Jupiter’s fifth moon, Io, is the most volcanically active body in the solar system. Plumes of sulfur spew upward as high as 190 miles (300 kilometers). The surface of Io is splotched with lava lakes and floodplains of liquid rock.
Io by the numbers
Age: Io is about 4.5 billion years old, about the same age as Jupiter.
Distance from Jupiter: Io is the fifth moon from Jupiter. Its orbital distance is about 262,000 miles (422,000 km). Io takes 1.77 Earth-days to orbit Jupiter. Io is tidally locked, so the same side always faces Jupiter.
Size: Io has a mean radius of 1,131.7 miles, making it slightly larger than Earth’s moon. It has a slight elliptical shape, with its longest axis directed toward Jupiter. Among the Galilean satellites Io ranks third, behind Ganymede and Callisto but ahead of Europa, in both mass and volume.
Temperature: Io's surface temperature averages about minus 202 degrees Fahrenheit (minus 130 Celsius), resulting in the formation of sulfur dioxide snowfields. But Io’s volcanoes can reach 3,000 F (1,649 C). Io is often referred to as a celestial body of fire and ice.
The Discovery of Io
Io was the first of Jupiter’s moons discovered by Galileo Galilei on Jan. 8, 1610. He actually discovered the moon the day prior, but could not differentiate between Io and Europa, another Jupiter moon, until the next night. The discovery, along with three other Jovian moons, was the first time a moon was discovered orbiting a planet other than Earth. Galileo’s discovery eventually led to the understanding that planets orbit the sun, instead of our solar system revolving around Earth.
Galileo first referred to this moon as Jupiter I. In the mid-1800s, the moon was renamed Io. In Greek mythology, Io was a priestess of Hera (Zeus' wife) and the daughter of Inachus, the king of Argos. Zeus (the counterpart for the Roman god Jupiter) fell in love with her, but turned her into a cow to avoid being caught with her by his wife, Hera (or Juno).
Several spacecraft have flown by Jupiter and its moons. Pioneer 10 arrived first, in 1973, followed by Pioneer 11 in 1974. Voyager 1 and Voyager 2 returned striking photos during their flybys. The Galileo spacecraft passed as low as 162 miles (261 km) over the surfaces of the Galilean moons and produced detailed images.
Characteristics of Io
The interior of Io is composed of an iron or iron sulfide core and a brown silicate outer layer, giving the planet a splotchy orange, yellow, black, red, and white appearance.
Based on data from scientific computer models, Io formed in a region around Jupiter where water ice was plentiful. Io’s heat, combined with the possibility that there was water on Io shortly after it was formed, could have made life possible, although Jupiter’s radiation would have removed the water from the surface.
The moon's most distinctive features are its volcanoes. Aside from Earth, Io is the only known body in the solar system to have observed active volcanoes. While Galileo had made some cryptic notes inferring possible volcanic activity, NASA's Voyager spacecraft discovered Io's volcanoes in 1979.
The volcanic activity is a result of Io being stretched and squeezed as it orbits Jupiter. Io's rock surface bulges up and down by as much as 100 meters (328 feet) during the process. This affects Io’s volcanic activity in a similar way to which Earth’s oceans react to the moon. Io’s irregularly elliptical orbit also heightens the tidal activity.
Because of the volcanic activity, Io’s atmosphere contains mostly sulphur dioxide. Io’s orbit cuts across Jupiter’s powerful magnetic lines of force, turning Io into an electric generator. As Jupiter rotates, the magnetic forces strip away about a ton (1,000 kg) of Io’s material every second. The material becomes ionized and forms a doughnut-shaped cloud of radiation called a plasma torus. Some of the ions are pulled into Jupiter’s upper atmosphere and create auroras.
Io's environment has come under intense scrutiny in recent years as scientists try to explain why the moon has the most active volcanoes in the solar system. The recent findings involve both observations of the moon and modeling of the interior, which can only be inferred.
A 2015 study explained why Io's most prolific volcanoes appear to be offset from where scientists expected they would be. While previous models suggested that the zones with the most intense heating would have more active volcanoes, the actual Io had its most active ones farther east. The study suggests that if there was an ocean mixed with molten and solid rock underneath the moon, the rock portions would rub against each other and create the offset zones scientists observed.
Insights into Io's surface may also come from a 2012 map published by the U.S. Geological Survey – the first to include the entire surface. The researchers said that volcanic activity would be among the things that could be studied with this map. The imagery includes observations from the Voyager 1 and Voyager 2 spacecraft, as well as Galileo.
While there is no mission specifically planned to look at Io, there will be other missions in the vicinity of the moon in future years, including Juno (2016), a planned NASA Europa mission (perhaps in the 2030s), and the European Space Agency's JUICE mission (JUpiter ICy Moons Explorer, which will focus on Europa, Ganymede and Callisto). Meanwhile, observations continue from the ground; sometimes Io's volcanoesare violent enough to produce spectacular pictures even from so far away.
Additional reporting by contributor Elizabeth Howell.