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Evolution of Solar System Models

Sep 3, 2025

Overview

This lecture traces the evolution of solar system models from the geocentric view to the heliocentric model, explaining key astronomical phenomena and their cultural impact.

The Geocentric Model

  • The geocentric model placed Earth at the center of the solar system for centuries.
  • Ptolemy improved the geocentric model by introducing epicycles (small circles superimposed on larger orbits) to explain retrograde motion.
  • Retrograde motion is when a planet appears to move backward in the sky for a short time.

The Heliocentric Model and Copernican Revolution

  • Copernicus revived the heliocentric model, placing the Sun at the center of the solar system.
  • The heliocentric model easily explains retrograde motion as Earth overtaking outer planets in its orbit.
  • Copernicus estimated planetary distances from the sun with geometric calculations.

Parallax and Evidence for Heliocentrism

  • Critics argued that if Earth orbits the Sun, the position of stars should shift (stellar parallax).
  • Stellar parallax is very small due to vast star distances and requires precise telescopes to detect.
  • Parallax is measured by observing a star from different points in Earth’s orbit and using trigonometry to calculate its distance.

Cultural and Philosophical Implications

  • The Copernican model challenged the idea that Earth and humanity are the center of the universe.
  • Giordano Bruno expanded on these ideas, suggesting stars are suns with their own planets.
  • The Catholic Church opposed these views; Bruno was executed for heresy.
  • The scientific revolution faced resistance but helped advance freedom of thought.

Key Terms & Definitions

  • Geocentric Model — Solar system model with Earth at the center.
  • Epicycle — A small circle on which a planet moves, itself moving along a larger orbital circle.
  • Heliocentric Model — Solar system model with the Sun at the center.
  • Retrograde Motion — Apparent backward movement of a planet as seen from Earth.
  • Parallax — Apparent shift in position of an object when viewed from different locations.
  • Astronomical Unit (AU) — Distance from Earth to the Sun (≈ 150 million km).

Action Items / Next Steps

  • Review trigonometry principles, especially regarding right triangles and angle calculations.
  • Continue with the next lecture to learn how astronomers developed the Copernican model further.