Overview

A dyke (sometimes spelled dike) is a sheetlike body of rock that forms when molten material forces its way through or between older rocks and solidifies. Most commonly this molten material is igneous in origin — magma or lava — that intrudes into cracks and bedding planes and then cools to form a tabular body that typically has a near-vertical orientation relative to the host rocks. Dykes range in thickness from a few centimetres to many metres or more, and they commonly cut across existing structures rather than following them.

Formation and characteristics

Dyke formation is an intrusive process: pressure in a subsurface magma source fractures the surrounding rock and drives molten material into the openings. When the molten rock cools and crystallizes it becomes a coherent mass with properties that often differ markedly from the surrounding country rock. Dykes commonly display a fine-grained or glassy chilled margin where rapid cooling occurred against cooler host rock, and they may show columnar jointing, variations in mineralogy, or contact metamorphism in adjacent rocks.

Because dykes cut across preexisting layers or structures — for example bedding or foliation — they are useful for relative dating in the field: a dyke must be younger than the rocks it intrudes. In sedimentary terrains, the relationship to layering (bedding) is often obvious. Not all vertical tabular bodies are igneous; some may form by sedimentary infill of vertical cracks or by tectonic processes, and those are distinguished by their texture and origin (sedimentary intrusions).

  • Sheet dykes: planar and tabular intrusions that can be traced for great distances.
  • Composite dykes: contain multiple injections or different rock types within a single fissure.
  • Breccia-filled fissures: in some settings fractures are filled with broken fragments and cement — for example breccia after seismic or volcanic activity.

In contrast to a sill, which parallels bedding and forms a concordant sheet, a dyke is typically discordant and transects bedding or other structures. Many volcanic events produce both dykes and sills as magma exploits weaknesses in different orientations.

Distribution, swarms and geological significance

Dykes are widespread in many rock sequences and are especially common in older Palaeozoic terrains where multiple pulses of magmatism occurred. Large concentrations of dykes are referred to as dyke swarms; these can extend for tens to hundreds of kilometres and are important markers of past extensional stress fields. Classic localities where dense networks of igneous dykes are exposed include parts of the British Isles such as the Isle of Arran, and similar patterns are found in many continental flood basalt provinces.

Uses, examples and planetary occurrences

Dykes are of interest beyond simple mapping: they can act as conduits for mineral-bearing fluids and sometimes localize ore deposits, influence permeability in hydrogeology and geothermal systems, and provide insights into the stress state of the crust at the time of emplacement. Dykes and dyke swarms have been recognized on other planetary bodies as well, indicating that comparable fracturing and intrusive processes have occurred on the Moon, Mars and elsewhere.

Notable facts and field recognition

  1. Dykes often display a clear crosscutting relationship against host rocks and therefore are useful in establishing relative ages of geological events, including in Palaeozoic successions.
  2. Textures such as chilled margins, vesicles, and mineral layering help distinguish igneous dykes from later sedimentary fills or tectonic features.
  3. Field examples and regional studies show that many magmatic systems produce networks of both vertical dykes and horizontal sills during different stages of an eruption or intrusion cycle.

Overall, dykes are fundamental components of the crustal plumbing system: records of magmatic activity, crustal stress, and fluid flow that are valuable to petrologists, structural geologists and economic geologists alike.