PIA02594: Io's Tvashtar Area in Infrared: Multiple Lava Flows


Io’s Tvashtar Area in Infrared: Multiple Lava Flows

Caption:

New and older lava flows clustered in the Tvashtar region of Jupiter's moon Io appear as hot spots in a temperature map from NASA's Galileo spacecraft.

The multiple hot spots indicate continuing shifts in the location of Tvashtar's eruptions since the region's volcanic activity was first seen in December 1999.

The temperature map (top) uses infrared observations made during Galileo's Aug. 6, 2001, flyby of Io. It is shown using landmarks from a February 2000 visible-light image (bottom) that Galileo's camera recorded of the Tvashtar area of bowl-like depressions in Io's northern hemisphere. The temperature map comes from Galileo's near-infrared mapping spectrometer.

Tvashtar has been a very active region since December 1999, when Galileo detected a major eruption from the location marked A (See insert image below). The eruption from A was interpreted as a row of lava fountains. When Galileo flew by Io again in February 2000, the eruption had shifted to the location marked B, where a lava flow shaped like a dolphin's tail is seen. The temperature map shows that volcanic activity is present at many locations in this region. The highest temperatures are found in the three locations marked x, where new lavas may have recently come to the surface. Temperatures (in Kelvin) displayed in the color bar are lower limits. (The range in Fahrenheit is from 460 degrees below zero to 530 degrees above zero.) Each picture element averages the characteristics of an area about 2 kilometers (1.2 miles) across; smaller patches may be hundreds of degrees higher. The Galileo camera did not obtain a visible-light image of the Tvashtar region during the August 2001 flyby. Based on the locations of the hottest materials detected by Galileo's near-infrared mapping spectrometer, volcanologists expect that significant surface changes have occurred.

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http://solarsystem.nasa.gov/galileo/ .

Background Info:

The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Galileo mission for NASA’s Office of Space Science, Washington, D.C. Additional information about the spacecraft and its discoveries is available on the Galileo home page at

Cataloging Keywords:

Name Value Additional Values
Target Io
System Jupiter
Target Type Satellite
Mission Galileo
Instrument Host Galileo Orbiter
Host Type Orbiter
Instrument Near-Infrared Mapping Spectrometer (NIMS)
Detector
Extra Keywords Color, Infrared, Map, Volcano
Acquisition Date
Release Date 2001-11-27
Date in Caption 2001-08-06
Image Credit NASA/JPL
Source photojournal.jpl.nasa.gov/catalog/PIA02594
Identifier PIA02594