Exploring Saturn’s largest moon, Titan, presents unique orbital challenges due to its dense atmosphere, gravitational perturbations, and limited sunlight. A new study proposes an innovative satellite constellation architecture based on […]
Saturn
Water-group Ion Irradiation Studies Of Enceladus Ice Analogues: Can Radiolysis Account For Material In And Around The South Polar Plume?
Saturn’s magnetosphere contains trapped plasma and energetic charged particles which constantly irradiate the surface of Enceladus.
Exploring Giant Planet Atmospheres with Habitable Worlds Observatory
Visible and ultraviolet imaging and spectroscopy of Solar System giant planets can set the paradigm for the atmospheric, ionospheric, and magnetospheric processes shaping the diversity of giant exoplanets, brown dwarfs, […]
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.
Catalog And Characterization Of Science Orbit Configurations For An Enceladus Orbiter
Saturn’s moon Enceladus is an exciting destination for future exploration missions due to the scientifically interesting geyser region located on its South pole.
Icy Ocean World Enceladus Orbits In The Ring It Makes Around Saturn
Saturn’s E ring is a huge, fuzzy, donut-shaped circle of particles around Saturn, that puzzled scientists for a long time.
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.
Cassini Proves The Existence Of Complex Chemistry Within Enceladus’ Ocean
Scientists digging through data collected by the Cassini spacecraft have found new complex organic molecules spewing from Saturn’s moon Enceladus. This is a clear sign that complex chemical reactions are […]
On the Detection Of Exorings in Reflected Light With JWST NIRCam
When directly imaging a cold giant exoplanet hosting a ring system, the reflected light from the rings can outshine the planet’s thermal emission and reflected-light in the near-infrared.
Study Questions Oceanic Origin Of Organics In Enceladus’s Plumes
Organic molecules detected in the watery plumes that spew out from cracks in the surface of Enceladus could be formed through exposure to radiation on Saturn’s icy moon, rather than […]
