caa a22 4500 477114458 CHVBK 20180405111618.0 cr unu---uuuuu 170330e19960801xx s 000 0 eng 10.1007/BF02327155 doi (NATIONALLICENCE)springer-10.1007/BF02327155 Speiser David CH-4144 Arlesheim Scuola Normale Superiore, Pisa aut The Kepler Problem from Newton to Johann Bernoulli [Elektronische Daten] [David Speiser] Summary: Newton solved what was called afterwards for a short time "the directKepler problem” ("le problème direct”): given a curve (e.g. an ellipse) and the center of attraction (e.g. the focus), what is the law of this attraction ifKepler's second law holds? The "problème inverse” (today: the "problème direct”) was attacked system-atically only later, first byJacob Hermann, then solved completely byJohann Bernoulli in 1710 and followingBernoulli byPierre Varignon. How didBernoulli solve the problem? What method did he use for this purpose and which of his accomplishments do we still follow today? In the second part various questions connected to the first part are dealt with from the point of view, Conflict and Cooperation, suggested byJ. van Maanen to the participants of the Groningen conference. Springer-Verlag, 1996 Archive for History of Exact Sciences Springer-Verlag 50/2(1996-08-01), 103-116 0003-9519 50:2<103 1996 50 407 https://doi.org/10.1007/BF02327155 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF02327155 text/html Onlinezugriff via DOI NATIONALLICENCE 100 1- Speiser David CH-4144 Arlesheim Scuola Normale Superiore, Pisa aut NATIONALLICENCE 773 0- Archive for History of Exact Sciences Springer-Verlag 50/2(1996-08-01), 103-116 0003-9519 50:2<103 1996 50 407 Metadata rights reserved Springer special CC-BY-NC licence nationallicence SWISSBIB 114763828 BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer