Well, hotter than they should be, for being so far from the sun. In a process called tidal heating, gravitational tugs from Jupiterâs moons and the planet itself stretch and squish the moons enough to warm them. As a result, some of the icy moons contain interiors warm enough to host oceans of liquid water, and in the case of the rocky moon Io, tidal heating melts rock into magma.
Researchers previously believed that the gas giant Jupiter was responsible for most of the tidal heating associated with the liquid interiors of the moons, but a new study published in Geophysical Research Letters found that moon-moon interactions may be more responsible for the heating than Jupiter alone.
âItâs surprising because the moons are so much smaller than Jupiter. You wouldnât expect them to be able to create such a large tidal response,â said the paperâs lead author Hamish Hay, a postdoctoral fellow at the Jet Propulsion Laboratory in Pasadena, California, who did the research when he was a graduate student in the University of Arizona Lunar and Planetary Laboratory.
Understanding how the moons influence each other is important because it can shed light on the evolution of the moon system as a whole. Jupiter has nearly 80 moons, the four largest of which are Io, Europe, Ganymede and Callisto.
âMaintaining subsurface oceans against freezing over geological times requires a fine balance between internal heating and heat loss, and yet we have several pieces of evidence that Europa, Ganymede, Callisto and other moons should be ocean worlds,â said co-author Antony Trinh, a postdoctoral research fellow in the Lunar and Planetary Lab. âIo, the moon closest to Jupiter, shows widespread volcanic activity, another consequence of tidal heating, but at a higher intensity likely experienced by other terrestrial planets, like Earth, in their early history. Ultimately, we want to understand the source of all this heat, both for its influence on the evolution and habitability of the many worlds across the solar system and beyond.â
âResonance creates loads more heating,â Hay said. âBasically, if you push any object or system and let go, it will wobble at its own natural frequency. If you keep on pushing the system at the right frequency, those oscillations get bigger and bigger, just like when youâre pushing a swing. If you push the swing at the right time, it goes higher, but get the timing wrong and the swingâs motion is dampened.â
âThese tidal resonances were known before this work, but only known for tides due to Jupiter, which can only create this resonance effect if the ocean is really thin (less than 300 meters or under 1,000 feet), which is unlikely,â Hay said. âWhen tidal forces act on a global ocean, it creates a tidal wave on the surface that ends up propagating around the equator with a certain frequency, or period.â
According to the researchers’ model, Jupiterâs influence alone canât create tides with the right frequency to resonate with the moons because the moons’ oceans are thought to be too thick. Itâs only when the researchers added in the gravitational influence of the other moons that they started to see tidal forces approaching the natural frequencies of the moons.
When the tides generated by other objects in Jupiterâs moon system match each moonâs own resonant frequency, the moon begins to experience more heating than that due to tides raised by Jupiter alone, and in the most extreme cases, this could result in the melting of ice or rock internally.
For moons to experience tidal resonance, their oceans must be tens to hundreds of kilometers â at most a few hundred miles â thick, which is in range of scientists’ current estimates. However, there are some caveats to the researchers’ findings.
Their model assumes that tidal resonances never get too extreme, Hay said. He and his team want to return to this variable in the model and see what happens when they lift that constraint.
Hay also is hoping that future studies will be able to infer the true depth of the oceans within these moons.
Natural satellite, Jupiter, Moon, Galilean moons, Tidal heating of Io, Europe
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