Station
Similar stations in Arakwibut
Surface Settlement (Odyssey) - 435 Ls
Arakwibut Systems
Murdoch's Workshop
Surface Settlement (Odyssey) - 435 Ls
Regulatory State of Arakwibut
Bray Synthetics Exchange
Surface Settlement (Odyssey) - 947 Ls
Black Widow
Nightingale Industrial Installation
Surface Settlement (Odyssey) - 948 Ls
Arakwibut Co
Bruneau Manufacturing Silo
Surface Settlement (Odyssey) - 949 Ls
Arakwibut Systems
Uniyal Synthetics Foundry
Surface Settlement (Odyssey) - 1,221 Ls
Arakwibut Co
Deshmukh Industrial Assembly
Surface Settlement (Odyssey) - 1,222 Ls
Black Widow
Maruyama Astrophysics Enterprise
Surface Settlement (Odyssey) - 1,227 Ls
Arakwibut Co
Nightingale Leisure District
Surface Settlement (Odyssey) - 1,227 Ls
Black Widow
Soulier Engineering Hub
Surface Settlement (Odyssey) - 1,227 Ls
Black Widow
Grushevsky Arms Stockade
Surface Settlement (Odyssey) - 1,228 Ls
Black Widow
Casari Synthetics Exchange
Surface Settlement (Odyssey) - 3,108 Ls
Arakwibut Co
Knowles's Haven
Surface Settlement (Odyssey) - 3,114 Ls
Black Widow
Ren Industrial Depot
Surface Settlement (Odyssey) - 3,118 Ls
Black Widow
Tavernier Industrial Moulding
Surface Settlement (Odyssey) - 3,127 Ls
Black Widow
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