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.
NASA's Cassini spacecraft peers down though layers of haze to glimpse the lakes of Titan's northern regions. Titan has a hydrological cycle similar to Earth's, but instead of water, Titan's lakes and seas are filled with liquid methane and ethane.
This artist's concept shows a possible model of Titan's internal structure that incorporates data from NASA's Cassini spacecraft. A model of Cassini is shown making a targeted flyby over Titan's cloudtops; Saturn and Enceladus appear at upper right.
Using a special spectral filter, NASA's Cassini spacecraft was able to peer through the hazy atmosphere of Saturn's moon Titan. This image features the largest seas and some of the many hydrocarbon lakes that are present on Titan's surface.