Parallax, the apparent shift of an object when viewed from two distinct perspectives, is a foundational concept in both astronomy and perception. It forms the basis for measuring distances in celestial observations, as astronomers employ Earth’s orbital path to determine stellar distances by analyzing angular changes. In optics and photography, it accounts for differences in visual alignment, while in human vision, it facilitates depth perception through stereopsis. Authors such as J. A.
Gillet highlighted its significance in celestial mechanics, pointing out that horizontal parallax is most pronounced at the horizon, while Samuel Pierpont Langley compared it to surveying methods. Mary Fairfax Somerville associated parallax with the determination of planetary distances, and Ernest Gallaudet Draper explained its angular changes in relation to altitude. These varied perspectives emphasize parallax’s dual function as a scientific instrument and a perceptual mechanism, connecting vast cosmic dimensions with everyday visual experience.