Mercury Surface Discovery Suggests A Far More Violent And Hotter Volcanic History
Astronomy

Mercury Surface Discovery Suggests A Far More Violent And Hotter Volcanic History

New infrared analysis reveals Mercury’s surface has far less silicon dioxide than previously thought, pointing to a much more intense volcanic history.

By Aisha Ahmed
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Mercury 3 Scaled

New analytical data suggests that the surface of Mercury is significantly less rich in silicon dioxide than scientists previously estimated. By refining how researchers interpret infrared signatures from planetary surfaces, a team has determined that silica makes up roughly 37% of the planet’s crust by mass—a reduction of up to 25% compared to earlier models.

The findings, detailed in the journal Planetary Research, offer a fresh perspective on the solar system’s smallest planet. Because silicon dioxide serves as a fundamental marker for identifying volcanic rock types and understanding crustal evolution, this shift in the data implies that Mercury’s interior may have undergone far more intense, deep-seated melting than previously hypothesized.

Three steps to Mercury. Step 1: Using laboratory measurements, the researchers established a relationship between infrared radiation and SiO2 content. Step 2: They verified this relationship using measurement data from the Moon and lunar samples. Step 3: Using infrared data from Mercury, the researchers were then able to determine the SiO2 content of Mercury’s surface.
Three steps to Mercury. Step 1: Using laboratory measurements, the researchers established a relationship between infrared radiation and SiO2 content. Step 2: They verified this relationship using measurement data from the Moon and lunar samples. Finally, Step 3: Using infrared data from Mercury, the researchers were then able to determine the SiO2 content of Mercury’s surface. (CREDIT: MPS / hormesdesign.de)

Reinterpreting the Hermean Crust

Led by experts from the Max Planck Institute for Solar System Research, the University of Münster, and the University of Göttingen, the research team focused on the “Christiansen Feature,” a specific mid-infrared spectral signal that shifts based on the mineral composition of a surface. By synthesizing laboratory glass beads with silica concentrations ranging from 0.5% to 97.6%, the scientists created a robust calibration scale to better translate remote infrared observations into chemical abundances.

Christian Renggli, lead author and director of the Experimental Laboratory Magma Ocean, noted that lower silica levels typically suggest that volcanic activity originated from deeper within the mantle. Alternatively, the results could point to a highly unusual chemical environment on Mercury where silicon exists in metallic or carbide forms, rather than being fully oxidized into SiO2.

To validate their methodology, the team applied their calibration to lunar data collected by NASA’s Lunar Reconnaissance Orbiter. By comparing their findings against physical rock samples retrieved during the Apollo, Luna, and Chang’e missions, the researchers confirmed their technique could reliably reconstruct the surface chemistry of worlds where direct sampling remains impossible.

First global map of the SiO2 content on the Moon’s surface. The white, labeled dots show the landing sites from which the Apollo, Luna, and Chang’e missions brought lunar samples back to Earth. The samples made it possible to verify the accuracy of the map.
First global map of the SiO2 content on the Moon’s surface. The white, labeled dots show the landing sites from which the Apollo, Luna, and Chang’e missions brought lunar samples back to Earth. The samples made it possible to verify the accuracy of the map. (CREDIT: Renggli et al.: Planetary Research (2026))

Preparing for BepiColombo

Previous estimates for Mercury’s silica content were largely derived from elemental ratios observed by the MESSENGER spacecraft, which often required complex assumptions about mineralogy. This new infrared-based approach provides an independent check that places the planet’s composition well below the previously accepted range of 49% to 60%.

This discrepancy is expected to be settled by the BepiColombo mission, a joint effort between the European Space Agency and the Japan Aerospace Exploration Agency. Currently on its approach to the planet, the mission is scheduled to enter orbit in late 2026, with full-scale scientific investigations slated for 2027.

One primary tool on the mission, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS), is specifically designed to analyze the 7-to-14-micrometer wavelength range. This allows the instrument to isolate the Christiansen Feature with unprecedented precision. According to Renggli, this new research provides the essential framework for interpreting the high-resolution data that will soon emerge from the MERTIS instrument, potentially clarifying why Mercury followed such a unique evolutionary path compared to its rocky neighbors.

The CF position in µm as a function of the SiO2 wt.% concentration in the glasses. Grey circles represent literature data. The black line with a grey error envelope represents the best fit second-order polynomial through all data including our new synthetic glasses and the literature values.
The CF position in µm as a function of the SiO2 wt.% concentration in the glasses. Grey circles represent literature data. The black line with a grey error envelope represents the best fit second-order polynomial through all data including our new synthetic glasses and the literature values. (CREDIT: Christian Renggli et al, Planetary Research)
Calculated SiO2 concentration map over the central mare region with highly silicic localities identified by Glotch et al. (2010). These silicic domes and craters exhibit SiO2 concentrations of up to 76 wt.% at Lassell Massif.
Calculated SiO2 concentration map over the central mare region with highly silicic localities identified by Glotch et al. (2010). These silicic domes and craters exhibit SiO2 concentrations of up to 76 wt.% at Lassell Massif. (CREDIT: Christian Renggli et al, Planetary Research)

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Reference(s)

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Ahmed, Aisha. “Mercury Surface Discovery Suggests A Far More Violent And Hotter Volcanic History.” BioScience. BioScience ISSN 2521-5760, 29 August 2026. <https://www.bioscience.com.pk/en/subject/astronomy/mercurys-surface-chemistry-reveals-clues-to-a-much-hotter-volcanic-past>. Ahmed, A. (2026, August 29). “Mercury Surface Discovery Suggests A Far More Violent And Hotter Volcanic History.” BioScience. ISSN 2521-5760. Retrieved August 29, 2026 from https://www.bioscience.com.pk/en/subject/astronomy/mercurys-surface-chemistry-reveals-clues-to-a-much-hotter-volcanic-past Ahmed, Aisha. “Mercury Surface Discovery Suggests A Far More Violent And Hotter Volcanic History.” BioScience. ISSN 2521-5760. https://www.bioscience.com.pk/en/subject/astronomy/mercurys-surface-chemistry-reveals-clues-to-a-much-hotter-volcanic-past (accessed August 29, 2026).
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