- Captain's Logs
- Feb 23, '22
- Sep 15, '17
- Sep 15, '15
- Jan 14, '15
- Dec 24, '14
- Jul 28, '14
- Jun 30, '14
- Nov 12, '13
- Jun 18, '13
- Dec 18, '12
- Jul 12, '12
- Apr 23, '12
- Nov 17, '11
- Jul 6, '11
- Nov 1, '10
- Sep 21, '09
- May 7, '09
- Apr 2, '09
- Mar 23, '09
- Dec 31, '08
- Nov 1, '08
- Jun 30, '08
- Mar 26, '08
- Dec 24, '07
- Oct 15, '07
- Mar 15, '07
- Dec 29, '06
- Sep 19, '06
- Jun 18, '06
- Mar 9, '06
- Dec 22, '05
- Jun 28, '05
- Jan 11, '05
- Dec 30, '04
- Nov 29, '04
- Oct 26, '04
- Sep 9, '04
- May 6, '04
- Feb 27, '04
- Dec 5, '03
- Nov 13, '03
- Nov 1, '02
- Mar 13, '02
- May 31, '01
- Oct 9, '00
- Feb 11, '00
- Sep 1, '99

|
 |
Io's Tvashtar Area in Infrared: Multiple Lava Flows
 PIA 02594
Image 468 x 620:
JPEG 39 KB
PNG 228 KB

Image (Labeled) 468x620:
JPEG 40 KB
|
|
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. 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.
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 http://galileo.jpl.nasa.gov.
Image Credit: NASA/JPL |
|