Rock Identifier
Red Scoria (Vesicular Basaltic Andesite) — igneous
igneous

Red Scoria

Vesicular Basaltic Andesite

Hardness: 5-6 Mohs. Color: Reddish-brown to dark red. Luster: Dull/Earthy. Structure: Highly vesicular (pitted with air bubbles). Specific Gravity: Approximately 1.5-2.0 (relatively lightweight due to vesicles).

Hardness
5-6 Mohs
Color
Reddish-brown to dark red
Luster
Dull/Earthy
Identified More igneous
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Physical properties

Hardness: 5-6 Mohs. Color: Reddish-brown to dark red. Luster: Dull/Earthy. Structure: Highly vesicular (pitted with air bubbles). Specific Gravity: Approximately 1.5-2.0 (relatively lightweight due to vesicles).

Formation & geological history

Formed from cooling lava that was rich in dissolved gases. As the magma reaches the surface, gases expand and form bubbles (vesicles) while the rock solidifies. Red coloration is caused by the oxidation of iron-bearing minerals (magnetite or olivine) during or after the eruption.

Uses & applications

Landscaping, drainage systems, gas grills, high-temperature insulation, and lightweight aggregate in concrete construction.

Geological facts

Scoria is similar to pumice but is denser and has larger vesicles. While pumice can often float on water, scoria usually sinks because its vesical walls are thicker and more mineral-rich.

Field identification & locations

Identified by its high porosity, rough abrasive texture, and many visible holes. It is commonly found in volcanic regions, cinder cones, and near the vents of basaltic volcanoes. Its red color is a key indicator of high iron oxidation.