Station
Similar stations in LP 399-165
Surface Settlement (Odyssey) - -
Yare Industrial Complex
Surface Settlement (Odyssey) - -
Koo's Laboratory
Surface Settlement (Odyssey) - 3,618 Ls
Union of LP 399-165 Union
Blayney Chemical Depot
Surface Settlement (Odyssey) - 3,709 Ls
Union of LP 399-165 Union
Chamapiwa Manufacturing Base
Surface Settlement (Odyssey) - 3,721 Ls
Union of LP 399-165 Union
Thakur Industrial Facility
Surface Settlement (Odyssey) - 3,726 Ls
Union of LP 399-165 Union
Skovoroda's Workshop
Surface Settlement (Odyssey) - 3,762 Ls
Union of LP 399-165 Union
Cho Analytics
Surface Settlement (Odyssey) - 3,777 Ls
Union of LP 399-165 Union
Mannan Excavation Station
Surface Settlement (Odyssey) - 3,791 Ls
Union of LP 399-165 Union
Moulin Engineering Exchange
Surface Settlement (Odyssey) - 3,794 Ls
Union of LP 399-165 Union
Hou's Laboratory
Surface Settlement (Odyssey) - 3,804 Ls
Union of LP 399-165 Union
Navarrete's Workshop
Surface Settlement (Odyssey) - 3,824 Ls
Union of LP 399-165 Union
Yoshida Engineering Facility
Surface Settlement (Odyssey) - 3,831 Ls
Union of LP 399-165 Union
Pettitt Synthetics
Surface Settlement (Odyssey) - 3,870 Ls
LP 399-165 Autocracy
Bernard Chemical Complex
Surface Settlement (Odyssey) - 3,874 Ls
Union of LP 399-165 Union
Abimbola Industrial Works
Surface Settlement (Odyssey) - 3,891 Ls
Union of LP 399-165 Union
Ferreira Industrial Foundry
Surface Settlement (Odyssey) - 4,076 Ls
Union of LP 399-165 Union
Gunther's Engineering
Surface Settlement (Odyssey) - 4,183 Ls
Union of LP 399-165 Union
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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