Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

Analogous to Earth's water cycle, Titan's methane-based hydrologic cycle supports standing
bodies of liquid and drives processes that result in common morphologic features including …

NASA's Dragonfly mission will send a rotorcraft lander to the surface of Titan in the mid-
2030s. Dragonfly's science themes include investigation of Titan's prebiotic chemistry …

Although there is evidence that liquids have flowed on the surface at Titan's equator in the
past, to date, liquids have only been confirmed on the surface at polar latitudes, and the vast …

Liquid water oceans are now predicted to exist beneath the icy shells of numerous worlds in
the outer solar system. These ocean worlds are prime targets in our search for evidence of …

Terrestrial analogue studies underpin almost all planetary missions and their use is
essential in the exploration of our Solar system and in assessing the habitability of other …

The last decade of Mars exploration produced a series of discoveries that provide
compelling evidence for the existence of sedimentary rocks on Mars. Previously, Mars was …

We construct the depth profile—the bathymetry—of Titan's large sea Ligeia Mare from
Cassini RADAR data collected during the 23 May 2013 (T91) nadir‐looking altimetry flyby …

Cassini's Imaging Science Subsystem (ISS) has been observing Titan since April 2004,
compiling a nearly global surface map and monitoring the surface and atmosphere for …

The existence of cryovolcanic features on Titan has been the subject of some controversy.
Here we use observations from the Cassini RADAR, including Synthetic Aperture Radar …