PIA22483: Spotting Dust Storms on Titan


Spotting Dust Storms on Titan

Caption:

Click here for animation

This animation -- based on images captured by the Visual and Infrared Mapping Spectrometer on NASA's Cassini mission during several Titan flybys in 2009 and 2010 -- shows clear bright spots appearing close to the equator around the equinox that have been interpreted as evidence of dust storms. The brightenings were visible only for a short period of time -- between 11 hours to five Earth weeks -- and cannot be seen in previous or subsequent images.

Background Info:

The Cassini spacecraft ended its mission on Sept. 15, 2017.

The Cassini mission is a cooperative project of NASA, ESA (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. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.

For more information about the Cassini-Huygens mission visit https://saturn.jpl.nasa.gov and https://www.nasa.gov/cassini . The Cassini imaging team homepage is at http://ciclops.org .

Cataloging Keywords:

Name Value Additional Values
Target Titan
System Saturn
Target Type Satellite
Mission Cassini-Huygens
Instrument Host Cassini Orbiter
Host Type Orbiter
Instrument Visual and Infrared Mapping Spectrometer (VIMS)
Detector
Extra Keywords Atmosphere, Color, Dust, Infrared, Storm
Acquisition Date
Release Date 2018-09-24
Date in Caption
Image Credit NASA/JPL-Caltech/University of Arizona/University Paris Diderot/IPGP
Source photojournal.jpl.nasa.gov/catalog/PIA22483
Identifier PIA22483