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Juno measured Io’s hidden heat for the first time, rising over 20 C within metres

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NASA’s Juno spacecraft made the first spatially resolved measurement of heat rising from roughly 2-6 metres below the surface of Jupiter’s moon Io.

Temperature increased by more than 20 C within the upper few metres, but the data still allow two explanations: broad conductive heat flow or scattered shallow lava and hot vents.

A Jupiter instrument looked under a rocky moon

Juno’s Microwave Radiometer was built to see below Jupiter’s thick clouds. During Io flybys in December 2023 and February 2024, it measured thermal emission from 0.6 to 22 GHz.

Lower frequencies probe deeper than infrared surface measurements. The lowest-frequency channels sampled roughly 2-6 metres below the surface.

A steep shallow temperature rise

Across the observed regions, the study found a temperature increase greater than 20 C within the upper few metres, a signal too steep to explain with sunlight alone.

The inferred density of the upper layer, below about 10 cm, was 0.7-1.1 g/cm3. That is consistent with a broad cover of porous volcanic material such as ash or pumice.

Produced image showing Juno sending microwaves into Io's shallow subsurface to measure heat
Produced image: ONEPRESS illustrates Juno’s microwave observations and Io’s shallow thermal structure. It is not an actual observation or measured geological cross-section.

Two ways the heat could rise

One model has internal heat moving steadily through a conductive crust at 1-3 W/m2. The other uses relatively fresh lava under five years old, or hot vents below thin crust, scattered across about 10% of the surface.

The present observations do not choose conclusively between them.

A first measurement, not a buried thermometer

This is a remote inference from microwave brightness temperature and dielectric properties, not a lander thermometer. Two flybys did not cover every region of Io.

Applying the technique to Earth volcano monitoring is also a proposal, not demonstrated eruption forecasting.

Why it matters

The result moves beyond surface infrared views and directly constrains how heat travels inside the most volcanically active world in the Solar System. Similar observations could probe shallow layers on other rocky and icy moons.

Official Primary Sources

Journal of Geophysical Research: Planets original study

NASA JPL: Juno takes Io’s temperature

NASA JPL subsurface heat map