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This is the timeline of the Universe from
Big Bang The Big Bang event is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models of the Big Bang explain the evolution of the observable universe from the ...
to
Heat Death Heat death may refer to: *Heat death of the universe, a proposed cosmological event ** Heat death paradox, a philosophical examination of the cosmological event *Hyperthermia, injury up to and including death, from excessive heat *Thermal shock ...
scenario. The different eras of the universe are shown. The heat death will occur in around 1.7×10106 years, if protons decay.


Timeline

ImageSize = width:840 height:2000 PlotArea = left:40 right:235 bottom:75 top:75 Colors = id:period1 value:rgb(1,1,0.7) # light yellow id:period2 value:rgb(0.7,0.7,1) # light blue id:events value:rgb(1,0.7,1) # light purple id:era1 Value:yellowgreen id:era2 value:lightorange id:time1 Value:coral id:time2 Value:lavender DateFormat = yyyy Period = from:-171 till:300 TimeAxis = format:yyyy orientation:vertical # order:reverse does not work ScaleMajor = unit:year increment:10 start:-170 ScaleMinor = unit:year increment:1 start:-171 AlignBars = justify BarData = bar:Clock bar:Dummy1 bar:Era bar:Dummy2 bar:Dummy3 bar:Periods bar:Dummy4 bar:Events TextData = fontsize:M pos:(365,75) text:"
Planck epoch The chronology of the universe describes the history and future of the universe according to Big Bang cosmology. Research published in 2015 estimates the earliest stages of the universe's existence as taking place 13.8 billion years ago, wit ...
" # pos:(210,50) pos:(205,50) text:"
Big Bang The Big Bang event is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models of the Big Bang explain the evolution of the observable universe from the ...
" pos:(20,50) text:"0: Linear time" pos:(10,1980) text:"Double-logarithmic time:" text:"100*log log year" pos:(200,1960) text:"
Heat Death Heat death may refer to: *Heat death of the universe, a proposed cosmological event ** Heat death paradox, a philosophical examination of the cosmological event *Hyperthermia, injury up to and including death, from excessive heat *Thermal shock ...
" PlotData= textcolor:black fontsize:M width:90 bar:Clock color:events align:right shift:(43,3) mark:(line,teal) at:-171 text:"1E-43 seconds" # at:-141 # at:-135 at:-129 text:"One picosecond" # at:-122 text:"One nanosecond" at:-113 text:"One microsecond" # at:-102 shift:(43,-13) text:"One millisecond" # at:-100 text:"1E-10 years" at:-88 text:"One second" at:-60 text:"One hour" at:0 text:"One year" at:48 text:"One thousand years" at:78 text:"One million years" at:95 text:"One billion years" # at:100 text:"1E10 years" at:108 text:"One trillion years" at:118 text:"One quadrillion years" # at:126 # at:132 at:200 text:"1E100 years" # at:200 text:"10100 years" at:300 shift:(43,-13) text:"1E1000 years" width:55 bar:Dummy1 width:130 bar:Era mark:(line,white) align:center shift:(0,0) from:-171 till:78 color:era1 text:" The Primordial Era" from:78 till:115 color:era2 text:" The Stelliferous Era~ZOOM IN" from:115 till:160 color:era1 text:"The Degenerate Era" from:160 till:200 color:era2 text:"The Black Hole Era" from:200 till:300 color:era1 text:"The Dark Era" width:55 bar:Dummy2 bar:Dummy3 width:165 bar:Periods align:center shift:(0,0) mark:(line,white) from:-171 till:-164 color:period1 text:
Grand unification epoch In physical cosmology, assuming that nature is described by a Grand Unified Theory, the grand unification epoch was the period in the evolution of the early universe following the Planck epoch, starting at about 10−43 seconds after the Big Bang, ...
# end at 10-37 seconds, not 10-33? from:-164 till:-129 color:period2 text:
Electroweak epoch In physical cosmology, the electroweak epoch was the period in the evolution of the early universe when the temperature of the universe had fallen enough that the strong force separated from the electroweak interaction, but was high enough for ele ...
from:-129 till:-113 color:period1 text:
Quark epoch In physical cosmology, the Quark epoch was the period in the evolution of the early universe when the fundamental interactions of gravitation, electromagnetism, the strong interaction and the weak interaction had taken their present forms, but th ...
from:-113 till:-88 shift:(-40,0) align:left color:period2 text: Hadron epoch Formation of hydrogen nuclei from:-88 till:-72 color:period1 shift:(0,0) text:
Lepton epoch In physical cosmology, the lepton epoch was the period in the evolution of the early universe in which the leptons dominated the mass of the Universe. It started roughly 1 second after the Big Bang, after the majority of hadrons and anti-hadrons a ...
from:-72 till:75 color:period2 shift:(0,0) text:
Photon epoch In physical cosmology, the photon epoch was the period in the evolution of the early universe in which photons dominated the energy of the universe. The photon epoch started after most leptons and anti-leptons were annihilated at the end of the ...
from:75 till:90 color:period1 text:" Dark Ages" from:90 till:93 color:period2 text:"
Reionization In the fields of Big Bang theory and cosmology, reionization is the process that caused matter in the universe to reionize after the lapse of the " dark ages". Reionization is the second of two major phase transitions of gas in the universe (t ...
" # 100-400 million years from:100 till:101 color:period1 text:"Life on Earth~ ZOOM IN MORE" width:55 bar:Dummy4 width:55 mark:(line,purple) textcolor:black fontsize:M bar:Events color:events align:left shift:(30,-2) at:-171 shift:(30,-15) text:" Planck time, the smallest observable unit of time ~and the time before which science is unable to ~describe the universe. At this point, the force of ~gravity separated from the electronuclear force." at:-164 shift:(30,-10) text:"Separation of the strong force from the ~electronuclear force." from:-164 till:-160 align:left shift:(-55,-3) color:time1 text:" Inflationary epoch. The Universe expands exponentially" at:-160 shift:(30,20) text:"Reheating after inflation populates universe ~with quarks and anti-quarks." at:-129 text:"The weak force separates from the ~electromagnetic force resulting in the four ~separate forces we know today." at:-113 text:"Quarks become confined within hadrons." at:-88 text:"Neutrinos cease to interact with other particles." at:-72 shift:(30,-11) text:"Lepton/anti-lepton pairs annihilate." from:-72 till:-65 align:center shift:(0,0) color:time2 text:"
Big Bang nucleosynthesis In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis) is the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) du ...
" at:-65 shift:(30,0) text:"3 to 20 minutes: Formation of helium nuclei" at: 69 shift:(30,-14) text:" 70,000 years: Matter domination" from:73 till:74 shift:(-65,-5) color:time1 mark:(line,white) text:" Recombination" at:75 shift:(30,35) text:"379,000 years: Hydrogen and helium nuclei ~capture electrons to form stable atoms. Photons ~are no longer able to interact strongly with atoms. ~
Cosmic microwave background radiation In Big Bang cosmology the cosmic microwave background (CMB, CMBR) is electromagnetic radiation that is a remnant from an early stage of the universe, also known as "relic radiation". The CMB is faint cosmic background radiation filling all space ...
streams ~freely." at:87 text:" 10-17 million years - Habitable epoch begins" at:90 text:"100 million years. First star began to shine." at: 94 text:" 600 million years. Formation of the first galaxy" # at:98 text:" 4 billion years. Earliest Population I stars" at:100 text:" 9.1 billion years. Formation of the Sun" shift:(30,-10) at:101 mark:(line,magenta) text:"13.8 billion years: this present day" # at:101 text:"19.1 billion years Sun becomes a red giant" at:115 text:"Formation of new stars ceases.~Stars cease to fuse." shift:(30,-7) at:118 text:"Solar systems no longer exist. Planets flung out ~of orbit or consumed by larger bodies.~ Sun has become a black dwarf." shift:(30,26) at:130 text:"Galaxies no longer exist. Stars flung out of orbit~or consumed by black holes." shift:(30,11) at:156 text:" Half of all protons have decayed." at:160 shift:(30,10) text:"All protons decay. The matter that stars and life~were built of no longer exists." at:182 text:"A black hole with the mass of the Sun~has evaporated." at:200 text:"A supermassive black hole with mass~10 billion solar masses has evaporated."
Usually the
logarithmic scale A logarithmic scale (or log scale) is a way of displaying numerical data over a very wide range of values in a compact way—typically the largest numbers in the data are hundreds or even thousands of times larger than the smallest numbers. Such a ...
is used for such timelines but it compresses the most interesting Stelliferous Era too much as
this This may refer to: * ''This'', the singular proximal demonstrative pronoun Places * This, or ''Thinis'', an ancient city in Upper Egypt * This, Ardennes, a commune in France People with the surname * Hervé This, French culinary chemist Arts, e ...
example shows. Therefore, a double-logarithmic scale ''s'' (''s*100'' in the graphics) is used instead. The minimum of it is only 1, not 0 as needed, and the negative outputs for inputs smaller than 10 are useless. Therefore, the time from 0.1 to 10 years is collapsed to a single point 0, but that does not matter in this case because nothing special happens in the history of the universe during that time. : s = \begin \log_ \log_ year & \mbox year > 10 \mbox year = 10^ \\ 0 & \mbox 0.1 \le year \le 10 \\ -\log_ (-\log_ year) & \mbox year < 0.1 \mbox year = 10^ \end The seconds in the timescale have been converted to years by second / 31 557 600 using the Julian year.


See also

* * * * * * * * * * * - Timeline uses the log scale for comparison with the double-logarithmic scale in this article.


References

* {{DEFAULTSORT:Graphical Timeline From Big Bang To Heat Death Big Bang to Heat Death Astrophysics Physical cosmology Astronomy timelines Big Bang