Station
Similar stations in HIP 43296
Installation (Government) - -
Justice Party of HIP 43296Bombelli Vista
Surface Settlement (Installation) - -
Justice Party of HIP 43296Dorsey Penal colony
Surface Settlement (Installation) - -
HIP 43296 LabourFrobisher Prospect
Surface Settlement (Installation) - -
Justice Party of HIP 43296Fu Landing +
Surface Settlement (Installation) - -
Macomb Installation
Surface Settlement (Installation) - -
Meikle Oasis
Surface Settlement (Installation) - -
HIP 43296 LabourNixon Prospect +++
Surface Settlement (Installation) - -
Regional Mobile Guard Network
Installation (Security) - -
Oulani Peacekeeping InitiativeRoosevelt Market
Installation (Tourist) - -
Tyurin Refinery
Surface Settlement (Installation) - -
Verne Lab
Surface Settlement (Installation) - -
Justice Party of HIP 43296Wells' Claim
Surface Settlement (Installation) - -
Justice Party of HIP 43296Krisjanis's Folly
Surface Settlement (Installation) - 1,361 Ls
HIP 43296 LabourThorn's Installation
Surface Settlement (Installation) - 1,361 Ls
Justice Party of HIP 43296
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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