Station
Similar stations in HIP 38129
Surface Settlement (Installation) - -
Klikumad ConfederationCarpini Beacon
Surface Settlement (Installation) - -
Christopher Oasis
Surface Settlement (Installation) - -
HIP 38129 Republic PartyCount
Installation (Civilian) - -
Diamond Beacon
Surface Settlement (Installation) - -
Klikumad ConfederationDrexler Works +++
Surface Settlement (Installation) - -
Fiennes Hub
Surface Settlement (Installation) - -
Klikumad ConfederationGalactic Project Satellite
Installation (Comms) - -
Hambly Works
Surface Settlement (Installation) - -
Klikumad ConfederationHoyle Prospect
Surface Settlement (Installation) - -
HIP 38129 Republic PartyPurple Galaxies Co.
- -
HIP 38129 Republic PartyRoddenberry Base
Surface Settlement (Installation) - -
The Order of The Black LionRusch's Progress
Surface Settlement (Installation) - -
Klikumad ConfederationZajdel Laboratory +++
Surface Settlement (Installation) - -
Klikumad ConfederationClute's Inheritance
Surface Settlement (Installation) - 156 Ls
The Order of The Black LionGeston Depot
Surface Settlement (Installation) - 156 Ls
Klikumad Confederation
Galpedia
Isaac Newton
Sir Isaac Newton PRS MP (/ˈnjuːtən/; 25 December 1642 – 20 March 1726/7) was an English physicist and mathematician (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time and as a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia Mathematica ("Mathematical Principles of Natural Philosophy"), first published in 1687, laid the foundations for classical mechanics. Newton made seminal contributions to optics, and he shares credit with Gottfried Leibniz for the development of calculus.
Newton's Principia formulated the laws of motion and universal gravitation, which dominated scientists' view of the physical universe for the next three centuries. By deriving Kepler's laws of planetary motion from his mathematical description of gravity, and then using the same principles to account for the trajectories of comets, the tides, the precession of the equinoxes, and other phenomena, Newton removed the last doubts about the validity of the heliocentric model of the cosmos. This work also demonstrated that the motion of objects on Earth and of celestial bodies could be described by the same principles. His prediction that the Earth should be shaped as an oblate spheroid was later vindicated by the measurements of Maupertuis, La Condamine, and others, which helped convince most Continental European scientists of the superiority of Newtonian mechanics over the earlier system of Descartes.
Wikipedia text is available under the Creative Commons Attribution/Share-Alike License; additional terms may apply. Wikipedia image: Wikipedia / CC-BY-SA-3.0