{"id":823328,"date":"2026-07-25T17:22:08","date_gmt":"2026-07-25T17:22:08","guid":{"rendered":"https:\/\/www.newsbeep.com\/au\/823328\/"},"modified":"2026-07-25T17:22:08","modified_gmt":"2026-07-25T17:22:08","slug":"jupiters-volcanic-moon-io-hides-intense-heat-beneath-its-porous-crust","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/au\/823328\/","title":{"rendered":"Jupiter\u2019s volcanic moon, Io, hides intense heat beneath its porous crust"},"content":{"rendered":"

NASA\u2019s Juno spacecraft<\/a> measured heat below Io\u2019s surface for the first time and found temperatures rise sharply just a few feet underground.Io\u2019s surface appears surprisingly smooth and covered in lightweight, porous material similar to pumice or fluffy volcanic ash.The findings may help scientists understand how heat moves through volcanic worlds, including Io, other moons, and possibly volcanoes on Earth.<\/p>\n

Io\u2019s surface may look like a frozen snapshot of volcanic chaos, but just a few feet below, the temperature rises sharply. NASA\u2019s Juno spacecraft has now measured that hidden heat directly, exposing how energy moves through Jupiter\u2019s most volcanic moon.<\/p>\n

The readings came from Juno\u2019s Microwave Radiometer during close flybys on Dec. 30, 2023, and Feb. 3, 2024. The spacecraft passed within about 930 miles of Io\u2019s surface both times.<\/p>\n

Published in the Journal of Geophysical Research: Planets<\/a>, the work marks the first direct measurement of thermal emission from beneath Io\u2019s surface. It also points to a landscape that is smoother and less dense than its rugged mountains suggest.<\/p>\n

\u201cThe Juno Microwave Radiometer directly observed Io\u2019s heat output by looking below the surface,\u201d said Scott Bolton, study coauthor and Juno\u2019s principal investigator at Southwest Research Institute<\/a> in San Antonio. \u201cThe surprising discovery that we could see below a rocky moon\u2019s surface has important implications for studying Earth\u2019s volcanoes.\u201d<\/p>\n

This graphic illustrates the areas of Io sampled by the Microwave Radiometer instrument aboard NASA\u2019s Juno spacecraft during two close flybys of the Jovian moon. (CREDIT: NASA\/JPL-Caltech\/SwRI\/USGS) Heat rising beneath a thin surface<\/p>\n

Io\u2019s volcanic activity comes from tidal heating. Jupiter\u2019s gravity repeatedly stretches and squeezes the moon as it follows a slightly elliptical orbit. That deformation generates immense internal heat.<\/p>\n

Earlier infrared observations measured only the uppermost surface. Juno\u2019s radiometer instead sampled microwave emission from depths ranging from a few inches to tens of feet.<\/p>\n

\u201cThe instrument measured Io\u2019s thermal emission at depths ranging from a few inches down to tens of feet,\u201d said lead author Shannon Brown of NASA\u2019s Jet Propulsion Laboratory<\/a>. \u201cEverywhere we looked, we found the temperature rising by more than 40 degrees Fahrenheit just several feet into the surface.\u201d<\/p>\n

Solar heating alone cannot explain that steep increase.<\/p>\n

The team considered two possible explanations. Heat may be moving steadily upward through a conductive crust. Under that model, the local heat flow measures about 1 to 3 watts per square meter.<\/p>\n

This map represents data captured by the Microwave Radiometer instrument aboard NASA\u2019s Juno, indicating heat rising from just beneath the surface of Jupiter\u2019s moon Io. The colors illustrate a distinct temperature gradient across the moon, with the most extreme, localized heat output in red. (CREDIT: NASA\/JPL-Caltech\/SwRI\/USGS) <\/p>\n

That sounds modest, roughly comparable to a small nightlight beneath each square yard. Across Io, however, it represents energy release up to 30 times Earth\u2019s average surface heat flow.<\/p>\n

A second possibility involves recent lava flows. About 10 percent of Io\u2019s surface may be covered at any time by cooling flows capped with roughly 30 to 35 feet of solidified crust.<\/p>\n

A microwave view of a rocky moon<\/p>\n

Juno\u2019s Microwave Radiometer was built to probe beneath Jupiter\u2019s clouds<\/a>. Its six antennas detect wavelengths from about half an inch to 20 inches, allowing each channel to sample a different depth.<\/p>\n

The instrument later observed Ganymede, Europa and Io during Juno\u2019s extended mission. At the icy moons, it probed tens of miles beneath the surface under assumptions about mostly pure water ice.<\/p>\n

Io presented a different challenge. Its surface contains volcanic rock, sulfur compounds and porous material. The team did not expect microwave signals to penetrate so effectively.<\/p>\n

MWR sampling and footprints on Io for PJ57 (black) and PJ58 (blue) for the 12\u00b0 beams. (CREDIT: Scott Bolton et. al, JGR Planets) <\/p>\n

\u201cThe technique is novel in that each wavelength explores different depths,\u201d Bolton said. \u201cAt Ganymede<\/a> and Europa, we explored tens of miles below the surface, assuming their ice shells were mostly pure water, but the ability to probe into the volcanic rock at Io was an unexpected discovery.\u201d<\/p>\n

The radiometer recorded a strong increase in brightness temperature at the lowest frequencies, which penetrate deepest. That pattern indicates warmer material below a cooler near-surface layer.<\/p>\n

The deepest channel sensed the upper several meters, with some signal coming from the upper tens of meters. The shallower channels showed weaker temperature changes.<\/p>\n

Io\u2019s plains look smoother than expected<\/p>\n

The flybys also revealed unusual surface properties.<\/p>\n

Io is known for mountains taller than 6 miles, yet most areas away from that topography reflected microwaves like a smooth surface. Some smooth regions may extend for 60 miles or more.<\/p>\n

Juno observed overlapping areas from different angles. The changing reflection pattern allowed the team to distinguish between a rough surface, which scatters radiation broadly, and a smooth one, which reflects it in favored directions.<\/p>\n

MWR brightness temperatures projected over the 3 dB footprint onto Io’s surface for PJ57 (top) and PJ58 (bottom). (CREDIT: Scott Bolton et. al, JGR Planets) <\/p>\n

The result favored mostly specular reflection, similar to the way sunlight flashes from an ocean or polished land surface at certain angles.<\/p>\n

\u201cAway from its mountains, the surface is more like the Great Plains of North America,\u201d Brown said. \u201cAnd even though Io is a rocky body, the surface material has a very low density, more like pumice or a fluffy volcanic ash than solid rock.\u201d<\/p>\n

The inferred density ranges from about 0.7 to 1.1 grams per cubic centimeter. That is consistent with porous volcanic ash<\/a>, pumice or scoria rather than dense rock.<\/p>\n

The upper layer may also sit above denser material several meters down. Lower microwave frequencies appeared to encounter a higher effective dielectric constant, which the team interpreted as a possible sign of increasing density with depth.<\/p>\n

Practical implications of the research<\/p>\n

These measurements give scientists a new way to study how heat escapes from a world shaped by tidal forces. Until now, observations mainly tracked eruptions or heat leaving the visible surface.<\/p>\n

Microwave measurements can instead follow the temperature gradient below that surface. They may help determine whether Io loses heat through broad conductive regions, repeated lava resurfacing, or both.<\/p>\n

\u201cIo provides a unique window into learning how tidal heating works throughout the cosmos,\u201d Bolton said. The same process also supplies energy to subsurface oceans on moons such as Europa<\/a> and Ganymede.<\/p>\n

The technique could guide future missions to rocky moons and ocean worlds. A higher-resolution radiometer with more frequencies and dual polarization could map heat flow and shallow structure in greater detail.<\/p>\n

The approach may also inform studies closer to home. Bolton said a similar instrument near an Earth volcano could detect subsurface temperature changes and provide new evidence about how volcanic systems move heat before it reaches the surface.<\/p>\n

Research findings are available online in the journal JGR Planets<\/a>.<\/p>\n

Related Stories<\/p>\n","protected":false},"excerpt":{"rendered":"NASA\u2019s Juno spacecraft measured heat below Io\u2019s surface for the first time and found temperatures rise sharply just…\n","protected":false},"author":2,"featured_media":823329,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[7],"tags":[64,63,397314,108263,17264,34842,397315,306788,397316,319364,2568,337,128,397317,397318,60678,109497,397319,129308,25643,397320],"class_list":["post-823328","post","type-post","status-publish","format-standard","has-post-thumbnail","category-science","tag-au","tag-australia","tag-heat-beneath-ios-surface","tag-io","tag-jupiter","tag-jupiter-moons","tag-microwave-radiometer","tag-nasa-jet-propulsion-laboratory","tag-nasa-juno-mission","tag-planetary-geology","tag-planetary-science","tag-research","tag-science","tag-scott-bolton","tag-shannon-brown","tag-southwest-research-institute","tag-space-news","tag-subsurface-heat","tag-tidal-heating","tag-volcanic-activity","tag-volcanic-moons"],"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/posts\/823328","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/comments?post=823328"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/posts\/823328\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/media\/823329"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/media?parent=823328"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/categories?post=823328"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/au\/wp-json\/wp\/v2\/tags?post=823328"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}