Galileo and his successors utilized various celestial bodies to demonstrate that the Earth orbits the Sun, a concept that would be challenging to prove in a hypothetical solar system devoid of moons and planets. The parallax method, where the apparent movement of nearby stars relative to distant ones is observed from different positions on Earth, serves as a key technique for establishing this heliocentric model. Observations of the phases of Venus and Mercury further support the heliocentric theory, as their phases cannot be explained by a geocentric model. Modern technology, such as telescopes and high-resolution photography, can facilitate these observations, although they require sophisticated equipment. Ultimately, the heliocentric model simplifies the explanation of celestial motions, making it easier to understand the dynamics of the solar system.