The Distance Of The Sun From The Earth Determined, By The Theory Of Gravity (1763)

Exploring the theory of gravity, this scientific treatise delves into the methods used to measure the distance between the Earth and the Sun. Matthew Stewart introduces gravity's role in planetary motion, detailing historical techniques like the transit of Venus and parallax. He presents his own mathematical approach, addressing factors influencing accuracy, supported by illustrations and historical context. This work serves as a significant resource for those interested in the evolution of scientific understanding in astronomy, preserved as a facsimile reprint.