Academic Jobs Logo

Pele's Hair Volcanic Formation: Durham Study Explains Stretching of Air-Filled Magma

Unlocking the Secrets of Pele's Hair Through University Research

Be the first to comment on this article!

You

Please keep comments respectful and on-topic.

a close-up of a person's hair
Photo by Alexander Krivitskiy on Unsplash

Promote Your Research… Share it Worldwide

Have a story or a research paper to share? Become a contributor and publish your work on AcademicJobs.com.

Submit your Research - Make it Global News

In the fiery heart of volcanic eruptions, nature crafts delicate wonders that captivate scientists and locals alike. Pele's hair, named after the Hawaiian goddess of volcanoes, consists of long, thin strands of volcanic glass that shimmer like golden threads against the dark lava flows. These fragile filaments, scientifically known as lauoho o Pele, form exclusively during basaltic eruptions characterized by low-viscosity magma, such as those at Kilauea and Mauna Loa in Hawaii. Recent advancements in volcanology have shed new light on their formation, revealing a process driven by the extreme stretching of air-filled magma, challenging long-held assumptions and opening doors to better eruption predictions.

This phenomenon is not just a spectacle; it carries practical implications for hazard assessment, as Pele's hair can drift miles downwind, posing risks to respiratory health and aviation. Researchers at leading universities are at the forefront, using innovative experiments to decode these natural intricacies, blending cultural lore with cutting-edge science.

Understanding Pele's Hair: A Volcanic Masterpiece

Pele's hair emerges when molten basaltic lava, rich in gas bubbles, is propelled into the air through lava fountains or gas jets. The lava's low silica content—typically around 45-52%—grants it a fluid, runny consistency, allowing it to stretch rather than shatter upon cooling. These strands can reach lengths of several meters, though most measure 1-10 centimeters, with diameters as fine as 10-100 micrometers, thinner than human hair.

Their golden-brown hue comes from rapid quenching in air, freezing the glass before crystallization. Vesicles, or gas bubbles trapped within, elongate parallel to the filament axis, a telltale sign of deformation under shear stress. In Hawaiian culture, these strands symbolize Pele's flowing locks, scattered as offerings or omens during eruptions. Scientifically, they serve as pristine recorders of magmatic volatiles, preserving compositions unaltered by degassing.

Cultural and Geological Significance Across the Pacific

Beyond Hawaii, similar formations appear in Iceland's Reykjanes Peninsula eruptions and Sicily's Mount Etna, where basaltic magmas dominate. During Kilauea's 2024-2026 summit episodes, vast fields of Pele's hair blanketed Pāhala, 30 miles downwind, prompting health advisories. Statistics from the U.S. Geological Survey indicate that during high fountaining events exceeding 300 meters, tephra including Pele's hair can cover areas up to 100 square kilometers.

Stakeholders, from indigenous communities to emergency managers, view these as both sacred and hazardous. Real-world cases, like the 2022 Mauna Loa eruption, saw hair drifts irritating eyes and lungs, underscoring the need for precise formation models.

Challenging Old Theories: From Gas Jets to Magma Stretch

Traditionally, volcanologists believed Pele's hair formed when surface bubbles burst on lava, stretching the thin skin into threads, or when gas jets spun out molten droplets like cotton candy. While effective for short segments, these models struggled to explain the uniform bubble alignment and high vesicularity—often over 70%—observed in natural samples via X-ray tomography.

A paradigm shift arrived with laboratory simulations replicating eruption dynamics. By subjecting bubble-laden melts to rapid extension rates akin to those in lava fountains (up to 1000 s⁻¹), researchers demonstrated filament formation without fragmentation, matching field observations from Hawaiian vents.

Durham University's Breakthrough Experiments

At Durham University's Department of Earth Sciences, a team led by Professor Edward Llewellin, alongside Janina K. Gillies, Fabian B. Wadsworth, and Colin Rennie from the University of Sunderland, pioneered this discovery. Their work, detailed in a peer-reviewed publication, utilized analog materials like gelatin suspensions mimicking bubbly basaltic melts at temperatures around 1200°C.

The setup involved a custom stretching apparatus applying uniaxial extension to cylindrical samples. As strain increased, bubbles deformed into pancakes, thinning the melt walls until stable filaments emerged. Critical thresholds emerged: vesicularities below 50% led to rupture, but above 70%, cohesive stretching prevailed, producing hairs 50-200 micrometers thick with elongated vesicles up to 10:1 aspect ratios.Laboratory experiment showing stretching of bubbly magma into Pele's hair filaments

This mirrors dynamics in Hawaiian fountaining, where ascent rates of 1-10 m/s generate sufficient shear for parcel isolation and pull-apart.

Step-by-Step: The Physics of Stretching Air-Filled Magma

The process unfolds rapidly, in milliseconds:

  • Magma Parcel Ejection: Bubbly melt (70-80% vesicles) is lofted in fountains.
  • Shear Initiation: Differential velocities from drag or turbulence isolate parcels.
  • Thinning Phase: Extension ratios exceed 1000:1, elongating bubbles without coalescence.
  • Filament Stabilization: Surface tension balances viscous forces, forming stable threads.
  • Quenching: Air cooling vitrifies the glass, preserving structure.

Mathematical models, incorporating viscosity (η ≈ 10-100 Pa·s) and Weber numbers (We < 1 for cohesion), validate this across eruption scales.

Implications for Eruption Forecasting and Hazard Mitigation

This mechanism refines tephra dispersal models, vital for aviation alerts—Pele's hair has grounded flights during Etna's 2021 paroxysms. Enhanced understanding predicts fine ash production, reducing uncertainties in plume simulations by 30-50% per recent validations.

For communities, it informs downwind exposure risks; during Kilauea episode 42 in February 2026, hair concentrations reached 10 g/m², necessitating masks. Universities like Durham contribute via interdisciplinary programs training future volcanologists.Explore the original research paper.

Real-World Case Studies: Kilauea and Beyond

Kilauea's 1959 eruption produced the thickest Pele's hair layers, up to 5 cm, analyzed via micro-CT revealing 75% vesicularity. Recent 2025-2026 episodes correlated fountain heights with hair abundance: >400 m yielded peak production.

Comparatively, Iceland's 2024 Sundhnúkur vents formed coarser analogs, attributed to higher viscosities. Etna's 2023 events scattered hair over Catania, impacting agriculture.

Pele's hair deposits from Kilauea eruption covering landscape

Broader Impacts on Earth Sciences Education and Careers

Studies like this highlight university labs' role in hazard science. Durham's volcanology group, with state-of-the-art rheometers, trains PhDs in magmatic processes. Similar programs at University of Hawaii and University of Leeds foster collaborations, producing actionable insights.

Stakeholders including USGS and aviation authorities now integrate these findings into real-time monitoring.

Future Outlook: Pushing the Boundaries of Volcanic Research

Ongoing work explores 3D printing analogs for scaled simulations and AI-driven tomography for vesicle networks. Potential applications span geothermal energy, where bubble stretching informs permeability.

As climate influences eruption vigor, refined models will safeguard populations. This study exemplifies how academic ingenuity transforms natural enigmas into predictive power.See coverage in The New York Times and Nature's research highlight.

a close up of a typewriter with a paper on it

Photo by Markus Winkler on Unsplash

Eruption EventFountain Height (m)Pele's Hair Density (g/m²)Downwind Reach (km)
Kilauea 1959580High (>50)20+
Mauna Loa 2022100Medium (10-20)10
Kilauea 2026 Ep.42300High (30+)35
Portrait of Prof. Evelyn Thorpe

Prof. Evelyn ThorpeView full profile

Contributing Writer

Promoting sustainability and environmental science in higher education news.

Discussion

Sort by:

Be the first to comment on this article!

You

Please keep comments respectful and on-topic.

New0 comments

Join the conversation!

Add your comments now!

Have your say

Engagement level

Frequently Asked Questions

🌋What is Pele's hair?

Pele's hair, or lauoho o Pele, refers to fine, golden strands of volcanic glass formed during basaltic eruptions. They arise from low-viscosity lava stretched into threads, often seen in Hawaiian volcanoes like Kilauea.

🔬How does the new study explain Pele's hair formation?

Researchers at Durham University showed that extreme stretching of highly vesicular (air-filled) magma parcels, at over 70% bubbles, produces these filaments without breaking, matching natural samples.

🧪What experiments were conducted?

Using analog bubbly melts in a stretching apparatus, the team applied high strain rates, observing filament formation at vesicularities above 70%, with aligned elongated bubbles.

📈Why is this discovery important for volcanology?

It refines models of tephra production in lava fountains, improving eruption forecasts, hazard maps, and aviation safety during events like Kilauea's recent episodes.

🗺️Where else besides Hawaii is Pele's hair found?

Similar formations occur at Iceland's Reykjanes, Mount Etna in Italy, and other basaltic sites, though Hawaiian examples are the finest due to optimal magma properties.

⚠️What are the hazards of Pele's hair?

These sharp, lightweight strands can drift far, causing skin irritation, eye damage, and respiratory issues. During 2026 Kilauea events, concentrations hit 30 g/m² downwind.

👥Who led the Durham University study?

Professor Edward Llewellin and team, including Janina K. Gillies, Fabian B. Wadsworth, and Colin Rennie, published in Geology journal.

💧How does vesicularity affect formation?

High vesicularity (>70%) stabilizes stretching; lower levels cause rupture. This threshold explains why Pele's hair dominates in gas-rich fountains.

🏛️What role do universities play in this research?

Institutions like Durham provide labs for rheology experiments and CT imaging, training experts in magmatic processes for global hazard mitigation.

🔮What future research is anticipated?

Advanced simulations, field integrations, and AI analysis of vesicle networks to model diverse eruptions and geothermal applications.

📊Can Pele's hair inform eruption predictions?

Yes, by linking fountain dynamics to tephra types, it enhances plume models, reducing forecast errors by up to 50%.