Station
Similar stations in LP 417-213
Surface Settlement (Odyssey) - -
Liberals of LP 417-213
Florianz Hydroponics Estate
Surface Settlement (Odyssey) - 14 Ls
The FatherhoodMacleod Nutrition Nursery
Surface Settlement (Odyssey) - 21 Ls
The FatherhoodOpeyemi Horticultural Estate
Surface Settlement (Odyssey) - 21 Ls
Traditional LP 417-213 Conservatives
Beausoleil Horticultural Enterprise
Surface Settlement (Odyssey) - 37 Ls
The FatherhoodBlakytny Hydroponics Exchange
Surface Settlement (Odyssey) - 37 Ls
LP 417-213 Power SolutionsWilliams Leisure
Surface Settlement (Odyssey) - 2,043 Ls
The Fatherhood
Gimenez's Horizon
Surface Settlement (Odyssey) - 2,076 Ls
The FatherhoodJenkerson Visitor Complex
Surface Settlement (Odyssey) - 2,323 Ls
The Fatherhood
Maruyama Lodgings
Surface Settlement (Odyssey) - 2,326 Ls
The Fatherhood
Soh Synthetics Workshop
Surface Settlement (Odyssey) - 2,342 Ls
Dominion of LP 417-213
Sosa's Dock
Surface Settlement (Odyssey) - 2,405 Ls
The FatherhoodGarcia Tourism Complex
Surface Settlement (Odyssey) - 2,471 Ls
LP 417-213 Power Solutions
Furnival Defence Enterprise
Surface Settlement (Odyssey) - 2,581 Ls
Liberals of LP 417-213
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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