9.2 Marine Minerals
The ocean floor hosts vast mineral deposits including polymetallic nodules, ferromanganese crusts, polymetallic sulfides, phosphorites, and methane hydrates. As terrestrial reserves diminish and demand for critical metals grows, deep-sea mining has become a frontier of resource extraction—raising profound environmental and governance challenges under the International Seabed Authority (ISA).
Polymetallic (Manganese) Nodules
Manganese nodules are potato-sized concretions found on abyssal plains at 4000–6000 m depth. They grow at rates of only a few millimeters per million years by precipitating dissolved metals from seawater (hydrogenous growth) and pore water (diagenetic growth). The growth rate can be estimated from radiometric dating using $^{10}\text{Be}$ or $^{230}\text{Th}$:
$$G = \frac{\Delta r}{\Delta t} \approx 1\text{--}10 \;\text{mm/Myr}$$
Among the slowest geological processes on Earth
Composition
Mn (27–30%), Fe (6%), Ni (1.3%), Cu (1.1%), Co (0.2%), plus trace REEs, Li, Mo, V, Te
Clarion-Clipperton Zone (CCZ)
Largest known deposit: ~21 billion tonnes of nodules across 4.5 million km² in the equatorial Pacific
The total metal resource in a deposit is estimated by integrating nodule abundance$\rho_A$ (kg/m²) over the survey area:
$$M_{\text{metal}} = \int\!\!\int_A \rho_A(x,y) \cdot g_{\text{metal}}(x,y) \, dA$$
$\rho_A$ = nodule abundance (kg/m²), $g$ = metal grade (weight fraction)
Ferromanganese Crusts & Polymetallic Sulfides
Ferromanganese Crusts
Form on seamount flanks at 800–2500 m depth by hydrogenous precipitation from cold, oxygenated seawater. Enriched in Co (up to 2%), Ni, REEs, Te, and Pt. Growth rate ~1–5 mm/Myr. Thickness ranges from 1 to 25 cm.
Global resource: ~7.5 billion tonnes of dry crust on ~1.7 million seamounts
Polymetallic Sulfides (SMS)
Form at hydrothermal vents on mid-ocean ridges and back-arc basins. Superheated fluids ($>350°C$) precipitate Cu, Zn, Au, Ag when mixing with cold ambient seawater causes rapid supersaturation.
Typical grades: Cu 1–15%, Zn 3–20%, Au 1–10 g/t, Ag 50–500 g/t
Metal precipitation from hydrothermal fluids occurs when the saturation index exceeds zero. The saturation index (SI) for a mineral phase is:
$$\text{SI} = \log_{10}\!\left(\frac{\text{IAP}}{K_{sp}(T, P)}\right), \quad \text{precipitation when SI} > 0$$
$\text{IAP}$ = ion activity product, $K_{sp}$ = solubility product (temperature and pressure dependent)
Methane Hydrates (Clathrates)
Methane hydrates are ice-like crystalline solids in which methane molecules are trapped within a cage lattice of hydrogen-bonded water molecules. They are stable under high-pressure, low-temperature conditions found in continental margins and permafrost regions. The three-phase (hydrate–liquid water–gas) equilibrium boundary follows:
$$\ln P_{eq} = \frac{A}{T} + B$$
$P_{eq}$ = equilibrium pressure (MPa), $T$ = temperature (K); for pure CH&sub4; in pure water: $A \approx -8534$, $B \approx 38.98$
~1800 Gt C
Estimated global methane hydrate carbon
164:1
Gas volume expansion upon dissociation
300–2000 m
Typical depth range of the GHSZ
The Clausius-Clapeyron relation governs the phase boundary slope for the dissociation reaction CH&sub4;·nH&sub2;O → CH&sub4;(g) + nH&sub2;O(l):
$$\frac{dP}{dT} = \frac{\Delta H}{T \, \Delta V}$$
$\Delta H \approx 54$ kJ/mol for Structure I methane hydrate
Deep-Sea Mining Technology & Governance
Mining System Components
Collector vehicles on the seafloor gather nodules or cut crust; a riser system transports slurry to a surface support vessel; dewatering and tailings management occur on board. The hydraulic power required to lift material through the riser is approximately:
$P_{\text{lift}} = \dot{m} \, g \, H \cdot (1 + f_{\text{loss}})$, where $f_{\text{loss}} \approx 0.2\text{--}0.4$ accounts for friction
Environmental Impact Assessment
Sediment plumes may extend hundreds of kilometers. Habitat destruction affects slow-growing communities with recovery timescales exceeding millions of years for nodule fields. Noise and light pollution disrupt deep-sea organisms adapted to the dark, quiet abyss.
ISA Regulatory Framework
The International Seabed Authority manages mineral resources in the "Area" (international seabed beyond national jurisdiction) under UNCLOS Part XI. Exploration contracts, environmental management plans, and Area-based management tools are required before any extraction.
Sand & Gravel Extraction
Shallow marine aggregates mined for construction at ~6 billion tonnes/year globally. Causes coastal erosion and habitat loss.
Rare Earth Elements in Deep-Sea Mud
Pacific deep-sea muds contain REE concentrations 2–5x terrestrial ores. Critical for electronics, wind turbines, and EV batteries.
Derivation: Resource Estimation from Survey Data
Step 1: Define Nodule Abundance as a Spatial Field
Nodule abundance $\rho_A(x,y)$ (kg/m$^2$) is a spatially varying quantity measured at discrete box-core sampling stations $(x_i, y_i)$. The total mass of nodules in the exploration area $A$ is:
$$M_{\text{total}} = \int\!\!\int_A \rho_A(x,y) \, dA$$
Step 2: Discretise Using Geostatistical Interpolation
With $n$ sample stations, we estimate $\rho_A$ at unsampled locations using kriging. The kriged estimate is a weighted linear combination of observations:
$$\hat{\rho}_A(\mathbf{x}_0) = \sum_{i=1}^{n} w_i \, \rho_A(\mathbf{x}_i), \quad \sum_i w_i = 1$$
Step 3: Incorporate Metal Grade
Each metal $m$ has a grade (weight fraction) $g_m(x,y)$ that also varies spatially. The total metal resource is the product of abundance and grade integrated over area:
$$M_m = \int\!\!\int_A \rho_A(x,y) \cdot g_m(x,y) \, dA \approx \sum_{k=1}^{N_{\text{cells}}} \hat{\rho}_A(\mathbf{x}_k) \cdot \hat{g}_m(\mathbf{x}_k) \cdot \Delta A_k$$
Step 4: Uncertainty via Kriging Variance
Kriging provides not just the best estimate but also the estimation variance $\sigma_k^2$ at each cell, allowing confidence intervals on the total resource:
$$\text{Var}(M_m) = \sum_{k=1}^{N_{\text{cells}}} \left[\hat{g}_m^2 \sigma_{\rho,k}^2 + \hat{\rho}_A^2 \sigma_{g,k}^2\right] (\Delta A_k)^2$$
Derivation: Manganese Nodule Growth Rate from Radiometric Dating
Step 1: Radioactive Decay Law
A radioisotope incorporated into the nodule during growth decays exponentially. For $^{10}\text{Be}$ ($t_{1/2} = 1.387$ Myr):
$$N(t) = N_0 \, e^{-\lambda t}, \quad \lambda = \frac{\ln 2}{t_{1/2}}$$
Step 2: Relate Depth in Nodule to Age
If the nodule grows radially at a constant rate $G$ (mm/Myr), then a layer at radial depth $r$ from the surface was deposited at time $t = r/G$ ago. The isotope activity at depth $r$ is:
$$A(r) = A_0 \, \exp\!\left(-\frac{\lambda \, r}{G}\right)$$
Step 3: Linearise by Taking the Logarithm
Taking the natural log gives a linear relationship between $\ln A$ and radial depth $r$. The slope of this line yields the growth rate:
$$\ln A(r) = \ln A_0 - \frac{\lambda}{G} \, r \quad \Longrightarrow \quad G = -\frac{\lambda}{\text{slope}}$$
Step 4: Typical Results
For CCZ nodules, measured $^{10}\text{Be}$ profiles yield slopes corresponding to $G \approx 1\text{--}10$ mm/Myr. Hydrogenous layers (seawater precipitation) grow at ~1--5 mm/Myr, while diagenetic layers (pore water) grow faster at ~5--10 mm/Myr. A 5 cm radius nodule therefore has an age of order 5--50 Myr.
Python: Mineral Grade Analysis & Economic Viability
Python: Mineral Grade Analysis & Economic Viability
Python!/usr/bin/env python3
Click Run to execute the Python code
Code will be executed with Python 3 on the server
Fortran: Methane Hydrate P–T Phase Diagram
This program computes the three-phase equilibrium boundary for Structure I methane hydrate and determines the gas hydrate stability zone (GHSZ) thickness given seafloor conditions and the local geothermal gradient.
Fortran: Methane Hydrate P–T Phase Diagram
FortranMethane hydrate P-T phase diagram and GHSZ calculation
Click Run to execute the Fortran code
Code will be compiled with gfortran and executed on the server
Phosphorites & Placer Deposits
Marine Phosphorites
Phosphatic sedimentary deposits on continental shelves and slopes. Form by upwelling-driven biological productivity and diagenetic phosphogenesis. Major deposits off Namibia, Peru, and eastern Australia. Primary mineral: francolite (carbonate fluorapatite).
Marine Placer Deposits
Heavy mineral concentrations in nearshore sediments including tin (cassiterite), titanium (ilmenite, rutile), zircon, and diamonds. Formed by wave and current sorting of terrestrial source material on continental shelves.