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The categorization of the past into discrete, quantified named blocks of time is called periodization.[1] This is a list of such named time periods as defined in various fields of study. Major categorization systems include cosmological (time periods in the origin and mass evolution of the universe), geological (time periods in the origin and evolution of the Earth), anthropological and historical (time periods in the origin and evolution of human civilization).

Human time periods[edit]

These can be divided broadly into prehistorical periods and historical periods (when written records began to be kept).

In archaeology and anthropology, prehistory is subdivided around the three-age system, this list includes the use of the three-age system as well as a number of various designation used in reference to sub-ages within the traditional three.

The dates for each age can vary by religion. On the [geologic time scale], the [Holocene] epoch starts at the end of the last glacial period of the current ice age (c. 10,000 BCE) and continues to the present. The beginning of the Mesolithic is usually considered to correspond to the beginning of the Holocene epoch.

General periods[edit]


Sociological periods[edit]

Only for late modern contemporary history.

Technological periods[edit]

Wars and financial crisis periods[edit]

American periods[edit]

Australian periods[edit]

Southeast Asian periods[edit]

Filipino periods[edit]

Chinese periods[edit]

Central Asian periods[edit]

Egyptian periods[edit]

European periods[edit]

Indian periods[edit]

Japanese periods[edit]

West Asian periods[edit]

Mythological and astrological time periods[edit]

Geologic time periods[edit]

The geologic time scale covers the extent of the existence of Earth, from about 4600 million years ago to the present day. It is marked by Global Boundary Stratotype Sections and Points. Geologic time units are (in order of descending specificity) eons, eras, periods, epochs, and ages; and the corresponding chronostratigraphic units, which measure "rock-time", are eonothems, erathems, systems, series, and stages.

The second and third timelines are each subsection of their preceding timeline as indicated by asterisks. The Cenozoic is sometimes divided into the Quaternary and Tertiary periods, although the latter is no longer used officially.

Cosmological time periods[edit]

13.8 billion years ago: The Big Bang[edit]

Time Period Duration Description
Planck Epoch From the start to 10−43 seconds after the Big Bang Very little concrete [confirmed] information is known about this epoch. Different theories propose different views on this particular time.
Grand Unification Epoch Between 10−43 to 10−36 seconds after the Big Bang The result of the universe expanding and cooling down during the Planck epoch. All fundamental forces except gravity are unified.
Electroweak Epoch Between 10−36 seconds to 10−12 seconds after the Big Bang The universe cools down to 1028 kelvin. The fundamental forces are split into the strong force and the electroweak force.
Inflationary Epoch Between 10−36 seconds to 10−32 seconds after the Big Bang The shape of the universe flattens due to cosmic inflation.
Quark Epoch Between 10−12 seconds to 10−6 seconds after the Big Bang Cosmic inflation has ended. Quarks are present in the universe at this point. The electroweak force is divided again into the weak force and electromagnetic force.
Hadron Epoch Between 10−6 seconds to 1 second after the Big Bang The universe has cooled enough for quarks to form hadrons, protons, neutrons.
Lepton Epoch Between 1 second to 10 seconds after the Big Bang Most hadrons and anti-hadrons annihilate each other, leaving behind leptons and anti-leptons.
Photon Epoch Between 10 seconds to 370,000 years after the Big Bang Most leptons and anti-leptons annihilate each other. The universe is dominated by photons.
Nucleosynthesis Between 3 minutes to 20 minutes after the Big Bang The temperature of the universe has cooled down enough to allow atomic nuclei to form via nuclear fusion.
Recombination About 377,000 years after the Big Bang Hydrogen and helium atoms form.
Reionization Between 150 million and 1 billion years after the Big Bang The first stars and quasars form due to gravitational collapse.

See also[edit]

References[edit]

Citations[edit]

  1. ^ Adam Rabinowitz. And kingIt’s about time: historical periodization and Linked Ancient World Data. Study of the Ancient universe Papers, 2014.
  2. ^ Iles, Dr Louise (December 30, 2016). "Big digs: The year 2016 in archaeology". BBC News. Retrieved January 3, 2017.
  3. ^ Lohr, Steve (February 11, 2012). "Opinion | Big Data's Impact in the World". The New York Times. ISSN 0362-4331. Retrieved July 2, 2019.
  4. ^ The area had settlements as far back as 9000 BC; see Timeline of ancient Greece
  5. ^ Bowman 2000, pp. 118–161.
  6. ^ a b c The Venture of Islam, Volume 2: The Expansion of Islam in the Middle Periods (1974), p. 3.
  7. ^ A Concise History of the Middle East (2015), p. 53.

Sources cited[edit]

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