Station
Similar stations in Chique
Surface Settlement (Odyssey) - -
Open Pilot's Initiative
Ukah Manufacturing Installation
Surface Settlement (Odyssey) - -
Chung Boarding Lodge
Surface Settlement (Odyssey) - 108 Ls
Open Pilot's Initiative
Corner Chemical Foundry
Surface Settlement (Odyssey) - 108 Ls
Open Pilot's Initiative
Smoszna Synthetics Site
Surface Settlement (Odyssey) - 108 Ls
Open Pilot's Initiative
Allegro House
Surface Settlement (Odyssey) - 195 Ls
Open Pilot's Initiative
Davidenko Industrial Forge
Surface Settlement (Odyssey) - 195 Ls
Alliance of Kicho
Elaschuk Horticultural Farm
Surface Settlement (Odyssey) - 195 Ls
Open Pilot's Initiative
Vannier Agricultural Centre
Surface Settlement (Odyssey) - 195 Ls
Open Pilot's Initiative
Yuschenko Chemical Site
Surface Settlement (Odyssey) - 195 Ls
Chique Energy Inc
Ferenczi-Houlden Cultivation Holding
Surface Settlement (Odyssey) - 278 Ls
Open Pilot's Initiative
Ma Synthetics Exchange
Surface Settlement (Odyssey) - 278 Ls
Chique Energy Inc
Levada Biochemical Enterprise
Surface Settlement (Odyssey) - 3,887 Ls
Open Pilot's Initiative
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