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.
Titan
Refractive Indices Of Photochemical Haze Analogs For Solar System And Exoplanet Applications: A Cross-laboratory Comparative Study Between The PAMPRE And COSmIC Experimental Set-ups
Previous observations of Titan, Pluto and Solar System gas giants along with recent observations of exoplanet atmospheres with the James Webb Space Telescope taught us that photochemical hazes are ubiquitous […]
Prebiotic Chemistry Insights for Dragonfly: Thermodynamics of Amino Acid Synthesis in Selk Crater on Titan
Saturnian moon Titan presents a compelling testbed for probing prebiotic chemistry beyond early Earth. Impact-generated melt pools provide transient aqueous habitats in an otherwise cryogenic environment.
Flower-like Satellite Constellations To Guide Future Missions Around TitanSatellite Navigation
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 […]
How Does Ice Shell Geometry Shape Ocean Dynamics On Icy Moons?
A poleward-thinning ice shell can drive circulation in the subsurface oceans of icy moons by imposing a meridional temperature gradient–colder at the equator than the pole–through the freezing point suppression […]
Growth, Physiology, And Metabolism Of Halomonas Meridiana In Aqueous Ammonium Sulfate With Implications For Icy Moon Astrobiology
The discovery of extraterrestrial reservoirs of liquid water has motivated missions to icy moons Europa and Titan.
Unexpected Discovery On Titan Challenges Our View On Chemistry Before Life Emerged
Researchers at Chalmers University of Technology in Sweden and the US space agency NASA have made an unexpected discovery that challenges one of the basic rules of chemistry and provides […]
Enceladus’ Tidal Heating: A Simple Approach
Saturn’s moon Enceladus has a global ocean that is covered by an ice shell. The moon’s eccentric orbit forces the shell to librate, which distorts the shell and thereby generates […]
Special Issue of Geosciences: “Worlds of the Solar System: Geological Evolution and Habitability of Planets and Moons”
The Special Issue of Geosciences entitled “Worlds of the Solar System: Geological Evolution and Habitability of Planets and Moons” aims to bring together the latest advances on the dynamic processes […]
Using SOFIA’s EXES To Search For C6H2 And C4N2 in Titan’s Atmosphere
In Titan’s atmosphere, the chemistry of small hydrocarbons and nitriles represent an important link from molecular species to the ubiquitous organic haze that gives Titan its characteristic yellow color.
