Media Information

 
 
 
Collection:
NASA Solarsystem Collection
title:
Titanic Volcano
description:
This high-resolution infrared image was taken during the Cassini spacecraft's closest approach to Titan on Oct. 26, 2004. These images were obtained by Cassini's visual and infrared mapping spectrometer instrument and show a bright, circular feature (8.5 degrees latitude, minus 143.5 degrees longitude) with two elongated wings extending westwards. Scientists think this feature might be a volcano.

The resolution in the image varies from 2.6 kilometers (1.6 miles) per pixel to 1.8 kilometers (1.1 miles) per pixel.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The visual and infrared mapping spectrometer team is based at the University of Arizona.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.na sa.gov. The visual and infrared mapping spectrometer team homepage is at http://wwwvims.lpl.a rizona.edu.
date:
10.26.2004
keywords:
Solar System Exploration
keywords:
SSE
keywords:
Space
keywords:
NASA
keywords:
National Aeronautics and Space Administration
keywords:
JPL
keywords:
Jet Propulsion Laboratory
keywords:
Planets
facet_what:
Saturn
facet_what:
Cassini
facet_what:
Spectrometer
facet_what:
Titan
facet_what:
Cassini-Huygens
facet_what:
Cassini Orbiter
facet_what:
Huygens Probe
facet_what:
Visual and Infrared Mapping Spectrometer (VIMS)
facet_where:
Jet Propulsion Laboratory
facet_where:
Saturn
facet_where:
California
facet_where:
Washington
facet_where:
Arizona
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_when:
10-26-2004
facet_when_year:
2004
UID:
SPD-SLRSY-4603
original url:

Titanic Volcano