Theorie der Bewegung der Himmelskörper Um die Sonne Buchkatalog

Excerpt from Theorie der Bewegung der Himmelskörper Um die Sonne: Nebst Deren Bahnbestimmung in Elementarer DarstellungEs stelle die Ellipse der Figur (fig. 1) die Bahn eines Planeten vor, im Brennpuncte S sei die Sonne. Ist A P die grosse Axel der Ellipse so ist der dem Brennpuncte S näher liegende Punct P zugleich derjenige Punct der Bahn, in welchem der Planet der Sonne am nächsten kommt, und wird daher das Perihelium oder die Sonnennähe ge naunt.About the PublisherForgotten Books publishes hundreds of thousands of rare and classic books. Find more at www.forgottenbooks.comThis book is a reproduction of an important historical work. Forgotten Books uses state-of-the-art technology to digitally reconstruct the work, preserving the original format whilst repairing imperfections present in the aged copy. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in our edition. We do, however, repair the vast majority of imperfections successfully, any imperfections that remain are intentionally left to preserve the state of such historical works.