Summary of Recent Research about the Early Earth

This page includes the following materials that have been drawn from research about the early earth:

Excerpts from the 2007 workshop on teaching about the early earth

At the workshop on Teaching about the Early Earth in April 2007, four invited researchers shared highlights and recent advances from their work. The talks illuminated new research in the areas of the solid earth, the atmosphere/climate system and the emergence and evolution of early life.

Title slide from Lindy Elkins-Tanton's presentation,  "The first 50 Ma: Planetary formation and the role of water"
The first 50 Ma: Planetary formation and the role of water (PowerPoint 4.7MB Apr25 07) by Lindy Elkins-Tanton, Massachusetts Institute of Technology 
This presentation describes how modeling of the crystallization of an early molten Earth can be used to test magma ocean models and the implications for the differentiation of early Earth, mars, and Moon.
Mantle overturn visualization - surface cooled from the top ( 1.5MB May16 07)
Mantle overturn visualization - surface insulated at the top ( 2.2MB May16 07)

References

  • Elkins-Tanton L.T., Continental magmatism, volatile recycling, and a heterogeneous mantle caused by lithospheric gravitational instabilities, accepted at Journal of Geophysical Research: Solid Earth, 2006.
  • Elkins-Tanton L.T., E.M. Parmentier, P.C. Hess, The formation of ancient crust on Mars through magma ocean processes, Journal of Geophysical Research 110, E12S01, doi:10.1029/2005JE002480, 2005

Title slide from James Kasting's presentation: Gaia Revisited - The Interplay Between Climate and Life on the Early Earth
Gaia Revisited: The Interplay Between Climate and Life on the Early Earth (PowerPoint 1MB Apr20 07) by James Kasting, The Pennsylvania State University
Dr. Kasting described the use of Sulfur isotopes to constrain processes at work in creating the early atmosphere, the nature of that atmosphere, and the resulting implications for the temperature and climate on the early Earth. For example, how did the early Earth remain warm enough to sustain liquid water and early life?


References

  • Kasting, J. F. and S. Ono, Paleoclimates: the first two billion years, Phil. Trans. Royal Soc. Lond. B.. 361, 917-929.
  • Kasting, J. F. and M. T. Howard, Atmospheric composition and climate on the early Earth, Phil. Trans. Royal Soc. Lond. B 361, 1733-1742 (2006).

Title slide from Lynn Margulis' presentation titled "Evolution in the pre-Phanerozoic Earth"
Evolution on the pre-Phanerozoic Earth (PowerPoint 2.1MB Jun7 07)
by Keynote speaker Lynn Margulis, University of Massachusetts, Amherst 
In this talk, Dr. Margulis showed how modern life forms can be used to infer evolutionary processes active in the past, particularly the importance of symbiosis-the inheritance of acquired genomes, and the implications of the mutual evolution of life and Earth.


Reference

  • Lynn Margulis, Dorion Sagan, 2002 Acquiring Genomes: A theory of the origins of species. New York: Basic Books

Title slide from Stan Awramik's presentation, "The Record of Life on the Early Earth"
The Record of Life on the Early Earth (PowerPoint 2.1MB Jun7 07),
by Stanley Awramik, University of California, Santa Barbara
This talk focused on the use of the early fossil record to constrain the evolution of the earliest life and also, the evaluation of uncertain evidence in scientific thinking.



Plate tectonics volume cover

Research volumes about the early earth

When did Plate Tectonics Begin on Planet Earth?

Edited by Kent C. Condie and Victoria Pease

Inspired by a GSA Penrose Conference held in Lander, Wyoming, June 14–18, 2006, this 2008 GSA volume discusses the beginning and evolution of plate tectonics on Earth, and gives readers an introduction to some of the uncertainties and controversies related to the evolution of the planet.


origin and evolution of Earth

Origin and Evolution of Earth: Research Questions for a Changing Planet

The National Research Council assembled a committee to propose and explore grand questions in geological and planetary science. This book captures, in a series of questions, the essential scientific challenges that constitute the frontier of Earth science at the start of the 21st century.

More information from the National Academies Press, including free pdf summaries and free online reading of this volume.


Elements special issue about the Early Earth, August 2006

cover of the Elements special issue on the Early Earth

The earliest Earth was a strange inhospitable world, yet transitions to a more familiar planet occurred within the first billion years. In spite of sparse preservation of an ambiguous rock record, recent studies refine the nature and timing of key events. This issue reviews current knowledge of the age of the Earth, massive early meteorite impacts, the early atmosphere and hydrosphere, the rock record, and the first life.

Contents and authors:

  • Introduction by John W. Valley, Guest Editor
  • The Origin of the Earth—What's New?by Alex N. Halliday
  • Impact Processes on the Early Earth by Christian Koeberl
  • Earth's Earliest Atmosphere by Kevin J. Zahnle
  • Antiquity of the Oceans and Continents by Allen P. Nutman
  • The First Billion Years: When Did Life Emerge? by J. William Schopf

A pdf file of this entire issue is available from the Elements web site

Archean Geodynamics and Environments

Image of the cover of the AGU special volume, "Archean Geodynamics and Environments"

Edited by Keith Benn, Jean-Claude Mareschal and Kent Condie

This AGU volume presents significant aspects of Archean geodynamics with 17 benchmark papers. Using data from the preserved Archean geological record and cutting-edge geodynamic and geophysical modeling, the book features discussion on:

  • Global geodynamics and plate tectonics: the Archean thermal regime and the nature of mantle convection
  • Thermomechanical evolution of continents
  • Subduction, accretion, and orogeny
  • Early environments and the evolution of life

Front matter
Ordering information from the American Geophysical Union bookstore

Cover image of the GSA special paper, "Processes on Early Earth"

Processes on the Early Earth - GSA Special Paper 405

Edited by Wolf Uwe Reimold and Roger L. Gibson
This Special Paper presents a collection of 19 papers contributed to a joint Field Forum organized by the Geological Society of America and the Geological Society of South Africa in July 2004 in the Barberton Greenstone Belt and the Vredefort Dome, South Africa. The papers cover a wide variety of themes, including Archean and Proterozoic crust formation and geodynamics (with an appraisal of evidence of Archean subduction processes); the significance of impacts in the evolution of the early Earth's crust; traces of early life in Archean environments of Australia and South Africa and related studies of depositional environments; and processes affecting the giant Witwatersrand gold deposit.

More information from the GSA bookstore

Cover of the GSA memoir: Evolution of Early Earth's Atmosphere, Hydrosphere, and Biosphere - Constraints from Ore Deposits

Evolution of Early Earth's Atmosphere, Hydrosphere, and Biosphere - Constraints from Ore Deposits

Edited by Stephen E. Kesler and Hiroshi Ohmoto
This GSA memoir contains 17 papers about the Earth's early atmosphere, hydrosphere, and biosphere, from Hadean through Proterozoic time. Topics include the early evolution of life, formation of the continents, oxygenation of the atmosphere, interpretation of the banded iron formations, and more.

More information from the GSA bookstore


Other Resources of Interest

A Cool Early Earth by John W. Valley, William H. Peck, Elizabeth M. King, and Simon A. Wilde 
This landmark paper describes the analysis of the oldest-known earth materials, 4.4 billion year old zircon grains. Studies of these zircons suggest that some continental crust formed as early as 4.4 Ga, 160 m.y. after accretion of the Earth, and that surface temperatures were low enough for liquid water.

Heterogeneous Hadean Hafnium: Evidence of Continental Crust at 4.4 to 4.5 Ga by T. M. Harrison, J. Blichert-Toft, W. Müller, F. Albarede, P. Holden, and S. J. Mojzsis
This Science paper tests the hypothesis of progressive continental growth beginning at 4 billion years ago. The authors measured initial 176Hf/177Hf values of 4.01- to 4.37-Ga detrital zircons from Jack Hills, Western Australia. Their results support the view that continental crust had formed by 4.4 to 4.5 Ga and was rapidly recycled into the mantle.

Comment on "Heterogeneous Hadean Hafnium: Evidence of Continental Crust at 4.4 to 4.5 Ga" by John W. Valley, Aaron J. Cavosie, Bin Fu, William H. Peck, and Simon A. Wilde
The authors of this response question the interpretations of Harrison et al (above) and draw less extreme conclusions. In their response, the authors interpret results for >4 Ga zircons to suggest the presence of granitic (sensu lato) crust by 4.4 Ga and oceans by 4.2 Ga. The composition of this crust is uncertain, although the preservation of these zircons requires at least some early buoyant crust.

Response to Comment on "Heterogeneous Hadean Hafnium: Evidence of Continental Crust at 4.4 to 4.5 Ga" by T. M. Harrison, J. Blichert-Toft, W. Müller, F. Albarede, P. Holden, and S. J. Mojzsis 
This response corrects some misrepresentations of their original work and continues to build the case for the presence of continental crust or plate boundary processes prior to 4 billion years ago.

Vestiges of a Beginning: Clues to the Emergent Biosphere Recorded in the Oldest Known Sedimentary Rocks by Stephen J. Mojzsis and T. Mark Harrison
This research paper describes findings from the oldest known rocks of marine sedimentary origin from the southwestern coast of Greenland. Evidence suggests that these rocks preserve a biogeochemical record of early life. On the basis of the age of these rocks, the emergence of the biosphere appears to overlap with a period of intense global bombardment. This finding could also be consistent with evidence from molecular biology that places the ancestry of primitive bacteria living in extreme thermal environments near the last common ancestor of all known life.

Emergence of an aerobic biosphere during the Archean-Proterozoic transition: Challenges of future research by Victor A. Melezhik, Anthony E. Fallick, Eero J. Hanski, Lee R. Kump, Aivo Lepland, Anthony R. Prave, and Harald Strauss
The earth system experienced a series of fundamental upheavals throughout the Archean-Paleoproterozoic transition (ca. 2500-2000 Ma). Most important were the establishment of an oxygen-rich atmosphere and the emergence of an aerobic biosphere. This paper describes evidence of the hallmark events of that transition.

Evidence for a gradual rise of oxygen between 2.6 and 2.5 Ga from Mo isotopes and Re-PGE signatures in shales by M. Wille, J.D. Kramers, T.F. Nägler, N.J. Beukes, S. Schröder, Th. Meisel, J.P. Lacassie, and A.R. Voegelin
This article reports geochemical findings concerning the question of how and when free oxygen started to accumulate in the Earth's atmosphere and hydrosphere. The authors report that the general increase in Mo concentrations and isotope fractionation indicates a gradual rise of oxygen between 2.64 and 2.5 Ga.

Earth-Like Planet Discovered in Libra This story from National Public Radio describes a discovery of a new planet in the constellation Libra. The small, rocky planet is special because it appears to have mild temperatures, like Earth. Researchers believe it looks like the first planet outside of our solar system that could be home to liquid water, and maybe even life.

Middle Archean volcano-hydrothermal sequence: Bacterial microfossil-bearing 3.2 Ga Dixon Island Formation, coastal Pilbara terrane, Australia by Shoichi Kiyokawa, Takashi Ito, Minoru Ikehara, and Fumio Kitajima
The 3.2 Ga Dixon Island Formation in the Cleaverville Group of the coastal Pilbara terrane, Australia, is one of the most complete and best-preserved examples of middle Archean oceanic stratigraphy and contains possible microbial material. Field observations and geochemical evidence suggest that this formation contains a low-temperature hydrothermal vent system with a biogenic microbial colony from the Archean ocean.

Hydrothermal Systems: Doorways to Early Biosphere Evolution by Jack Farmer
Hydrothermal systems provide important environments for the synthesis of simple precursor carbon compounds that may have been important in the origin of living systems. Such environments probably also played a primary role in the early evolution of the biosphere.


For references, resources and images useful for teaching early earth topics, proceed to references for teaching the early earth.

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