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Today's featured article

Callisto

Callisto is a moon of the planet Jupiter, discovered in 1610 by Galileo Galilei. It is the third-largest moon in the Solar System and the second largest in the Jovian system, after Ganymede. It does not form part of the orbital resonance that affects three inner Galilean satellites—Io, Europa and Ganymede—and thus does not experience appreciable tidal heating. Callisto rotates synchronously with its orbital period, so the same face is always turned toward Jupiter. Callisto is composed of approximately equal amounts of rock and ices, with a mean density of about 1.83 g/cm3. Compounds detected spectroscopically on the surface include water ice, carbon dioxide, silicates, and organic compounds. Investigation by the Galileo spacecraft revealed that Callisto may have a small silicate core and possibly a subsurface ocean of liquid water at depths greater than 100 km. Prominent surface features include multi-ring structures, variously shaped impact craters, and chains of craters and associated scarps, ridges and deposits. Callisto is surrounded by an extremely thin atmosphere composed of carbon dioxide and probably molecular oxygen, as well as by a rather intense ionosphere. (more...)

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Port Vell, Barcelona

An aerial panoramic view of Port Vell, Barcelona, Spain, from atop the Columbus Monument. The area has been in use as a port since the 4th century BC, when it was settled by the Laietani. The current incarnation was built as part of an urban renewal program prior to the 1992 Barcelona Olympics. It is now a focal point of the city and tourist attraction, drawing up to 16 million visitors a year.

Photo credit: David Iliff

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