
University of Queensland researchers have identified a chemical signature in tiny plagioclase crystals that signals when magma is ready to erupt.
PhD candidate Daniela Parra- Encalada (School of the Environment) and senior author Associate Professor Teresa Ubide led the work, published in Nature Communications.
They studied plagioclase, a common white mineral that grows in magma a few kilometres below the surface and responds to changes in temperature, water content, and composition, from Andean volcanoes in Chile and Argentina (across a ~230 km stretch) spanning different ages, eruptive styles, and activity levels.
Key findings
- The smallest, newest crystals (microcrysts, roughly the width of a human hair) that form in the final stages before eruption share a consistent chemical signature across the studied volcanoes and other Pacific Ring of Fire datasets.
- Modelling links this signature to hot, deeper magma injecting into a shallower reservoir. This destabilises the volcanic plumbing system and can trigger eruption.
- The team named the geochemical pattern the “plagioclase eruptibility field”.
- Earlier-formed plagioclase with lower calcium content often records non-eruptible magma that is cooling and accumulating in the crust (relevant for metal enrichment, such as copper and gold, and only rarely involved in super-eruptions).
Researchers analysed thin sections of 28 representative rocks from seven volcanoes plus two ancient super- eruptions using microscopy and laser-based chemical mapping. Similar microcryst signatures appear more widely around the Ring of Fire, pointing to a common triggering process.
This crystal “fingerprint” could help identify volcanoes (including seemingly quiet ones) that merit closer monitoring because their magma systems show signs of eruptibility. Future work will test whether the pattern holds in oceanic volcanoes and explore links to critical-mineral accumulation.
Plagioclase acts like a recorder of a volcano’s recent history because its composition and zoning (growth layers) change with magmatic conditions.
Focusing on the tiniest crystals isolates the final pre- eruption stage more clearly than bulk- rock chemistry.

Magma crystallization is the process by which molten rock (magma) cools and solidifies into solid minerals (crystals), eventually forming igneous rock.
1. What is magma?
Magma is a hot, mobile mixture of:
- Liquid silicate melt (the dominant component)
- Suspended crystals
- Dissolved gases (mainly water vapor, CO₂, sulfur gases)
- Sometimes solid rock fragments
Temperatures typically range from ~700 °C (rhyolitic, silicic magma) to >1200 °C (basaltic and mafic magma).
2. How crystallization begins
Crystallization starts when the temperature drops below the liquidus (the temperature at which the first crystals begin to form). As cooling continues, the magma moves toward the solidus (the temperature at which it becomes completely solid).
The process involves two main stages:
- Nucleation: Tiny clusters of atoms arrange into stable crystal “seeds.”
- Crystal growth: Atoms attach to these seeds, causing crystals to enlarge.
3. Sequence of crystallization (Bowen’s Reaction Series)
Minerals do not all form at once. They crystallize in a predictable order based on temperature and composition:
Discontinuous series (mafic minerals):
Olivine → Pyroxene → Amphibole → Biotite mica
Continuous series (plagioclase feldspar):
Calcium- rich plagioclase (high anorthite, An-rich) → progressively more sodium -rich plagioclase (lower An)
Later- forming minerals (lower temperature):
Potassium feldspar, muscovite mica, and quartz.
This is why volcanic rocks often contain a mix of early- formed (larger, sometimes resorbed) crystals and late- formed microcrysts.
4. Key factors that control crystallization
- Cooling rate: Slow cooling (deep underground) produces large crystals (phaneritic texture, e.g., granite). Fast cooling (eruption at the surface) produces small crystals or glass (aphanitic or glassy texture, e.g., basalt or obsidian).
- Composition: Higher silica content raises viscosity and lowers crystallization temperature.
- Pressure: Higher pressure generally raises melting points; decompression can trigger crystallization.
- Water and volatiles: Dissolved water lowers the melting temperature and can suppress or promote certain minerals (e.g., plagioclase stability expands as magma degasses near the surface).
- Magma mixing and recharge: Injection of hotter, more mafic magma can dissolve existing crystals or cause new ones to grow with different compositions (producing zoning).
5. Crystal zoning and records of history
Crystals often grow in layers (like tree rings). Changes in temperature, pressure, water content, or melt composition produce compositional zoning.
In plagioclase, for example, the anorthite (Ca) content decreases as the melt evolves or increases when hotter mafic magma recharges the system. These zones preserve a detailed timeline of magma conditions, exactly the “crystal records” used in the recent research on eruptibility.
6. Final outcomes
- If magma fully crystallizes underground → intrusive (plutonic) rock.
- If it erupts before full crystallization → volcanic (extrusive) rock containing a mixture of phenocrysts (early crystals), microcrysts (late crystals formed during ascent), and groundmass (fine crystals or glass).
In short, magma crystallization is a progressive, temperature- and composition- driven process that turns liquid melt into a solid crystalline rock, while recording the physical and chemical history of the magma system in the crystals themselves.
Crystal records of erupted vs. trapped magma in volcanic arcs
Arc andesites form by mixing of mafic and silicic magmas. The silicic end-member is hard to constrain because it is underrepresented in erupted products.
Using textural, elemental, and isotopic records in plagioclase, the authors distinguish trapped crystal mush from erupted magma. They define the plagioclase eruptibility field, a narrow, recurrent anorthite range (An ≈ 61), that marks the melt that actually erupts across Central Andes volcanoes after mafic recharge.
Recycled plagioclase cargo is dominated by lower- An compositions (An ≈ 43), recording prolonged crystallisation and assimilation in silicic mushes.
The same pattern appears in continental and composite arcs globally, indicating strong eruptive filtering: most felsic and mafic mushes remain dormant and contribute to crustal growth, though felsic mushes can occasionally remobilise to produce super- eruptions.
Key findings
- Samples: 28 fresh lava and tephra samples from a ~230 km transect in the Central Andes (main-arc and back-arc settings). Includes polygenetic stratovolcanoes (Lascar, Socompa, Tuzgle), monogenetic centres (El Negrillar, Cerro Overo, Back-Arc Monogenetic Volcanism fields), and older flare-up ignimbrites.
- Plagioclase populations:
- Microcrysts (small crystals formed from the final erupted melt during ascent/degassing) and phenocryst rims cluster tightly around An 61 ± 7 (labradorite). This is the “plagioclase eruptibility field.”
- These crystals also show elevated Mg and Fe, consistent with rapid growth from relatively mafic, recharged melt.
- The broader crystal cargo (cores, mantles, mush fragments, lithics) is dominated by lower-An plagioclase (average ~An 43- 45), recording silicic (rhyolitic) mushes that largely remain trapped.
- Interpretation: Mafic recharge into shallow reservoirs homogenises and mobilises intermediate (andesitic) melt that can erupt. The eruptibility field is remarkably consistent across volcano ages, styles (effusive/explosive), and tectonic settings in the study area and appears in other arc datasets.
- Trapped vs. erupted: Most of the crystal cargo records non-eruptible (or rarely eruptible) felsic mush that contributes to crustal growth and can host metal enrichment. Only under special conditions (e.g., flare-ups) do these mushes remobilise for large eruptions.
- Supporting data include EPMA, LA -Q- ICP- MS elemental mapping, Sr- isotope analyses, and thermodynamic modelling of equilibrium melts.
Broader implications
The plagioclase eruptibility field offers a petrographic and geochemical indicator of magma that is primed for eruption. It helps explain the prevalence of andesites in arcs (selective filtering of intermediate compositions) and highlights the large volume of unerupted mush.
Future work may test the pattern in oceanic arcs and explore links to critical-metal accumulation in trapped mushes.
The full paper (open access) includes detailed figures of crystal textures, compositional distributions, elemental maps, and global comparisons. A PDF download is available on the Nature page.
Journal: Nature Communications, volume 17, Article number: 11203 (2026)
DOI: 10.1038/s41467-026-78932-9
Provided: University of Queensland
Published: 09 November 2026
Authors: Daniela Parra-Encalada,
Teresa Ubide,
Gideon Rosenbaum,
Yujin Jegal,
Patricia Larrea,
Emilce Bustos &
Catharine Wang
Abstract
Arc andesites are hybrids generated by mixing of mafic and silicic magmas. The silicic endmember can contribute to crustal growth or trigger explosive eruptions, yet remains difficult to constrain due to limited representation in the erupted record. Here, we show that textural, elemental and isotopic records preserved in plagioclase can distinguish between trapped and erupted crystal mush, thus constraining conditions of magma storage vs. eruption in arc systems. We define the plagioclase eruptibility field, a narrow and recurrent anorthite range (An~61) that represents erupted melt across Central Andes volcanoes upon mafic recharge. The recycled plagioclase cargo is dominantly An~43, recording prolonged crystallisation and assimilation within silicic mushes. This pattern repeats in continental and composite arcs globally, indicating strong eruptive filtering of arc magmas and widespread occurrence of dormant felsic and mafic mushes that, in most cases, contribute to crustal growth; yet exceptionally, felsic mushes can rapidly remobilise to generate super-eruptions.




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