Station
Similar stations in Devata Baru
Surface Settlement (Odyssey) - -
Traditional Devata Baru Movement
Vasylyshin's Constructions
Surface Settlement (Odyssey) - -
Flanagan Excavation Exchange
Surface Settlement (Odyssey) - 189 Ls
Confederacy of Devata Baru
Fletcher Industrial Complex
Surface Settlement (Odyssey) - 189 Ls
Confederacy of Devata Baru
Uniyal Chemical Silo
Surface Settlement (Odyssey) - 189 Ls
Confederacy of Devata Baru
Gallardo Biochemical Installation
Surface Settlement (Odyssey) - 285 Ls
Confederacy of Devata Baru
Craig Botanical Habitat
Surface Settlement (Odyssey) - 286 Ls
Confederacy of Devata Baru
Favre Manufacturing Site
Surface Settlement (Odyssey) - 286 Ls
Confederacy of Devata Baru
Nnamani Mining Exploration
Surface Settlement (Odyssey) - 286 Ls
Confederacy of Devata Baru
Yi Industrial Holdings
Surface Settlement (Odyssey) - 565 Ls
Confederacy of Devata Baru
Benoit's Workshop
Surface Settlement (Odyssey) - 803 Ls
Deep Space Pirate Federation
Imai Analytics Site
Surface Settlement (Odyssey) - 803 Ls
Unionists of Brynhilo
Li's Chemicals
Surface Settlement (Odyssey) - 803 Ls
Bastogne Private Security Firm
Cheng Industrial Holdings
Surface Settlement (Odyssey) - 10,839 Ls
Confederacy of Devata Baru
Beauregard Engineering Hub
Surface Settlement (Odyssey) - 11,037 Ls
Confederacy of Devata Baru
Yamada's Forge
Surface Settlement (Odyssey) - 11,082 Ls
Confederacy of Devata Baru
Datta Biochemical Installation
Surface Settlement (Odyssey) - 11,354 Ls
Confederacy of Devata Baru
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.
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