Station
Similar stations in Indians
Surface Settlement (Odyssey) - 1,368 Ls
Indians Network
Nnadi's Manufacturings
Surface Settlement (Odyssey) - 1,379 Ls
Ironheart Corporation
Iglesias Biochemical Facility
Surface Settlement (Odyssey) - 1,382 Ls
Ironheart Corporation
Leclerc Engineering Base
Surface Settlement (Odyssey) - 1,383 Ls
Ironheart Corporation
Elaschuk Biochemical Institution
Surface Settlement (Odyssey) - 1,384 Ls
Indians Coordinated
Crellin-Davies Industrial Holdings
Surface Settlement (Odyssey) - 1,913 Ls
Ironheart Corporation
Chevalier's Constructions
Surface Settlement (Odyssey) - 1,916 Ls
Protectorate of the Northern Hemisphere
Shao Genetics Assembly
Surface Settlement (Odyssey) - 1,917 Ls
Indians Network
Sasaki Industrial Assembly
Surface Settlement (Odyssey) - 1,922 Ls
Ironheart Corporation
Soria Biochemical Facility
Surface Settlement (Odyssey) - 1,932 Ls
Ironheart Corporation
Motrienko Formulations
Surface Settlement (Odyssey) - 3,515 Ls
Indians Coordinated
Ferreyra Biological
Surface Settlement (Odyssey) - 3,521 Ls
Indians Coordinated
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