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NASAscientists have revealed the closed book of the most volcanic consistence in oursolar organization , according to fresh inquiry . The uncovering clear a 44 - class - honest-to-goodness mystery of why , and how , Jupiter ’s violent moon , Io , became so volcanically active .

Io is only somewhat heavy than our moonlight , with a diam of 2,237 mile ( 3,600 kilometers ) , and has anestimated 400 volcanoes , fit in toNASA.Plumes from these volcano ' eruption can stretch for miles out into blank space , and can even be seen from Earth when viewed through large scope .

Image shows the north polar region of Jupiter’s volcanic moon Io as captured by NASA’s Juno during the spacecraft’s 57th close pass of the gas giant on Dec. 30, 2023.

Jupiter’s moon Io is the most volcanically active world in our solar system. But the reason for this activity has left astronomers scratching their heads.

This dramatic volcanism was first identified in 1979 by scientist Linda Morabito , then at NASA ’s Jet Propulsion - Laboratory , inan imagetaken byNASA ’s Voyager 1 ballistic capsule .

" Since Morabito ’s discovery , planetary scientist have wondered how the volcanoes were feed from the lava underneath the surface,“Scott Bolton , principal research worker for NASA ’s Juno space vehicle from the Southwest Research Institute in San Antonio , said in astatement . " Was there a shallow sea of white - hot magma fueling the volcano , or was their generator more localize ? "

TheJuno space vehicle , which was launched in 2011 to learn Jupiter and the moons that orbit it , made two very tight flybys of Io in 2023 and 2024 , approach within 930 miles ( 1,500 km ) of its bubble surface . " We knew datum from Juno ’s two very close flybys could give us some insights on how this tortured moonshine actually worked , " Bolton said .

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During these approaches , the spacecraft collected data point that grant scientists to value Io ’s sobriety .

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Io orbits close to Jupiter at an average aloofness of 262,000 miles ( 422,000 km ) , completing its oval-shaped round once every 42.5 hour . Due to the shape of its eye socket , the moon ’s distance from its parent planet alter , and so too does Jupiter ’s gravitational pull . This means the moonlight is ceaselessly being shove and released like a stress globe in a process known as tidal flexing .

a close-up of a storm on Jupiter�s surface

" This never-ending flexing creates Brobdingnagian energy [ in the form of warmth , ] which literally fade portions of Io ’s interior , " Bolton said .

In the past times , it was thought that , because of this flexing , Io ’s interior might be home to a big magma ocean , stretch out beneath its entire Earth’s surface like a layer of tiramisu . However , enquiry lead by Bolton , publish Dec. 12 in the journalNature , suggest that this is not the case .

" If Io has a globose magma sea , we bed the signature of its tidal contortion would be much prominent than a more rigid , mostly solid interior , " Bolton said .

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a picture of the Cerro Uturuncu volcano

Instead , the squad ’s information suggested that Jupiter ’s volcanic lunar month has a mostly strong interior , with each of Io ’s volcanoes cause their own hush-hush chamber of roiling magma .

" Juno ’s discovery that tidal forces do not always create globular magma oceans does more than prompt us to rethink what we fuck about Io ’s inside , " survey lead authorRyan Park , a Juno co - research worker and supervisory program of the Solar System Dynamics Group at NASA ’s Jet Propulsion Laboratory , suppose in the affirmation .

The survey findings have implications for Jupiter ’s moonEuropaand Saturn ’s moonEnceladus , as well exoplanets beyond our solar organisation . " Our new findings render an opportunity to rethink what we know about planetary formation and phylogenesis , " Park said .

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