Station
Similar stations in Hoora Ating
Surface Settlement (Odyssey) - 497 Ls
LTT 8657 Patron's Principles
Richter Cultivation Base
Surface Settlement (Odyssey) - 497 Ls
Independents of Hoora Ating
Richards Industrial Foundry
Surface Settlement (Odyssey) - 3,967 Ls
LTT 8657 Patron's Principles
Pereyra Forge
Surface Settlement (Odyssey) - 3,975 Ls
Imperial Grey Wolves
Yi's Command
Surface Settlement (Odyssey) - 30,343 Ls
Imperial Grey Wolves
Anderson Industrial Complex
Surface Settlement (Odyssey) - 30,528 Ls
Society of Hoora Ating
Godoy Excavation Facility
Surface Settlement (Odyssey) - 30,651 Ls
Ixchertha Services
Miyamoto Excavation Platform
Surface Settlement (Odyssey) - 30,651 Ls
Imperial Grey Wolves
Lagarde's Drilling
Surface Settlement (Odyssey) - 30,659 Ls
Imperial Grey Wolves
Holloway Military Barracks
Surface Settlement (Odyssey) - 30,704 Ls
Imperial Grey Wolves
Deloney Mining Complex
Surface Settlement (Odyssey) - 30,790 Ls
Imperial Grey Wolves
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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