This global digital map of Saturn's moon Titan was created using images taken by NASA's Cassini spacecraft's. The map was produced in June 2015 using data collected through Cassini's flyby, known as 'T100,' on April 7, 2014.
Titan and Saturn share a hazy appearance in this image from NASA's Cassini spacecraft, though Saturn is a gas giant with no solid surface to speak of, and Titan's atmosphere is a blanket surrounding an icy, solid body.
Titan may be a 'large' moon -- its name even implies it -- but it is still dwarfed by its parent planet, Saturn. As it turns out, this is perfectly normal. This image is from NASA's Cassini spacecraft.
Named after a Japanese paradise, NASA's Cassini spacecraft spies the Senkyo region of Titan), a bit less welcoming than its namesake with a very inhospitable average temperature of approximately 290 degrees below zero Fahrenheit (-180 degrees Celsius).
Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view, at left, and one made using a new technique for handling electronic noise that results in clearer views of Titan's surface, at right.
This montage from NASA's Cassini Synthetic Aperture Radar (SAR) images of the surface of Titan shows four examples of how a newly developed technique for handling noise results in clearer, easier to interpret views.
These views from NASA's Cassini Synthetic Aperture Radar (SAR) present a side-by-side comparisons of a traditional view and one made using a new technique called despeckling for handling electronic noise that results in clearer views of Titan's surface.
This diagram depicts conditions observed by NASA's Cassini spacecraft during a flyby in Dec. 2013, when Saturn's magnetosphere was highly compressed, exposing Titan to the full force of the solar wind.
The view was obtained during NASA's Cassini orbiter's flyby on July 24, 2012, also called the 'T85' flyby by the Cassini team. This was the most intense specular reflection that Cassini had seen to date.
These three images, created from NASA's Cassini Synthetic Aperture Radar (SAR) data, show the appearance and evolution of a mysterious feature in Ligeia Mare, one of the largest hydrocarbon seas on Saturn's moon Titan.
Scientists modeled how methane rainfall runoff would interact with the porous, icy crust of Saturn's moon Titan and found that a subsurface methane 'aquifer' might have its composition changed over time due to the formation of materials called clathrates.
Only a sharp and careful eye can make out the subtle variations in Titan's clouds when viewed in visible light by NASA's Cassini spacecraft. This infrared image clearly reveals a band around the Titan's north pole.