Abstract
The Archean atmosphere was likely a weakly reduced mixture composed predominantly of N2 and CO2, with smaller concentrations of H2, CO, and CH4. Both CO2 and N2 may have been present in abundances exceeding today's values, by a factor of 2 or more for N2 and by factors of 100 or more for CO2. Published upper limits on CO2 from paleosols and banded iron formations are probably invalid; hence, CO2 could have been the dominant greenhouse gas that compensated for the fainter young Sun. The Archean greenhouse effect was likely supplemented by CH4, which could have risen to levels of 1000ppmv or more once methanogens had evolved. Warming by CH4 was limited to approximately 10-12°, however, by formation of organic haze. The key to analyzing Archean atmospheric composition is to understand the hydrogen budget of the atmosphere in which outgassing of H2 and other reduced gases from volcanoes was balanced by loss of hydrogen to space and burial of organic carbon in sediments. The mixing ratio of O2 in such a weakly reduced atmosphere would have been extremely low, roughly 10-13 at the surface, increasing to ~10-3 in the upper stratosphere. A rise in O2 just after the end of the Archean may have eliminated the methane greenhouse and triggered the Paleoproterozoic glaciations.
| Original language | English (US) |
|---|---|
| Title of host publication | Treatise on Geochemistry |
| Subtitle of host publication | Second Edition |
| Publisher | Elsevier Inc. |
| Pages | 157-175 |
| Number of pages | 19 |
| Volume | 6 |
| ISBN (Print) | 9780080983004 |
| DOIs | |
| State | Published - Nov 1 2013 |
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All Science Journal Classification (ASJC) codes
- Environmental Science(all)
- Earth and Planetary Sciences(all)
- Chemistry(all)
Cite this
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Modeling the Archean Atmosphere and Climate. / Kasting, James.
Treatise on Geochemistry: Second Edition. Vol. 6 Elsevier Inc., 2013. p. 157-175.Research output: Chapter in Book/Report/Conference proceeding › Chapter
TY - CHAP
T1 - Modeling the Archean Atmosphere and Climate
AU - Kasting, James
PY - 2013/11/1
Y1 - 2013/11/1
N2 - The Archean atmosphere was likely a weakly reduced mixture composed predominantly of N2 and CO2, with smaller concentrations of H2, CO, and CH4. Both CO2 and N2 may have been present in abundances exceeding today's values, by a factor of 2 or more for N2 and by factors of 100 or more for CO2. Published upper limits on CO2 from paleosols and banded iron formations are probably invalid; hence, CO2 could have been the dominant greenhouse gas that compensated for the fainter young Sun. The Archean greenhouse effect was likely supplemented by CH4, which could have risen to levels of 1000ppmv or more once methanogens had evolved. Warming by CH4 was limited to approximately 10-12°, however, by formation of organic haze. The key to analyzing Archean atmospheric composition is to understand the hydrogen budget of the atmosphere in which outgassing of H2 and other reduced gases from volcanoes was balanced by loss of hydrogen to space and burial of organic carbon in sediments. The mixing ratio of O2 in such a weakly reduced atmosphere would have been extremely low, roughly 10-13 at the surface, increasing to ~10-3 in the upper stratosphere. A rise in O2 just after the end of the Archean may have eliminated the methane greenhouse and triggered the Paleoproterozoic glaciations.
AB - The Archean atmosphere was likely a weakly reduced mixture composed predominantly of N2 and CO2, with smaller concentrations of H2, CO, and CH4. Both CO2 and N2 may have been present in abundances exceeding today's values, by a factor of 2 or more for N2 and by factors of 100 or more for CO2. Published upper limits on CO2 from paleosols and banded iron formations are probably invalid; hence, CO2 could have been the dominant greenhouse gas that compensated for the fainter young Sun. The Archean greenhouse effect was likely supplemented by CH4, which could have risen to levels of 1000ppmv or more once methanogens had evolved. Warming by CH4 was limited to approximately 10-12°, however, by formation of organic haze. The key to analyzing Archean atmospheric composition is to understand the hydrogen budget of the atmosphere in which outgassing of H2 and other reduced gases from volcanoes was balanced by loss of hydrogen to space and burial of organic carbon in sediments. The mixing ratio of O2 in such a weakly reduced atmosphere would have been extremely low, roughly 10-13 at the surface, increasing to ~10-3 in the upper stratosphere. A rise in O2 just after the end of the Archean may have eliminated the methane greenhouse and triggered the Paleoproterozoic glaciations.
UR - http://www.scopus.com/inward/record.url?scp=84903797059&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84903797059&partnerID=8YFLogxK
U2 - 10.1016/B978-0-08-095975-7.01306-1
DO - 10.1016/B978-0-08-095975-7.01306-1
M3 - Chapter
AN - SCOPUS:84903797059
SN - 9780080983004
VL - 6
SP - 157
EP - 175
BT - Treatise on Geochemistry
PB - Elsevier Inc.
ER -