Io, the second smallest and innermost of Jupiter's four Galilean moons, was first observed by Galileo Galilei in January 1610. Along with moons Ganymede, Europa, and Callisto, Io challenged the belief that Earth was the center of the universe. These moons seemed to orbit Jupiter rather than Earth, which revolutionized our understanding of the cosmos. Although Galileo kept his discovery secret for a time due to the influence of the Catholic Church, his documentation of Io set the stage for some extraordinary discoveries in the centuries that followed.
Known as Jupiter's 'pizza moon' for its bright, patchy surface, Io is often described as a world of fire and ice. Despite being located in one of the coldest regions of our solar system (nearly 400 million miles from the Sun), Io produces immense amounts of heat. This heat is generated by intense volcanic activity, making Io one of the most geologically active bodies in the solar system. Its dramatic and fiery landscape truly makes it a hellish moon unlike any other.
In a nod to science fiction, Galileo originally named Io 'Jupiter I.' However, it wasn't until the mid-1800s that the moon received its mythological name, after the Greek priestess Io, who was pursued by Zeus (Jupiter in Roman mythology). In the myth, Io transforms into a cow to escape Hera, Zeus's wife, which mirrors the moon's bizarre and constantly changing features. Below are ten incredible facts about Io, one of the most mysterious moons in the universe.
10. Lacking Water

Io is one of the driest worlds in the solar system. When it was first formed around Jupiter, it emerged from a region that contained water ice. While it's believed that water may have once been present on Io, any trace of it has been long erased by Jupiter's powerful radiation.
This doesn't entirely dismiss the possibility of life on Io, though not on its surface. If life were to exist on 'Jupiter I,' it would likely be found deep within the moon's crust. So, if you're hoping to find extraterrestrial life on Io, you might have better luck digging underground to escape the harsh radiation!
9. Towering Volcanoes

Io is one of the most volcanically active places in the solar system. We are familiar with events like the Mount St. Helens eruption in 1980, the eruption of Mount Vesuvius in AD 79 that engulfed Pompeii in ash, or the Yellowstone supervolcano beneath Wyoming. However, these eruptions are nothing compared to what happens on Io. In fact, hundreds of volcanoes dot the surface of this small moon, and they are the main force behind Io's weather patterns.
The volcanic eruptions on Io are so intense that they can be observed from telescopes on Earth. These explosions are so powerful they can cover vast areas in seconds. Some eruptions release up to 20 trillion watts of energy, ejecting plumes of debris that fly off the moon’s surface and into space. These plumes, which can be made of sulfur, rock, and other debris, sometimes reach altitudes of 400 kilometers (250 miles) above the surface. The eruptions on Io are typically thousands of times more powerful than anything on Earth, and after these eruptions, rivers of lava can stretch for hundreds of miles.
8. Ocean of Lava

Below Io’s surface, there exists vast seas of magma. This molten rock, constantly shifting beneath the moon’s crust, powers Io’s extreme volcanism. The surface of Io essentially floats on top of this liquid rock, which is about 50 kilometers (30 miles) thick. This molten reservoir is the reason Io holds the title of the most volcanically active body in the solar system.
Recent studies show that Io, though only about the size of North America, produces 100 times more lava than all the volcanoes on Earth combined. One of its regions, Loki Patera, named after the Norse trickster god, features a massive volcanic depression measuring 204 kilometers (127 miles) across, constantly filled with magma. This region, thought to be an exposed lava sea, dwarfs any lava sea found on Earth by millions of times.
7. Temperature Extremes on Io

Io experiences dramatic temperature changes. Out of all the moons in the solar system, it may have the most extreme temperature variations. In areas dominated by volcanic activity, temperatures can soar to a staggering 1,700 degrees Celsius (3,100 °F), hotter than Mercury’s surface. With the harsh radiation from Jupiter and these high temperatures, anyone visiting Io would need some serious sun protection. However, despite these hotspots, the majority of Io remains a frigid world.
Away from the volcanic regions, Io's surface temperature can plunge to a chilling –153 degrees Celsius (–243 °F). NASA’s Galileo spacecraft found that temperatures at night are nearly the same across Io’s equator and poles. This is a stark contrast to Earth, where equatorial regions typically experience much higher temperatures than the polar areas due to the varying amounts of sunlight.
6. It’s a Stinky Place

Io could easily claim the title of the smelliest place in the solar system. As if the freezing temperatures, scorching hot spots, and the absence of water weren’t enough to make life unbearable on Io, it also has a distinctly unpleasant odor—like rotten eggs. The cause? Io's thin atmosphere is largely composed of sulfur dioxide, which is constantly released from its volcanoes. The few other elements in the atmosphere allow the sulfur dioxide to linger, giving Io its foul scent.
The continuous volcanic eruptions on Io act as massive factories of gases, contributing to its less-than-pleasant smell. But these gases are also responsible for creating Io’s atmosphere (even if it’s stinky), setting it apart from most moons, which have no atmosphere at all. So, which would you prefer: air that smells of rotten eggs, or the cold void of space? Either way, you won’t survive without proper protection.
5. Intense Magnetism

Io’s atmosphere, primarily composed of sulfur dioxide, creates a highly ionized environment. As Io orbits Jupiter, it passes through powerful magnetic fields, transforming it into a giant electrical generator. But what’s even more astonishing isn’t just the charged atmosphere causing massive lightning storms, it’s the fact that Jupiter's magnetic forces strip away about a ton of surface material from Io every second. Talk about some extreme weight loss!
The material that gets stripped off Io is quickly ionized, creating a cloud of intense radiation that surrounds the moon. This phenomenon is called a plasma torus. Io is one of the rare places in our solar system where such an event occurs, adding to the list of the moon’s many peculiarities. Unfortunately, scientists believe the radiation levels make it unlikely for life to exist on Io, though they haven’t entirely ruled out the possibility. Compared to other moons around Jupiter, like the icy Europa, Io’s chances of supporting life are slim.
4. Io’s Short Year

Io experiences one of the fastest years in the solar system. If you think time flies on Earth, wait until you hear this: Io’s year (the time it takes to orbit Jupiter) lasts only 42 Earth hours.
While Earth’s moon takes around 27 days to complete one orbit, Io's year is incredibly short in comparison! Interestingly, the length of Io’s year is almost identical to the duration of its day, which is just 1.8 Earth days.
3. Io Helps Us Understand Earth’s History

Io, one of Jupiter’s moons, is arguably one of the most bizarre places in our solar system, with its massive volcanoes, molten seas, foul-smelling atmosphere (when present), and constant bombardment by Jupiter’s powerful radiation. But what really captures the attention of Earth-bound scientists is not its strange geology but how it offers us valuable insights into the history of Earth itself.
Over four billion years ago, Earth began its existence as a massive, molten sphere, constantly bombarded by asteroids crashing into its lava seas. It's fascinating to think that such a distant, alien world offers us the opportunity to study volcanic processes that may have occurred on our own planet during its early formation. As this list of ten incredible facts about Io shows, Jupiter’s innermost moon is truly a cosmic oddity.
2. Sulfur Snow

Every day on Io, sulfur snow falls to its surface. Unlike Earth’s water crystals, which freeze and fall to the ground, Io’s version of ‘snow’ is much stranger. For two hours every year, Io passes through Jupiter’s immense shadow, cutting off sunlight from warming the moon’s thin atmosphere. During this shadowed period, the plummeting temperatures cause sulfur dioxide in the air to freeze and settle as sulfur snow. The sulfur released by Io’s volcanoes also quickly freezes, adding to the snowfall.
Moreover, this shadow-induced phenomenon results in a truly alien occurrence: Io’s atmosphere essentially collapses during these brief Jovian eclipses. After two hours, as sunlight returns, the atmosphere is rejuvenated, and the sulfur snow evaporates back into gas (a process called sublimation). This leads to an endless cycle of collapse and rebirth for Io’s atmosphere, influenced by sunlight’s effect on both the surface temperature and the very presence of the atmosphere.
1. Constantly Stretched and Compressed

Here's something quite unusual: Io's surface endures relentless distortion due to Jupiter’s immense gravity. It’s almost like kneading dough. The moon is continually stretched and compressed by the forces from Jupiter, forcing its shape to fluctuate as the magma beneath behaves like squishy gelatin. Known as tidal heating, this phenomenon causes Io’s surface to rise and sink by hundreds of feet each day.
Tidal heating is also experienced by other moons such as Europa and Enceladus. On Europa, this results in vast ice fractures, while on Enceladus, it triggers the eruption of ice geysers.