This volume reproduces mathematically significant extracts from the
extant manuscript record of Newton's researches during 1684-5 into the
dynamical motion of bodies under the deviating action of a central
force, and his subsequent struggles thereby to explain the observed
motions of solar comets and of the moon. The short tract De motu
Corporum, which Newton initially composed on this topic in the early
autumn of 1684, was primarily built around his earlier proof that in the
absence of external perturbation a planetary eclipse may be traversed
under an inverse-square force pull to its solar focus, but also
discussed the simplest case of resisted ballistic motion. In epilogue,
excerpts from his abandoned grand scheme for revising the Principia in
the early 1690s detail Newton's planned refinements to his printed
exposition of central force, both simplifying and extending it,
introducing therein a novel general fluxional measure of such force -
but failing adequately to apply it to the primary case of conic motion.