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Timeline of the far future

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A dark gray and red sphere representing the Earth lies against a black background to the right of an orange circular object representing the Sun
Artist's concept of the Earth several billion years from now, when the Sun is a red giant.

While the future cannot be predicted with certainty, present understanding in various scientific fields allows for the prediction of some far-future events, if only in the broadest outline.[1][2] 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 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 rise over time.[3] Stars will eventually exhaust their supply of hydrogen fuel and burn out. Close encounters between astronomical objects gravitationally fling planets from their star systems, and star systems from galaxies.[4]

Physicists expect that matter itself will eventually come under the influence of radioactive decay, as even the most stable materials break apart into subatomic particles.[5] Current data suggest that the universe has a flat geometry (or very close to flat), and thus will not collapse in on itself after a finite time,[6] and the infinite future allows for the occurrence of a number of massively improbable events, such as the formation of Boltzmann brains.[7]

The timelines displayed here cover events from the beginning of the 4th millennium (which begins in 3001 CE) to the furthest reaches of future time. A number of alternative future events are listed to account for questions still unresolved, such as whether humans will become extinct, whether protons decay, and whether the Earth survives when the Sun expands to become a red giant.


Astronomy and astrophysics Astronomy and astrophysics
Geology and planetary science Geology and planetary science
Biology Biology
Particle physics Particle physics
Mathematics Mathematics
Technology and culture Technology and culture

Earth, the Solar System and the universe[edit]

Key.svg Years from now Event
Astronomy and astrophysics 2,000 The average length of a solar day is likely to exceed 86,400¹⁄₃₀ SI seconds due to lunar tides decelerating the Earth's rotation, making the current UTC standard of inserting a leap second only at the end of a UTC month insufficient to keep UTC within one second of UT1 at all times. To compensate, either leap seconds will have to be added at multiple times during the month or multiple leap seconds will have to be added at the end of some or all months.[8]
Geology and planetary science 10,000 If a failure of the Wilkes Subglacial Basin "ice plug" in the next few centuries were to endanger the East Antarctic Ice Sheet, it would take up to this long to melt completely. Sea levels would rise 3 to 4 metres.[9] One of the potential long-term effects of global warming, this is separate from the shorter-term threat of the West Antarctic Ice Sheet.
Astronomy and astrophysics 10,000[note 1] The red supergiant star Antares will likely have exploded in a supernova. The explosion should be easily visible on Earth in daylight.[10]
Astronomy and astrophysics 13,000 By this point, halfway through the precessional cycle, Earth's axial tilt will be reversed, causing summer and winter to occur on opposite sides of Earth's orbit. This means that the seasons in the Northern Hemisphere, which experiences more pronounced seasonal variation due to a higher percentage of land, will be even more extreme, as it will be facing towards the Sun at Earth's perihelion and away from the Sun at aphelion.[11]
Geology and planetary science 15,000 According to the Sahara pump theory, the precession of Earth's poles will move the North African Monsoon far enough north to convert the Sahara back into having a tropical climate, as it had 5,000–10,000 years ago.[12][13]
Geology and planetary science 17,000[note 1] Best-guess recurrence rate for a "civilization-threatening" supervolcanic eruption large enough to spew 1,000 gigatonnes of pyroclastic material.[14][15]
Geology and planetary science 25,000 The northern Martian polar ice cap could recede as Mars reaches a warming peak of the northern hemisphere during the c. 50,000-year perihelion precession aspect of its Milankovitch cycle.[16][17]
Astronomy and astrophysics 36,000 The small red dwarf Ross 248 will pass within 3.024 light-years of Earth, becoming the closest star to the Sun.[18] It will recede after about 8,000 years, making first Alpha Centauri (again) and then Gliese 445 the nearest stars[18] (see timeline).
Geology and planetary science 50,000 According to Berger and Loutre (2002), the current interglacial period will end,[19] sending the Earth back into a glacial period of the current ice age, regardless of the effects of anthropogenic global warming.

According to more recent studies however (2016), the effects of anthropogenic global warming may delay this otherwise expected glacial period by another 50,000 years, effectively skipping it.[20]

The Niagara Falls will have eroded away the remaining 32 km to Lake Erie, and will cease to exist.[21]

The many glacial lakes of the Canadian Shield will have been erased by post-glacial rebound and erosion.[22]

Astronomy and astrophysics 50,000 The length of the day used for astronomical timekeeping reaches about 86,401 SI seconds due to lunar tides decelerating the Earth's rotation. Under the present-day timekeeping system, either a leap second would need to be added to the clock every single day, or else by then, in order to compensate, the length of the day would have had to have been officially lengthened by one SI second.[8]
Astronomy and astrophysics 100,000 The proper motion of stars across the celestial sphere, which results from their movement through the Milky Way, renders many of the constellations unrecognizable by someone used to today's configuration.[23]
Astronomy and astrophysics 100,000[note 1] The hypergiant star VY Canis Majoris will likely have exploded in a supernova.[24]
Biology 100,000 Native North American earthworms, such as Megascolecidae, will have naturally spread north through the United States Upper Midwest to the Canada–US border, recovering from the Laurentide Ice Sheet glaciation (38°N to 49°N), assuming a migration rate of 10 metres per year.[25] (However, humans have already introduced non-native invasive earthworms of North America on a much shorter timescale, causing a shock to the regional ecosystem.)
Geology and planetary science > 100,000 As one of the long-term effects of global warming, 10% of anthropogenic carbon dioxide will still remain in a stabilized atmosphere.[26]
Geology and planetary science 250,000 Lōʻihi, the youngest volcano in the Hawaiian–Emperor seamount chain, will rise above the surface of the ocean and become a new volcanic island.[27]
Astronomy and astrophysics c. 300,000[note 1] At some point in the next few hundred thousand years, the Wolf–Rayet star WR 104 may explode in a supernova. There is a small chance WR 104 is spinning fast enough to produce a gamma-ray burst, and an even smaller chance that such a GRB could pose a threat to life on Earth.[28][29]
Astronomy and astrophysics 500,000[note 1] Earth will likely have been hit by an asteroid of roughly 1 km in diameter, assuming that it cannot be averted.[30]
Geology and planetary science 500,000 The rugged terrain of Badlands National Park in South Dakota will have eroded away completely.[31]
Geology and planetary science 1 million Meteor Crater, a large impact crater in Arizona considered the "freshest" of its kind, will have eroded away.[32]
Astronomy and astrophysics 1 million[note 1] Highest estimated time until the red supergiant star Betelgeuse explodes in a supernova. For at least a few months, the supernova will be visible on Earth in daylight. Studies suggest this supernova will occur within a million years, and perhaps even as little as the next 100,000 years.[33][34]
Astronomy and astrophysics 1 million[note 1] Desdemona and Cressida, moons of Uranus, will likely have collided.[35]
Astronomy and astrophysics 1.28 ± 0.05 million The star Gliese 710 will pass as close as 0.0676 parsecs—0.221 light-years (14,000 astronomical units)[36] to the Sun before moving away. This will gravitationally perturb members of the Oort cloud, a halo of icy bodies orbiting at the edge of the Solar System, thereafter raising the likelihood of a cometary impact in the inner Solar System.[37]
Biology 2 million Estimated time for the recovery of coral reef ecosystems from human-caused ocean acidification; the recovery of marine ecosystems after the acidification event that occurred about 65 million years ago took a similar length of time.[38]
Geology and planetary science 2 million+ The Grand Canyon will erode further, deepening slightly, but principally widening into a broad valley surrounding the Colorado River.[39]
Astronomy and astrophysics 2.7 million Average orbital half-life of current centaurs, that are unstable because of gravitational interaction of the several outer planets.[40] See predictions for notable centaurs.
Astronomy and astrophysics 3 million Due to the gradual slowing down of Earth's rotation, a day on Earth will be one minute longer than it is today.[41]
Geology and planetary science 10 million The widening East African Rift valley is flooded by the Red Sea, causing a new ocean basin to divide the continent of Africa[42] and the African Plate into the newly formed Nubian Plate and the Somali Plate.
Biology 10 million Estimated time for full recovery of biodiversity after a potential Holocene extinction, if it were on the scale of the five previous major extinction events.[43]

Even without a mass extinction, by this time most current species will have disappeared through the background extinction rate, with many clades gradually evolving into new forms.[44][45]

Astronomy and astrophysics 10 million – 1 billion[note 1] Cupid and Belinda, moons of Uranus, will likely have collided.[35]
Astronomy and astrophysics 50 million Maximum estimated time before the moon Phobos collides with Mars.[46]
Geology and planetary science 50 million According to Christopher R. Scotese, the movement of the San Andreas Fault will cause the Gulf of California to flood into the Central Valley. This will form a new inland sea on the West Coast of North America, causing the current locations of Los Angeles and San Francisco to merge.[47] The Californian coast will begin to be subducted into the Aleutian Trench.[48]

Africa's collision with Eurasia will close the Mediterranean Basin and create a mountain range similar to the Himalayas.[49]

The Appalachian Mountains peaks will largely erode away,[50] weathering at 5.7 Bubnoff units, although topography will actually rise as regional valleys deepen at twice this rate.[51]

Geology and planetary science 50–60 million The Canadian Rockies will erode away to a plain, assuming a rate of 60 Bubnoff units.[52] The Southern Rockies in the United States are eroding at a somewhat slower rate.[53]
Geology and planetary science 50–400 million Estimated time for Earth to naturally replenish its fossil fuel reserves.[54]
Geology and planetary science 80 million The Big Island will have become the last of the current Hawaiian Islands to sink beneath the surface of the ocean, while a more recently formed chain of "new Hawaiian Islands" will then have emerged in their place.[55]
Astronomy and astrophysics 100 million[note 1] Earth will likely have been hit by an asteroid comparable in size to the one that triggered the K–Pg extinction 66 million years ago, assuming this cannot be averted.[56]
Geology and planetary science 100 million According to the Pangaea Proxima Model created by Christopher R. Scotese, a new subduction zone will open in the Atlantic Ocean and the Americas will begin to converge back toward Africa.[47]
Geology and planetary science 100 million Upper estimate for lifespan of the rings of Saturn in their current state.[57]
Astronomy and astrophysics 110 million The Sun's luminosity has increased by 1%.[58]
Astronomy and astrophysics 180 million Due to the gradual slowing down of Earth's rotation, a day on Earth will be one hour longer than it is today.[59]
Mathematics 230 million Prediction of the orbits of the planets is impossible over greater time spans than this, due to the limitations of Lyapunov time.[60]
Astronomy and astrophysics 240 million From its present position, the Solar System completes one full orbit of the Galactic Center.[61]
Geology and planetary science 250 million According to Christopher R. Scotese, due to the northward movement of the West Coast of North America, the coast of California will collide with Alaska.[47]
Geology and planetary science 250–350 million All the continents on Earth may fuse into a supercontinent. Three potential arrangements of this configuration have been dubbed Amasia, Novopangaea, and Pangaea Ultima.[47][62] This will likely result in a glacial period, lowering sea levels and increasing oxygen levels, further lowering global temperatures.[63][64]
Biology > 250 million Rapid biological evolution may occur due to the formation of a supercontinent causing lower temperatures and higher oxygen levels.[64] Increased competition between species due to the formation of a supercontinent, increased volcanic activity and less hospitable conditions due to global warming from a brighter Sun could result in a mass extinction event from which plant and animal life may not fully recover.[65]
Geology and planetary science 300 million Due to a shift in the equatorial Hadley cells to roughly 40° north and south, the amount of arid land will increase by 25%.[65]
Geology and planetary science 300–600 million Estimated time for Venus's mantle temperature to reach its maximum. Then, over a period of about 100 million years, major subduction occurs and the crust is recycled.[66]
Geology and planetary science 350 million According to the extroversion model first developed by Paul F. Hoffman, subduction ceases in the Pacific Ocean Basin.[67][68][62]
Geology and planetary science 400–500 million The supercontinent (Pangaea Ultima, Novopangaea, or Amasia) will likely have rifted apart.[62] This will likely result in higher global temperatures, similar to the Cretaceous period.[64]
Astronomy and astrophysics 500 million[note 1] Estimated time until a gamma-ray burst, or massive, hyperenergetic supernova, occurs within 6,500 light-years of Earth; close enough for its rays to affect Earth's ozone layer and potentially trigger a mass extinction, assuming the hypothesis is correct that a previous such explosion triggered the Ordovician–Silurian extinction event. However, the supernova would have to be precisely oriented relative to Earth to have any such effect.[69]
Astronomy and astrophysics 600 million Tidal acceleration moves the Moon far enough from Earth that total solar eclipses are no longer possible.[70]
Geology and planetary science 500–600 million The Sun's increasing luminosity begins to disrupt the carbonate–silicate cycle; higher luminosity increases weathering of surface rocks, which traps carbon dioxide in the ground as carbonate. As water evaporates from the Earth's surface, rocks harden, causing plate tectonics to slow and eventually stop once the oceans evaporate completely. With less volcanism to recycle carbon into the Earth's atmosphere, carbon dioxide levels begin to fall.[71] By this time, carbon dioxide levels will fall to the point at which C3 photosynthesis is no longer possible. All plants that utilize C3 photosynthesis (≈99 percent of present-day species) will die.[72] The extinction of C3 plant life is likely to be a long-term decline rather than a sharp drop. It is likely that plant groups will die one by one well before the critical carbon dioxide level is reached. The first plants to disappear will be C3 herbaceous plants, followed by deciduous forests, evergreen broad-leaf forests and finally evergreen conifers.[65]
Biology 500–800 million[note 1] As Earth begins to rapidly warm and carbon dioxide levels fall, plants—and, by extension, animals—could survive longer by evolving other strategies such as requiring less carbon dioxide for photosynthetic processes, becoming carnivorous, adapting to desiccation, or associating with fungi. These adaptations are likely to appear near the beginning of the moist greenhouse.[65] The death of most plant life will result in less oxygen in the atmosphere, allowing for more DNA-damaging ultraviolet radiation to reach the surface. The rising temperatures will increase chemical reactions in the atmosphere, further lowering oxygen levels. Flying animals would be better off because of their ability to travel large distances looking for cooler temperatures.[73] Many animals may be driven to the poles or possibly underground. These creatures would become active during the polar night and aestivate during the polar day due to the intense heat and radiation. Much of the land would become a barren desert, and plants and animals would primarily be found in the oceans.[73]
Biology 800–900 million Carbon dioxide levels will fall to the point at which C4 photosynthesis is no longer possible.[72] Without plant life to recycle oxygen in the atmosphere, free oxygen and the ozone layer will disappear from the atmosphere allowing for intense levels of deadly UV light to reach the surface. In the book The Life and Death of Planet Earth, authors Peter D. Ward and Donald Brownlee state that some animal life may be able to survive in the oceans. Eventually, however, all multicellular life will die out.[74] At most, animal life could survive about 100 million years after plant life dies out, with the last animals being animals that do not depend on living plants such as termites or those near hydrothermal vents such as worms of the genus Riftia.[65] The only life left on the Earth after this will be single-celled organisms.
Geology and planetary science 1 billion[note 2] 27% of the ocean's mass will have been subducted into the mantle. If this were to continue uninterrupted, it would reach an equilibrium where 65% of present-day surface water would be subducted.[75]
Geology and planetary science 1.1 billion The Sun's luminosity will have risen by 10%, causing Earth's surface temperatures to reach an average of around 320 K (47 °C; 116 °F). The atmosphere will become a "moist greenhouse", resulting in a runaway evaporation of the oceans.[71][76] This would cause plate tectonics to stop completely, if not already stopped before this time.[77] Pockets of water may still be present at the poles, allowing abodes for simple life.[78][79]
Biology 1.2 billion High estimate until all plant life dies out, assuming some form of photosynthesis is possible despite extremely low carbon dioxide levels. If this is possible, rising temperatures will make any animal life unsustainable from this point on.[80][81][82]
Biology 1.3 billion Eukaryotic life dies out on Earth due to carbon dioxide starvation. Only prokaryotes remain.[74]
Astronomy and astrophysics 1.5–1.6 billion The Sun's rising luminosity causes its circumstellar habitable zone to move outwards; as carbon dioxide rises in Mars's atmosphere, its surface temperature rises to levels akin to Earth during the ice age.[74][83]
Biology 1.6 billion Lower estimate until all prokaryotic life will go extinct.[74]
Geology and planetary science 2 billion High estimate until the Earth's oceans evaporate if the atmospheric pressure were to decrease via the nitrogen cycle.[84]
Geology and planetary science 2.3 billion The Earth's outer core freezes if the inner core continues to grow at its current rate of 1 mm (0.039 in) per year.[85][86] Without its liquid outer core, the Earth's magnetic field shuts down,[87] and charged particles emanating from the Sun gradually deplete the atmosphere.[88]
Astronomy and astrophysics 2.55 billion The Sun will have reached a maximum surface temperature of 5,820 K (5,550 °C; 10,020 °F). From then on, it will become gradually cooler while its luminosity will continue to increase.[76]
Geology and planetary science 2.8 billion Earth's surface temperature will reach around 420 K (147 °C; 296 °F), even at the poles.[71][89]
Biology 2.8 billion All life, which by now had been reduced to unicellular colonies in isolated, scattered microenvironments such as high-altitude lakes or caves, goes extinct.[71][89]
Astronomy and astrophysics c. 3 billion[note 1] There is a roughly 1-in-100,000 chance that the Earth might be ejected into interstellar space by a stellar encounter before this point, and a 1-in-3-million chance that it will then be captured by another star. Were this to happen, life, assuming it survived the interstellar journey, could potentially continue for far longer.[90]
Astronomy and astrophysics 3 billion Median point at which the Moon's increasing distance from the Earth lessens its stabilising effect on the Earth's axial tilt. As a consequence, Earth's true polar wander becomes chaotic and extreme, leading to dramatic shifts in the planet's climate due to the changing axial tilt.[91]
Astronomy and astrophysics 3.3 billion 1% chance that Jupiter's gravity may make Mercury's orbit so eccentric as to collide with Venus, sending the inner Solar System into chaos. Possible scenarios include Mercury colliding with the Sun, being ejected from the Solar System, or colliding with Earth.[92]
Geology and planetary science 3.5–4.5 billion All water currently present in oceans (if not lost earlier) evaporates. The greenhouse effect caused by the massive, water-rich atmosphere, combined with the Sun's luminosity reaching roughly 35–40% above its present value, will result in Earth's surface temperature rising to 1,400 K (1,130 °C; 2,060 °F)—hot enough to melt some surface rock.[77][84][93][94]
Astronomy and astrophysics 3.6 billion Neptune's moon Triton falls through the planet's Roche limit, potentially disintegrating into a planetary ring system similar to Saturn's.[95]
Astronomy and astrophysics 4 billion Median point by which the Andromeda Galaxy will have collided with the Milky Way, which will thereafter merge to form a galaxy dubbed "Milkomeda".[96] There is also a small chance of the Solar System being ejected.[97][98] The planets of the Solar System will almost certainly not be disturbed by these events.[99][100][101]
Geology and planetary science 4.5 billion Mars reaches the same solar flux the Earth did when it first formed, 4.5 billion years ago from today.[83]
Astronomy and astrophysics 5.4 billion With the hydrogen supply exhausted at its core, the Sun leaves the main sequence and begins to evolve into a red giant.[102]
Geology and planetary science 6.5 billion Mars reaches the same solar radiation flux as Earth today, after which it will suffer a similar fate to the Earth as described above.[83]
Astronomy and astrophysics 7.5 billion Earth and Mars may become tidally locked with the expanding subgiant Sun.[83]
Astronomy and astrophysics 7.59 billion The Earth and Moon are very likely destroyed by falling into the Sun, just before the Sun reaches the tip of its red giant phase and its maximum radius of 256 times the present-day value.[102][note 3] Before the final collision, the Moon possibly spirals below Earth's Roche limit, breaking into a ring of debris, most of which falls to the Earth's surface.[103]

During this era, Saturn's moon Titan may reach surface temperatures necessary to support life.[104]

Astronomy and astrophysics 7.9 billion The Sun reaches the tip of the red-giant branch of the Hertzsprung–Russell diagram, achieving its maximum radius of 256 times the present-day value.[105] In the process, Mercury, Venus, and very likely Earth are destroyed.[102]
Astronomy and astrophysics 8 billion The Sun becomes a carbon–oxygen white dwarf with about 54.05% its present mass.[102][106][107][108] At this point, if somehow the Earth survives, temperatures on the surface of the planet, as well as other remaining planets in the Solar System, will begin dropping rapidly, due to the white dwarf Sun emitting much less energy than it does today.
Astronomy and astrophysics 22 billion The end of the Universe in the Big Rip scenario, assuming a model of dark energy with w = −1.5.[109][110] If the density of dark energy is less than −1, then the Universe's expansion would continue to accelerate and the Observable Universe would continue to get smaller. Around 200 million years before the Big Rip, galaxy clusters like the Local Group or the Sculptor Group would be destroyed. Sixty million years before the Big Rip, all galaxies will begin to lose stars around their edges and will completely disintegrate in another 40 million years. Three months before the Big Rip, all star systems will become gravitationally unbound, and planets will fly off into the rapidly expanding universe. Thirty minutes before the Big Rip, planets, stars, asteroids and even extreme objects like neutron stars and black holes will evaporate into atoms. One hundred zeptoseconds (10−19 seconds) before the Big Rip, atoms would break apart. Ultimately, once rip reaches the Planck scale, cosmic strings would be disintegrated as well as the fabric of spacetime itself. The universe would enter into a "rip singularity" when all distances become infinitely large. Whereas in a "crunch singularity" all matter is infinitely concentrated, in a "rip singularity" all matter is infinitely spread out.[111] However, observations of galaxy cluster speeds by the Chandra X-ray Observatory suggest that the true value of w is c. −0.991, meaning the Big Rip will not occur.[112]
Astronomy and astrophysics 50 billion If the Earth and Moon are not engulfed by the Sun, by this time they will become tidelocked, with each showing only one face to the other.[113][114] Thereafter, the tidal action of the white dwarf Sun will extract angular momentum from the system, causing the lunar orbit to decay and the Earth's spin to accelerate.[115]
Astronomy and astrophysics 65 billion The Moon may end up colliding with the Earth due to the decay of its orbit, assuming the Earth and Moon are not engulfed by the red giant Sun.[116]
Astronomy and astrophysics 100–150 billion The Universe's expansion causes all galaxies beyond the former Milky Way's Local Group to disappear beyond the cosmic light horizon, removing them from the observable universe.[117]
Astronomy and astrophysics 150 billion The cosmic microwave background cools from its current temperature of c. 2.7 K (−270.45 °C; −454.81 °F) to 0.3 K (−272.850 °C; −459.130 °F), rendering it essentially undetectable with current technology.[118]
Astronomy and astrophysics 325 billion Estimated time by which the expansion of the universe isolates all gravitationally bound structures within their own cosmological horizon. At this point, the universe has expanded by a factor of more than 100 million, and even individual exiled stars are isolated.[119]
Astronomy and astrophysics 450 billion Median point by which the c. 47 galaxies[120] of the Local Group will coalesce into a single large galaxy.[5]
Astronomy and astrophysics 800 billion Expected time when the net light emission from the combined "Milkomeda" galaxy begins to decline as the red dwarf stars pass through their blue dwarf stage of peak luminosity.[121]
Astronomy and astrophysics 1012 (1 trillion) Low estimate for the time until star formation ends in galaxies as galaxies are depleted of the gas clouds they need to form stars.[5]

The Universe's expansion, assuming a constant dark energy density, multiplies the wavelength of the cosmic microwave background by 1029, exceeding the scale of the cosmic light horizon and rendering its evidence of the Big Bang undetectable. However, it may still be possible to determine the expansion of the universe through the study of hypervelocity stars.[117]

Astronomy and astrophysics 1.05×1012 (1.05 trillion) Estimated time by which the Universe will have expanded by a factor of more than 1026, reducing the average particle density to less than one particle per cosmological horizon volume. Beyond this point, particles of unbound intergalactic matter are effectively isolated, and collisions between them cease to affect the future evolution of the Universe.[119]
Astronomy and astrophysics 2×1012 (2 trillion) Estimated time by which all objects beyond our Local Group are redshifted by a factor of more than 1053. Even the highest energy gamma rays are stretched so that their wavelength is greater than the physical diameter of the horizon.[122]
Astronomy and astrophysics 4×1012 (4 trillion) Estimated time until the red dwarf star Proxima Centauri, the closest star to the Sun at a distance of 4.25 light-years, leaves the main sequence and becomes a white dwarf.[123]
Astronomy and astrophysics 1013 (10 trillion) Estimated time of peak habitability in the universe, unless habitability around low-mass stars is suppressed.[124]
Astronomy and astrophysics 1.2×1013 (12 trillion) Estimated time until the red dwarf VB 10, as of 2016 the least massive main sequence star with an estimated mass of 0.075 M, runs out of hydrogen in its core and becomes a white dwarf.[125][126]
Astronomy and astrophysics 3×1013 (30 trillion) Estimated time for stars (including the Sun) to undergo a close encounter with another star in local stellar neighborhoods. Whenever two stars (or stellar remnants) pass close to each other, their planets' orbits can be disrupted, potentially ejecting them from the system entirely. On average, the closer a planet's orbit to its parent star the longer it takes to be ejected in this manner, because it is gravitationally more tightly bound to the star.[127]
Astronomy and astrophysics 1014 (100 trillion) High estimate for the time by which normal star formation ends in galaxies.[5] This marks the transition from the Stelliferous Era to the Degenerate Era; with no free hydrogen to form new stars, all remaining stars slowly exhaust their fuel and die.[4] By this time, the universe will have expanded by a factor of approximately 102554.[119]
Astronomy and astrophysics 1.1–1.2×1014 (110–120 trillion) Time by which all stars in the universe will have exhausted their fuel (the longest-lived stars, low-mass red dwarfs, have lifespans of roughly 10–20 trillion years).[5] After this point, the stellar-mass objects remaining are stellar remnants (white dwarfs, neutron stars, black holes) and brown dwarfs.

Collisions between brown dwarfs will create new red dwarfs on a marginal level: on average, about 100 stars will be shining in what was once the Milky Way. Collisions between stellar remnants will create occasional supernovae.[5]

Astronomy and astrophysics 1015 (1 quadrillion) Estimated time until stellar close encounters detach all planets in star systems (including the Solar System) from their orbits.[5]

By this point, the Sun will have cooled to 5 K (−268.15 °C; −450.67 °F).[128]

Astronomy and astrophysics 1019 to 1020
(10–100 quintillion)
Estimated time until 90–99% of brown dwarfs and stellar remnants (including the Sun) are ejected from galaxies. When two objects pass close enough to each other, they exchange orbital energy, with lower-mass objects tending to gain energy. Through repeated encounters, the lower-mass objects can gain enough energy in this manner to be ejected from their galaxy. This process eventually causes the Milky Way to eject the majority of its brown dwarfs and stellar remnants.[5][129]
Astronomy and astrophysics 1020 (100 quintillion) Estimated time until the Earth collides with the black dwarf Sun due to the decay of its orbit via emission of gravitational radiation,[130] if the Earth is not ejected from its orbit by a stellar encounter or engulfed by the Sun during its red giant phase.[130]
Astronomy and astrophysics 1023 (100 sextillion) Around this timescale most stellar remnants and other objects are ejected from the remains of their galactic cluster.[131]
Astronomy and astrophysics 1030 (1 nonillion) Estimated time until those stellar remnants not ejected from galaxies (1–10%) fall into their galaxies' central supermassive black holes. By this point, with binary stars having fallen into each other, and planets into their stars, via emission of gravitational radiation, only solitary objects (stellar remnants, brown dwarfs, ejected planetary-mass objects, black holes) will remain in the universe.[5]
Particle physics 2×1036 Estimated time for all nucleons in the observable universe to decay, if the hypothesized proton half-life takes its smallest possible value (8.2×1033 years).[132][133][note 4]
Particle physics 3×1043 Estimated time for all nucleons in the observable universe to decay, if the hypothesized proton half-life takes the largest possible value, 1041 years,[5] assuming that the Big Bang was inflationary and that the same process that made baryons predominate over anti-baryons in the early Universe makes protons decay.[133][note 4] By this time, if protons do decay, the Black Hole Era, in which black holes are the only remaining celestial objects, begins.[4][5]
Particle physics 1065 Assuming that protons do not decay, estimated time for rigid objects, from free-floating rocks in space to planets, to rearrange their atoms and molecules via quantum tunneling. On this timescale, any discrete body of matter "behaves like a liquid" and becomes a smooth sphere due to diffusion and gravity.[130]
Particle physics 2×1066 Estimated time until a black hole of 1 solar mass decays into subatomic particles by Hawking radiation.[134]
Particle physics 6×1099 Estimated time until the supermassive black hole of TON 618, as of 2018 the most massive known with a mass of 66 billion solar masses, dissipates by the emission of Hawking radiation,[134] assuming zero angular momentum (that it does not rotate).
Particle physics 1.7×10106 Estimated time until a supermassive black hole with a mass of 20 trillion solar masses decays by Hawking radiation.[134] This marks the end of the Black Hole Era. Beyond this time, if protons do decay, the Universe enters the Dark Era, in which all physical objects have decayed to subatomic particles, gradually winding down to their final energy state in the heat death of the universe.[4][5]
Particle physics 10139 2018 estimate of Standard Model lifetime before collapse of a false vacuum; 95% confidence interval is 1058 to 10241 years due in part to uncertainty about the top quark mass.[135]
Particle physics 10200 Estimated high time for all nucleons in the observable universe to decay, if they do not via the above process, through any one of many different mechanisms allowed in modern particle physics (higher-order baryon non-conservation processes, virtual black holes, sphalerons, etc.) on time scales of 1046 to 10200 years.[4]
Particle physics 101100-32000 Estimated time for those black dwarfs with masses at or above 1.2 times the mass of the Sun to undergo supernovae as a result of slow silicon-nickel-iron fusion, as the declining electron fraction lowers their Chandrasekhar limit, assuming protons do not decay.[136]
Particle physics 101500 Assuming protons do not decay, the estimated time until all baryonic matter in stellar-mass objects has either fused together via muon-catalyzed fusion to form iron-56 or decayed from a higher mass element into iron-56 to form an iron star.[130]
Particle physics [note 5][note 6] Conservative estimate for the time until all iron stars collapse via quantum tunnelling into black holes, assuming no proton decay or virtual black holes.[130]

On this vast timescale, even ultra-stable iron stars will have been destroyed by quantum tunnelling events. First iron stars of sufficient mass (somewhere between 0.2 M and the Chandrasekhar limit[137]) will collapse via tunnelling into neutron stars. Subsequently, neutron stars and any remaining iron stars heavier than the Chandrasekhar limit collapse via tunnelling into black holes. The subsequent evaporation of each resulting black hole into subatomic particles (a process lasting roughly 10100 years), and subsequent shift to the Dark Era is on these timescales instantaneous.

Particle physics [note 1][note 6][note 7] Estimated time for a Boltzmann brain to appear in the vacuum via a spontaneous entropy decrease.[7]
Particle physics [note 6] High estimate for the time until all iron stars collapse into black holes, assuming no proton decay or virtual black holes,[130] which then (on these timescales) instantaneously evaporate into subatomic particles.

This is also the highest estimate possible time for Black Hole Era (and subsequent Dark Era) to finally commence. Beyond this point, it is almost certain that Universe will contain no more baryonic matter and will be an almost pure vacuum (possibly accompanied with the presence of a false vacuum) until it reaches its final energy state, assuming it does not happen before this time.

Particle physics [note 6] Highest estimate for the time it takes for the universe to reach its final energy state, even in the presence of a false vacuum.[7]
Particle physics [note 1][note 6] Time for quantum effects to generate a new Big Bang, resulting in a new universe. Around this vast timeframe, quantum tunnelling in any isolated patch of the now-empty universe could generate new inflationary events, resulting in new Big Bangs giving birth to new universes.[138]

(Because the total number of ways in which all the subatomic particles in the observable universe can be combined is ,[139][140] a number which, when multiplied by , disappears into the rounding error, this is also the time required for a quantum-tunnelled and quantum fluctuation-generated Big Bang to produce a new universe identical to our own, assuming that every new universe contained at least the same number of subatomic particles and obeyed laws of physics within the landscape predicted by string theory.)[141][142]


Key.svg Years from now Event
technology and culture 10,000 Most probable estimated lifespan of technological civilization, according to Frank Drake's original formulation of the Drake equation.[143]
Biology 10,000 If globalization trends lead to panmixia, human genetic variation will no longer be regionalized, as the effective population size will equal the actual population size.[144]
Mathematics 10,000 Humanity has a 95% probability of being extinct by this date, according to Brandon Carter's formulation of the controversial Doomsday argument, which argues that half of the humans who will ever have lived have probably already been born.[145]
technology and culture 20,000 According to the glottochronology linguistic model of Morris Swadesh, future languages should retain just 1 out of 100 "core vocabulary" words on their Swadesh list compared to that of their current progenitors.[146]
Geology and planetary science 100,000+ Time required to terraform Mars with an oxygen-rich breathable atmosphere, using only plants with solar efficiency comparable to the biosphere currently found on Earth.[147]
Technology and culture 1 million Estimated shortest time by which humanity could colonize our Milky Way galaxy and become capable of harnessing all the energy of the galaxy, assuming a velocity of 10% the speed of light.[148]
Biology 2 million Vertebrate species separated for this long will generally undergo allopatric speciation.[149] Evolutionary biologist James W. Valentine predicted that if humanity has been dispersed among genetically isolated space colonies over this time, the galaxy will host an evolutionary radiation of multiple human species with a "diversity of form and adaptation that would astound us".[150] This would be a natural process of isolated populations, unrelated to potential deliberate genetic enhancement technologies.
Mathematics 7.8 million Humanity has a 95% probability of being extinct by this date, according to J. Richard Gott's formulation of the controversial Doomsday argument.[151]
technology and culture 100 million Maximal estimated lifespan of technological civilization, according to Frank Drake's original formulation of the Drake equation.[152]
Astronomy and astrophysics 1 billion Estimated time for an astroengineering project to alter the Earth's orbit, compensating for the Sun's rising brightness and outward migration of the habitable zone, accomplished by repeated asteroid gravity assists.[153][154]

Spacecraft and space exploration[edit]

To date five spacecraft (Voyager 1, Voyager 2, Pioneer 10, Pioneer 11 and New Horizons) are on trajectories which will take them out of the Solar System and into interstellar space. Barring an extremely unlikely collision with some object, the craft should persist indefinitely.[155]

Key.svg Years from now Event
Astronomy and astrophysics 1,000 The SNAP-10A nuclear satellite, launched in 1965 to an orbit 700 km (430 mi) above Earth, will return to the surface.[156][157]
Astronomy and astrophysics 16,900 Voyager 1 passes within 3.5 light-years of Proxima Centauri.[158]
Astronomy and astrophysics 18,500 Pioneer 11 passes within 3.4 light-years of Alpha Centauri.[158]
Astronomy and astrophysics 20,300 Voyager 2 passes within 2.9 light-years of Alpha Centauri.[158]
Astronomy and astrophysics 25,000 The Arecibo message, a collection of radio data transmitted on 16 November 1974, reaches the distance of its destination, the globular cluster Messier 13.[159] This is the only interstellar radio message sent to such a distant region of the galaxy. There will be a 24-light-year shift in the cluster's position in the galaxy during the time it takes the message to reach it, but as the cluster is 168 light-years in diameter, the message will still reach its destination.[160] Any reply will take at least another 25,000 years from the time of its transmission (assuming faster-than-light communication is impossible).
Astronomy and astrophysics 33,800 Pioneer 10 passes within 3.4 light-years of Ross 248.[158]
Astronomy and astrophysics 34,400 Pioneer 10 passes within 3.4 light-years of Alpha Centauri.[158]
Astronomy and astrophysics 42,200 Voyager 2 passes within 1.7 light-years of Ross 248.[158]
Astronomy and astrophysics 44,100 Voyager 1 passes within 1.8 light-years of Gliese 445.[158]
Astronomy and astrophysics 46,600 Pioneer 11 passes within 1.9 light-years of Gliese 445.[158]
Astronomy and astrophysics 50,000 The KEO space time capsule, if it is launched, will reenter Earth's atmosphere.[161]
Astronomy and astrophysics 90,300 Pioneer 10 passes within 0.76 light-years of HIP 117795.[158]
Astronomy and astrophysics 306,100 Voyager 1 passes within 1 light-year of TYC 3135-52-1.[158]
Astronomy and astrophysics 492,300 Voyager 1 passes within 1.3 light-years of HD 28343.[158]
Astronomy and astrophysics 800,000–8 million Low estimate of Pioneer 10 plaque lifespan, before the etching is destroyed by poorly-understood interstellar erosion processes.[162]
Astronomy and astrophysics 1.2 million Pioneer 11 comes within 3 light-years of Delta Scuti.[158]
Astronomy and astrophysics 1.3 million Pioneer 10 comes within 1.5 light-years of HD 52456.[158]
Astronomy and astrophysics 2 million Pioneer 10 passes near the bright star Aldebaran.[163]
Astronomy and astrophysics 4 million Pioneer 11 passes near one of the stars in the constellation Aquila.[163]
Astronomy and astrophysics 8 million The LAGEOS satellites' orbits will decay, and they will re-enter Earth's atmosphere, carrying with them a message to any far future descendants of humanity, and a map of the continents as they are expected to appear then.[164]
Astronomy and astrophysics 1 billion Estimated lifespan of the two Voyager Golden Records, before the information stored on them is rendered unrecoverable.[165]
Astronomy and astrophysics 1020 (100 quintillion) Estimated timescale for the Pioneer and Voyager spacecraft to collide with a star (or stellar remnant).[158]

Technological projects[edit]

Key.svg Date or years from now Event
technology and culture 3015 CE A camera, placed at the ASU Art Museum in 2015 by Jonathon Keats, will finish its 1,000-year-long exposure of the city of Tempe, Arizona.[166]
technology and culture 3183 CE The Time Pyramid, a public art work started in 1993 at Wemding, Germany, is scheduled for completion.[167]
technology and culture 6939 CE The Westinghouse Time Capsules from the years 1939 and 1964 are scheduled to be opened.[168]
technology and culture 7000 CE The last Expo '70 Time Capsule from the year 1970, buried under a monument near Osaka Castle, Japan is scheduled to be opened.[169]
technology and culture 28 May 8113 CE The Crypt of Civilization, a time capsule located at Oglethorpe University in Atlanta, Georgia, is scheduled to be opened after being sealed before World War II.[170][171]
technology and culture 10,000 Planned lifespan of the Long Now Foundation's several ongoing projects, including a 10,000-year clock known as the Clock of the Long Now, the Rosetta Project, and the Long Bet Project.[172]

Estimated lifespan of the HD-Rosetta analog disc, an ion beam-etched writing medium on nickel plate, a technology developed at Los Alamos National Laboratory and later commercialized. (The Rosetta Project uses this technology, named after the Rosetta Stone.)

Biology 10,000 Projected lifespan of Norway's Svalbard Global Seed Vault.[173]
technology and culture 1 million Estimated lifespan of Memory of Mankind (MOM) self storage-style repository in Hallstatt salt mine in Austria, which stores information on inscribed tablets of stoneware.[174]
technology and culture 1 million Planned lifespan of the Human Document Project being developed at the University of Twente in the Netherlands.[175]
technology and culture 292,278,994 CE
(292 million)
Numeric overflow in system time for Java computer programs.[176]
technology and culture 1 billion Estimated lifespan of "Nanoshuttle memory device" using an iron nanoparticle moved as a molecular switch through a carbon nanotube, a technology developed at the University of California at Berkeley.[177]
technology and culture > 13 billion Estimated lifespan of "Superman memory crystal" data storage using femtosecond laser-etched nanostructures in glass, a technology developed at the University of Southampton.[178][179]
technology and culture 292,277,026,596 CE
(292 billion)
Numeric overflow in system time for 64-bit Unix systems.[180]

Human constructs[edit]

Key.svg Years from now Event
Geology and planetary science 50,000 Estimated atmospheric lifetime of tetrafluoromethane, the most durable greenhouse gas.[181]
Geology and planetary science 1 million Current glass objects in the environment will be decomposed.[182]

Various public monuments composed of hard granite will have eroded one metre, in a moderate climate, assuming a rate of 1 Bubnoff unit (1 mm in 1,000 years, or ≈1 inch in 25,000 years).[183]

Without maintenance, the Great Pyramid of Giza will erode into unrecognizability.[184]

On the Moon, Neil Armstrong's "one small step" footprint at Tranquility Base will erode by this time, along with those left by all twelve Apollo moonwalkers, due to the accumulated effects of space weathering.[185][186] (Normal erosion processes active on Earth are not present due to the Moon's almost complete lack of atmosphere.)

Geology and planetary science 7.2 million Without maintenance, Mount Rushmore will erode into unrecognizability.[187]
Geology and planetary science 100 million Future archaeologists should be able to identify an "Urban Stratum" of fossilized great coastal cities, mostly through the remains of underground infrastructure such as building foundations and utility tunnels.[188]

Nuclear power[edit]

Key.svg Years from now Event
Particle physics 10,000 The Waste Isolation Pilot Plant, for nuclear weapons waste, is planned to be protected until this time, with a "Permanent Marker" system designed to warn off visitors through both multiple languages (the six UN languages and Navajo) and through pictograms.[189] The Human Interference Task Force has provided the theoretical basis for United States plans for future nuclear semiotics.
Particle physics 24,000 The Chernobyl Exclusion Zone, the 2,600-square-kilometre (1,000 sq mi) area of Ukraine and Belarus left deserted by the 1986 Chernobyl disaster, will return to normal levels of radiation.[190]
Geology and planetary science 30,000 Estimated supply lifespan of fission-based breeder reactor reserves, using known sources, assuming 2009 world energy consumption.[191]
Geology and planetary science 60,000 Estimated supply lifespan of fission-based light-water reactor reserves if it is possible to extract all the uranium from seawater, assuming 2009 world energy consumption.[191]
Particle physics 211,000 Half-life of technetium-99, the most important long-lived fission product in uranium-derived nuclear waste.
Particle physics 250,000 The estimated minimum time at which the spent plutonium stored at New Mexico's Waste Isolation Pilot Plant will cease to be radiologically lethal to humans.[192]
Particle physics 15.7 million Half-life of iodine-129, the most durable long-lived fission product in uranium-derived nuclear waste.
Geology and planetary science 60 million Estimated supply lifespan of fusion power reserves if it is possible to extract all the lithium from seawater, assuming 1995 world energy consumption.[193]
Geology and planetary science 5 billion Estimated supply lifespan of fission-based breeder reactor reserves if it is possible to extract all the uranium from seawater, assuming 1983 world energy consumption.[194]
Geology and planetary science 150 billion Estimated supply lifespan of fusion power reserves if it is possible to extract all the deuterium from seawater, assuming 1995 world energy consumption.[193]

Graphical timelines[edit]

For graphical, logarithmic timelines of these events see:

See also[edit]


  1. ^ a b c d e f g h i j k l m n This represents the time by which the event will most probably have happened. It may occur randomly at any time from the present.
  2. ^ Units are short scale.
  3. ^ This has been a tricky question for quite a while; see the 2001 paper by Rybicki, K. R. and Denis, C. However, according to the latest calculations, this happens with a very high degree of certainty.
  4. ^ a b Around 264 half-lives. Tyson et al. employ the computation with a different value for half-life.
  5. ^ is 1 followed by 1026 (100 septillion) zeroes
  6. ^ a b c d e Although listed in years for convenience, the numbers beyond this point are so vast that their digits would remain unchanged regardless of which conventional units they were listed in, be they nanoseconds or star lifespans.
  7. ^ is 1 followed by 1050 (100 quindecillion) zeroes


  1. ^ Rescher, Nicholas (1998). Predicting the future: An introduction to the theory of forecasting. State University of New York Press. ISBN 978-0791435533.
  2. ^ "" (PDF).
  3. ^ Nave, C.R. "Second Law of Thermodynamics". Georgia State University. Retrieved 3 December 2011.
  4. ^ a b c d e Adams, Fred; Laughlin, Greg (1999). The Five Ages of the Universe. New York: The Free Press. ISBN 978-0684854229.
  5. ^ a b c d e f g h i j k l Adams, Fred C.; Laughlin, Gregory (1997). "A dying universe: the long-term fate and evolution of astrophysical objects". Reviews of Modern Physics. 69 (2): 337–372. arXiv:astro-ph/9701131. Bibcode:1997RvMP...69..337A. doi:10.1103/RevModPhys.69.337. S2CID 12173790.
  6. ^ Komatsu, E.; Smith, K. M.; Dunkley, J.; et al. (2011). "Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation". The Astrophysical Journal Supplement Series. 192 (2): 18. arXiv:1001.4731. Bibcode:2011ApJS..192...19W. doi:10.1088/0067-0049/192/2/18. S2CID 17581520.
  7. ^ a b c Linde, Andrei (2007). "Sinks in the Landscape, Boltzmann Brains and the Cosmological Constant Problem". Journal of Cosmology and Astroparticle Physics. 2007 (1): 022. arXiv:hep-th/0611043. Bibcode:2007JCAP...01..022L. CiteSeerX doi:10.1088/1475-7516/2007/01/022. S2CID 16984680.
  8. ^ a b Finkleman, David; Allen, Steve; Seago, John; Seaman, Rob; Seidelmann, P. Kenneth (June 2011). "The Future of Time: UTC and the Leap Second". American Scientist. 99 (4): 312. arXiv:1106.3141. Bibcode:2011arXiv1106.3141F. doi:10.1511/2011.91.312. S2CID 118403321.
  9. ^ Mengel, M.; Levermann, A. (4 May 2014). "Ice plug prevents irreversible discharge from East Antarctica". Nature Climate Change. 4 (6): 451–455. Bibcode:2014NatCC...4..451M. doi:10.1038/nclimate2226.
  10. ^ Hockey, T.; Trimble, V. (2010). "Public reaction to a V = −12.5 supernova". The Observatory. 130 (3): 167. Bibcode:2010Obs...130..167H.
  11. ^ Plait, Phil (2002). Bad Astronomy: Misconceptions and Misuses Revealed, from Astrology to the Moon Landing "Hoax". John Wiley and Sons. pp. 55–56.[ISBN missing]
  12. ^ Mowat, Laura (14 July 2017). "Africa's desert to become lush green tropics as monsoons MOVE to Sahara, scientists say". Daily Express. Retrieved 23 March 2018.
  13. ^ "Orbit: Earth's Extraordinary Journey". ExptU. 23 December 2015. Archived from the original on 14 July 2018. Retrieved 23 March 2018.
  14. ^ "'Super-eruption' timing gets an update – and not in humanity's favour". Nature. 30 November 2017. p. 8. doi:10.1038/d41586-017-07777-6. Retrieved 28 August 2020.
  15. ^ "Scientists predict a volcanic eruption that would destroy humanity could happen sooner than previously thought". The Independent. Retrieved 28 August 2020.
  16. ^ Schorghofer, Norbert (23 September 2008). "Temperature response of Mars to Milankovitch cycles". Geophysical Research Letters. 35 (18): L18201. Bibcode:2008GeoRL..3518201S. doi:10.1029/2008GL034954.
  17. ^ Beech, Martin (2009). Terraforming: The Creating of Habitable Worlds. Springer. pp. 138–142.
  18. ^ a b Matthews, R. A. J. (Spring 1994). "The Close Approach of Stars in the Solar Neighborhood". Quarterly Journal of the Royal Astronomical Society. 35 (1): 1. Bibcode:1994QJRAS..35....1M.
  19. ^ Berger, A & Loutre, MF (2002). "Climate: an exceptionally long interglacial ahead?". Science. 297 (5585): 1287–1288. doi:10.1126/science.1076120. PMID 12193773. S2CID 128923481.
  20. ^ "Human-made climate change suppresses the next ice age – Potsdam Institute for Climate Impact Research". Retrieved 21 October 2020.
  21. ^ "Niagara Falls Geology Facts & Figures". Niagara Parks. Archived from the original on 19 July 2011. Retrieved 29 April 2011.
  22. ^ Bastedo, Jamie (1994). Shield Country: The Life and Times of the Oldest Piece of the Planet. Komatik Series, ISSN 0840-4488. 4. Arctic Institute of North America of the University of Calgary. p. 202. ISBN 9780919034792.
  23. ^ Tapping, Ken (2005). "The Unfixed Stars". National Research Council Canada. Archived from the original on 8 July 2011. Retrieved 29 December 2010.
  24. ^ Monnier, J. D.; Tuthill, P.; Lopez, GB; et al. (1999). "The Last Gasps of VY Canis Majoris: Aperture Synthesis and Adaptive Optics Imagery". The Astrophysical Journal. 512 (1): 351–361. arXiv:astro-ph/9810024. Bibcode:1999ApJ...512..351M. doi:10.1086/306761. S2CID 16672180.
  25. ^ Schaetzl, Randall J.; Anderson, Sharon (2005). Soils: Genesis and Geomorphology. Cambridge University Press. p. 105. ISBN 9781139443463.
  26. ^ David Archer (2009). The Long Thaw: How Humans Are Changing the Next 100,000 Years of Earth's Climate. Princeton University Press. p. 123. ISBN 978-0-691-13654-7.
  27. ^ "Frequently Asked Questions". Hawai'i Volcanoes National Park. 2011. Retrieved 22 October 2011.
  28. ^ Tuthill, Peter; Monnier, John; Lawrance, Nicholas; Danchi, William; Owocki, Stan; Gayley, Kenneth (2008). "The Prototype Colliding-Wind Pinwheel WR 104". The Astrophysical Journal. 675 (1): 698–710. arXiv:0712.2111. Bibcode:2008ApJ...675..698T. doi:10.1086/527286. S2CID 119293391.
  29. ^ Tuthill, Peter. "WR 104: Technical Questions". Retrieved 20 December 2015.
  30. ^ Bostrom, Nick (March 2002). "Existential Risks: Analyzing Human Extinction Scenarios and Related Hazards". Journal of Evolution and Technology. 9 (1). Retrieved 10 September 2012.
  31. ^ "Badlands National Park – Nature & Science – Geologic Formations".
  32. ^ Landstreet, John D. (2003). Physical Processes in the Solar System: An introduction to the physics of asteroids, comets, moons and planets. Keenan & Darlington. p. 121. ISBN 9780973205107.
  33. ^ Sessions, Larry (29 July 2009). "Betelgeuse will explode someday". EarthSky Communications, Inc. Retrieved 16 November 2010.
  34. ^ "A giant star is acting strange, and astronomers are buzzing". National Geographic. 26 December 2019. Retrieved 15 March 2020.
  35. ^ a b "Uranus's colliding moons". 2017. Retrieved 23 September 2017.
  36. ^ Bailer-Jones, C.A.L.; Rybizki, J; Andrae, R.; Fouesnea, M. (2018). "New stellar encounters discovered in the second Gaia data release". Astronomy & Astrophysics. 616: A37. arXiv:1805.07581. Bibcode:2018A&A...616A..37B. doi:10.1051/0004-6361/201833456. S2CID 56269929.
  37. ^ Filip Berski; Piotr A. Dybczyński (25 October 2016). "Gliese 710 will pass the Sun even closer". Astronomy and Astrophysics. 595 (L10): L10. Bibcode:2016A&A...595L..10B. doi:10.1051/0004-6361/201629835.
  38. ^ Goldstein, Natalie (2009). Global Warming. Infobase Publishing. p. 53. ISBN 9780816067695. The last time acidification on this scale occurred (about 65 mya) it took more than 2 million years for corals and other marine organisms to recover; some scientists today believe, optimistically, that it could take tens of thousands of years for the ocean to regain the chemistry it had in preindustrial times.
  39. ^ "Grand Canyon – Geology – A dynamic place". Views of the National Parks. National Park Service.
  40. ^ Horner, J.; Evans, N.W.; Bailey, M. E. (2004). "Simulations of the Population of Centaurs I: The Bulk Statistics". Monthly Notices of the Royal Astronomical Society. 354 (3): 798–810. arXiv:astro-ph/0407400. Bibcode:2004MNRAS.354..798H. doi:10.1111/j.1365-2966.2004.08240.x. S2CID 16002759.
  41. ^ Jillian Scudder. "How Long Until The Moon Slows The Earth to a 25 Hour Day?". Forbes. Retrieved 30 May 2017.
  42. ^ Haddok, Eitan (29 September 2008). "Birth of an Ocean: The Evolution of Ethiopia's Afar Depression". Scientific American. Retrieved 27 December 2010.
  43. ^ Kirchner, James W.; Weil, Anne (9 March 2000). "Delayed biological recovery from extinctions throughout the fossil record". Nature. 404 (6774): 177–180. Bibcode:2000Natur.404..177K. doi:10.1038/35004564. PMID 10724168. S2CID 4428714.
  44. ^ Wilson, Edward O. (1999). The Diversity of Life. W.W. Norton & Company. p. 216. ISBN 9780393319408.
  45. ^ Wilson, Edward Osborne (1992). "The Human Impact". The Diversity of Life. London: Penguin UK (published 2001). ISBN 9780141931739. Retrieved 15 March 2020.
  46. ^ Bills, Bruce G.; Gregory A. Neumann; David E. Smith; Maria T. Zuber (2005). "Improved estimate of tidal dissipation within Mars from MOLA observations of the shadow of Phobos". Journal of Geophysical Research. 110 (E7). E07004. Bibcode:2005JGRE..110.7004B. doi:10.1029/2004je002376.
  47. ^ a b c d Scotese, Christopher R. "Pangea Ultima will form 250 million years in the Future". Paleomap Project. Retrieved 13 March 2006.
  48. ^ Garrison, Tom (2009). Essentials of Oceanography (5th ed.). Brooks/Cole. p. 62.[ISBN missing]
  49. ^ "Continents in Collision: Pangea Ultima". NASA. 2000. Retrieved 29 December 2010.
  50. ^ "Geology". Encyclopedia of Appalachia. University of Tennessee Press. 2011. Archived from the original on 21 May 2014. Retrieved 21 May 2014.
  51. ^ Hancock, Gregory; Kirwan, Matthew (January 2007). "Summit erosion rates deduced from 10Be: Implications for relief production in the central Appalachians" (PDF). Geology. 35 (1): 89. Bibcode:2007Geo....35...89H. doi:10.1130/g23147a.1.
  52. ^ Yorath, C. J. (2017). Of rocks, mountains and Jasper: a visitor's guide to the geology of Jasper National Park. Dundurn Press. p. 30. ISBN 9781459736122. [...] 'How long will the Rockies last?' [...] The numbers suggest that in about 50 to 60 million years the remaining mountains will be gone, and the park will be reduced to a rolling plain much like the Canadian prairies.
  53. ^ Dethier, David P.; Ouimet, W.; Bierman, P. R.; Rood, D. H.; et al. (2014). "Basins and bedrock: Spatial variation in 10Be erosion rates and increasing relief in the southern Rocky Mountains, USA" (PDF). Geology. 42 (2): 167–170. Bibcode:2014Geo....42..167D. doi:10.1130/G34922.1.
  54. ^ Patzek, Tad W. (2008). "Can the Earth Deliver the Biomass-for-Fuel we Demand?". In Pimentel, David (ed.). Biofuels, Solar and Wind as Renewable Energy Systems: Benefits and Risks. Springer. ISBN 9781402086533.
  55. ^ Perlman, David (14 October 2006). "Kiss that Hawaiian timeshare goodbye / Islands will sink in 80 million years". San Francisco Chronicle.
  56. ^ Nelson, Stephen A. "Meteorites, Impacts, and Mass Extinction". Tulane University. Retrieved 13 January 2011.
  57. ^ Lang, Kenneth R. (2003). The Cambridge Guide to the Solar System. Cambridge University Press. p. 329. ISBN 9780521813068. [...] all the rings should collapse [...] in about 100 million years.
  58. ^ Schröder, K.-P.; Connon Smith, Robert (2008). "Distant future of the Sun and Earth revisited". Monthly Notices of the Royal Astronomical Society. 386 (1): 155–63. arXiv:0801.4031. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x. S2CID 10073988.
  59. ^ Jillian Scudder. "How Long Until The Moon Slows The Earth to a 25 Hour Day?". Forbes. Retrieved 30 May 2017.
  60. ^ Hayes, Wayne B. (2007). "Is the Outer Solar System Chaotic?". Nature Physics. 3 (10): 689–691. arXiv:astro-ph/0702179. Bibcode:2007NatPh...3..689H. CiteSeerX doi:10.1038/nphys728. S2CID 18705038.
  61. ^ Leong, Stacy (2002). "Period of the Sun's Orbit Around the Galaxy (Cosmic Year)". The Physics Factbook. Retrieved 2 April 2007.
  62. ^ a b c Williams, Caroline; Nield, Ted (20 October 2007). "Pangaea, the comeback". New Scientist. Archived from the original on 13 April 2008. Retrieved 2 January 2014.
  63. ^ Calkin & Young 1996, pp. 9–75.
  64. ^ a b c Thompson & Perry 1997, pp. 127–128.
  65. ^ a b c d e O'Malley-James, Jack T.; Greaves, Jane S.; Raven, John A.; Cockell, Charles S. (2014). "Swansong Biosphere II: The final signs of life on terrestrial planets near the end of their habitable lifetimes". International Journal of Astrobiology. 13 (3): 229–243. arXiv:1310.4841. Bibcode:2014IJAsB..13..229O. doi:10.1017/S1473550413000426. S2CID 119252386.
  66. ^ Strom, Robert G.; Schaber, Gerald G.; Dawson, Douglas D. (25 May 1994). "The global resurfacing of Venus". Journal of Geophysical Research. 99 (E5): 10899–10926. Bibcode:1994JGR....9910899S. doi:10.1029/94JE00388.
  67. ^ Nield 2007, pp. 20–21.
  68. ^ Hoffman 1992, pp. 323–327.
  69. ^ Minard, Anne (2009). "Gamma-Ray Burst Caused Mass Extinction?". National Geographic News. Retrieved 27 August 2012.
  70. ^ "Questions Frequently Asked by the Public About Eclipses". NASA. Archived from the original on 12 March 2010. Retrieved 7 March 2010.
  71. ^ a b c d O'Malley-James, Jack T.; Greaves, Jane S.; Raven, John A.; Cockell, Charles S. (2012). "Swansong Biospheres: Refuges for life and novel microbial biospheres on terrestrial planets near the end of their habitable lifetimes". International Journal of Astrobiology. 12 (2): 99–112. arXiv:1210.5721. Bibcode:2013IJAsB..12...99O. doi:10.1017/S147355041200047X. S2CID 73722450.
  72. ^ a b Heath, Martin J.; Doyle, Laurance R. (2009). "Circumstellar Habitable Zones to Ecodynamic Domains: A Preliminary Review and Suggested Future Directions". arXiv:0912.2482 [astro-ph.EP].
  73. ^ a b Ward & Brownlee 2003, pp. 117-128.
  74. ^ a b c d Franck, S.; Bounama, C.; Von Bloh, W. (November 2005). "Causes and timing of future biosphere extinction" (PDF). Biogeosciences Discussions. 2 (6): 1665–1679. Bibcode:2005BGD.....2.1665F. doi:10.5194/bgd-2-1665-2005.
  75. ^ Bounama, Christine; Franck, S.; Von Bloh, David (2001). "The fate of Earth's ocean". Hydrology and Earth System Sciences. 5 (4): 569–575. Bibcode:2001HESS....5..569B. doi:10.5194/hess-5-569-2001.
  76. ^ a b Schröder, K.-P.; Connon Smith, Robert (1 May 2008). "Distant future of the Sun and Earth revisited". Monthly Notices of the Royal Astronomical Society. 386 (1): 155–163. arXiv:0801.4031. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x. S2CID 10073988.
  77. ^ a b Brownlee 2010, p. 95.
  78. ^ Brownlee 2010, p. 79.
  79. ^ Li King-Fai; Pahlevan, Kaveh; Kirschvink, Joseph L.; Yung, Luk L. (2009). "Atmospheric pressure as a natural climate regulator for a terrestrial planet with a biosphere". Proceedings of the National Academy of Sciences of the United States of America. 106 (24): 9576–9579. Bibcode:2009PNAS..106.9576L. doi:10.1073/pnas.0809436106. PMC 2701016. PMID 19487662.
  80. ^ Caldeira, Ken; Kasting, James F. (1992). "The life span of the biosphere revisited". Nature. 360 (6406): 721–23. Bibcode:1992Natur.360..721C. doi:10.1038/360721a0. PMID 11536510. S2CID 4360963.
  81. ^ Franck, S. (2000). "Reduction of biosphere life span as a consequence of geodynamics". Tellus B. 52 (1): 94–107. Bibcode:2000TellB..52...94F. doi:10.1034/j.1600-0889.2000.00898.x.
  82. ^ Lenton, Timothy M.; von Bloh, Werner (2001). "Biotic feedback extends the life span of the biosphere". Geophysical Research Letters. 28 (9): 1715–1718. Bibcode:2001GeoRL..28.1715L. doi:10.1029/2000GL012198.
  83. ^ a b c d Kargel, Jeffrey Stuart (2004). Mars: A Warmer, Wetter Planet. Springer. p. 509. ISBN 978-1852335687. Retrieved 29 October 2007.
  84. ^ a b Li, King-Fai; Pahlevan, Kaveh; Kirschvink, Joseph L.; Yung, Yuk L. (16 June 2009). "Atmospheric pressure as a natural climate regulator for a terrestrial planet with a biosphere". Proceedings of the National Academy of Sciences of the United States of America. 106 (24): 9576–9579. Bibcode:2009PNAS..106.9576L. doi:10.1073/pnas.0809436106. PMC 2701016. PMID 19487662.
  85. ^ Waszek, Lauren; Irving, Jessica; Deuss, Arwen (20 February 2011). "Reconciling the Hemispherical Structure of Earth's Inner Core With its Super-Rotation". Nature Geoscience. 4 (4): 264–267. Bibcode:2011NatGe...4..264W. doi:10.1038/ngeo1083.
  86. ^ McDonough, W. F. (2004). "Compositional Model for the Earth's Core". Treatise on Geochemistry. 2. pp. 547–568. Bibcode:2003TrGeo...2..547M. doi:10.1016/B0-08-043751-6/02015-6. ISBN 978-0080437514.
  87. ^ Luhmann, J. G.; Johnson, R. E.; Zhang, M. H. G. (1992). "Evolutionary impact of sputtering of the Martian atmosphere by O+ pickup ions". Geophysical Research Letters. 19 (21): 2151–2154. Bibcode:1992GeoRL..19.2151L. doi:10.1029/92GL02485.
  88. ^ Quirin Shlermeler (3 March 2005). "Solar wind hammers the ozone layer". News@nature. doi:10.1038/news050228-12.
  89. ^ a b Adams 2008, pp. 33–47.
  90. ^ Adams 2008, pp. 33–44.
  91. ^ Neron de Surgey, O.; Laskar, J. (1996). "On the Long Term Evolution of the Spin of the Earth". Astronomy and Astrophysics. 318: 975. Bibcode:1997A&A...318..975N.
  92. ^ "Study: Earth May Collide With Another Planet". Fox News Channel. 11 June 2009. Archived from the original on 4 November 2012. Retrieved 8 September 2011.
  93. ^ Guinan, E. F.; Ribas, I. (2002). Montesinos, Benjamin; Gimenez, Alvaro; Guinan, Edward F. (eds.). "Our Changing Sun: The Role of Solar Nuclear Evolution and Magnetic Activity on Earth's Atmosphere and Climate". ASP Conference Proceedings. 269: 85–106. Bibcode:2002ASPC..269...85G.
  94. ^ Kasting, J. F. (June 1988). "Runaway and moist greenhouse atmospheres and the evolution of earth and Venus". Icarus. 74 (3): 472–494. Bibcode:1988Icar...74..472K. doi:10.1016/0019-1035(88)90116-9. PMID 11538226.
  95. ^ Chyba, C. F.; Jankowski, D. G.; Nicholson, P. D. (1989). "Tidal Evolution in the Neptune-Triton System". Astronomy and Astrophysics. 219 (1–2): 23. Bibcode:1989A&A...219L..23C.
  96. ^ Cox, J. T.; Loeb, Abraham (2007). "The Collision Between The Milky Way And Andromeda". Monthly Notices of the Royal Astronomical Society. 386 (1): 461–474. arXiv:0705.1170. Bibcode:2008MNRAS.386..461C. doi:10.1111/j.1365-2966.2008.13048.x. S2CID 14964036.
  97. ^ Cain, Fraser (2007). "When Our Galaxy Smashes into Andromeda, What Happens to the Sun?". Universe Today. Archived from the original on 17 May 2007. Retrieved 16 May 2007.
  98. ^ Cox, T. J.; Loeb, Abraham (2008). "The Collision Between The Milky Way And Andromeda". Monthly Notices of the Royal Astronomical Society. 386 (1): 461–474. arXiv:0705.1170. Bibcode:2008MNRAS.386..461C. doi:10.1111/j.1365-2966.2008.13048.x. S2CID 14964036.
  99. ^ "NASA's Hubble Shows Milky Way is Destined for Head-On Collision". NASA. 31 May 2012. Retrieved 13 October 2012.
  100. ^ Dowd, Maureen (29 May 2012). "Andromeda Is Coming!". The New York Times. Retrieved 9 January 2014. [NASA's David Morrison] explained that the Andromeda-Milky Way collision would just be two great big fuzzy balls of stars and mostly empty space passing through each other harmlessly over the course of millions of years.
  101. ^ Braine, J.; Lisenfeld, U.; Duc, P. A.; et al. (2004). "Colliding molecular clouds in head-on galaxy collisions". Astronomy and Astrophysics. 418 (2): 419–428. arXiv:astro-ph/0402148. Bibcode:2004A&A...418..419B. doi:10.1051/0004-6361:20035732. S2CID 15928576.
  102. ^ a b c d Schroder, K. P.; Connon Smith, Robert (2008). "Distant Future of the Sun and Earth Revisited". Monthly Notices of the Royal Astronomical Society. 386 (1): 155–163. arXiv:0801.4031. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x. S2CID 10073988.
  103. ^ Powell, David (22 January 2007). "Earth's Moon Destined to Disintegrate". Tech Media Network. Retrieved 1 June 2010.
  104. ^ Lorenz, Ralph D.; Lunine, Jonathan I.; McKay, Christopher P. (1997). "Titan under a red giant sun: A new kind of "habitable" moon" (PDF). Geophysical Research Letters. 24 (22): 2905–2908. Bibcode:1997GeoRL..24.2905L. CiteSeerX doi:10.1029/97GL52843. PMID 11542268. Retrieved 21 March 2008.
  105. ^ Rybicki, K. R.; Denis, C. (2001). "On the Final Destiny of the Earth and the Solar System". Icarus. 151 (1): 130–137. Bibcode:2001Icar..151..130R. doi:10.1006/icar.2001.6591.
  106. ^ Balick, Bruce. "Planetary Nebulae and the Future of the Solar System". University of Washington. Archived from the original on 19 December 2008. Retrieved 23 June 2006.
  107. ^ Kalirai, Jasonjot S.; et al. (March 2008). "The Initial-Final Mass Relation: Direct Constraints at the Low-Mass End". The Astrophysical Journal. 676 (1): 594–609. arXiv:0706.3894. Bibcode:2008ApJ...676..594K. doi:10.1086/527028. S2CID 10729246.
  108. ^ Kalirai et al. 2008, p. 16. Based upon the weighted least-squares best fit with the initial mass equal to a solar mass.
  109. ^ "Universe May End in a Big Rip". CERN Courier. 1 May 2003. Retrieved 22 July 2011.
  110. ^ "Ask Ethan: Could The Universe Be Torn Apart In A Big Rip?".
  111. ^ Caldwell, Robert R.; Kamionkowski, Marc; Weinberg, Nevin N. (2003). "Phantom Energy and Cosmic Doomsday". Physical Review Letters. 91 (7): 071301. arXiv:astro-ph/0302506. Bibcode:2003PhRvL..91g1301C. doi:10.1103/PhysRevLett.91.071301. PMID 12935004.
  112. ^ Vikhlinin, A.; Kravtsov, A.V.; Burenin, R.A.; et al. (2009). "Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints". The Astrophysical Journal. 692 (2): 1060–1074. arXiv:0812.2720. Bibcode:2009ApJ...692.1060V. doi:10.1088/0004-637X/692/2/1060.
  113. ^ Murray, C.D. & Dermott, S.F. (1999). Solar System Dynamics. Cambridge University Press. p. 184. ISBN 978-0-521-57295-8.
  114. ^ Dickinson, Terence (1993). From the Big Bang to Planet X. Camden East, Ontario: Camden House. pp. 79–81. ISBN 978-0-921820-71-0.
  115. ^ Canup, Robin M.; Righter, Kevin (2000). Origin of the Earth and Moon. The University of Arizona space science series. 30. University of Arizona Press. pp. 176–177. ISBN 978-0-8165-2073-2.
  116. ^ Dorminey, Bruce (31 January 2017). "Earth and Moon May Be on Long-Term Collision Course". Forbes. Retrieved 11 February 2017.
  117. ^ a b Loeb, Abraham (2011). "Cosmology with Hypervelocity Stars". Journal of Cosmology and Astroparticle Physics. Harvard University. 2011 (4): 023. arXiv:1102.0007. Bibcode:2011JCAP...04..023L. doi:10.1088/1475-7516/2011/04/023. S2CID 118750775.
  118. ^ Chown, Marcus (1996). Afterglow of Creation. University Science Books. p. 210.[ISBN missing]
  119. ^ a b c Busha, Michael T.; Adams, Fred C.; Wechsler, Risa H.; Evrard, August E. (20 October 2003). "Future Evolution of Structure in an Accelerating Universe". The Astrophysical Journal. 596 (2): 713–724. arXiv:astro-ph/0305211. doi:10.1086/378043. ISSN 0004-637X. S2CID 15764445.
  120. ^ "The Local Group of Galaxies". Students for the Exploration and Development of Space. Retrieved 2 October 2009.
  121. ^ Adams, F. C.; Graves, G. J. M.; Laughlin, G. (December 2004). García-Segura, G.; Tenorio-Tagle, G.; Franco, J.; Yorke, H. W. (eds.). "Gravitational Collapse: From Massive Stars to Planets. / First Astrophysics meeting of the Observatorio Astronomico Nacional. / A meeting to celebrate Peter Bodenheimer for his outstanding contributions to Astrophysics: Red Dwarfs and the End of the Main Sequence". Revista Mexicana de Astronomía y Astrofísica, Serie de Conferencias. 22: 46–49. Bibcode:2004RMxAC..22...46A. See Fig. 3.
  122. ^ Krauss, Lawrence M.; Starkman, Glenn D. (March 2000). "Life, The Universe, and Nothing: Life and Death in an Ever-Expanding Universe". The Astrophysical Journal. 531 (1): 22–30. arXiv:astro-ph/9902189. Bibcode:2000ApJ...531...22K. doi:10.1086/308434. ISSN 0004-637X. S2CID 18442980.
  123. ^ Fred C. Adams; Gregory Laughlin; Genevieve J. M. Graves (2004). "RED Dwarfs and the End of The Main Sequence" (PDF). Revista Mexicana de Astronomía y Astrofísica, Serie de Conferencias. 22: 46–49.
  124. ^ Loeb, Abraham; Batista, Rafael; Sloan, W. (2016). "Relative Likelihood for Life as a Function of Cosmic Time". Journal of Cosmology and Astroparticle Physics. 2016 (8): 040. arXiv:1606.08448. Bibcode:2016JCAP...08..040L. doi:10.1088/1475-7516/2016/08/040. S2CID 118489638.
  125. ^ "Why the Smallest Stars Stay Small". Sky & Telescope (22). November 1997.
  126. ^ Adams, F. C.; P. Bodenheimer; G. Laughlin (2005). "M dwarfs: planet formation and long term evolution". Astronomische Nachrichten. 326 (10): 913–919. Bibcode:2005AN....326..913A. doi:10.1002/asna.200510440.
  127. ^ Tayler, Roger John (1993). Galaxies, Structure and Evolution (2nd ed.). Cambridge University Press. p. 92. ISBN 978-0521367103.
  128. ^ Barrow, John D.; Tipler, Frank J. (19 May 1988). The Anthropic Cosmological Principle. foreword by John A. Wheeler. Oxford: Oxford University Press. ISBN 978-0192821478. LC 87-28148.
  129. ^ Adams, Fred; Laughlin, Greg (1999). The Five Ages of the Universe. New York: The Free Press. pp. 85–87. ISBN 978-0684854229.
  130. ^ a b c d e f Dyson, Freeman J. (1979). "Time Without End: Physics and Biology in an Open Universe". Reviews of Modern Physics. 51 (3): 447–460. Bibcode:1979RvMP...51..447D. doi:10.1103/RevModPhys.51.447. Retrieved 5 July 2008.
  131. ^ John Baez (7 February 2016). "The End of the Universe".
  132. ^ Nishino H, et al. (Super-K Collaboration) (2009). "Search for Proton Decay via




    in a Large Water Cherenkov Detector". Physical Review Letters. 102 (14): 141801. arXiv:0903.0676. Bibcode:2009PhRvL.102n1801N. doi:10.1103/PhysRevLett.102.141801. PMID 19392425. S2CID 32385768.
  133. ^ a b Tyson, Neil de Grasse; Tsun-Chu Liu, Charles; Irion, Robert (2000). One Universe: At Home in the Cosmos. Joseph Henry Press. ISBN 978-0309064880.
  134. ^ a b c Page, Don N. (1976). "Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole". Physical Review D. 13 (2): 198–206. Bibcode:1976PhRvD..13..198P. doi:10.1103/PhysRevD.13.198. See in particular equation (27).
  135. ^ Andreassen, Anders; Frost, William; Schwartz, Matthew D. (12 March 2018). "Scale-invariant instantons and the complete lifetime of the standard model". Physical Review D. 97 (5): 056006. arXiv:1707.08124. Bibcode:2018PhRvD..97e6006A. doi:10.1103/PhysRevD.97.056006. S2CID 118843387.
  136. ^ M. E. Caplan (7 August 2020). "Black Dwarf Supernova in the Far Future" (PDF). MNRAS. 000 (1–6): 4357–4362. arXiv:2008.02296. Bibcode:2020MNRAS.497.4357C. doi:10.1093/mnras/staa2262. S2CID 221005728.
  137. ^ K. Sumiyoshi; S. Yamada; H. Suzuki; W. Hillebrandt (21 July 1997). "The fate of a neutron star just below the minimum mass: does it explode?". Astronomy and Astrophysics. 334: 159. arXiv:astro-ph/9707230. Bibcode:1998A&A...334..159S. Given this assumption... the minimum possible mass of a neutron star is 0.189
  138. ^ Carroll, Sean M.; Chen, Jennifer (27 October 2004). "Spontaneous Inflation and the Origin of the Arrow of Time". arXiv:hep-th/0410270.
  139. ^ Tegmark, M (7 February 2003). "Parallel universes. Not just a staple of science fiction, other universes are a direct implication of cosmological observations". Sci. Am. 288 (5): 40–51. arXiv:astro-ph/0302131. Bibcode:2003SciAm.288e..40T. doi:10.1038/scientificamerican0503-40. PMID 12701329.
  140. ^ Max Tegmark (7 February 2003). "Parallel Universes". In "Science and Ultimate Reality: From Quantum to Cosmos", Honoring John Wheeler's 90th Birthday. J. D. Barrow, P.C.W. Davies, & C.L. Harper Eds. 288 (5): 40–51. arXiv:astro-ph/0302131. Bibcode:2003SciAm.288e..40T. doi:10.1038/scientificamerican0503-40. PMID 12701329.
  141. ^ M. Douglas (21 March 2003). "The statistics of string / M theory vacua". JHEP. 0305 (46): 046. arXiv:hep-th/0303194. Bibcode:2003JHEP...05..046D. doi:10.1088/1126-6708/2003/05/046. S2CID 650509.
  142. ^ S. Ashok; M. Douglas (2004). "Counting flux vacua". JHEP. 0401 (60): 060. arXiv:hep-th/0307049. Bibcode:2004JHEP...01..060A. doi:10.1088/1126-6708/2004/01/060. S2CID 1969475.
  143. ^ Smith, Cameron; Davies, Evan T. (2012). Emigrating Beyond Earth: Human Adaptation and Space Colonization. Springer. p. 258.[ISBN missing]
  144. ^ Klein, Jan; Takahata, Naoyuki (2002). Where Do We Come From?: The Molecular Evidence for Human Descent. Springer. p. 395.[ISBN missing]
  145. ^ Carter, Brandon; McCrea, W. H. (1983). "The anthropic principle and its implications for biological evolution". Philosophical Transactions of the Royal Society of London. A310 (1512): 347–363. Bibcode:1983RSPTA.310..347C. doi:10.1098/rsta.1983.0096. S2CID 92330878.
  146. ^ Greenberg, Joseph (1987). Language in the Americas. Stanford University Press. pp. 341–342.[ISBN missing]
  147. ^ McKay, Christopher P.; Toon, Owen B.; Kasting, James F. (8 August 1991). "Making Mars habitable". Nature. 352 (6335): 489–496. Bibcode:1991Natur.352..489M. doi:10.1038/352489a0. PMID 11538095. S2CID 2815367.
  148. ^ Kaku, Michio (2010). "The Physics of Interstellar Travel: To one day, reach the stars". Retrieved 29 August 2010.
  149. ^ Avise, John; D. Walker; G. C. Johns (22 September 1998). "Speciation durations and Pleistocene effects on vertebrate phylogeography". Philosophical Transactions of the Royal Society B. 265 (1407): 1707–1712. doi:10.1098/rspb.1998.0492. PMC 1689361. PMID 9787467.
  150. ^ Valentine, James W. (1985). "The Origins of Evolutionary Novelty And Galactic Colonization". In Finney, Ben R.; Jones, Eric M. (eds.). Interstellar Migration and the Human Experience. University of California Press. p. 274.[ISBN missing]
  151. ^ J. Richard Gott, III (1993). "Implications of the Copernican principle for our future prospects". Nature. 363 (6427): 315–319. Bibcode:1993Natur.363..315G. doi:10.1038/363315a0. S2CID 4252750.
  152. ^ Bignami, Giovanni F.; Sommariva, Andrea (2013). A Scenario for Interstellar Exploration and Its Financing. Springer. p. 23.[ISBN missing]
  153. ^ Korycansky, D. G.; Laughlin, Gregory; Adams, Fred C. (2001). "Astronomical engineering: a strategy for modifying planetary orbits". Astrophysics and Space Science. 275 (4): 349–366. arXiv:astro-ph/0102126. Bibcode:2001Ap&SS.275..349K. doi:10.1023/A:1002790227314. hdl:2027.42/41972. S2CID 5550304. Astrophys.Space Sci.275:349-366,2001.
  154. ^ Korycansky, D. G. (2004). "Astroengineering, or how to save the Earth in only one billion years" (PDF). Revista Mexicana de Astronomía y Astrofísica. 22: 117–120. Bibcode:2004RMxAC..22..117K.
  155. ^ "Hurtling Through the Void". Time. 20 June 1983. Retrieved 5 September 2011.
  156. ^ Staub, D.W. (25 March 1967). SNAP 10 Summary Report. Atomics International Division of North American Aviation, Inc., Canoga Park, California. NAA-SR-12073.
  157. ^ "U.S. ADMISSION : Satellite mishap released rays". The Canberra Times. 52 (15, 547). Australian Capital Territory, Australia. 30 March 1978. p. 5. Retrieved 12 August 2017 – via National Library of Australia., ...Launched in 1965 and carrying about 4.5 kilograms of uranium 235, Snap 10A is in a 1,000-year orbit....
  158. ^ a b c d e f g h i j k l m n Coryn, A.L.; Bailer-Jones, Davide Farnocchia (3 April 2019). "Future stellar flybys of the Voyager and Pioneer spacecraft". Research Notes of the American Astronomical Society. 3 (59): 59. arXiv:1912.03503. Bibcode:2019RNAAS...3...59B. doi:10.3847/2515-5172/ab158e. S2CID 134524048.
  159. ^ "Cornell News: "It's the 25th Anniversary of Earth's First (and only) Attempt to Phone E.T."". Cornell University. 12 November 1999. Archived from the original on 2 August 2008. Retrieved 29 March 2008.
  160. ^ Dave Deamer. "In regard to the email from". Science 2.0. Archived from the original on 24 September 2015. Retrieved 14 November 2014.
  161. ^ "KEO FAQ". Retrieved 14 October 2011.
  162. ^ Lasher, Lawrence. "Pioneer Mission Status". NASA. Archived from the original on 8 April 2000. [Pioneer's speed is] about 12 km/s... [the plate etching] should survive recognizable at least to a distance ≈10 parsecs, and most probably to 100 parsecs.
  163. ^ a b "The Pioneer Missions". NASA. Retrieved 5 September 2011.
  164. ^ "LAGEOS 1, 2". NASA. Retrieved 21 July 2012.
  165. ^ Jad Abumrad and Robert Krulwich (12 February 2010). Carl Sagan And Ann Druyan's Ultimate Mix Tape (Radio). NPR.
  166. ^ "This Camera Will Capture a 1,000-Year Exposure That Ends in 3015 for History's Slowest Photo". PetaPixel. Retrieved 14 December 2015.
  167. ^ Conception Official Zeitpyramide website. Retrieved 14 December 2010.
  168. ^ The Book of Record of the Time Capsule of Cupaloy. New York City: Westinghouse Electric and Manufacturing Company. 1938. p. 6.
  169. ^ "Time Cpsue Expo 1970". Retrieved 15 October 2020.
  170. ^ "The New Georgia Encyclopedia – Crypt of Civilization". Retrieved 29 June 2008.
  171. ^ "History of the Crypt of Civilization". Retrieved 22 October 2015.
  172. ^ "The Long Now Foundation". The Long Now Foundation. 2011. Retrieved 21 September 2011.
  173. ^ "A Visit to the Doomsday Vault". CBS News. 20 March 2008.
  174. ^ "Memory of Mankind". Retrieved 4 March 2019.
  175. ^ "Human Document Project 2014".
  176. ^ "When will System.currentTimeMillis() overflow?". Stack Overflow.
  177. ^ Begtrup, G. E.; Gannett, W.; Yuzvinsky, T. D.; Crespi, V. H.; et al. (13 May 2009). "Nanoscale Reversible Mass Transport for Archival Memory" (PDF). Nano Letters. 9 (5): 1835–1838. Bibcode:2009NanoL...9.1835B. CiteSeerX doi:10.1021/nl803800c. PMID 19400579. Archived from the original (PDF) on 22 June 2010.
  178. ^ Zhang, J.; Gecevičius, M.; Beresna, M.; Kazansky, P. G. (2014). "Seemingly unlimited lifetime data storage in nanostructured glass". Phys. Rev. Lett. 112 (3): 033901. Bibcode:2014PhRvL.112c3901Z. doi:10.1103/PhysRevLett.112.033901. PMID 24484138.
  179. ^ Zhang, J.; Gecevičius, M.; Beresna, M.; Kazansky, P. G. (June 2013). "5D Data Storage by Ultrafast Laser Nanostructuring in Glass" (PDF). CLEO: Science and Innovations: CTh5D–9. Archived from the original (PDF) on 6 September 2014.
  180. ^ "Date/Time Conversion Contract Language" (PDF). Office of Information Technology Services, New York (state). 19 May 2019. Retrieved 16 October 2020.
  181. ^ Artaxo, Paulo; Berntsen, Terje; Betts, Richard; Fahey, David W.; Haywood, James; Lean, Judith; Lowe, David C.; Myhre, Gunnar; Nganga, John; Prinn, Ronald; Raga, Graciela; Schulz, Michael; van Dorland, Robert (February 2018). "Changes in Atmospheric Constituents and in Radiative Forcing" (PDF). International Panel on Climate Change. p. 212. Retrieved 17 March 2021.
  182. ^ "Time it takes for garbage to decompose in the environment" (PDF). New Hampshire Department of Environmental Services. Archived from the original (PDF) on 9 June 2014. Retrieved 23 May 2014.
  183. ^ Lyle, Paul (2010). Between Rocks And Hard Places: Discovering Ireland's Northern Landscapes. Geological Survey of Northern Ireland.[ISBN missing]
  184. ^ Weisman, Alan (10 July 2007). The World Without Us. New York: Thomas Dunne Books/St. Martin's Press. pp. 171–172. ISBN 978-0-312-34729-1. OCLC 122261590.
  185. ^ "Apollo 11 – First Footprint on the Moon". Student Features. NASA.
  186. ^ Meadows, A. J. (2007). The Future of the Universe. Springer. pp. 81–83.[ISBN missing]
  187. ^ Weisman, Alan (10 July 2007). The World Without Us. New York: Thomas Dunne Books/St. Martin's Press. p. 182. ISBN 978-0-312-34729-1. OCLC 122261590.
  188. ^ Zalasiewicz, Jan (25 September 2008). The Earth After Us: What legacy will humans leave in the rocks?. Oxford University Press., Review in Stanford Archaeology
  189. ^ "Permanent Markers Implementation Plan" (PDF). United States Department of Energy. 30 August 2004. Archived from the original (PDF) on 28 September 2006.
  190. ^ Time: Disasters that Shook the World. New York City: Time Home Entertainment. 2012. ISBN 978-1-60320-247-3.
  191. ^ a b Fetter, Steve (March 2009). "How long will the world's uranium supplies last?".
  192. ^ Biello, David (28 January 2009). "Spent Nuclear Fuel: A Trash Heap Deadly for 250,000 Years or a Renewable Energy Source?". Scientific American.
  193. ^ a b Ongena, J; G. Van Oost (2004). "Energy for future centuries – Will fusion be an inexhaustible, safe and clean energy source?" (PDF). Fusion Science and Technology. 2004. 45 (2T): 3–14. doi:10.13182/FST04-A464. S2CID 15368449.
  194. ^ Cohen, Bernard L. (January 1983). "Breeder Reactors: A Renewable Energy Source" (PDF). American Journal of Physics. 51 (1): 75. Bibcode:1983AmJPh..51...75C. doi:10.1119/1.13440.