- Stage
- 000.0°
- Field
- —
- Light
- crossed polars
Slide 07 / 09 · Spherulitic obsidian
Lipari obsidian
The youngest rock in the tray: a flow of volcanic glass that ran down the north-east of Lipari some eight hundred years ago.
Glass has no crystal structure, so between crossed polars it is black. The spheres are spherulites: fans of feldspar and silica needles that crystallised radially in the cooling glass, strung along its flow bands. Like the ooids of Portland, each shows a fixed dark cross. In plane light, look for the curved perlitic cracks and the trains of tiny microlites that trace how the lava moved.
Under the microscope
What to look for
- 01 · crossed polars · ×4Spherulite crossesRadiating fibres: the cross stays aligned with the polarisers while the stage turns.
- 02 · plane light · ×10Perlitic cracksOnion-skin cracks in the glass, from contraction as it cooled and hydrated.
- 03 · tint plate · ×4Tint plateWith the gypsum plate in, opposite quadrants of each spherulite turn blue and yellow.
The whole section
Plane light | crossed polars
The same slice of rock with the analyser out and in. Drag the line.
Mode, by eye
What it is made of
| Mineral | Share | δ | Γ max at 30 µm | Strongest colour |
|---|---|---|---|---|
| volcanic glass | 70% | — | 0 nm | dark at every angle |
| spherulites | 27% | 0.008 | 240 nm | first-order grey–white |
| sanidine, microlites | 3% | 0.007 | 210 nm | first-order grey–white |
Γ (retardation) = thickness × birefringence δ. Swatches are computed by the same optics that draw the microscope.