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 Online History sources include Online History sources include
-  * [[ http://www.bartleby.com/86/ | A Short History of the World, HG Wells, 1922 ]] +  * [[ http://en.wikipedia.org/wiki/History_of_the_universe | Wikipedia History of the Universe ]]
-  * [[http://www.bartleby.com/67 | Encyclopedia of World History, Peter Stearns, 2001]] +
-  * [[ http://en.wikibooks.org/wiki/Astronomy/Short_History_of_the_Universe | A short History of the Universe ]]+
   * [[http://www.pbs.org/wgbh/nova/origins/universe.html | PBS Nova History of the Universe]]   * [[http://www.pbs.org/wgbh/nova/origins/universe.html | PBS Nova History of the Universe]]
   * [[ http://www.pbs.org/deepspace/timeline/index.html | PBS Deep Space Timeline]]   * [[ http://www.pbs.org/deepspace/timeline/index.html | PBS Deep Space Timeline]]
-  * [[ http://en.wikipedia.org/wiki/History_of_the_universe || Wikipedia History of the Universe ]]+  * [[ http://en.wikibooks.org/wiki/Astronomy/Short_History_of_the_Universe | A short History of the Universe ]] 
 + 
 +  * [[http://en.wikipedia.org/wiki/Prehistoric_life | Wikipedia History of Life ]] 
 +  * [[http://www.pbs.org/wgbh/nova/link/history.html | PBS History of Life ]] 
 +  * [[http://www.ucmp.berkeley.edu/exhibits/index.php | University of California Paleontology Online]] 
 +  * [[ http://en.wikipedia.org/wiki/History_of_Earth | Wikipedia History of the Earth]] 
 + 
 +  * [[http://www.bartleby.com/67 | Encyclopedia of World History, Peter Stearns, 2001]] 
 +  * [[ http://www.bartleby.com/86/ | A Short History of the World, HG Wells, 1922 ]]
  
 ===== History of The Universe ===== ===== History of The Universe =====
  
   * 13.7 Billion Years ago - Big Bang   * 13.7 Billion Years ago - Big Bang
-    * - 10<sup>-32</sup> second - hyper-inflation+    * - 10<sup>-32</sup> second after Big Bang (abb) - hyper-inflation
     * 10<sup>-32</sup> - 10<sup>-6</sup>second - inflation slows, gravity emerges followed by strong , weak and electromagnetic forces. Matter consists of fundamental particles including quarks, electrons, photons, and neutrinos.     * 10<sup>-32</sup> - 10<sup>-6</sup>second - inflation slows, gravity emerges followed by strong , weak and electromagnetic forces. Matter consists of fundamental particles including quarks, electrons, photons, and neutrinos.
-    * 10<sup>-6</sup> - 1 second - hadrons (protons and neutrons) form +    * 10<sup>-6</sup> - 1 second abb - hadrons (protons and neutrons) form 
-    * 3-20 minutes - deuteron, helium and lithium nuclei form. 3 times as much hydrogen than helium by mass. Only traces of other nuclei. +    * 3 - 20 minutes abb- deuteron, helium and lithium nuclei form. 3 times as much hydrogen than helium by mass. Only traces of other nuclei. 
-    * 300,000 years after big bang - expanding cloud of gas cools enough for electrons to associate with nuclei forming atoms +    * 300,000 years abb - expanding cloud of gas cools enough for electrons to associate with nuclei forming atoms 
-    * .5 - 1 billion years after big bang - earliest stars and galaxies form +    * .5 - 1 billion years abb - earliest stars and galaxies form 
-    * 1 - 3 billion years after big bang - larger galaxies with black holes and quasars at their centre form +    * 1 - 3 billion years abb - larger galaxies with black holes and quasars at their centre form 
-  * 7 - 10 billion years ago - Milky Way galaxy forms +  * 7 - 10 billion years ago (bya)- Milky Way galaxy forms 
-  * 4.5-5 billion years ago - Sun and Earth form +  * 4.6 bya - Solar System forms 
-  * 3.7 billion years ago - first life on Earth +  * 3.7 bya - first life on Earth 
-  * 1.7 billion years ago - multicellular life on Earth+  * 1.7 bya - multi-cellular life on Earth
   * ---------------------   * ---------------------
-  * 3.3 billion years in the future - Milky Way collides with Andromeda +  * 3.3 billion years from now - Milky Way collides with Andromeda 
-  * 6.3 billion years in the future - Sun dies +  * 6.3 billion years from now - Sun dies 
-  * 100 trillion years in the future - Stars have all blown up and collapsed into black holes and neutron stars, or have withered into white dwarfs. +  * 100 trillion years from now - Stars have all blown up and collapsed into black holes and neutron stars, or have withered into white dwarfs. 
-  * 10<sup>37</sup> years in the future - After an epoch of proton decay, the only stellar-like objects remaining are evaporating black holes. +  * 10<sup>37</sup> years from now - After an epoch of proton decay, the only stellar-like objects remaining are evaporating black holes. 
-  * 10<sup>100</sup> years in the future - Black holes have evaporated. Only fundamental particles remain:  photons of colossal wavelength, neutrinos, electrons, and positrons.+  * 10<sup>100</sup> years from now - Black holes have evaporated. Only fundamental particles remain:  photons of colossal wavelength, neutrinos, electrons, and positrons.
  
 ===== History of Life ===== ===== History of Life =====
  
 +  * Hadean Eon : 4.6 - 3.8 billion years ago (bya) 
 +    * 4.6 bya - Earth forms 
 +    * 4.4 bya - Earth's crust forms 
 +    * 4 bya - Clouds, rain and oceans 
 +  * Archean Eon : 3.8 - 2.5 bya 
 +    * 3.8 bya - first life on Earth 
 +    * 3.5 bya - photosynthesis starts 
 +  * Proterozoic Eon : 2.5 bya - 550 mya 
 +    * 2.4 bya - oxygen becomes significant component of the atmosphere 
 +    * 1 bya - multicellular plants (algae) and animals 
 +    * 770 - 750 mya - first ice age 
 +  * before 550 mya is aka the Precambrian Period or Supereon. After 550 mya is aka the Phanerozoic Eon. 
 +  * **Paleozoic (Primary) Era** : 550 - 250 mya 
 +    * Cambrian - small shelled animals, corals 
 +    * Ordovician - starfish, jawless fish 
 +    * Silurian - land plants, ferns, sharks, fish 
 +    * Devonian - first tetrapods - evolution of fish onto land 
 +    * Carboniferous - reptiles, amphibians, spiders, conifers, amniotic eggs (340 mya), synapsids 
 +    * Permian - more synapsids (proto-mammalian reptiles).  
 +  * 250 mya - Extinction event, 83% of species die off 
 +  * 300 mya - 250 mya - last supercontinent Pangaea exists 
 +  * **Mesozoic (Secondary) Era** : 250 - 65 mya 
 +    * Triassic - turtles, lizards, dinosaurs, mammals 
 +    * Extinction event 200 mya allows dinosaurs to start to become dominant. Kills > 50 % of species. 
 +    * Jurassic - squids, frogs, birds 
 +    * Cretaceous - more dinosaurs, flowering plants, snakes, modern fish, toothed birds 
 +  * 65 mya - Meterorite extinction event (off Yucatan peninsula) kills off most large animals 
 +  * **Cenozoic Era** : 65 mya - present 
 +    * Tertiary - more mammals, grasses, apes, hominids 
 +    * Quaternary 
 +      * Pleistocene (1.8 mya - 8000 ya) - mammoths, Neanderthals 
 +      * Holocene (8000 ya - now) - modern humans
notes/history.1793661401.txt.gz · Last modified: 2026/11/02 15:16 by 171.236.48.62