Basic differences in Earth physics[change | change source]
Because the Earth was only half as old as now, there were some basic differences from today. Heat in the Earth's interior was greater than today. This was mainly due to the higher abundance of radioactive isotopes, which decay as time passes.
Temperatures at the surface were also higher, due to radiation from the Earth's interior, and due to a methane and carbon dioxide-based greenhouse atmosphere. During the previous eon, the Archaean, the oceans were hot (55–85 °C). This was only partly balanced by the fact that the Sun's radiation was lower at that time.
Paleontological evidence on the Earth's rotational history suggests that ~1.8 billion years ago, there were about 450 days in a year, implying 20 hour days. Further back, the Earth day had about 17 hours, and there were 514±33 days per year. The Earth–Moon distance for the earliest Palaeoproterozoic was 51.9±3.3 Earth radii (compared to 60.27 at present).
Supercontinent[change | change source]
Climate[change | change source]
Drop in methane[change | change source]
There are clear indications that the era saw a drop in atmospheric methane:
- "The collapse of methane from formerly high levels in the Archaean atmosphere probably plays a large role, not only the oxygenation history, but also the occurrence of Palaeoproterozoic ice ages. The data point to 2.4–2.3 billion years ago as host to a ‘Great Oxidation Event’, during which Earth's surface environment changed profoundly and irreversibly".
The buildup of oxygen[change | change source]
Oxygen was produced by the cyanobacteria, but it was mostly used up by chemical sinks. These were the unoxidized sulfur and iron. Until roughly 2.3 billion years ago, oxygen was probably only 1% to 2% of its current level.p323
Banded iron formations, which provide most of the world's iron ore, were formed by the oxygen forming compounds with iron; most accumulation ceased after 1.9 billion years ago. Red beds, which are colored by hematite, indicate an increase in atmospheric oxygen after 2 billion years ago; they are not found in older rocks.p324
Ice ages[change | change source]
There were three major ice ages, with ice deep into the tropics. Undoubtedly, they happened as a result of reduced greenhouse gases in the atmosphere, and the rise of oxygen production.
There is what researchers call "a puzzling interval of ~1,400 million years with no verified glaciation between early Palaeoproterozoic glaciations at 2400–2200 mya in North America, South Africa, Scandinavia and Australia and the Neoproterozoic glaciations that affected all continents at 800–600 mya".
Meteorite strikes[change | change source]
There were major bolide impacts during the era, two of which caused the largest impact crators on Earth. There are also three smaller (equal or more than 30 kilometers diameter) in the time zone of 3.0 to 1.2 billion years ago.
Origin of eukaryotes[change | change source]
The origin of the eukaryotic cell was a milestone in the evolution of life, since they include all complex cells and almost all multi-cellular organisms. The timing of this series of events is hard to determine; Knoll suggests they developed approximately 1.6–2.1 billion years ago. Some acritarchs are known from at least 1650 million years ago, and the possible alga Grypania has been found as far back as 2100 million years ago.
References[change | change source]
- Reddy S.M. and Evans D.A.D. 2009. Palaeoproterozoic supercontinents and global evolution: correlations from core to atmosphere. Geological Society. 203, 1–26. 
- Giorgio Pannella 1972. Paleontological evidence on the Earth's rotational history since early precambrian Archived 2020-07-06 at the Wayback Machine Astrophysics and Space Science 16.2 p212
- Williams G.E. 2000. Geological constraints on the Precambrian history of Earth's rotation and the moon's orbit. Reviews of Geophysics 38:37–59.
- Rogers J.J.W. and Santosh M. 2002. Configuration of Columbia, a Mesoproterozoic supercontinent. Gondwana Research. 5, 5-22
- Zhao, Gochun; et al. (2002). "Review of global 2.1–1.8 Ga orogens: implications for a pre-Rodinia supercontinent". Earth-Science Reviews. 59 (1–4): 125–162. Bibcode:2002ESRv...59..125Z. doi:10.1016/S0012-8252(02)00073-9. Retrieved 2007-01-07.
- Cloud P.E. 1968. Atmospheric and hydrospheric evolution on the primitive Earth. Science 160:729–736.
- Holland H.D. 2006. The oxygenation of the atmosphere and oceans. Philosophical Transactions of the Royal Society B: Biological Sciences 361:903–915.
- Stanley, Steven M. 1999. Earth system history. New York: W.H. Freeman. ISBN 0-7167-2882-6.
- Evans D.A., Beukes N.J., Kirschvink J.L. 1997. Low-latitude glaciation in the Palaeoproterozoic era. Nature 386:262–266.
- Williams G.E. 2005. Subglacial meltwater channels and glaciofluvial deposits in the Kimberley Basin, Western Australia: 1.8 Ga low-latitude glaciation coeval with continental assembly. Journal of the Geological Society 162:111–124. 
- Grieve R. and Therriault A. 2000. Vredefort, Sudbury, Chicxulub: three of a kind? Annual Review of Earth and Planetary Sciences 28:305–338.
- Knoll, Andrew H. 2004. Life on a young planet: the first three billion years of evolution on Earth. Princeton University Press. ISBN 0-691-12029-3
- Knoll, A.H; Javaux, E.J; Hewitt, D.; Cohen, P. (2006). "Eukaryotic organisms in Proterozoic oceans". Philosophical Transactions of the Royal Society of London, Part B. 361 (1470): 1023–38. doi:10.1098/rstb.2006.1843. PMC 1578724. PMID 16754612.