PIA02567: Giant Lava Flow on Io, in Color
 Target Name:  Io
 Is a satellite of:  Jupiter
 Mission:  Galileo
 Spacecraft:  Galileo Orbiter
 Instrument:  Solid-State Imaging 
 Product Size:  413 x 900 pixels (w x h)
 Produced By:  University of Arizona
 Addition Date:  2000-10-26
 Primary Data Set:  Galileo EDRs
 Full-Res TIFF:  PIA02567.tif (1.187 MB)
 Full-Res JPEG:  PIA02567.jpg (44.4 kB)

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Original Caption Released with Image:

This mosaic combines images collected in February 2000 and the summer of 1999 by NASA's Galileo spacecraft to highlight new details of the longest active lava flow known in the solar system.

The area, called Amirani, has been known to be the home of a number of volcanic hot spots ever since NASA's two Voyager spacecraft flew by Jupiter in 1979. Images collected by Galileo in 1999 showed that these hot areas were part of a single immense lava flow field. The newest images confirm that the Amirani flow field is indeed a quilt work of dark lava flows. The most recent lavas are darkest because they are too hot to be covered by sulfur-dioxide plumes. Fresh lava is leaking out of at least five areas at the northern end of the Amirani flow field and at least three places in the middle. However, it is likely that the lava first comes to the surface near the southern end of the flow field. The liquid lava travels under a frozen layer of older lava, breaking out onto the surface only after traveling hundreds of kilometers (hundreds of miles) from the vent. The "small" breakouts produce lava flows larger than the current eruption on Earth at Kilauea Volcano in Hawaii. These observations are helping to explain how very large, ancient lava flows formed on the Earth.

While the behavior of the lava once it is on the surface makes sense, how it comes to the surface is more complicated. Small, white, diffuse halos surrounding the darkest lava flows are probably sulfur-dioxide-rich snows and frosts that have been vaporized by the hot lava. The bright red material to the south of the Amirani flow field is likely to contain a large fraction of sulfur droplets. Sulfur-rich gas appears to be bubbling out all along the east-west crack at the southern end of Amirani. This may be the crack along which the lava rises to the surface. The main Amirani plume appears to emanate from a fuzzy, purplish area within the southern part of the flow field. This is a plausible alternative location for the lava to come to the surface.

The mosaic shows an area 500 kilometers (310 miles) long and 180 kilometers (110 miles) wide. Black and white images at 210 meters (690 feet) per picture element were combined with color data at 1.3 kilometers (.8 miles) per picture element. This computer wizardry allows us to learn much more than either set of pictures alone. North is to the top of the picture.

The Jet Propulsion Laboratory, Pasadena, Calif., manages the mission for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology in Pasadena.

This image and other images and data received from Galileo are posted on the Galileo mission home page at http://solarsystem.nasa.gov/galileo/. Background information and educational context for the images can be found at http://galileo.jpl.nasa.gov/gallery/io.cfm.

Image Credit:
NASA/JPL/University of Arizona

Image Addition Date: