Io (moon)

Io (IPA: [ˈaɪoʊ], eye'-oe, Greek Ιώ) is the innermost of the four Galilean moons of Jupiter. It is named after the Greek mythological figure Io, one of the many lovers of Zeus (who is also known as Jupiter in the Roman mythology).

Although the name "Io" was suggested by Simon Marius soon after its discovery in 1610, this name and the names of the other Galilean satellites fell into disfavor for a considerable time, and were not revived in common use until the mid-20th century. In much of the earlier astronomical literature, Io is simply referred to by its Roman numeral designation as "Jupiter I", or simply as "the first satellite of Jupiter".

Volcanism

File:Io moon 475px.jpg

Galileo orbiter images reveal active volcanoes. The eruption in the top inset reaches 140km high, the other is 75km high.

Io is most noteworthy for its volcanic nature; it is the most volcanically active body in the Solar System. Similarly to volcanoes on Earth, Ionian volcanoes emit sulfur and sulfur dioxide. Originally it was thought that many lava flows consisted of sulfurous substances. However, nowadays it is thought that many of them are molten silicate rock like on the Earth.

The energy for this activity probably derives from tidal interactions among Io, Jupiter, and two other moons of Jupiter, Europa and Ganymede. The three moons are locked into Laplace-resonant orbits such that Io orbits twice for each orbit of Europa, which in turn orbits twice for each orbit of Ganymede; furthermore, Io always keeps the same face towards Jupiter. The gravitational interaction of Europa, Ganymede and Jupiter cause Io to "stretch" and "bend" by as much as 100 meters, a process which generates heat through internal friction.

Some of Io's volcanic plumes have been measured rising over 300 km above the surface before falling back, with material ejected from the surface at approximately one kilometre per second. The volcanic eruptions change rapidly; in just four months between the arrivals of Voyager 1 and Voyager 2 some eruptions stopped and others began. The deposits surrounding the vents also changed visibly during this time.

Another source of energy is that Io cuts across Jupiter's magnetic field lines, generating an electric current. Though not a large source of energy compared to the tidal heating, this current may carry more than 1,000 gigawatts with a potential of 400 kilovolts. It also strips ionized atoms from Io at the rate of a thousand kilograms per second. Due to the rapid rotation of Jupiter's magnetic field, these particles are swept along the orbit in front of Io where they form a torus of intense radiation around Jupiter that glows brightly in the ultraviolet. Particles escaping from this torus are partially responsible for Jupiter's unusually large magnetosphere, their outward pressure inflating it from within. Recent data from the Galileo orbiter indicate that Io might have its own magnetic field.

The location of Io with respect to the Earth and Jupiter has a strong influence on the Jovian radio emissions as seen from the earth: When Io is visible, radio signals from Jupiter increase considerably.

In February 2001, the largest recorded volcanic eruptions in the solar system occurred on Io [1].

Physical characteristics

Unlike most moons in the outer solar system, Io may be somewhat similar in bulk composition to the terrestrial planets, primarily composed of molten silicate rock. Recent data from the Galileo orbiter indicates that Io has a core of iron (perhaps mixed with iron sulfide), the core's radius being at least 900 km.

When Voyager 1 first returned images of Io in 1979, scientists expected to see numerous craters, the density of which across Io's surface would give clues to the moon's age. However, they were surprised to discover that Io's surface is almost completely lacking in craters, due to the tremendous amount of volcanic activity constantly reshaping the landscape. Since the surface features visible today were formed relatively recently, the Ionian surface is described as "young", as is the terrestrial surface. In contrast, celestial bodies with heavily cratered features, such as Earth's Moon, are considered to have "old" surfaces, since they have remained in their current state for billions of years.

In addition to volcanoes, Io's surface includes nonvolcanic mountains, numerous lakes of molten sulfur, calderas up to several kilometres deep, and extensive flows hundreds of kilometres long of low-viscosity fluid (possibly some form of molten sulfur or silicate). Sulfur and its compounds take on a wide range of colors and are responsible for Io's variegated appearance.

Analysis of the Voyager images led scientists to believe that the lava flows on Io's surface were composed mostly of various compounds of molten sulfur. However, subsequent ground-based infrared studies indicate that they are too hot for liquid sulfur; some of the hottest spots on Io may reach temperatures as high as 2000 kelvins, 1300 kelvins higher than the boiling point of sulfur, although though the average is much lower, at around 130 K. One current theory is that Io's lavas are molten silicate rock. Recent Hubble Space Telescope observations indicate that the material may be rich in sodium. There may be a variety of different materials in different locations.

Io has a thin atmosphere composed of sulfur dioxide and perhaps other gases.

Unlike the other Galilean satellites, Io has little or no water. This is probably because Jupiter was hot enough early in the evolution of the solar system to drive off the volatile elements in the vicinity of Io, but not hot enough to do so farther out.

Io in fiction

Peter Hyams, the director of 2010, had previously made a film called Outland (1981), set in a mining colony on Io, although the moon itself had little importance to the plot.
Io plays an important role in both the book and the film of Arthur C. Clarke's 2010: Odyssey Two (1984). A spacecraft is found tumbling end over end in orbit around Io, coated with sulfur from the erupting volcanoes beneath it.
In the television cartoon saga Exosquad (1993–1995), Io is the location of an Exofleet base and the scene of several critical battles between Terran and "Neosapien" forces.
In the science fiction TV series Babylon 5 (1993–), Io is home to an Earth Alliance colony, second in size only to the colony on Mars.
Michael Swanwick's Hugo award-winning short story "The Very Pulse of the Machine" (1998) is set on Io, and features elements of the volcanic, sulfurous landscape, as well as the powerful electrical flux between Io and Jupiter.
In the BBC docudrama Space Odyssey: Voyage To The Planets (2005), about a possible manned mission to various points of the Solar System, one astronaut lands on Io to collect samples of its rocks. However, due to radiation risks and the astronaut becoming exhausted, the EVA on Io is aborted early and the samples are abandoned.

External links

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Volcanism

Physical characteristics

Io in fiction

See also

External links