Station
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Surface Settlement (Odyssey) - 34 Ls
The Altruists
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Surface Settlement (Odyssey) - 34 Ls
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Surface Settlement (Odyssey) - 34 Ls
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Surface Settlement (Odyssey) - 34 Ls
Freedom Party of Ho Hsi
Nakamura Excavation Territory
Surface Settlement (Odyssey) - 34 Ls
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Tapia Manufacturing
Surface Settlement (Odyssey) - 34 Ls
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Surface Settlement (Odyssey) - 1,109 Ls
Ho Hsi Jet Comms Limited
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Surface Settlement (Odyssey) - 1,109 Ls
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Surface Settlement (Odyssey) - 1,110 Ls
Ho Hsi Jet Comms LimitedTakeda's Foundry
Surface Settlement (Odyssey) - 1,111 Ls
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Surface Settlement (Odyssey) - 1,112 Ls
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Surface Settlement (Odyssey) - 1,112 Ls
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Prieto's Hold
Surface Settlement (Odyssey) - 1,112 Ls
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Yamashita Chemical Holdings
Surface Settlement (Odyssey) - 1,112 Ls
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Ibanez Forge
Surface Settlement (Odyssey) - 1,113 Ls
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Surface Settlement (Odyssey) - 1,133 Ls
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Mendoza Entertainment Complex
Surface Settlement (Odyssey) - 2,639 Ls
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Dyachenko Leisure Resort
Surface Settlement (Odyssey) - 2,642 Ls
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Maier Heights
Surface Settlement (Odyssey) - 2,642 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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