This study presents the trajectory design for a mission touring Saturn’s Inner Large Moons (Rhea, Dione, Tethys, Enceladus, and Mimas) engineered to meet observational requirements, including full surface coverage, while […]
Tethys
Icy Worlds: Moons And Dwarf Planets
In the outer solar system beyond Jupiter, water ice is a dominant component of planetary bodies, and most solid objects in this region are classified as icy bodies.
Deuterated Water Ice On The Satellites Of Saturn
The deuterium to hydrogen ratio in water ice in a planetary body carries important information on the history of water processing and delivery in the protostellar nebula.
A JWST Study Of CO2 On The Satellites Of Saturn
Solid state CO2 has been detected throughout the outer solar system, even at temperatures where crystalline CO2 is unstable, requiring that the CO2 be trapped in a separate host material.
The Evolution Of A Young Ocean Within Mimas
The fractured, young surfaces on confirmed ocean worlds such as Europa and Enceladus suggest that ocean-bearing moons with relatively thin overlying ice shells should be easy to identify. Hence, the […]
'Snow-Cannon' Enceladus Shines Up Saturn's Super-Reflective Moons
Radar observations of Saturn’s moons, Mimas, Enceladus and Tethys, show that Enceladus is acting as a ‘snow-cannon,’ coating itself and its neighbours with fresh water-ice particles to make them dazzlingly […]
