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Volatile Ice Deposits in Lunar Polar Regions and Their Sources
An amalgamation of code adapted from Schorghofer  and Moores  was used to simulate the movement of volatiles on the present-day surface of the Moon. The trapping of volatiles in permanently shadowed regions ...
Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars
Science fiction has long teased our imaginations with tales of planets with two suns. How these planets form and evolve, and their survival prospects, are active fields of research. Expanding on previous work, four new ...