Station
Similar stations in HIP 51877
Surface Settlement (Odyssey) - -
HIP 51877 StakeholdersChoi Botanical Plantation
Surface Settlement (Odyssey) - -
Gallo Prospecting
Surface Settlement (Odyssey) - -
Osnovianenko Botanical Facility
Surface Settlement (Odyssey) - -
HIP 51877 Silver BrotherhoodWerner Dredging Base
Surface Settlement (Odyssey) - -
Gabri LabourVaaler Prospecting Installation
Surface Settlement (Odyssey) - 2,147 Ls
Natural Mehit Liberty Party
Kosach Dredging Hub
Surface Settlement (Odyssey) - 2,148 Ls
HIP 51877 Silver Brotherhood
Akpabio Mineralogic Enterprise
Surface Settlement (Odyssey) - 2,156 Ls
Natural Mehit Liberty Party
Oshpak Metallurgic Territory
Surface Settlement (Odyssey) - 2,165 Ls
Natural Mehit Liberty Party
Rawlinson Mining Exchange
Surface Settlement (Odyssey) - 2,181 Ls
Natural Mehit Liberty Party
Lymar's Minerals
Surface Settlement (Odyssey) - 2,183 Ls
Natural Mehit Liberty Party
Webb Drilling Facility
Surface Settlement (Odyssey) - 3,668 Ls
HIP 51877 Silver Brotherhood
Blakytny Nutrition Holdings
Surface Settlement (Odyssey) - 3,672 Ls
HIP 51877 Silver Brotherhood
Lugun Excavation Prospect
Surface Settlement (Odyssey) - 3,672 Ls
HIP 51877 Silver Brotherhood
Bevis Dredging Enterprise
Surface Settlement (Odyssey) - 3,682 Ls
HIP 51877 Silver Brotherhood
Ferraro Metallurgic Base
Surface Settlement (Odyssey) - 3,682 Ls
HIP 51877 Silver Brotherhood
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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