List of time periods

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

These can be divided broadly into prehistorical (before history began to be recorded) 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 region. 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 Mesolithic is usually considered to correspond to the beginning of the Holocene epoch.

General periods

  • Pre-History – Period between the appearance of Homo ("humans"; first stone tools c. three million years ago) and the invention of writing systems (for the Ancient Near East: c. five thousand years ago).
    • Stone Age
      • Paleolithic – is the earliest period of the Stone Age
      • Mesolithic (Epipaleolithic) – was a period in the development of human technology between the Palaeolithic and Neolithic periods.
      • Neolithic – a period of primitive technological and social development, beginning about 10,200 BCE in parts of the Middle East, and later in other parts of the world.
      • Chalcolithic (or "Eneolithic", "Copper Age") – this period was still largely Neolithic in and civilizations who had adopted or developed a writing system.
    • Protohistory – Period between prehistory and history, during which a culture or civilization has not yet developed writing but other cultures have already noted its existence in their own writings; the absolute time scale of "protohistory" varies widely depending on the region, from the late 4th millennium BCE in the Ancient Near East to the present in the case of uncontacted peoples.
  • Ancient History – Aggregate of past events from the beginning of recorded human history and extending as far as the Early Middle Ages or the Postclassical Era. The span of recorded history is roughly less than five thousand years, beginning with the earliest linguistic records in the third millennium BCE in Mesopotamia and China
    • Classical Antiquity – Broad term for a long period of cultural history centered on the Mediterranean Sea, comprising the interlocking civilizations of ancient Greece and ancient Rome, collectively known as the Greco-Roman world. It is the period in which Greek and Roman society flourished and wielded great influence throughout Europe, North Africa and the Middle East.
  • Post-Classical History – Period of time that immediately followed ancient history. Depending on the continent, the era generally falls between the years CE 200–600 and CE 1200–1500. The major classical civilizations the era follows are Han China (ending in 220), the Western Roman Empire (in 476), the Gupta Empire (in the 550s), and the Sasanian Empire (in 651).
  • Modern History – After the post-classical era

Socio-cultural periods

Only for Late Modern Contemporary history.

Technology periods

Wars and crisis periods

American periods

Southeast Asian periods

Filipino periods

Chinese periods

Central Asian periods

Egyptian periods

European periods

Indian periods

Japanese periods

West Asian periods

Mythological and astrological time periods

  • Astrological Ages
  • Greek Mythology (See also: Ages of Man)
    • Golden Age (self-sufficient)
    • Silver Age (self-indulgent)
    • Bronze Age (warlike)
    • Heroic Age (nobly aspirant)
    • Iron Age (violent)
  • Aztec Mythology
    • Nahui-Ocelotl, Destroyed by Jaguars
    • Nahui-Ehécatl, Destroyed by Hurricane
    • Nahuiquiahuitl, Destroyed by Flaming Rain
    • Nahui-Atl, Destroyed by Flood
    • Nahui-Ollin, the one we are in now, Destroyed by Earthquakes (the end was said to be in 2012, but that did not occur)

Geologic time periods

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 subsections 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

13.8 billion years ago: The Big Bang

Time PeriodDurationDescription
Planck EpochFrom the start to 10−43 seconds after the Big BangVery little concrete [confirmed] information is known about this epoch. Different theories propose different views on this particular time.
Grand Unification EpochBetween 10−43 to 10−36 seconds after the Big BangThe result of the universe expanding and cooling down during the Planck epoch. All fundamental forces except gravity are unified.
Electroweak EpochBetween 10−36 seconds to 10−12 seconds after the Big BangThe universe cools down to 1028 kelvin. The fundamental forces are split into the strong force and the electroweak force.
Inflationary EpochBetween 10−36 seconds to 10−32 seconds after the Big BangThe shape of the universe flattens due to cosmic inflation.
Quark EpochBetween 10−12 seconds to 10−6 seconds after the Big BangCosmic 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 EpochBetween 10−6 seconds to 1 second after the Big BangThe universe has cooled enough for quarks to form hadrons, protons, neutrons.
Lepton EpochBetween 1 second to 10 seconds after the Big BangMost hadrons and anti-hadrons annihilate each other, leaving behind leptons and anti-leptons.
Photon EpochBetween 10 seconds to 370,000 years after the Big BangMost leptons and anti-leptons annihilate each other. The universe is dominated by photons.
NucleosynthesisBetween 3 minutes to 20 minutes after the Big BangThe temperature of the universe has cooled down enough to allow atomic nuclei to form via nuclear fusion.
RecombinationAbout 377,000 years after the Big BangHydrogen and helium atoms form.
ReionizationBetween 150 million and 1 billion years after the Big BangThe first stars and quasars form due to gravitational collapse.

See also

References

Citations

  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. 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

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