Reconciling atmospheric temperatures in the early Archean: AGU2012 P11G-05

Research output: Contribution to conferenceConference abstract for conferenceResearch

Standard

Reconciling atmospheric temperatures in the early Archean : AGU2012 P11G-05. / Pope, Emily Catherine; Bird, Dennis K.; Rosing, Minik Thorleif; Albarede, Francis.

2012. Abstract from American Geophysical Union Fall Meeting, San Francisco, United States.

Research output: Contribution to conferenceConference abstract for conferenceResearch

Harvard

Pope, EC, Bird, DK, Rosing, MT & Albarede, F 2012, 'Reconciling atmospheric temperatures in the early Archean: AGU2012 P11G-05', American Geophysical Union Fall Meeting, San Francisco, United States, 03/12/2012 - 07/12/2012. <http://abstractsearch.agu.org/meetings/2012/FM/sections/P/sessions/P11G/abstracts/P11G-05.html>

APA

Pope, E. C., Bird, D. K., Rosing, M. T., & Albarede, F. (2012). Reconciling atmospheric temperatures in the early Archean: AGU2012 P11G-05. Abstract from American Geophysical Union Fall Meeting, San Francisco, United States. http://abstractsearch.agu.org/meetings/2012/FM/sections/P/sessions/P11G/abstracts/P11G-05.html

Vancouver

Pope EC, Bird DK, Rosing MT, Albarede F. Reconciling atmospheric temperatures in the early Archean: AGU2012 P11G-05. 2012. Abstract from American Geophysical Union Fall Meeting, San Francisco, United States.

Author

Pope, Emily Catherine ; Bird, Dennis K. ; Rosing, Minik Thorleif ; Albarede, Francis. / Reconciling atmospheric temperatures in the early Archean : AGU2012 P11G-05. Abstract from American Geophysical Union Fall Meeting, San Francisco, United States.1 p.

Bibtex

@conference{ad961355b4f344c7a51fef654024d89d,
title = "Reconciling atmospheric temperatures in the early Archean: AGU2012 P11G-05",
abstract = "Average surface temperatures of Earth in the Archean remain unresolved despite decades of diverse approaches to the problem. As in the present, early Earth climates were complex systems dependent on many variables. With few constraints on such variables, climate models must be relatively simplistic, and consider only one or two factors that drive Archean climate (e.g. a fainter young sun, a low albedo, the extent and effect of cloud cover, or the presence and abundance of a wide array of greenhouse and icehouse gasses). Compounded on the limitations of modeling is the sparse and often ambiguous Archean rock record. The goal of this study is to compile and reconcile Archean geologic and geochemical features that are in some way controlled by surface temperature and/or atmospheric composition, so that at the very least paleoclimate models can be checked by physical limits. Data used to this end include the oxygen isotope record of chemical sediments and ancient ocean crust, chemical equilibria amongst primary phases in banded iron formations (BIFs), sedimentary features indicative of temperate or glacial environments, and paleosol indicators of atmospheric CO2. Further, we explore the extent to which hydrogen isotopes contribute to the geologic record as a signal for glaciations, continental growth and atmospheric methane levels. Oceanic serpentinites and subduction-related volcanic and hydrothermal environments obtain their hydrogen isotope signature from seawater, and thus may be used to calculate secular variation in δDSEAWATER which may fluctuate significantly due to hydrogen escape, continental growth and large-scale glaciation events. Further, ancient records of low-δD meteoric fluids signal both cooler temperatures and the emergence of large continents (increasing the effects of continental weathering on climate). Selective alteration of δD in Isua rocks to values of -130 to -100‰ post-dates ca. 3.55Ga Ameralik dikes, but may be associated with a poorly defined 2.6-2.8Ga metamorphic event that is coincident with the amalgamation of the “Kenorland supercontinent.”",
keywords = "Faculty of Science, Evolution of the atmosphere, Geochemical cycles, Stable isotope geochemistry, Archean",
author = "Pope, {Emily Catherine} and Bird, {Dennis K.} and Rosing, {Minik Thorleif} and Francis Albarede",
year = "2012",
language = "English",
note = "American Geophysical Union Fall Meeting, AGU2012 ; Conference date: 03-12-2012 Through 07-12-2012",

}

RIS

TY - ABST

T1 - Reconciling atmospheric temperatures in the early Archean

T2 - American Geophysical Union Fall Meeting

AU - Pope, Emily Catherine

AU - Bird, Dennis K.

AU - Rosing, Minik Thorleif

AU - Albarede, Francis

PY - 2012

Y1 - 2012

N2 - Average surface temperatures of Earth in the Archean remain unresolved despite decades of diverse approaches to the problem. As in the present, early Earth climates were complex systems dependent on many variables. With few constraints on such variables, climate models must be relatively simplistic, and consider only one or two factors that drive Archean climate (e.g. a fainter young sun, a low albedo, the extent and effect of cloud cover, or the presence and abundance of a wide array of greenhouse and icehouse gasses). Compounded on the limitations of modeling is the sparse and often ambiguous Archean rock record. The goal of this study is to compile and reconcile Archean geologic and geochemical features that are in some way controlled by surface temperature and/or atmospheric composition, so that at the very least paleoclimate models can be checked by physical limits. Data used to this end include the oxygen isotope record of chemical sediments and ancient ocean crust, chemical equilibria amongst primary phases in banded iron formations (BIFs), sedimentary features indicative of temperate or glacial environments, and paleosol indicators of atmospheric CO2. Further, we explore the extent to which hydrogen isotopes contribute to the geologic record as a signal for glaciations, continental growth and atmospheric methane levels. Oceanic serpentinites and subduction-related volcanic and hydrothermal environments obtain their hydrogen isotope signature from seawater, and thus may be used to calculate secular variation in δDSEAWATER which may fluctuate significantly due to hydrogen escape, continental growth and large-scale glaciation events. Further, ancient records of low-δD meteoric fluids signal both cooler temperatures and the emergence of large continents (increasing the effects of continental weathering on climate). Selective alteration of δD in Isua rocks to values of -130 to -100‰ post-dates ca. 3.55Ga Ameralik dikes, but may be associated with a poorly defined 2.6-2.8Ga metamorphic event that is coincident with the amalgamation of the “Kenorland supercontinent.”

AB - Average surface temperatures of Earth in the Archean remain unresolved despite decades of diverse approaches to the problem. As in the present, early Earth climates were complex systems dependent on many variables. With few constraints on such variables, climate models must be relatively simplistic, and consider only one or two factors that drive Archean climate (e.g. a fainter young sun, a low albedo, the extent and effect of cloud cover, or the presence and abundance of a wide array of greenhouse and icehouse gasses). Compounded on the limitations of modeling is the sparse and often ambiguous Archean rock record. The goal of this study is to compile and reconcile Archean geologic and geochemical features that are in some way controlled by surface temperature and/or atmospheric composition, so that at the very least paleoclimate models can be checked by physical limits. Data used to this end include the oxygen isotope record of chemical sediments and ancient ocean crust, chemical equilibria amongst primary phases in banded iron formations (BIFs), sedimentary features indicative of temperate or glacial environments, and paleosol indicators of atmospheric CO2. Further, we explore the extent to which hydrogen isotopes contribute to the geologic record as a signal for glaciations, continental growth and atmospheric methane levels. Oceanic serpentinites and subduction-related volcanic and hydrothermal environments obtain their hydrogen isotope signature from seawater, and thus may be used to calculate secular variation in δDSEAWATER which may fluctuate significantly due to hydrogen escape, continental growth and large-scale glaciation events. Further, ancient records of low-δD meteoric fluids signal both cooler temperatures and the emergence of large continents (increasing the effects of continental weathering on climate). Selective alteration of δD in Isua rocks to values of -130 to -100‰ post-dates ca. 3.55Ga Ameralik dikes, but may be associated with a poorly defined 2.6-2.8Ga metamorphic event that is coincident with the amalgamation of the “Kenorland supercontinent.”

KW - Faculty of Science

KW - Evolution of the atmosphere

KW - Geochemical cycles

KW - Stable isotope geochemistry

KW - Archean

M3 - Conference abstract for conference

Y2 - 3 December 2012 through 7 December 2012

ER -

ID: 101697553