Station
Similar stations in Primpo
Surface Settlement (Odyssey) - -
Independents of HIP 9599Morita Foods
Surface Settlement (Odyssey) - 22 Ls
People's HIP 10175 for Equality
Knowles Cultivation Centre
Surface Settlement (Odyssey) - 30 Ls
People's HIP 10175 for Equality
Hawkins Hydroponics
Surface Settlement (Odyssey) - 37 Ls
People's HIP 10175 for Equality
Schneider Prospecting Exchange
Surface Settlement (Odyssey) - 43 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 43 Ls
Independents of HIP 9599
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Surface Settlement (Odyssey) - 44 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 49 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 52 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 52 Ls
People's HIP 10175 for Equality
Ele Dredging Exchange
Surface Settlement (Odyssey) - 412 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 412 Ls
People's HIP 10175 for Equality
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Surface Settlement (Odyssey) - 633 Ls
People's HIP 10175 for Equality
Jayashankar's Biological
Surface Settlement (Odyssey) - 2,523 Ls
Earls of Primpo
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Surface Settlement (Odyssey) - 3,579 Ls
People's HIP 10175 for Equality
Abe Industrial Silo
Surface Settlement (Odyssey) - 3,627 Ls
People's HIP 10175 for Equality
Lavigne Chemical Base
Surface Settlement (Odyssey) - 3,802 Ls
Confederacy of Primpo
Eames Research Institution
Surface Settlement (Odyssey) - 3,909 Ls
Confederacy of Primpo
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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