Modeling Black Body Radiation with Python and Pint

Translating complex physics equations into clean, runnable code can be challenging, especially when managing physical units. This course bridges the gap by showing you how to model black body radiation and star radiance using Python. You will transition from theoretical physics equations to active computational models. By combining core scientific principles with modern Python libraries, you will learn how to automate unit conversions, perform precise thermodynamic calculations, and generate clear, accurate plots of stellar radiance. What you'll learn: - Understand the fundamental physics of black body radiation, Planck's law, and stellar radiance - Manage physical units seamlessly in Python using the pint library to prevent calculation errors - Apply modern Python type hints to scientific functions for cleaner, self-documenting code - Calculate spectral radiance across different temperatures and wavelengths - Graph scientific data clearly using modern plotting best practices - Analyze how temperature shifts affect the peak emission wavelength of stars The course starts with essential physics terminology and foundational concepts before moving into writing clean Python code, managing units, and plotting your final scientific results. This course is designed for beginners to scientific computing and physics students who want to learn Python application; no advanced programming experience is required. Start translating physics theory into functional Python models today.