Station
Similar stations in Rudjer Boskovic
Surface Settlement (Odyssey) - 540 Ls
B.I.G. - Balkan Intergalactic Guerilla
Rayne Hydroponics Biome
Surface Settlement (Odyssey) - 540 Ls
B.I.G. - Balkan Intergalactic Guerilla
Yuan Agricultural Farm
Surface Settlement (Odyssey) - 540 Ls
B.I.G. - Balkan Intergalactic Guerilla
Mulford Chemical Enterprise
Surface Settlement (Odyssey) - 3,519 Ls
B.I.G. - Balkan Intergalactic Guerilla
Scholz's Shelter
Surface Settlement (Odyssey) - 3,519 Ls
B.I.G. - Balkan Intergalactic Guerilla
Schaeffer Industries
Surface Settlement (Odyssey) - 3,521 Ls
B.I.G. - Balkan Intergalactic Guerilla
Rhee Industrial Complex
Surface Settlement (Odyssey) - 3,526 Ls
B.I.G. - Balkan Intergalactic Guerilla
Mangal Biological Installation
Surface Settlement (Odyssey) - 5,091 Ls
B.I.G. - Balkan Intergalactic Guerilla
Maslo Chemical Facility
Surface Settlement (Odyssey) - 5,091 Ls
B.I.G. - Balkan Intergalactic Guerilla
Sibanda's Dream
Surface Settlement (Odyssey) - 5,091 Ls
Enigma Dyson Syndicate
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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