Station
Similar stations in Daisamaskap
Surface Settlement (Odyssey) - -
Zeng Mineralogic Territory
Surface Settlement (Odyssey) - -
Kohli's Mine
Surface Settlement (Odyssey) - 2,086 Ls
Steven Gordon Jolliffe
Goloborodko Prospecting Territory
Surface Settlement (Odyssey) - 2,089 Ls
Steven Gordon Jolliffe
Mori Metallurgic Base
Surface Settlement (Odyssey) - 2,094 Ls
Steven Gordon Jolliffe
Stein Extraction Rigs
Surface Settlement (Odyssey) - 2,803 Ls
Steven Gordon Jolliffe
Salinas's Reserve
Surface Settlement (Odyssey) - 2,807 Ls
Steven Gordon Jolliffe
Rivas Cultivation Site
Surface Settlement (Odyssey) - 4,099 Ls
Freedom Party of Daisamaskap
Richter Nurseries
Surface Settlement (Odyssey) - 4,109 Ls
Steven Gordon Jolliffe
Babu Nutrition Biome
Surface Settlement (Odyssey) - 4,112 Ls
Steven Gordon Jolliffe
Shen Cultivation Habitat
Surface Settlement (Odyssey) - 4,112 Ls
Steven Gordon Jolliffe
Hahm Mining Facility
Surface Settlement (Odyssey) - 4,114 Ls
Steven Gordon Jolliffe
Oluwusi Hydroponics Habitat
Surface Settlement (Odyssey) - 43,618 Ls
Daisamaskap Ring
Staff Extraction Territory
Surface Settlement (Odyssey) - 44,855 Ls
Steven Gordon Jolliffe
Rodgers Horticultural Exchange
Surface Settlement (Odyssey) - 45,119 Ls
Steven Gordon Jolliffe
Parkhomenko Mining Platform
Surface Settlement (Odyssey) - 45,581 Ls
Steven Gordon Jolliffe
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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