Station
Similar stations in HIP 116710
Surface Settlement (Odyssey) - 140 Ls
HIP 116710 Guardians
Klein Agricultural Biosphere
Surface Settlement (Odyssey) - 140 Ls
ELITE UNITED WORLDS
Mohanty Horticultural Biosphere
Surface Settlement (Odyssey) - 140 Ls
HIP 116710 Guardians
Munn's Habitat
Surface Settlement (Odyssey) - 140 Ls
HIP 116710 Guardians
Durand Botanical Complex
Surface Settlement (Odyssey) - 260 Ls
HIP 116710 Transport Network
Figueroa Horticultural Market
Surface Settlement (Odyssey) - 260 Ls
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Rey Cultivation Hub
Surface Settlement (Odyssey) - 260 Ls
HIP 116710 Guardians
Rybalka Nutrition Facility
Surface Settlement (Odyssey) - 260 Ls
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Yakimchuk Nutrition Biome
Surface Settlement (Odyssey) - 260 Ls
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Datta Manufacturing Base
Surface Settlement (Odyssey) - 1,657 Ls
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Lafitte's Vista
Surface Settlement (Odyssey) - 1,657 Ls
HIP 116710 GuardiansShao Industrial Site
Surface Settlement (Odyssey) - 1,657 Ls
Likedeeler of Michel
Song Synthetics Base
Surface Settlement (Odyssey) - 1,657 Ls
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Beauchene Horticultural Farm
Surface Settlement (Odyssey) - 10,641 Ls
HIP 116710 Guardians
Okwo Horticultural Estate
Surface Settlement (Odyssey) - 10,686 Ls
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Lugun Botanical Market
Surface Settlement (Odyssey) - 10,745 Ls
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Colley Cultivation Holding
Surface Settlement (Odyssey) - 10,765 Ls
Likedeeler of Michel
Mofu Cultivation Enterprise
Surface Settlement (Odyssey) - 10,782 Ls
HIP 116710 Guardians
Knowles Nutrition Centre
Surface Settlement (Odyssey) - 10,800 Ls
HIP 116710 Transport Network
Otanez Synthetics Depot
Surface Settlement (Odyssey) - 10,807 Ls
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Surface Settlement (Odyssey) - 10,895 Ls
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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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