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A Plain Method Of Determining The Parallax Of Venus, by James Ferguson, details a method for calculating the parallax of Venus during its transit across the Sun. This work further explains how, through analogy, to derive the parallax and distance of the Sun and all other planets. This historical text offers insights into 18th-century astronomical methods and understanding of the solar system. It remains relevant for those interested in the history of astronomy and the evolution of our understanding of planetary distances.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
