Station
Similar stations in LTT 18075
Surface Settlement (Odyssey) - -
Chauhan Biological
Surface Settlement (Odyssey) - -
LTT 18075 Progressive PartyHidalgo Horticultural Farm
Surface Settlement (Odyssey) - -
NODE 6
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Surface Settlement (Odyssey) - -
30 Lyncis InterstellarOgawa Cultivation Biosphere
Surface Settlement (Odyssey) - -
LTT 18075 Progressive PartyScholey Hydroponics Base
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Surface Settlement (Odyssey) - 697 Ls
Movement for Caraceni Future
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Surface Settlement (Odyssey) - 697 Ls
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Surface Settlement (Odyssey) - 700 Ls
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LTT 18075 Progressive Party
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Surface Settlement (Odyssey) - 704 Ls
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Surface Settlement (Odyssey) - 705 Ls
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Surface Settlement (Odyssey) - 705 Ls
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Surface Settlement (Odyssey) - 705 Ls
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Surface Settlement (Odyssey) - 705 Ls
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Surface Settlement (Odyssey) - 706 Ls
Movement for Caraceni Future
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Surface Settlement (Odyssey) - 707 Ls
Movement for Caraceni Future
Bell Cultivation Estate
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LTT 18075 Progressive PartyQuiroga Research Expedition
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Surface Settlement (Odyssey) - 1,326 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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