Citizen / General public
Researcher
Student / Future student
Company
Public partner
Journalist
Teacher / Pupil

A new machine learning model for predicting magma viscosity

A team of researchers led by Charles Le Losq (IPGP, IUF) has developed an innovative machine learning model capable of predicting the viscosity of magmas over a wide range of compositions, temperatures and pressures. This work represents a major advance in our understanding of magmatic processes, both on Earth and on exoplanets.

A new machine learning model for predicting magma viscosity

Molten magma on an exoplanet (generated by AI)

Publication date: 04/03/2025

Press, Research

An unprecedented database and a precise model

To train this model, the researchers compiled an exhaustive database containing almost 29,000 measurements of the viscosity of molten silicates, including high-pressure data up to 30 GPa. The model combines artificial neural networks with Gaussian processes, enabling accurate prediction of magma viscosity, even under extreme conditions such as those encountered on exoplanets.

Application to the exoplanet K2-141 b

By applying this model to the exoplanet K2-141 b, the team demonstrated the dominant role of temperature in controlling the viscosity of a magma ocean located on its diurnal surface. In addition, they determined that this planet probably has a thin atmosphere of rock vapour with a pressure of around 0.1 bar within a radius of 40° of the substellar point.
A notable result of the study is the interpretation of the night-time temperatures of K2-141 b. With values above 400 K, the researchers suggest the presence of a partially molten mantle beneath the surface, providing new insights into the internal structure and dynamics of lava planets.

An open-source library for the scientific community

The model developed is available in the form of an open-source Python library, gpvisc, enabling researchers around the world to explore the viscosity of magmas in various planetary and industrial contexts. This breakthrough opens up new perspectives for modelling magmatic processes and characterising rocky exoplanets.
This work was funded by the Labex UnivEarthS, ANR-10-LABX-0023 and ANR-18-IDEX-0001.

Publication link

Latest news
Discovery of a crustal lithosphere-asthenosphere boundary (LAB) topping a large magma reservoir at Axial volcano in the Eastern Pacific
Discovery of a crustal lithosphere-asthenosphere boundary (LAB) topping a large magma reservoir at Axial volcano in the Eastern Pacific
A team from the United States and Institut de physique du globe de Paris (IPGP) has imaged a crustal lithosphere-asthenosphere boundary (LAB) as the t...
The isotopic composition of oxygen in the solar system finally explained
The isotopic composition of oxygen in the solar system finally explained
A multidisciplinary team of French and British researchers—affiliated with the Institut de physique du globe de Paris (Université Paris Cité/IPGP/CNRS...
The rivers of titan: physical laws similar to those on earth
The rivers of titan: physical laws similar to those on earth
Researchers from the Institut de Physique du Globe de Paris (Université Paris Cité/CNRS/IPGP) have demonstrated for the first time that the rivers of ...
The Institute receives a precious sample of lunar basalt from the Chinese Chang'e-5 mission
The Institute receives a precious sample of lunar basalt from the Chinese Chang'e-5 mission
Frédéric Moynier has just been awarded a sample of lunar basalt collected by the Chinese Chang'e-5 mission, following an international call for propos...