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This is the timeline of the stelliferous era but also partly charts the primordial era, and charts more of the degenerate era of the heat death scenario. The scale is 10 \times \log_\ where \ is the time since the Big Bang expressed in years. Example: one million years is \ = 1000000;\ \ 10 \times \log_\ = 10\times 6 = 60.


Timeline

ImageSize = width:720 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:era2 value:lightorange id:era1 Value:yellowgreen DateFormat = yyyy Period = from:56 till:200 TimeAxis = format:yyyy orientation:vertical ScaleMajor = unit:year increment:10 start:60 ScaleMinor = unit:year increment:1 start:56 AlignBars = justify BarData = bar:Era bar:Dummy2 bar:Dummy3 bar:Periods bar:Dummy4 bar:Events TextData = fontsize:M pos:(250,75) text:" Photon epoch" pos:(260,657) text:" ZOOM IN" pos:(107,1645) text:" NEXT" pos:(65,1630) text:"The Degenerate Era" pos:(65,120) text:" The Primordial Era" pos:(85,105) text:"PREVIOUS" PlotData= textcolor:black fontsize:M width:165 bar:Era mark:(line,white) align:center shift:(0,0) from:60 till:140 color:era2 text:" The Stelliferous Era" width:55 bar:Dummy2 bar:Dummy3 width:165 bar:Periods align:center shift:(0,0) mark:(line,white) from:56 till:80 color:period1 text:" Dark Ages" from:80 till:90 color:period2 text:" Reionization" from:98 till:100 color:period1 text:" Formation of the Milky Way~galactic disk" shift:(0,2) from:100 till:102 color:period2 text:"Life on Earth" from:190 till:200 color:period1 width:55 bar:Dummy4 width:55 mark:(line,purple) textcolor:black fontsize:M bar:Events color:events align:left shift:(30,-4) at: 56 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 forms." shift:(30,-15) at: 60 text:"One million years" at: 80 text:"100 million years. First star began to shine." at: 88 text:"600 million years ~ Formation of the first galaxy" at: 90 text:"One billion years" at: 96 text:"4 billion years ~ earliest Population I stars" at:100 text:" 9.1 billion years Formation of Earth~ and Sun" at:101 mark:(line,magenta) text:"13.7 billion years, the present day" # at:102 shift:(30,10) text:" 16.7 billion years Collision of Milky Way and~Andromeda galaxies" at:103 shift:(30,0) text:" 19.1 billion years. Sun becomes a red giant ~ and shortly thereafter a white dwarf" at:120 text:"One trillion years" at:140 text:"Formation of new stars ceases.~Stars cease to fuse. " at:150 text:"One quadrillion years. ~Solar systems no longer exist. Planets flung ~out of orbit or consumed by larger bodies.~ Sun has become a~ black dwarf." at:180 text:"One quintillion years" at:195 text:"Galaxies no longer exist. Stars flung out of orbit ~or consumed by black holes." mark:(line,white)


See also

*
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 ...
* Cyclic model * Dyson's eternal intelligence * Final anthropic principle * Future of an expanding universe * Graphical timeline from Big Bang to Heat Death. Timeline uses double-logarithmic scale. *
Graphical timeline of the Big Bang This timeline of the Big Bang shows a sequence of events as currently theorized by scientists. It is a logarithmic scale that shows 10 \cdot \log_ ''second'' instead of ''second''. For example, one microsecond is 10 \cdot \log_ 0.000 001 = 10 \ ...
*
Graphical timeline of the universe This more than 20-billion-year timeline of our universe shows the best estimates of major events from the universe's beginning to anticipated future events. Zero on the scale is the present day. A large step on the scale is one billion years; a s ...
. Timeline uses linear time. * Heat death of the universe * List of other end scenarios than Heat Death *
1 E19 s and more An order of magnitude of time is usually a decimal prefix or decimal order-of-magnitude quantity together with a base unit of time, like a microsecond or a million years. In some cases, the order of magnitude may be implied (usually 1), like a ...
* Second law of thermodynamics * Ultimate fate of the Universe * The Last Question, story by
Isaac Asimov yi, יצחק אזימאװ , birth_date = , birth_place = Petrovichi, Russian SFSR , spouse = , relatives = , children = 2 , death_date = , death_place = Manhattan, New York City, U.S. , nationality = Russian (1920–1922)Soviet (192 ...
which considers the oncome of heat death in the universe and how it may be reversed. {{DEFAULTSORT:Graphical Timeline Of The Stelliferous Era Stelliferous Era Astrophysics Physical cosmology