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Cassini Image of Titan’s North Pole Showing Day and Night – Natural Color View from NASA. Image Credit: NASA/JPL
Updated on June 27, 2025 | By Jameswebb Discovery Editorial Team
Titan (Saturn) and Europa (Jupiter) are two of the most fascinating moons in our solar system, and both are being heavily researched. Now, imagine trying to predict the weather in a world where it rains liquid methane or where huge geysers shoot out of solid icy crusts above the surface, possibly even into space. That’s the kind of fun scientists are having right now.
Titan is the largest of all Saturn’s moons, and it has lakes, clouds, and even storms. Of course, the storms aren’t the kind we have here on Earth. Europa is one of Jupiter’s moons and, although it doesn’t really have an atmosphere, it has massive plumes of what might be water vapor that burst through cracks of its frozen surface. Both of these worlds are very extreme, very unpredictable, and very, very far away.
So, how do you even begin to forecast anything there? Well, you start on Earth because you have no other choice.
In this article, you’ll see how researchers used Earth’s weather data to simulate what might be happening on Titan and Europa, so read on.
When it comes to weather in our solar system (if you’re willing to stretch the definition of weather a little), Titan and Europa are the most exciting places to look at.
Titan has a thick nitrogen atmosphere (approx 95% nitrogen with a methane component), and its weather system is strange, to say the least – it’s built around methane instead of water. It’s freezing, with temperatures around -290°F, but there are still clouds, rain, and even lakes on the surface. Thanks to the Cassini-Huygens missions, we got a real look at this world and its seasons, storms, and atmospheric patterns that feel kind of familiar, just flipped on their head.
Note: seasons on Titan take about 7 Earth years to shift due to its 29.5-year solar orbit. That’s quite the long summer.
There’s no thick atmosphere on Europa, but it’s far from peaceful and quiet. There may be a salty ocean beneath its icy shell and, every now and then, plumes of water vapor seem to erupt through cracks in the ice. It seems to be something like cryovolcanic geysers.
The thing that makes moons so important is what they represent. With Titan, you get a glimpse of what early Earth might have looked like. Europa could teach us how subsurface oceans work on icy worlds. Unfortunately, we can’t observe them directly all the time, so we have to turn to simulations, which fill in the blanks and prepare for missions like Dragonfly and Europa Clipper.
Scientists don’t start from scratch when they want to simulate weather on other worlds – they start with the same models we use to study Earth. These are called General Circulation Models, or GCMs, and they’re basically complex weather engines that take into account wind, temperature, pressure, etc.
Of course, you have to make them work for places like Titan or Europa, so researchers adjust the inputs (gravity, sunlight, atmospheric makeup, and surface temperature) to get the model to behave more like a target moon.
For Titan, that means that they replace Earth’s water cycle with one based on methane. The model has to reflect how methane evaporates, forms clouds, and rains down on the surface under extremely cold conditions. It also has to account for the low energy coming from the distant Sun.
On Europa, the focus is more on the weather activity under the ice. There’s no thick atmosphere to model, but there are possible water vapor plumes that are driven by the heat from the inside. Researchers simulate how and when those plumes might erupt and, to make it more accurate, they use Earth-based examples like deep-sea vents or polar ice studies.
This is supported by current models, making it plausible, but note that it hasn’t been definitively observed yet. Weather APIs are widely used for Earth-based modeling, but they aren’t built for planetary simulations. So, if you search ‘weather API free’, you won’t find tools suited for modeling weather on moons like Titan or Europa. Not outside of Earth, anyway.
For that, you’d have to go for a specialized one with specialized datasets and simulation tools, which may cost you, and are (usually) unavailable to the general public.
Imagination and math both have a part to play, but researchers need more than that, so they use real data collected here on Earth.
These moons are, of course, very different from our planet, but some of the patterns and processes can still be studied using Earth-based information.
Data from NOAA, ERA5, and ECMWF show long-term patterns in wind, pressure, and temperature. These are scaled to match Titan’s thick, layered atmosphere or Europa’s thin surface gases.
Europa’s frozen surface is often compared to the polar regions on Earth. Data from Antarctica and the Arctic helps simulate how ice reflects sunlight, absorbs heat, and responds to the changes in temperature.
Scientists use geothermal data from Earth’s geysers and deep-sea vents to study Europa’s possible plumes. These systems give clues about how pressure builds and how material might escape through ice.
It will be a long time before we pack an umbrella for Titan, but thanks to Earth-based models and datasets, at least we can understand its weather. Sort of.
And what we see on both Europa and Titan is a mix of the familiar and completely bizarre, but just the fact that we can stretch the tools made for Earth to study moons that are millions of miles away?
You have to admit, that’s pretty awesome.