Paleoproterozoic

Paleoproterozoic
Paleoproterozoic stromatolites
Chronology
Proposed redefinition(s)2420–1780 Ma
Gradstein et al., 2012
Proposed subdivisionsOxygenian Period, 2420–2250 Ma

Gradstein et al., 2012
Jatulian/Eukaryian Period, 2250–2060 Ma
Gradstein et al., 2012
Columbian Period, 2060–1780 Ma

Gradstein et al., 2012
Etymology
Name formalityFormal
Alternate spelling(s)Palaeoproterozoic
Usage information
Celestial bodyEarth
Regional usageGlobal (ICS)
Time scale(s) usedICS Time Scale
Definition
Chronological unitEra
Stratigraphic unitErathem
Time span formalityFormal
Lower boundary definitionDefined Chronometrically
Lower GSSA ratified1991[1]
Upper boundary definitionDefined Chronometrically
Upper GSSA ratified1991[1]

The Paleoproterozoic Era[4] (also spelled Palaeoproterozoic) is the first of the three sub-divisions (eras) of the Proterozoic eon, and also the longest era of the Earth's geological history, spanning from 2,500 to 1,600 million years ago (2.5–1.6 Ga). It is further subdivided into four geologic periods, namely the Siderian, Rhyacian, Orosirian and Statherian.

Paleontological evidence suggests that the Earth's rotational rate ~1.8 billion years ago equated to 20-hour days, implying a total of ~450 days per year.[5] It was during this era that the continents first stabilized.[clarification needed]

  1. ^ a b Plumb, K. A. (June 1, 1991). "New Precambrian time scale". Episodes. 14 (2): 139–140. doi:10.18814/epiiugs/1991/v14i2/005.
  2. ^ "palaeo-". Lexico UK English Dictionary. Oxford University Press. Archived from the original on 2020-06-18. "Proterozoic". Lexico UK English Dictionary. Oxford University Press. Archived from the original on 2020-06-17.
  3. ^ "Proterozoic". Merriam-Webster.com Dictionary.
  4. ^ There are several ways of pronouncing Paleoproterozoic, including IPA: /ˌpæliˌprtərəˈzɪk, ˌp-, -liə-, -ˌprɒt-, -ər-, -trə-, -tr-/ PAL-ee-oh-PROH-tər-ə-ZOH-ik, PAY-, -⁠PROT-, -⁠ər-oh-, -⁠trə-, -⁠troh-.[2][3]
  5. ^ Pannella, Giorgio (1972). "Paleontological evidence on the Earth's rotational history since early precambrian". Astrophysics and Space Science. 16 (2): 212. Bibcode:1972Ap&SS..16..212P. doi:10.1007/BF00642735. S2CID 122908383.

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