The image in the upper part of the table represents a raw view of a portion of Saturn's largest moon Titan obtained on July 25, 2015 from the Cassini spacecraft on the basis of the CL1 filter and of the CB3 filter. The view whose file name is N00244673.jpg had not been validated or calibrated at the time of the observation and a validated or calibrated version was going to be archived with the Planetary Data System proposed by NASA. One can notice the sharp contrast between bright areas and dark areas in particular. The dark areas found in the low or mid-latitudes are generally dominated by linear and parallel dunes extending over long distances. The eyes of the Cassini orbiter can discern surface features in the infrared or near-infrared spectrum. The view in the lower part of the table represents a colorized version of the original image.

Credit for the original view: NASA/JPL-Caltech/Space Science Institute.
Credit for the colorization process of the original view: Marc Lafferre, 2021.

The image in the upper part of the table reveals a portion of Titan's landscape acquired from the Cassini orbiter on June 17, 2014. The view whose file name is N00225354.jpg was obtained on the basis of the CL1 filter and of the CB3 filter. The image had not been validated or calibrated at the time of the observation and a validated or calibrated version was going to be archived with the Planetary Data System proposed by NASA. One can notice the contrast between relatively bright areas and relatively dark areas. The image in the lower part of the table represents a colorized version of the original view.

Credit for the original view: NASA/JPL-Caltech/Space Science Institute.
Credit for the colorization process of the original view: Marc Lafferre, 2021.