laser Heated Diamond Anvil Cell (LHDAC) was employed, utilizing 300 ”m culet diamond anvils and a T301 stainless steel gasket.
  3. Heating Source: A continuous wave (CW) diode-pumped Ytterbium fiber optic laser (1.070 ”m) was used to heat the sample, creating a localized hotspot.
  4. Steady-State Confirmation: The system was allowed 5-10 minutes to stabilize after heating initiation to ensure steady-state heat flow conditions were achieved before measurement.
  5. Temperature Gradient Measurement: The temperature profile across the sample surface was measured by translating a 50 ”m pinhole attached to a spectrometer across the magnified image of the sample. Temperature was determined by fitting Planck’s radiation function (650-900 nm range).
  6. Heat Energy Calculation: The heat energy ($Q$) absorbed by the metal foil at the hotspot was calculated using the thermodynamic equation: $Q = m C_{p} (T_{hotspot} - T_{room}) \nu$, where $m$ is the mass, $C_{p}$ is the specific heat capacity, and $\nu$ is the modulation frequency (50 kHz).
  7. Thermal Conductivity Simulation: The finite-element software COMSOL Multiphysics was used to simulate the steady-state temperature distribution based on the heat conduction equation. The thermal conductivity ($\kappa$) of the sample was determined iteratively by varying $\kappa$ until the computed temperature profile matched the experimentally measured temperature gradient.
  8. Melting Point Determination: The melting temperature ($T_{m}$) at a given pressure was identified by the sudden, sharp drop in the calculated $\kappa$ value, marking the solid-to-liquid phase transition.

The findings are primarily relevant to fundamental research in planetary science and high-pressure physics, providing critical data for large-scale geophysical models and simulations:

  • Planetary Geophysics and Core Modeling:
    • Geodynamo Lifetime: The low, constant thermal conductivity of liquid Fe and Ni directly impacts the thermal evolution and cooling rate of planetary cores (Earth, Mercury, Mars). A lower $\kappa$ implies a slower heat loss, which is essential for sustaining the magnetic field (geodynamo) over geological timescales.
    • Core-Mantle Boundary Heat Flux: Providing accurate, experimentally derived $\kappa$ values for Fe and Ni at conditions relevant to the Mercury core-mantle boundary (5-8 GPa, 1850-2200 K) to refine models of Mercury’s weak dynamo.
  • High-Pressure Materials Science:
    • Transport Property Prediction: Establishing reliable experimental benchmarks for the thermal transport properties of transition metals (Fe, Ni) across phase transitions under extreme pressure, validating or challenging ab initio theoretical calculations.
    • Alloy Design for Extreme Environments: The observed invariance of $\kappa$ in the liquid state provides insight into electron scattering mechanisms in molten transition metals, which is valuable for designing alloys intended for high P-T applications where thermal management is critical.