Juno meri temperaturo Jupiterjeve ognjene lune Io.

NASA's Juno spacecraft has gathered unprecedented data on the internal temperatures of Jupiter's moon Io, offering new insights into its volcanic activity and geological structure. During two close flybys, on December 30, 2023, and February 3, 2024—the spacecraft passed within approximately 930 miles (1,500 kilometers) of Io's surface, collecting measurements using its Microwave Radiometer (MWR) instrument. These readings reveal significant heating beneath the moon's surface, with temperature increases of over 40 degrees Fahrenheit occurring just a few feet below the surface. This finding challenges previous assumptions about how Io's heat is generated and distributed. The research, published in the Journal of Geophysical Research: Planets, marks the first time scientists have obtained direct measurements of subsurface temperatures on a rocky celestial body other than Earth. Io, known for being the most volcanically active object in the solar system, experiences intense internal heating due to tidal forces exerted by Jupiter. As Io orbits the gas giant, gravitational pull stretches and compresses the moon, creating friction and generating vast amounts of heat. Prior knowledge of this process relied almost entirely on infrared observations, which only detect surface temperatures. The MWR instrument, however, allows researchers to look deeper, peering through the moon's crust to uncover hidden thermal patterns. Scott Bolton, Juno's principal investigator at Southwest Research Institute in San Antonio, emphasized the significance of the findings. “The Juno Microwave Radiometer directly observed Io's heat output by looking below the surface,” he said. “The surprising discovery that we could see below a rocky moon's surface has important implications for studying Earth's volcanoes.” He noted that similar techniques used on Earth could yield new understanding of how terrestrial volcanoes function, particularly in regions where magma movement is difficult to observe directly. The MWR instrument, originally designed to study Jupiter's atmosphere, proved unexpectedly effective in probing Io's subsurface. It uses six microwave antennas operating at varying wavelengths, from about half an inch to 20 inches (1.3 to 51 centimeters), allowing it to explore different depths. While earlier missions focused on icy moons such as Ganymede and Europa, where the instruments probed tens of miles beneath the surface, the application of the same technology to Io revealed a completely different geological landscape. The data showed that Io's surface is relatively smooth and composed of materials with low density, suggesting a unique combination of volcanic and tectonic processes shaping its terrain. Shannon Brown, the lead author of the study from NASA's Jet Propulsion Laboratory in Southern California, explained that the temperature gradients detected by the MWR indicate a much more complex heat distribution mechanism than previously thought. “Everywhere we looked, we found the temperature rising by more than 40 degrees Fahrenheit just several feet into the surface, a gradient far steeper than solar heating alone can explain,” she said. This suggests that internal heat sources, rather than just surface-level phenomena, play a critical role in Io's geology. Scientists are considering multiple explanations for the observed thermal signatures. One possibility is that the heat originates from extensive lava flows or magma chambers located just beneath the surface. Another theory involves the interaction of Io's crust with volatile substances, such as sulfur dioxide or silicate minerals, which could alter the thermal properties of the moon's surface. Both hypotheses require further investigation, potentially involving additional flybys or complementary data from other space observatories. The findings from Juno's recent encounters with Io will likely influence future planetary science missions, especially those targeting other geologically active bodies in the solar system. Researchers hope to apply similar microwave radiometry techniques to study the interiors of moons like Enceladus or Titan, where subsurface oceans and potential habitability remain key scientific questions. For now, the data from Io provide a rare glimpse into the dynamic processes that shape some of the most extreme environments beyond Earth.