2026 Astrobiology Science Conference | 18 May 2026
Effect of fluid tidal dissipation on the long-term persistence of icy-moon oceans
Inside some icy moons around the giant planets of the outer solar system (Jupiter, Saturn, Uranus, Neptune), there are oceans of liquid water. It's been a puzzle understanding...
2026 Astrobiology Science Conference | 21 May 2026
Thermodynamic Stability of Organic Molecules in the Interior of Icy Moons: Insights from Meteorite Analogs
Beneath icy moons’ surfaces, interactions between water and rock can create energetic environments that may support life. Organic molecules, including the building blocks...
2026 Astrobiology Science Conference | 18 May 2026
Laboratory Investigations of Ocean Transport in Icy Moons
Several icy moons in the outer solar system are confirmed (e.g. Europa, Enceladus) or are likely (e.g. Ganymede, Titan, Callisto, etc.) to host subsurface oceans with stable...
2026 Astrobiology Science Conference | 21 May 2026
Role of boundary layers in shaping the circulation in icy-moon oceans
Europa and Enceladus are ice-covered moons of Jupiter and Saturn that hide deep oceans beneath a thick ice shell. These oceans may host conditions suitable for life, possibly...
Journal of Geophysical Research: Planets VOL.131 ISSUE 5 | 5 May 2026
Electrical Conductivity of Almandine‐Rich Garnet at High Pressures and Temperatures: Constrains on the Conductivity Profile of the Moon and Mars
Duojun Wang + kewei shen
Despite the existence of several geophysical models for Mars and the Moon, the composition and structure of their mantles require further constraints; thus, the elastic and...