Galileo NIMS Observes Amirani | |
by NASA | |
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This image is the highest-resolution thermal, or heat | |
image, ever made of Amirani, a large volcano on Jupiter's | |
moon Io. It was taken on October 10, 1999, by the near- | |
infrared mapping spectrometer onboard NASA's Galileo | |
spacecraft. Amirani is on the side of Io that permanently | |
faces away from Jupiter. This image of Amirani was taken | |
at a distance of less than 25,000 kilometers (16,000 | |
miles). The picture scale is approximately 6.5 kilometers | |
(4 miles) per spectrometer pixel. The center and right | |
images show views of Amirani as seen by the spectrometer | |
at two wavelengths, 1.0 and 4.6 microns. These images can | |
be compared with a visible wavelength image (on the left) | |
of the same area obtained by Galileo's camera during a | |
previous orbit. The visible light image shows extensive | |
lava flows and a dark-floored caldera with associated | |
bright red deposits of material fed from the volcano. The | |
spectrometer observation was made in daylight. The center | |
image, taken at a wavelength of 1 micron, shows light and | |
dark areas on the surface that can be used to line up the | |
spectrometer data with the camera image. The image on the | |
right shows the same area at a wavelength of 4.6 microns, | |
which reveals the thermal emission from three separate | |
volcanic areas. The locations of these three "hot spots" | |
correspond to the darkest features in the camera image, | |
reinforcing a previously held belief by Galileo | |
scientists that there is a correlation between the dark | |
areas and the hot spots. The three spectrometer hot spots | |
are located at the eastern edge of the caldera at the | |
bottom of the camera image, and two locations along the | |
massive Amirani flows. These are most likely active lava | |
flows on the surface. Launched in October 1989, Galileo | |
entered orbit around Jupiter on December 7, 1995 on a | |
mission to study the giant planet, its largest moons and | |
its magnetic environment. JPL manages the mission for | |
NASA's Office of Space Science, Washington, DC. JPL is a | |
division of the California Institute of Technology, | |
Pasadena, CA. This image and other images and data | |
received from Galileo are posted on the World Wide Web, | |
on the Galileo mission home page at <a | |
href="http://galile | |
o.jpl.nasa.gov">http://galileo.jpl.nasa.gov</a>. | |
Background information and educational context for the | |
images can be found at <a | |
href="http://galileo.jpl.nasa.gov/gallery/io.cfm" | |
class="external free" | |
target="wpext">http://galileo.jpl.na | |
sa.gov/gallery/io.cfm</a>. | |
Date Published: 2009-10-14 05:11:13 | |
Identifier: PIA02516 | |
Item Size: 56808 | |
Media Type: image | |
# Topics | |
What -- Moon | |
What -- Io | |
What -- Near Infrared Mapping Spectro... | |
What -- Spectrometer | |
What -- Galileo | |
What -- Jupiter | |
What -- Visible Light | |
Where -- Jet Propulsion Laboratory (JPL) | |
Where -- Washington | |
Where -- California | |
# Collections | |
nasa | |
planetaryphotojournalcollection | |
# Uploaded by | |
@bonniereal | |
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