Station
Similar stations in HIP 62686
Surface Settlement (Odyssey) - -
Karpenko Agricultural Estate
Surface Settlement (Odyssey) - -
Otto Chemical
Surface Settlement (Odyssey) - -
Yang Horticultural Site
Surface Settlement (Odyssey) - -
Poirier Dredging Reserve
Surface Settlement (Odyssey) - 1,400 Ls
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Surface Settlement (Odyssey) - 1,403 Ls
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Surface Settlement (Odyssey) - 1,404 Ls
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Surface Settlement (Odyssey) - 1,408 Ls
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Surface Settlement (Odyssey) - 1,410 Ls
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Surface Settlement (Odyssey) - 1,416 Ls
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Surface Settlement (Odyssey) - 1,422 Ls
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Surface Settlement (Odyssey) - 1,425 Ls
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Surface Settlement (Odyssey) - 1,426 Ls
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Surface Settlement (Odyssey) - 1,427 Ls
Posse of HIP 62686
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Surface Settlement (Odyssey) - 1,432 Ls
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Surface Settlement (Odyssey) - 1,442 Ls
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Surface Settlement (Odyssey) - 1,443 Ls
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Faconti Industrial Assembly
Surface Settlement (Odyssey) - 1,444 Ls
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Suarez Agricultural Holdings
Surface Settlement (Odyssey) - 2,066 Ls
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Avery Agricultural Habitat
Surface Settlement (Odyssey) - 2,095 Ls
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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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