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・ Timeline of the development of tectonophysics (before 1954)
・ Timeline of the discovery and classification of minerals
・ Timeline of the Eastern Front of World War II
・ Timeline of the economy of the Indian subcontinent
・ Timeline of the Egyptian Crisis under Mohamed Morsi
・ Timeline of the Egyptian Crisis under the Supreme Council of the Armed Forces
・ Timeline of the Egyptian Revolution of 2011
・ Timeline of the electric motor
・ Timeline of the English Civil War
・ Timeline of the English Poor Law system
・ Timeline of the English Reformation
・ Timeline of the Eurofighter Typhoon
・ Timeline of the Euromaidan
・ Timeline of the European colonization of North America
・ Timeline of the evolutionary history of life
Timeline of the far future
・ Timeline of the flag of the United States
・ Timeline of the formation of the Universe
・ Timeline of the French Revolution
・ Timeline of the Front de libération du Québec
・ Timeline of the Fukushima Daiichi nuclear disaster
・ Timeline of the future
・ Timeline of the future of the universe
・ Timeline of the Gallipoli Campaign
・ Timeline of the Gaza War (2008–09)
・ Timeline of the geologic history of the United States
・ Timeline of the Gezi Park protests
・ Timeline of the governorship of Ezenwo Nyesom Wike
・ Timeline of the Great Depression
・ Timeline of the Great Purge


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Timeline of the far future : ウィキペディア英語版
Timeline of the far future

While scientific predictions of the future can never be absolutely certain, present understanding in various fields allows for the prediction of far future events, if only in the broadest strokes. These fields include astrophysics, which has revealed how planets and stars form, interact, and die; particle physics, which has revealed how matter behaves at the smallest scales; evolutionary biology, which predicts how life will evolve over time; and plate tectonics, which shows how continents shift over millennia.
All projections of the future of the Earth, the Solar System, and the Universe must account for the second law of thermodynamics, which states that entropy, or a loss of the energy available to do work, must increase over time.〔 Stars eventually must exhaust their supply of hydrogen fuel and burn out. Close encounters gravitationally fling planets from their star systems, and star systems from galaxies.〔 Eventually, matter itself is expected to come under the influence of radioactive decay, as even the most stable materials break apart into subatomic particles.〔 Current data suggests that the Universe is flat, and thus, will not collapse in on itself after a finite time,〔 and the infinite future potentially allows for the occurrence of a number of massively improbable events, such as the formation of a Boltzmann brain.〔
The timelines displayed here cover events from roughly eight thousand years from now to the furthest reaches of future time. A number of alternate future events are listed to account for questions still unresolved, such as whether humans will become extinct, whether protons decay, or whether Earth will survive the Sun's expansion into a red giant.
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抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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