But data from NASA’s Galileo spacecraft in the 1990s revealed Callisto may have a secret: a salty ocean beneath its surface. In the past, some scientists thought of Callisto as a boring “ugly duckling moon” and a “hunk of rock and ice.” That’s because the crater-covered world didn’t seem to have much going on-no active volcanoes or shifting tectonic plates. This study was funded by NASA’s Habitable Worlds program.Callisto is Jupiter’s second largest moon and the third largest moon in our solar system. Hay, Antony Trinh and Isamu Matsuyama, 19 July 2020, Geophysical Research Letters. Reference: “Powering the Galilean Satellites with Moon‐Moon Tides” by Hamish C. Hay also is hoping that future studies will be able to infer the true depth of the oceans within these moons. He and his team want to return to this variable in the model and see what happens when they lift that constraint. Their model assumes that tidal resonances never get too extreme, Hay said. However, there are some caveats to the researchers’ findings. When the tides generated by other objects in Jupiter’s moon system match each moon’s 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.įor moons to experience tidal resonance, their oceans must be tens to hundreds of kilometers – at most a few hundred miles – thick, which is in range of scientists’ current estimates. It’s 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 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.”Īccording to the researchers’ model, Jupiter’s influence alone can’t create tides with the right frequency to resonate with the moons because the moons’ oceans are thought to be too thick. “These 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,” Hay said. If you push the swing at the right time, it goes higher, but get the timing wrong and the swing’s motion is dampened.”Įach moon’s natural frequency depends on the depth of its ocean. ![]() If you keep on pushing the system at the right frequency, those oscillations get bigger and bigger, just like when you’re pushing a swing. “Basically, if you push any object or system and let go, it will wobble at its own natural frequency. “Resonance creates loads more heating,” Hay said. ![]() The trick to tidal heating is a phenomenon called tidal resonance. 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.” Tidal Resonance “Maintaining 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,” said co-author Antony Trinh, a postdoctoral research fellow in the Lunar and Planetary Lab. “Io, the Galilean 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. Jupiter has nearly 80 moons, the four largest of which are Io, Europa, Ganymede and Callisto. ![]() Understanding how the moons influence each other is important because it can shed light on the evolution of the moon system as a whole. You wouldn’t expect them to be able to create such a large tidal response,” said the paper’s 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. “It’s surprising because the moons are so much smaller than Jupiter. 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.
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