Moon Evolution Odyssey is a project focused on exploring and comparing the Moon, Europa, and Enceladus. It covers theoretical and observational astronomy, advancing into simulations and data analysis. The main goals are to study surface and subsurface features, tidal forces, and habitability potential. By mapping geological and thermal characteristics and applying simulations, SelenoQuest aims to reveal unique traits and potential for life on these celestial bodies. This project is a step toward understanding moons that may expand humanity’s knowledge of the cosmos. Ready to take the jump and uncover the secrets of the solar system's moons? Join us!!

WHAT LIES BENEATH THE SURFACE?

Objectives Geological and Subsurface Analysis: Compare surface features and subsurface compositions of the Moon, Europa, and Enceladus.

Tidal Forces and Thermal Simulations: Model tidal interactions to understand their impact on internal heating and potential habitability.

Habitability Assessment: Evaluate conditions that could support life on Europa and Enceladus, and contrast them with the Moon’s environment.

Simulation and Data Analysis: Utilize Python for simulations and data visualization, analyzing temperature gradients, orbital dynamics, and surface features to draw insights about the moons' potential for life and geological activity.