Multispectral and hyperspectral imaging
ASTER, Sentinel-2, Landsat; EMIT, EnMAP, PRISMA; airborne and field spectrometers
Identifies certain minerals at the exposed surface by their absorption features. It sees the top micrometres to millimetres of rock and soil — nothing beneath.
SCHEMATIC — NOT TO SCALE
Technical sheet — principle, instrument, reach, resolution, limits
- Physical principle
- Minerals absorb sunlight at characteristic wavelengths. Electronic transitions in iron give broad features in the visible and near-infrared (hematite near 0.86 µm, goethite near 0.91 µm); vibrations of Al–OH, Mg–OH and carbonate bonds give narrow features in the shortwave infrared (the kaolinite doublet near 2.165 and 2.205 µm, alunite's main feature near 2.17 µm, calcite near 2.34 µm). Multispectral sensors sample a few broad bands and can separate mineral groups; hyperspectral sensors (imaging spectroscopy) sample hundreds of narrow, contiguous bands and can separate individual minerals.
- Instrument and platform
- Multispectral: ASTER on Terra — its shortwave-infrared detectors stopped producing usable data in 2008 after overheating, but the earlier archive remains valuable — Sentinel-2 MSI and Landsat 8 and 9 OLI. Hyperspectral from orbit: NASA's EMIT on the International Space Station (60 m pixels, about 380–2500 nm), Germany's EnMAP (30 m, about 420–2450 nm, 224 bands) and Italy's PRISMA (30 m, 400–2500 nm). Airborne imaging spectrometers and handheld field spectrometers give finer detail.
- What it measures directly
- Reflected sunlight as a function of wavelength — a spectrum — for each pixel, after atmospheric correction.
- What it allows us to infer
- Surface mineralogy — clays (kaolinite, illite/sericite), sulphates (alunite, jarosite), carbonates, iron oxides — and from their patterns, hydrothermal alteration zones that surround some ore systems.
- Reach and depth (conditional)
- Surface only: the uppermost micrometres to millimetres. Vegetation, soil, lichen, desert varnish, water and cloud hide or dilute the signal. Works best in arid, sparsely vegetated terrain.
- Resolution and error sources
- Pixels from 10–30 m (Sentinel-2, Landsat, EnMAP, PRISMA, ASTER) to 60 m (EMIT); a mineral covering part of a pixel is mixed with everything else in it. Errors from atmospheric correction, illumination and topography, mixtures and look-alike minerals.
- Real mining application
- A standard first step in arid regions: mapping alteration around porphyry copper and epithermal gold systems, iron oxides over gossans and iron-rich rocks, carbonates for limestone and dolomite, and clays for industrial minerals; also used on mine waste and tailings to map iron oxides and secondary minerals.
- Limitations
- It does not see metals: copper, gold or lithium have no usable signature from orbit; it maps minerals that may accompany them. Alteration is not ore — many altered areas are barren — and a few centimetres of soil hide everything.
- Status
- OPERATIONAL. An established mapping tool; its detections are surface indications, never a grade.