Stellar Evolution, Nucleosynthesis, and Cosmology

Model and explain diurnal cycles, seasonal changes, lunar phase progression, eclipses, and ocean tides through orbital geometry and gravitational interactions.

Examine the physical properties of Solar System bodies and apply gravitational laws and Keplerian mechanics to explain orbital dynamics.

Analyze the astrophysical and geochemical factors that make Earth capable of supporting life and evaluate scientific models for the origins of the cosmos and biosphere.

Explain mantle convection, lithospheric plate boundaries, seafloor spreading, mountain orogeny, and seismological and volcanic hazards.

Evaluate renewable and non-renewable energy resources, analyze watershed and soil nutrient dynamics, and assess strategies for waste and pollution mitigation.

Trace stellar life cycles across mass regimes, explain stellar nucleosynthesis, and analyze evidence supporting the Big Bang and cosmic expansion.