Earth's Flips of State
The co-evolution of life and planet

(2026) , Oxford University Press,
x + 380 pages, 42 figures,
hardback, £82 / US$127, ISBN 978-0-197-82536-5
paperback (medium octavo), £31.99 / US$49,
ISBN 978-0-197-82537-2.
DOI:10.1093/9780197825402.001.0001

30% discount offer below.

Earth's Flips of State: The Co-evolution of Life and Planet
Earth's Flips of State
The co-evolution of life and
planet

-- Cover descriptor --

Our present is shaped by the past. Beyond living history, exactly how is something we rarely consider in any depth, let alone on the grandest of scales over the billions of years of Earth’s existence. This book looks at how life and our planet have together co-evolved to the present. This book also takes a glimpse as to a possible future.

The Earth has not always been in its present state: it has existed in other states and ‘rapidly’ (in the broadest geological sense) flipped from one state to another. Each new state has seen a different form of life dominate, and so a co-evolution of life and planet narrative has developed. Indeed, all our planet's flips of state have certain characteristics. All these characteristics can be seen today, which raises the question as to whether we are about to see the Earth system transition (flip) to a new state as evolutionarily significant as the rise of multicellular life: one in which the planet’s state is determined by a single species and its technological complex. Whether or not this dominance is sustainable is a key issue.

Another question arises: if the afore co-evolution of life and planet narrative took place on our planet, could it take place elsewhere? There are implications for life elsewhere in Solar system and the Galaxy. It might even explain the Fermi Paradox!

 

Contents very briefly described

The first section (chapters 1 and 2) sets the scene with the length of Earth's history and the planet's origins and early biosphere. It also introduces the concepts of stability and transition – especially critical transitions – between one state and another.

The second section (chapters 3, 4 and 5) looks at two critical transitions in Earth's history with each marked by millions of years of the planet being in a Snowball Earth state. How these came about through the development of simple bacteria-like life (prokaryotes) into more complex (eukaryotic) life and the rise of oxygen-generating photosynthesis as well as multicellular life. It shows how biological evolution shapes the planet and how planetary evolution (such as with plate tectonics) impacts biological evolution: there is a co-evolution of life and planet. Snowball Earth II, and its associated events, is looked at in detail.

The third section (chapters 6 and 7) notes that not all critical transition in Earth's history are driven by key biological evolutionary developments, but by other, more random, acts. It then returns to the co-evolution of life and planet narrative and looks at the defining characteristics of the key, biological-evolution-driven transitions before considering what this narrative implies as to the probability of life on other worlds.

The final section (chapters 8 and 9) considers our current time and whether we might be in the midst of another critical transition driven by biological evolution: the rise of a technology wielding species. It details the evolution of Homo sapiens and how this was driven by climate change critical transitions. It also introduces another characteristic of all the biological evolutionary driven critical transitions, that of each successive transition seeing the Earth have a greater amount of 'information'. Finally, it looks at the implications of our current transition both for us, the planet, and the possibility of advanced life elsewhere.

 

 

Contents

Introduction &Acknowledgements

1     The young Earth
      A sense of scale
      The formation of the Earth–Moon–Sun system
      Evolution of the Earth–Moon system
      The Earth and early biosphere
      References

2     Towards A Flip
      Carbon and the early biosphere
      Energising early life
      Biosphere stability
      Flips – Thresholds – Critical transitions (and Chaos)
      References

3     Towards a Snowball
      Prokaryote (the first cell type) evolution and early photosynthesis
      The evolution of oxygenic photosynthesis
      Oxygen in the atmosphere
      Summary of the evolution of bacterial photosynthesis
      The first big flip
      Snowball Earth I (~2.4 - 2.2 bya)
      References

4     A billion years towards the second flip
      The un-‘boring’ billion
      Turbocharging life
      The evolution of the eukaryotes 2.5 – 1.5 bya(?)
      When did the first and the more complex eukaryotes evolve?
      Going multicellular
      Multicellular life and the world
      References

5     The second flip and other Snowballs
      When did multicellularity arise?
      The move to land
      The second flip and another Snowball
      After Snowball II
      Alternative Snowballs
      Alternative Snowballs vs. the new narrative
      Merging the old and new narratives
      References

6     Jokers and Wild Cards
      Large igneous provinces (LIPs)
      The end-Permian event (251 mya)
      The Cretaceous-Tertiary extinction (66 mya)
      The initial Eocene CIE (~56 mya)
      The characteristics of life-driven flips of Earth state
      References

7     Exobiological implications
      Implications for possible life elsewhere in the Solar System
      The possibility of life on Venus
      The possibility of life on Mars
      The possibilities for life elsewhere in the Solar System
      Life beyond the Solar system
      References

8     A new flip?
      The present-day carbon isotope excursion and climate change
      Other human impacts on the carbon cycle
      New mineral species
      Information processing and the rise of humans
      Biological information and information technology
      The prospect of a new flip
      References

9     Implications
      A current critical transition
      The need to manage the future
      Problems in avoiding or managing the transition
      Fermi re-visited. Who will inherit?
      Possible solutions
      Looking at information-processing in the future
      Testability
      In conclusion
      References

Appendix I: Abbreviations & Symbols
Appendix 2: Nomenclature, Data and Terms
Appendix 3: Bio- Geological Timescale
Subject Index

 

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