Lecture
This lecture focuses on the properties and applications of ellipses in both astronomy and mathematics. It begins with a historical overview, highlighting Kepler's significant contributions to the understanding of planetary motion, specifically the elliptical orbits of planets around the sun. The instructor explains the transition from the geocentric model to the heliocentric model, emphasizing Kepler's three laws of planetary motion. The discussion then shifts to the mathematical definition of an ellipse, detailing its five fundamental parameters: the semi-major axis, semi-minor axis, focal distance, eccentricity, and the directrix. The lecture illustrates how these parameters relate to the geometric properties of ellipses and their representation in conic sections. The instructor also introduces practical applications of ellipses in architecture and stereotomy, demonstrating how these mathematical concepts can be applied in real-world scenarios. The session concludes with a focus on the construction of ellipses using various methods, including the gardener's string method, and the importance of understanding these shapes in both theoretical and practical contexts.