Abstract
Big History, the study of the entire time span of the universe in an integrated way, is essentially a study of increasing complexity. Complexity grows exponentially with the Golden Ratio, Phi, and has done so unabruptly since the beginning of time, and will continue to do so until the end of time.
Introduction
Complexity is a notoriously difficult concept to define. Its linguistical origin lies in the Latin word complexus, meaning entwined or twisted together, suggesting that what we consider to be complex are entities that consist of components that operate together, inseparately. Furthermore, these inseparable components have unique properties that the components themselves do not exhibit.
I like to relate entropy to complexity. In the universe entropy is set to increase, because more chaotic, or high entropic configurations, are more likely. Complexity then, can be defined as what happens when entities travel the opposite direction, they export entropy to keep there own entropy low.
It is of course, a relative concept, e.g. when the first molecules formed, they were the most complex, but they are simple, in comparison with multicellar life. It is also impossible to measure, difficult to quantify and often a mere qualitative concept in use. That hasn’t deterred people from making the credible claim that the human brain is the most complex structure in the known universe (1), where signals can travel over a combined 176,000 km of axons or roughly half the distance from here to the moon and neurons are able to make more interactions than there are atoms in the universe. It is also the most complex structure in known history, but it will possibly be usurped in complexity by the worldwide web in the near future. This bar the fact, that we still have no mathematical way to tell if a Boeing 767 or a cucumber is the more complex of the two (after Kevin Kelly (2)).
The rise of complexity is the story behind the Big History, it is the red thread to it and I would like to take it a step further, and call it the driving force behind it; a driving force with a deterministic and constant exponential value.
Every increase in complexity will allow an even faster increase of complexity from there on. The creation of atoms, allowed the creation of the more complex molecule, which in turn allowed the construction of cellular life, which all occurred at an ever faster pace. It is subject to the Law of Accelerating Returns, as proposed by Ray Kurzeil, which states that future increases will be greater than those of the past, because growth is dependent on your starting point (3). I will rewrite this definition, and claim that future growth is just as dependent on your starting point now, as past growth was dependent on your starting point then. In other words, the ratio of the sum of the quantities to the larger quantity is equal to the ratio of the larger quantity to the smaller one, which than is the definition of the Golden Ratio, or Phi (see figure 1).
Where the universe can be defined as a system that is in a constant process of increasing its entropy or its amount of randomness. Complexity and life, travel the complete opposite road, they have negentropy or negative entropy, which is the entropy that it exports to keep its own entropy low. It seems that it is these two forces that are shaping the “Big Future”.
Phi, the Golden Ratio
The rate with which complexity grows is the only rate that ensures exponential growth on equal terms at any point in time; the Golden Ratio, or Phi, which is 1.6180339887. Phi is observed in many objects that exhibit growth and are unrestricted by resource limits; such as plants, trees, celestial bodies and human bodies (e.g. a children’s illness can hamper growth and cause deviations from phi, which are perceived as malformations).
This is because Phi is the only number that allows equal growth independent of scale. No matter where you are in time, future C, will always be equal to starting point B + past complexity A, in the same way that the starting complexity B was obtained from past complexity A + the complexity before it.
Where we to mark each transition in discrete intervals n, one could describe the length of each colored line below as Phi to the power n, which leads to another interesting mathematical ability of Phi, namely 
Hypothesis
The greater complexities of today will cause an increase in complexities of tomorrow at a same rate as the complexities of yesterday caused those of today.
To investigate the rate of complexity growth, I turn to an idea by Ray Kurzweil, to select several key events in our existence, and see how much time it takes to the next, from which an idea of accelerating pace of complexity growth can be obtained. To the left I posted a table with what were in my opinion key events that pointed to an increase in complexity. Subsequently I plotted those on a graph (figure 2). A trendline was added. In red one can find the logarithmic function of the Golden Ratio, Phi, its trendline is x/Phi (or x/1.61803 = 0.6180x).
Because of the subjective nature of the so-called landmark events, I plotted the data accumulated by several sources, listed in the addendum. Projected are several key events in the history of man, from the Big Bang, 13.8 billion years ago, to the origin of life, 3.8 billion years ago and the rise of Homo Sapiens a couple of thousands years ago (data and idea by Ray Kurzweil). Plotted are how many years ago the event took place on one hand, and on the other, how much time it took to the next event. The axes are logarithmic, meaning that the increasing occurrences of landmark events are in fact governed by exponential growth. I also plotted several exponential power functions, with in red f(x) = Phi to the power of x, with Phi =1.61803 (Golden Ratio) and in black to compare a power function 1.25 to the power x and 3 to the power x.
There is the illusion that the graph will hit zero in a few years, marking the onset of the technical singularity. I dispute that and state that the graph will always have looked as if the singularity was near and it always will look as such. This is the nature of exponential complexity growth; it will look impressively steep in comparison with the past, but drudgingly slow compared with the future (4). The Golden Ratio ensures that this comparison between the past, the present and the future is always in the same ratio (see figure 1).
I further propose that on any point in time our ancestor was the most complex object in the known universe. From the near infinite possibilities of change of all the different matter in the universe, there always will be a significant chunk of that getting as fast as possible more complex. Our ancestor, as far as you can speak of it, was the first atom, the first heavy element, the first molecule, the first cellular life, the first sexual reproduced being, the first oxygen using organism, the first mammal, etc. As is the case with the many different genera of Homo that lived from 2 millions ago to up to a couple of thousands years ago, such as Homo Neanderthalis and Homo Erectus, there would be trial and error to decide of several more or less equally complex beings, before this process determined a optimum form; with parts incorporated from other genera, such as Neanderthal genes in ours (similarly there is a theory that viruses are in essence co-evolved with the first RNA, perhaps as an alternative to it, and finally incorporated into the more successful RNA structures).
Here the principle of uniformitarianism can be applied; the present is the key to the past, the same rules and reasonings that are at play now, would have been in place in the past. Any future complex entity can only be imagined to come from us. It is inconceivable that we will be surpassed by any other species we know in complexity. Similarly, it would have been so in the past, and so it will be in the future, as well.
The faith of the Universe, and other implications of a deterministic complexity increase
Asking us to understand the complexity of the future is the equivalent theoretical exercise as to ask the first primates to describe the internet. But I will attempt nonetheless.
Complexity growth seem to be unperturbed by either major paradigm shifts, as the beginning of life, nor by major catastrophic events, such as the end Cretaceous mass extinction, as is evidenced by the remarkable straight line through all events. Also in recent times events such as the Plague, or World War 1 and 2, seem to not have halted technological and economic progress in the long run.
|
Figure 3: Imagine an increasing complex entity underpinning all biodiversity, enabling the creation of an ever wider range of different genera with time (5). |
|
Figure 4: Major catastrophic historic events are not visible on GDP per capita growth, implying an underlying robustness to progress. |
A second point to make is on the existence of extraterrestrial life. On many places you would expect life of lower complexity (perhaps even on other bodies in our own solar system), but on planets that have similar goldilocks conditions as ours has had, that would also have had uninterrupted complexity growth, life would have had the exact same path towards complexity as we had, exactly as fast, and at this point in time, would be exactly as complex as we are now.
Taking these assumptions, one can take them to their ultimate conclusions.
Complexity will grow indefinitely; ever complexer entities will interlink ever more to form even greater complexity. We are at the onset of the great interlinking of our brains, the internet is the first glimpse of that trend. Billions of equally complex brains will merge to form a single complex entity. This entity will than merge with billions of entities of equal complexity across the galaxy, which in the end will merge with all other complex entities in all galaxies until its complexity will rival the Universe. It will encompass all.
References:
(1) http://www.economist.com/node/21537050
(2) What Technology Wants, Kevin Kelly
(3) http://www.kurzweilai.net/the-law-of-accelerating-returns
(4) http://www.kk.org/thetechnium/archives/2006/02/the_singularity.php
(5) http://en.wikipedia.org/wiki/File:Phanerozoic_Biodiversity.png
Addendum:
| Paradigm Shifts for 15 Lists of Key Events, Time to Next Event (Years), Logarithmic Plot | |||
| Paradigm Shifts | |||
| Source (List) | Event | Time Before Present (Years) | Time to Next Event (Years) |
| Carl Sagan | Big Bang |
15000000000 |
5000000000 |
| Carl Sagan | Origin of Milky Way Galaxy |
10000000000 |
5400000000 |
| Carl Sagan | Origin of the Solar System |
4600000000 |
200000000 |
| Carl Sagan | Formation of the Earth |
4400000000 |
400000000 |
| Carl Sagan | Origin of life on Earth |
4000000000 |
300000000 |
| Carl Sagan | Formation of the oldest rocks known on Earth |
3700000000 |
300000000 |
| Carl Sagan | Date of oldest fossils (bacteria and blue-green algae) |
3400000000 |
900000000 |
| Carl Sagan | Invention of sex (by microorganisms) |
2500000000 |
500000000 |
| Carl Sagan | Oldest fossil photosynthetic plants |
2000000000 |
100000000 |
| Carl Sagan | Eukaryotes (first cells with nuclei) flourish |
1900000000 |
700000000 |
| Carl Sagan | Significant oxygen atmosphere begins to develop on Earth |
1200000000 |
200000000 |
| Carl Sagan | Extensive volcanism and channel formation on Mars |
1000000000 |
380000000 |
| Carl Sagan | First worms |
620000000 |
50000000 |
| Carl Sagan | Precambrian ends. Paleozoic Era and Cambrian Period begin. Invertebrates flourish |
570000000 |
40000000 |
| Carl Sagan | First oceanic plankton. Trilobites flourish. |
530000000 |
40000000 |
| Carl Sagan | Ordovician Period. First fish, first vertebrates. |
490000000 |
40000000 |
| Carl Sagan | Silurian Period. First vascular plants. Plants begin colonization of land |
450000000 |
40000000 |
| Carl Sagan | Devonian Period begins. First insects. Animals begin colonization of land |
410000000 |
40000000 |
| Carl Sagan | First amphibians. First winged insects. |
370000000 |
40000000 |
| Carl Sagan | Carboniferous Period. First trees. First reptiles. |
330000000 |
40000000 |
| Carl Sagan | Permian Period begins. First dinosaurs. |
290000000 |
40000000 |
| Carl Sagan | Paleozoic Era ends. Mesozoic Era Begins. |
250000000 |
40000000 |
| Carl Sagan | Triassic Period. First mammals. |
210000000 |
50000000 |
| Carl Sagan | Jurassic Period. First birds. |
160000000 |
40000000 |
| Carl Sagan | Cretaceous Period. First flowers. Dinosaurs become extinct. |
120000000 |
38000000 |
| Carl Sagan | Mesozoic Era ends. Cenozoic Era Tertiary Period begins. First cetaceans. First primates. |
82000000 |
41000000 |
| Carl Sagan | First evolution of frontal lobes in the brain of primates. First hominids. Giant mammals flourish. |
41000000 |
23000000 |
| Carl Sagan | Origin of Proconsul and Ramapithecus, probable ancestors of apes and men |
18000000 |
15400000 |
| Carl Sagan | First humans |
2600000 |
900000 |
| Carl Sagan | Widespread use of stone tools |
1700000 |
1290000 |
| Carl Sagan | Domestication of fire by Peking man |
410000 |
290000 |
| Carl Sagan | Beginning of most recent glacial period |
120000 |
62000 |
| Carl Sagan | Seafarers settle Australia |
58000 |
29000 |
| Carl Sagan | Extensive cave painting in Europe |
29000 |
10000 |
| Carl Sagan | Invention of agriculture |
19000 |
7000 |
| Carl Sagan | Neolithic civilization; first cities |
12000 |
7200 |
| Carl Sagan | First dynasties in Summer, Ebla, and Egypt; development of astronomy |
4800 |
500 |
| Carl Sagan | Invention of the alphabet; Akkadian Empire |
4300 |
500 |
| Carl Sagan | Hammurabic legal codes in Babylon; Middle Kingdom in Egypt |
3800 |
400 |
| Carl Sagan | Bronze metallurgy; Mycenaean culture; Trojan War; Olmec culture; invention of the compass |
3400 |
500 |
| Carl Sagan | Iron metallurgy; First Assyrian Empire; Kingdom of Israel; founding of Carthage by Phoenicia |
2900 |
500 |
| Carl Sagan | Asokan India; Ch’in Dynasty China; Periclean Athens; birth of Buddha |
2400 |
500 |
| Carl Sagan | Euclidian geometry; Archimedean physics; Ptolemaic astronomy; Roman Empire; Christ |
1900 |
500 |
| Carl Sagan | Zero and decimals invented in Indian arithmetic; Rome falls; Moslem conquests |
1400 |
400 |
| Carl Sagan | Mayan civilization; Sung Dynasty China; Byzantine empire; Mongol invasion; crusades |
1000 |
500 |
| Carl Sagan | Renaissance in Europe; voyages of discovery from Europe and from Ming Dynasty China; emergence of the experimental method in science |
500 |
499 |
| Carl Sagan | Widespread development of science and technology; emergence of global culture; acquisition of the means of self-destruction of the human species; first steps in space craft planetary exploration and the search of extraterrestrial intelligence |
1 |
|
| AmericanMuseum of Natural History | Big Bang |
13000000000 |
3000000000 |
| AmericanMuseum of Natural History | Milky Way forms |
10000000000 |
5500000000 |
| AmericanMuseum of Natural History | Sun and planets form |
4500000000 |
700000000 |
| AmericanMuseum of Natural History | Oldest known life (single cell) |
3800000000 |
2800000000 |
| AmericanMuseum of Natural History | First multicellular organisms |
1000000000 |
450000000 |
| AmericanMuseum of Natural History | Cambrian Explosion (burst of new life forms) |
550000000 |
70000000 |
| AmericanMuseum of Natural History | Emergence of first vertebrates |
480000000 |
40000000 |
| AmericanMuseum of Natural History | Early land plants |
440000000 |
50000000 |
| AmericanMuseum of Natural History | Variety of insects begin to flourish |
390000000 |
160000000 |
| AmericanMuseum of Natural History | First dinosaurs appear |
230000000 |
40000000 |
| AmericanMuseum of Natural History | First mammalian ancestors appear |
190000000 |
50000000 |
| AmericanMuseum of Natural History | First known birds |
140000000 |
75000000 |
| AmericanMuseum of Natural History | Dinosaurs wiped out by asteroid or comet |
65000000 |
49000000 |
| AmericanMuseum of Natural History | Apes appear |
16000000 |
12100000 |
| AmericanMuseum of Natural History | First human ancestors to walk upright |
3900000 |
2100000 |
| AmericanMuseum of Natural History | Homo erectus appears |
1800000 |
1785000 |
| AmericanMuseum of Natural History | Anatomically modern humans appear |
15000 |
8700 |
| AmericanMuseum of Natural History | Invention of writing |
6300 |
1700 |
| AmericanMuseum of Natural History | Pyramids built in Egypt |
4600 |
4092 |
| AmericanMuseum of Natural History | Voyage of Christopher Columbus |
508 |
|
| Encyclopaedia Britannica | Oldest prokaryotic fossils |
3500000000 |
1000000000 |
| Encyclopaedia Britannica | Oxygen begins to accumulate in atmosphere |
2500000000 |
400000000 |
| Encyclopaedia Britannica | Oldest eukaryotic fossils |
2100000000 |
1400000000 |
| Encyclopaedia Britannica | Simple multicellular organisms evolve |
700000000 |
280000000 |
| Encyclopaedia Britannica | Plants colonize land |
420000000 |
50000000 |
| Encyclopaedia Britannica | Amphibians appear |
370000000 |
10000000 |
| Encyclopaedia Britannica | First insects |
360000000 |
20000000 |
| Encyclopaedia Britannica | Reptiles appear |
340000000 |
60000000 |
| Encyclopaedia Britannica | Mass extinction |
280000000 |
50000000 |
| Encyclopaedia Britannica | First dinosaurs and mammals |
230000000 |
30000000 |
| Encyclopaedia Britannica | Birds evolve from reptiles |
200000000 |
60000000 |
| Encyclopaedia Britannica | First flowering plants |
140000000 |
74000000 |
| Encyclopaedia Britannica | Mass extinction |
66000000 |
63600000 |
| Encyclopaedia Britannica | Ice age |
2400000 |
2300000 |
| Encyclopaedia Britannica | Advent of modern humans |
100000 |
99999 |
| Encyclopaedia Britannica | Present |
1 |
|
| ERAPS at University of Arizona | No life; shallow seas |
4000000000 |
200000000 |
| ERAPS at University of Arizona | Origin of simple cells |
3800000000 |
300000000 |
| ERAPS at University of Arizona | Origin of cyanobacteria |
3500000000 |
1000000000 |
| ERAPS at University of Arizona | Oxygen accumulates in atmosphere |
2500000000 |
800000000 |
| ERAPS at University of Arizona | Protists and green algae |
1700000000 |
700000000 |
| ERAPS at University of Arizona | Simple multicellular life (sponges, seaweeds) |
1000000000 |
300000000 |
| ERAPS at University of Arizona | More invertebrates (flatworms, jellyfish) |
700000000 |
180000000 |
| ERAPS at University of Arizona | Early animals with hard parts in oceans |
520000000 |
110000000 |
| ERAPS at University of Arizona | Planets invade land |
410000000 |
60000000 |
| ERAPS at University of Arizona | Vertebrates invade land |
350000000 |
50000000 |
| ERAPS at University of Arizona | Coal forming forests, amphibians, BIG insects |
300000000 |
70000000 |
| ERAPS at University of Arizona | Mass extinction (trilobites) |
230000000 |
30000000 |
| ERAPS at University of Arizona | Pangaea, first mammals, first reptiles |
200000000 |
135000000 |
| ERAPS at University of Arizona | Mass extinction (including dinosaurs) |
65000000 |
35000000 |
| ERAPS at University of Arizona | Small mammals, humanoids |
30000000 |
28000000 |
| ERAPS at University of Arizona | Early Humans |
2000000 |
1999999 |
| ERAPS at University of Arizona | Us |
1 |
|
| Paul Boyer | Big bang |
15000000000 |
10200000000 |
| Paul Boyer | Solar system forms |
4800000000 |
200000000 |
| Paul Boyer | Earth forms |
4600000000 |
600000000 |
| Paul Boyer | Nitrogen atmosphere (for winds) is present or acquired |
4000000000 |
100000000 |
| Paul Boyer | Abundant water is present or acquired, Organic precursors for life forms accumulate, Primitive living organisms arise or (less likely) come from space |
3900000000 |
400000000 |
| Paul Boyer | Land temperature stabilizes so that most of the water is liquid |
3500000000 |
300000000 |
| Paul Boyer | Some life forms get energy from oxidationreduction reactions |
3200000000 |
200000000 |
| Paul Boyer | Organisms evolve to gain many present biochemical characteristics |
3000000000 |
300000000 |
| Paul Boyer | Photosynthetic capacity is acquired, and oxygen evolution begins |
2700000000 |
100000000 |
| Paul Boyer | Land surfaces form and plate tectonics established |
2600000000 |
200000000 |
| Paul Boyer | Evolution produces organisms that can use oxygen to make ATP |
2400000000 |
300000000 |
| Paul Boyer | Abundant microorganisms colonize the entire earth. |
2100000000 |
1400000000 |
| Paul Boyer | Multicellular organisms arise with increased capacity for structural differentiation |
700000000 |
300000000 |
| Paul Boyer | Primitive plant forms begin to evolve stems, roots, and leaves |
400000000 |
397400000 |
| Paul Boyer | First humans |
2600000 |
900000 |
| Paul Boyer | Widespread use of stone tools |
1700000 |
700000 |
| Paul Boyer | Acquisition of spoken language |
1000000 |
995000 |
| Paul Boyer | Acquisition of written language |
5000 |
4500 |
| Paul Boyer | They learn that knowledge comes from observation and experiment (scientific method) |
500 |
300 |
| Paul Boyer | Ability to control nature gives rise to a human population explosion |
200 |
100 |
| Paul Boyer | The above abilities give rise to a remarkable understanding of nature |
100 |
|
| Barrow and Silk | Big Bang |
20000000000 |
1500000000 |
| Barrow and Silk | Galaxies begin to form |
18500000000 |
1500000000 |
| Barrow and Silk | Galaxies begin to cluster |
17000000000 |
1000000000 |
| Barrow and Silk | Our protogalaxy collapses; first stars form |
16000000000 |
1000000000 |
| Barrow and Silk | Quasars are born; Population II stars form |
15000000000 |
5000000000 |
| Barrow and Silk | Population I stars form |
10000000000 |
5200000000 |
| Barrow and Silk | Our parent interstellar cloud forms |
4800000000 |
100000000 |
| Barrow and Silk | Collapse of protosolar nebula |
4700000000 |
100000000 |
| Barrow and Silk | Planets form; rock solidifies |
4600000000 |
300000000 |
| Barrow and Silk | Intense cratering of planets |
4300000000 |
400000000 |
| Barrow and Silk | Oldest terrestrial rocks form |
3900000000 |
900000000 |
| Barrow and Silk | Microscopic life forms |
3000000000 |
1000000000 |
| Barrow and Silk | Oxygen rich atmosphere develops |
2000000000 |
1000000000 |
| Barrow and Silk | Macroscopic life forms |
1000000000 |
400000000 |
| Barrow and Silk | Earliest fossil record |
600000000 |
150000000 |
| Barrow and Silk | First fishes |
450000000 |
50000000 |
| Barrow and Silk | Early land plants |
400000000 |
100000000 |
| Barrow and Silk | Ferns, conifers |
300000000 |
100000000 |
| Barrow and Silk | First mammals |
200000000 |
50000000 |
| Barrow and Silk | First birds |
150000000 |
90000000 |
| Barrow and Silk | First primates |
60000000 |
10000000 |
| Barrow and Silk | Mammals increase |
50000000 |
49900000 |
| Barrow and Silk | Homo sapiens |
100000 |
|
| Jean Heidmann | Big Bang, etc. |
15000000000 |
7000000000 |
| Jean Heidmann | Age of most distant galaxies |
8000000000 |
3500000000 |
| Jean Heidmann | Formation of the Sun and the Earth |
4500000000 |
1000000000 |
| Jean Heidmann | First bacteria |
3500000000 |
2000000000 |
| Jean Heidmann | First eucaryotic organisms |
1500000000 |
1000000000 |
| Jean Heidmann | Explosion of life in the Cambria era |
500000000 |
496500000 |
| Jean Heidmann | The dawn of Australopithecus |
3500000 |
1000000 |
| Jean Heidmann | Homo habili uses tools |
2500000 |
1500000 |
| Jean Heidmann | Homo erectus masters the use of fire |
1000000 |
960000 |
| Jean Heidmann | Invention of writing |
40000 |
38000 |
| Jean Heidmann | Eratosthenes measures the size of the Earth |
2000 |
1600 |
| Jean Heidmann | Copernicus, Galileo |
400 |
|
| IGPP Symposium | Formation of the Earth |
4600000000 |
600000000 |
| IGPP Symposium | Origin of Life on Earth |
4000000000 |
200000000 |
| IGPP Symposium | Formation of the oldest rocks known on Earth |
3800000000 |
300000000 |
| IGPP Symposium | Date of oldest fossils and stromatolites |
3500000000 |
700000000 |
| IGPP Symposium | Abundant cyanobacteria and stromatolites |
2800000000 |
300000000 |
| IGPP Symposium | Abundant iron formations |
2500000000 |
400000000 |
| IGPP Symposium | Latest detrital uraninite/pyrite |
2100000000 |
200000000 |
| IGPP Symposium | Atmospheric oxygen |
1900000000 |
100000000 |
| IGPP Symposium | Nucleated cells (phytoplankton) |
1800000000 |
700000000 |
| IGPP Symposium | Complex (sexual) phytoplankton |
1100000000 |
250000000 |
| IGPP Symposium | Seaweeds and protozoans |
850000000 |
250000000 |
| IGPP Symposium | Animals without backbones |
600000000 |
100000000 |
| IGPP Symposium | Fish |
500000000 |
100000000 |
| IGPP Symposium | Land plants and animals |
400000000 |
100000000 |
| IGPP Symposium | Coal swamps |
300000000 |
100000000 |
| IGPP Symposium | Dinosaurs and birds |
200000000 |
100000000 |
| IGPP Symposium | Flowering plants |
100000000 |
98000000 |
| IGPP Symposium | Humans |
2000000 |
|
| Phillip Tobias | Divergence of orangutan lineage from Hominoidea |
16000000 |
8500000 |
| Phillip Tobias | Divergence of gorilla from other African hominoids |
7500000 |
1500000 |
| Phillip Tobias | Uplift, cooling, and aridification of Africa |
6000000 |
300000 |
| Phillip Tobias | Chimpanzee hominid divergence, inferred appearance of Hominidae |
5700000 |
200000 |
| Phillip Tobias | “Messinian crisis”, the drying up of the Mediterranean / Spread of African savannah / etc. |
5500000 |
700000 |
| Phillip Tobias | Earliest known fossils identifiable as probable hominid |
4800000 |
1000000 |
| Phillip Tobias | Earliest fossil evidence of hominid bipedalism |
3800000 |
1000000 |
| Phillip Tobias | Hominid fossils known |
2800000 |
100000 |
| Phillip Tobias | Differentiation of postulated “derived A. africanus” |
2700000 |
100000 |
| Phillip Tobias | One or more splittings of hominid lineage; earliest known Australopithecus boisei fossils; earliest known stone cultural remains. |
2600000 |
300000 |
| Phillip Tobias | Acquisition of spoken language (as here inferred); many changes in mammalian fauna of Africa (baboons, elephants, pigs, bovids, hippopotami, sabertoothed cats, rodents) |
2300000 |
200000 |
| Phillip Tobias | Earliest known Homo habilis fossils |
2100000 |
100000 |
| Phillip Tobias | Earliest modern human brain form; earliest signs of marked brain enlargement in hominids. |
2000000 |
200000 |
| Phillip Tobias | Movement of hominids from Africa to Asia and Europe |
1800000 |
100000 |
| Phillip Tobias | Emergence of Homo erectus |
1700000 |
400000 |
| Phillip Tobias | Acquisition of fire by H. erectus |
1300000 |
100000 |
| Phillip Tobias | Extinction of robust and hyperrobust australopithecines |
1200000 |
700000 |
| Phillip Tobias | Emergence of Homo sapiens |
500000 |
390000 |
| Phillip Tobias | Earliest known “anatomically modern Homo sapiens” |
110000 |
10000 |
| Phillip Tobias | Earliest burial of the dead |
100000 |
60000 |
| Phillip Tobias | Emergence of “modern human culture) |
40000 |
5000 |
| Phillip Tobias | Earliest rock art; earliest protowriting |
35000 |
30000 |
| Phillip Tobias | Earliest writing |
5000 |
|
| David Nelson | Planet earth forms |
4500000000 |
500000000 |
| David Nelson | Planet surface cools and bombardment from space slows, so life has the possibility of existing on the planet. Oldest earth rocks dated by radioactivity. |
4000000000 |
100000000 |
| David Nelson | Evidence for life seen in Greenland rocks enriched in C12 isotope. Prokaryotes diverge from archaea. Chlorophyll and photosynthesis evolve in the bacterial lineage. |
3900000000 |
200000000 |
| David Nelson | First banded iron formation seen. Implies oxygen made by photosynthesis |
3700000000 |
200000000 |
| David Nelson | First stromatolites seen. |
3500000000 |
1400000000 |
| David Nelson | First tentative evidence of a eukaryotic microfossil |
2100000000 |
100000000 |
| David Nelson | Oxygen begins to rise in the atmosphere after oxygen sinks saturated. |
2000000000 |
500000000 |
| David Nelson | Oxygen level in the atmosphere reaches present day level and stabilizes. More convincing evidence of eukaryotic microfossils. Chloroplasts and mitochondria present. |
1500000000 |
300000000 |
| David Nelson | Major eukaryotic phyla diverge. Plants branched before animals/fungi |
1200000000 |
600000000 |
| David Nelson | Invertebrates and vertebrates diverge. Hox gene cluster exists. |
600000000 |
70000000 |
| David Nelson | Cambrian explosion of fossil record. |
530000000 |
130000000 |
| David Nelson | Fish and other vertebrates diverge. Plants and fungi invade the land |
400000000 |
20000000 |
| David Nelson | Vertebrates move onto land |
380000000 |
20000000 |
| David Nelson | Gymnosperms (naked seed plants) diverge from angiosperms (flowering plants) |
360000000 |
60000000 |
| David Nelson | Birds and other vertebrates diverge. |
300000000 |
120000000 |
| David Nelson | Monocots diverge from dicots |
180000000 |
40000000 |
| David Nelson | Oldest angiosperm fossil |
140000000 |
80000000 |
| David Nelson | Last common ancestor of all polymorphism sequences |
60000000 |
55000000 |
| David Nelson | Chimpanzees and humans diverge |
5000000 |
3300000 |
| David Nelson | Homo sapiens |
1700000 |
1500000 |
| David Nelson | Last common ancestor of all human mitochondrial DNA types |
200000 |
141000 |
| David Nelson | Modern humans |
59000 |
|
| Goran Burenhult (ed.) | Purgatorius |
60000000 |
5000000 |
| Goran Burenhult (ed.) | Petrolemuridae |
55000000 |
10000000 |
| Goran Burenhult (ed.) | Adapiformes, omomylformes |
45000000 |
5000000 |
| Goran Burenhult (ed.) | Aegyptopithecus, Propliapithecus, Oligopithecus, Catopithecus |
40000000 |
2000000 |
| Goran Burenhult (ed.) | Afrotarsius |
38000000 |
11000000 |
| Goran Burenhult (ed.) | Omomylformes, Branisella |
27000000 |
9000000 |
| Goran Burenhult (ed.) | Prohylobates, Micropithecus, Afropithecus Proconsul |
18000000 |
3000000 |
| Goran Burenhult (ed.) | Kenyopithecus, Dryopithecus |
15000000 |
4000000 |
| Goran Burenhult (ed.) | Krishnapithecus |
11000000 |
1000000 |
| Goran Burenhult (ed.) | Sivapithecus |
10000000 |
500000 |
| Goran Burenhult (ed.) | Ouranopithecus |
9500000 |
3000000 |
| Goran Burenhult (ed.) | Samburu maxilla |
6500000 |
1500000 |
| Goran Burenhult (ed.) | Gigantopithecus |
5000000 |
3200000 |
| Goran Burenhult (ed.) | Orangutans, emergence of stone tools |
1800000 |
300000 |
| Goran Burenhult (ed.) | Appearance of the erectines |
1500000 |
870000 |
| Goran Burenhult (ed.) | Acheulian technology |
630000 |
80000 |
| Goran Burenhult (ed.) | Homo erectus |
550000 |
200000 |
| Goran Burenhult (ed.) | Homo heidelbergensis |
350000 |
120000 |
| Goran Burenhult (ed.) | Control of fire |
230000 |
30000 |
| Goran Burenhult (ed.) | Homo sapiens, modern humans |
200000 |
70000 |
| Goran Burenhult (ed.) | Neanderthalis |
130000 |
60000 |
| Goran Burenhult (ed.) | Mousterian technology |
70000 |
35000 |
| Goran Burenhult (ed.) | Art |
35000 |
|
| Johanson and Edgar | Ardipithecus ramidus |
4400000 |
200000 |
| Johanson and Edgar | Australopithecus anamensis |
4200000 |
300000 |
| Johanson and Edgar | Australopithecus afarensis |
3900000 |
1100000 |
| Johanson and Edgar | Australopithecus africanus |
2800000 |
100000 |
| Johanson and Edgar | Australopithecus aethiopicus |
2700000 |
200000 |
| Johanson and Edgar | Homo sp? |
2500000 |
100000 |
| Johanson and Edgar | Homo rudolfensis |
2400000 |
100000 |
| Johanson and Edgar | Australopithecus boisei |
2300000 |
400000 |
| Johanson and Edgar | Homo habilis / Australopithecus habilis |
1900000 |
100000 |
| Johanson and Edgar | Homo ergaster |
1800000 |
600000 |
| Johanson and Edgar | Homo erectus |
1200000 |
600000 |
| Johanson and Edgar | Homo heldelbergensis |
600000 |
300000 |
| Johanson and Edgar | Homo neanderthalensis |
300000 |
200000 |
| Johanson and Edgar | Homo sapiens |
100000 |
|
| Modis 2002 | Big Bang / quarks / protons & neutrons / atoms of elements |
15000000000 |
3000000000 |
| Modis 2002 | First stars |
12000000000 |
7400000000 |
| Modis 2002 | First planets / rock solidification / solar system |
4600000000 |
800000000 |
| Modis 2002 | First life / cooling of Earth / formation of first rocks / water forms |
3800000000 |
2800000000 |
| Modis 2002 | First multicellular life (sponges, seaweeds) |
1000000000 |
470000000 |
| Modis 2002 | Cambrian explosion / invertebrates / vertebrates |
530000000 |
330000000 |
| Modis 2002 | First mammals |
200000000 |
135000000 |
| Modis 2002 | First primates / asteroid collision |
65000000 |
48000000 |
| Modis 2002 | First orangutan |
17000000 |
11000000 |
| Modis 2002 | First hominids |
6000000 |
3400000 |
| Modis 2002 | First stone tools |
2600000 |
1600000 |
| Modis 2002 | Development of speech / Homo sapiens |
1000000 |
500000 |
| Modis 2002 | Discovery of fire / hunting gathering society |
500000 |
400000 |
| Modis 2002 | Emergence of “modern humans” / earliest burial of the dead / agrarian pastoral / sociocultural systems |
100000 |
65000 |
| Modis 2002 | Rock art / protowriting |
35000 |
25000 |
| Modis 2002 | Agriculture / prehistoric nomadic bands / techniques for starting fire |
10000 |
5000 |
| Modis 2002 | Discovery of the wheel / writing / archaic empires / large civilizations / Egypt / Mesopotamia |
5000 |
2500 |
| Modis 2002 | Democracy / city states / Greeks / Buddha |
2500 |
500 |
| Modis 2002 | Christianity |
2000 |
1325 |
| Modis 2002 | Gunpowder |
675 |
175 |
| Modis 2002 | Renaissance (printing press) / discovery of new world / the scientific method |
500 |
275 |
| Modis 2002 | Industrial revolution (steam engine) / political revolutions (French, USA) |
225 |
125 |
| Modis 2002 | Modern physics / radio / electricity / automobile / airplane / capitalism & colonialism |
100 |
50 |
| Modis 2002 | DNA / transistor / nuclear energy / W.W.II / cold war / sputnik |
50 |
45 |
| Modis 2002 | Internet / human genome sequenced |
5 |
|
| Richard Coren | Big Bang |
15000000000 |
11500000000 |
| Richard Coren | Solidification of Earth Prokaryotic life |
3500000000 |
2750000000 |
| Richard Coren | Eukaryotic radiation |
750000000 |
575000000 |
| Richard Coren | Appearance of class Mammalia |
175000000 |
142500000 |
| Richard Coren | Appearance of superfamily Hominoidea |
32500000 |
25500000 |
| Richard Coren | Appearance of family Hominidae |
7000000 |
5250000 |
| Richard Coren | Appearance of genus Homo |
1750000 |
1500000 |
| Richard Coren | Appearance of archaic Homo sapiens |
250000 |
180000 |
| Richard Coren | Appearance of H. sapiens sapiens |
70000 |
55000 |
| Richard Coren | Development of communal villages |
15000 |
11000 |
| Richard Coren | Development of writing |
4000 |
3441 |
| Richard Coren | Development of printing |
559 |
500 |
| Richard Coren | Development of digital electronics and computing |
59 |
|
| Modis 2003 | Big Bang |
15500000000 |
5500000000 |
| Modis 2003 | Origin of Milky Way |
10000000000 |
6000000000 |
| Modis 2003 | Origin of life on Earth |
4000000000 |
2000000000 |
| Modis 2003 | First eukaryotes |
2000000000 |
1000000000 |
| Modis 2003 | First multicellular life |
1000000000 |
570000000 |
| Modis 2003 | Cambrian explosion |
430000000 |
220000000 |
| Modis 2003 | First mammals |
210000000 |
71000000 |
| Modis 2003 | First flowering plants |
139000000 |
84400000 |
| Modis 2003 | Asteroid collision |
54600000 |
26100000 |
| Modis 2003 | First hominids |
28500000 |
12000000 |
| Modis 2003 | First orangutan |
16500000 |
11400000 |
| Modis 2003 | Chimpanzees and humans diverge |
5100000 |
2900000 |
| Modis 2003 | First stone tools |
2200000 |
1645000 |
| Modis 2003 | Emergence of Homo Sapiens |
555000 |
230000 |
| Modis 2003 | Domestication of fire |
325000 |
125000 |
| Modis 2003 | Differentiation of human DNA types |
200000 |
94300 |
| Modis 2003 | Emergence of “modern humans” |
105700 |
69900 |
| Modis 2003 | Rock art, protowriting |
35800 |
16600 |
| Modis 2003 | Invention of agriculture |
19200 |
8200 |
| Modis 2003 | Techniques for starting fire |
11000 |
6093 |
| Modis 2003 | Development of the wheel, writing |
4907 |
2470 |
| Modis 2003 | Democracy |
2437 |
997 |
| Modis 2003 | Zero and decimals invented in Indian arithmetic |
1440 |
901 |
| Modis 2003 | Renaissance (printing press) |
539 |
314 |
| Modis 2003 | Industrial Revolution (steam engine) |
225 |
125 |
| Modis 2003 | Modern physics |
100 |
50 |
| Modis 2003 | DNA structure described, transistor invented, nuclear energy |
50 |
45 |
| Modis 2003 | Internet, human genome sequenced |
5 |
|
























