EXTREMOPHILES as Astrobiological Models

EXTREMOPHILES as Astrobiological Models
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The data in this book are new or updated, and will serve also as Origin of Life and evolutionary studies. Endospores of bacteria have a long history of use as model organisms in astrobiology, including survival in extreme environments and interplanetary transfer of life. Numerous other bacteria as well as archaea, lichens, fungi, algae and tiny animals (tardigrades, or water bears) are now being investigated for their tolerance to extreme conditions in simulated or real space environments. Experimental results from exposure studies on the International Space Station and space probes for up to 1.5 years are presented and discussed. Suggestions for extaterrestrial energy sources are also indicated.

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Группа авторов. EXTREMOPHILES as Astrobiological Models

Table of Contents

List of Illustrations

Tables

Guide

Pages

Extremophiles as Astrobiological Models

Preface. Foreword

Who and what is in this new book?

Conclusions

Acknowledgments

References

1. Volcanic Steam Vents: Life at Low pH and High Temperature

1.1 Introduction

1.2 Steam Cave and Vent Sites

1.3 Steam Cave and Vent Sample Collection

1.3.1 Steam Collection

1.3.2 Steam Deposit Collection

1.3.3 Steam and Steam Deposit Collection: Control Methods. Steam Controls

Steam Deposit Controls

1.4 Culture Isolation

1.5 Cell Structure of Isolates

1.6 Environmental Models

1.7 Conclusions

Acknowledgments

References

2. Rio Tinto: An Extreme Acidic Environmental Model of Astrobiological Interest

2.1 Introduction

2.2 Acidic Chemolithotrophy

2.3 Rio Tinto Basin

2.4 Biodiversity in the Tinto Basin

2.5 Tinto Basin Sedimentary Geomicrobiology

2.6 The Iberian Pyrite Belt Dark Biosphere

2.7 Methanogenesis in Non-Methanogenic Conditions

2.8 Rio Tinto: A Geochemical and Mineralogical Terrestrial Analog of Mars

2.9 Conclusions

References

3. Blossoms of Rot: Microbial Life in Saline Organic-Rich Sediments

3.1 Introduction

3.2 Overview of Saline Aquatic Systems

3.3 Prerequisites of Organic Carbon-Rich Sediment Genesis in Saline Lakes

3.4 Chemistry of Recent Organic Carbon-Rich Sediments in Saline Water Bodies

3.5 Microbial Life in Saline Sapropels

3.5.1 Higher-Order Microbial Taxonomy Detected in Modern Saline Sapropels

3.5.2 Anaerobic Organic Matter Degradation in Saline Organic Carbon-Rich Sediments

3.5.2.1 Hydrolysis of Biomacromolecules

3.5.2.2 Primary and Secondary Fermentation of Low Molecular Weight Molecules

3.5.2.3 Methanogenesis

3.5.2.4 Biological Sulfur Reduction and Oxidation

3.5.2.5 Nitrogen Cycling

3.5.3 Uncultured Microbial Diversity of Saline Sapropels and Its Putative Ecological Roles

3.5.3.1 Uncultured Bacteria

3.5.3.2 Uncultured Archaea

3.6 Relevance of Saline Sapropels

3.7 Concluding Remarks

Acknowledgments

References

4. The Haloarchaea of Great Salt Lake as Models for Potential Extant Life on Mars

4.1 The Great Salt Lake System in the Bonneville Basin. 4.1.1 A Significant Terminal Lake in North America

4.1.2 Great Salt Lake as an Extreme Environment

The North Arm is a Zone of Salt-Saturation

Ultraviolet Light Flux at Great Salt Lake

4.1.3 The Declining Elevation of Great Salt Lake

Ancient Lake Bonneville Becomes Great Salt Lake

The Modern Terminal Lake Shrinks and Swells

4.1.4 Pertinent Mineralogy of Great Salt Lake and the Bonneville Basin

4.2 The Transformation of an Ancient Wet Mars to a Modern Hostile Environment

4.2.1 Global Climatic Change on Mars

4.2.2 The Ancient Lacustrine Environments of Mars

4.2.3 Brine on the Martian Surface

4.2.4 Mars is a Hostile Environment for Life

Low and Unstable Temperature

Ultraviolet Radiation Flux

4.3 Life in Evaporitic Minerals on Earth

4.3.1 Formation of Halite and Gypsum Primary Crystals in Aquatic Environments

4.3.2 Haloarchaea May Be Entombed in Halite

4.3.3 Haloarchaea May Be Entombed in Gypsum

4.3.4 Haloarchaea Can Survive over Geologic Time in Fluid Inclusions

4.4 Great Salt Lake Haloarchaea

4.5 Haloarchaea Have Superpowers for Extreme Lifestyles

4.5.1 Haloarchaea May Show Versatility with Respect to Temperature and pH

4.5.2 Haloarchaea are Metabolically Versatile

4.5.3 Haloarchaea Are Adapted to High Salinity and Desiccating Conditions

4.5.4 Haloarchaea Are Resistant to Ultraviolet Radiation

4.5.5 Haloarchaea Are Resistant to Ionizing Radiation

4.5.6 Haloarchaea May Have Novel Nutrient Attainment Strategies for Dormancy Periods

4.5.7 Haloarchaea Are Resistant to Space Conditions

4.6 Extant or Extinct Haloarchaea on Mars?

4.6.1 Haloarchaea as Extant Life

4.6.2 Haloarchaea as Extinct Life

Nucleic Acids as Biosignatures

Proteins as Biosignatures

Carbohydrates as Biosignatures

Lipids as Biosignatures

Contamination and Biosignatures

4.7 Conclusions and Insights

Acknowledgments

References

5. Arsenic-and Light Hydrocarbon-Rich Hypersaline Soda Lakes and Their Resident Microbes as Possible Models for Extraterrestrial Biomes

5.1 Introduction

First, however, a personal digression

5.2 Mars

5.3 Enceladus

5.4 Titan

References

6. Antarctic Bacteria as Astrobiological Models

Abbreviations

6.1 Introduction

6.2 Antarctica as an Analogous Environment for Astrobiology

6.2.1 Temperature

6.2.2 Soil as a Life-Supporting Medium

6.2.3 Soil Salinity

6.3 Astrobiological Environments of Interest

6.4 Bacterial Adaptations to Extreme Environments as Analogues for Astrobiology

6.4.1 Psychrophiles

6.5 Antarctic Bacteria as Analogues for Astrobiology

6.6 Endemic Antarctic Bacteria used in Astrobiology

6.7 Cosmopolitan Bacteria Found in Antarctica and used in Astrobiology

6.8 Conclusion

References

7. Extremophilic Life in Our Oceans as Models for Astrobiology

7.1 Introduction

7.2 Southern Ocean Ecosystem: West Antarctic Peninsula Region

7.3 Sea Ice Decline in WAP and Ice Shelf Collapse in Amundsen Sea

7.4 Deoxygenation Leading toward Hypoxic Zone in Amundsen Sea

7.5 Microbial Extremophiles in Southern Ocean

7.6 Chemosynthetic Abyssal Ecosystems. 7.6.1 Methane Cold Seep Deep-Sea Communities in the Abyss

7.6.2 Are Hydrothermal Vents Abyssal Gold Mines?

7.7 Hydrothermal Activity in Hrad Vallis on Mars

7.8 Why Chemosynthetic Ecosystems Remind Us of Environmental Conditions When Life Originated in the Universe

7.9 Ultra-Abyssal Ecosystem: Puerto Rico Trench

7.10 Affiliations of Abyssal Life to Astrobiology: Some Perspectives

7.11 Can We Find Protozoans Such as Xenophyophores on Other Planets?

7.12 Barophilic Organisms in the Deep-Sea

Acknowledgments

References

8. Challenging the Survival Thresholds of a Desert Cyanobacterium under Laboratory Simulated and Space Conditions

8.1 Introduction

8.2 Endurance of Chroococcidiopsis Under Air-Drying and Space Vacuum

8.3 Endurance of Chroococcidiopsis Under Laboratory Simulated and Space Radiation

8.4 The Use of Chroococcidiopsis’s Survival Thresholds for Future Astrobiological Experiments

Acknowledgments

References

9. Lichens as Astrobiological Models: Experiments to Fathom the Limits of Life in Extraterrestrial Environments

9.1 Introduction

9.2 Survival of Lichens in Outer Space

9.3 Space Environment: Relevance in Space Science

9.3.1 Space Radiation

9.3.2 Temperature

9.3.3 Microgravity

9.4 Biological Effects of Space. 9.4.1 Extraterrestrial Solar UV Radiation

9.4.2 Cosmic Radiation

9.4.3 Space Vacuum

9.4.4 Microgravity

9.5 Current and Past Astrobiological Facilities for Experiments with Lichens

9.6 Space Experiments with Lichens. 9.6.1 The BIOPAN Experiments: Exposure to Outer Space Conditions. Lichens Experiment

LITHOPANSPERMIA and LITHOPANSPERMIA/STONE Experiments

9.6.2 EXPOSE Facility On Board the ISS: Experiments at Space- and Mars-Like Conditions

LIFE Experiment

BIOMEX Experiment

9.7 Simulation Studies

9.8 Summary and Conclusions

9.9 Future Possibilities and Recommendations

References

10. Resistance of the Archaeon Halococcus morrhuae and the Biofilm-Forming Bacterium Halomonas muralis to Exposure to Low Earth Orbit for 534 Days

Introduction

10.2 Material and Methods. 10.2.1 Cultivation

10.2.2 UV-C Radiation and Desiccation Resistance

10.2.3 Sample Preparation for Exposure

10.2.4 Pre-Flight Ground Tests

10.2.5 Flight Preparation and Mission Ground Reference (MGR) Preparation

10.2.6 Mission EXPOSE-R2 – Flight Parameters and Conditions

10.2.7 Survival

10.2.8 Stability of Genomic DNA

10.2.9 Integrity of 16S rRNA Gene

Results

10.3.1 Survival EVT/SVT

10.3.2 Survival and Genetic Integrity Following Space Flight

10.4 Discussion

Acknowledgments

References

11. The Amazing Journey of Cryomyces antarcticus from Antarctica to Space

11.1 Introduction

11.2 The McMurdo Dry Valleys

11.3 Cryptoendolithic Communities

11.4 The Black Microcolonial Yeast-like Fungus Cryomyces antarcticus

11.5 The Polyextremotolerance of Cryomyces antarcticus

11.6 Cryomyces antarcticus and its Resistance to Radiation in Ground-Based Simulated Studies

11.7 C. antarcticus and its Resistance to Actual Space Exposure in Low Earth Orbit

11.7.1. LIFE Experiment on EXPOSE-E on Board the International Space Station

11.7.2. BIOMEX Experiment on EXPOSE-R2 on Board the International Space Station

11.8 Conclusion

11.9 Future Perspectives

Acknowledgments

References

12. Tardigrades – Evolutionary Explorers in Extreme Environments

12.1 Introduction

12.2 The Evolutionary Transition Towards Cryptobiotic Adaptations in Tardigrades

12.3 Cryptobiosis as an Evolutionary Adaptive Strategy

12.4 Defining Life in Cryptobiotic Animals

12.5 A Resilience Approach to the Cryptobiotic State

12.6 Molecular Mechanisms for Structural Stability in the Dry State

12.7 Tardigrades as Astrobiological Models

12.8 Tardigrades – Extremotolerants or Extremophiles?

Acknowledgments

References

13. Spore-Forming Bacteria as Model Organisms for Studies in Astrobiology

13.1 Introduction

13.2 Historical Beginnings

13.2.1 Evolution and the Origin of Life

13.2.2 Panspermia

13.2.3 Microbiology

13.2.4 Bacterial Spores

13.3 Revival of Lithopanspermia

13.4 Testing Lithopanspermia Experimentally

13.4.1 Impact-Mediated Launch

13.4.2 Transit Through Interplanetary Space

13.4.3 Atmospheric Entry and Deposition

13.5 Lithopanspermia, Spores, and the Origin of Life

13.6 Interstellar Lithopanspermia

13.7 Humans as Agents of Panspermia

13.8 Survival and Growth of Spores in the Mars Environment

Acknowledgments

References

14. Potential Energy Production and Utilization Pathways of the Martian Subsurface: Clues from Extremophilic Microorganisms on Earth

14.1. Introduction

14.2. Energy Sources

14.2.1 Hydrogen

Extremophiles Using Hydrogen

14.2.2 Methane

Extremophiles Using Methane

14.2.3 Iron

Extremophiles Using Iron

14.2.4 Sulfur and Associated Compounds

Extremophiles Using Sulfur

14.2.5 Other Potential Energy Sources. Nitrogen

Manganese

Perchlorate

Organics

Special Mention: Oxygen

14.3. Conclusion

References

15. Origin of Initial Communities of Thermophilic Extremophiles on Earth by Efficient Response to Oscillations in the Environment

15.1 Introduction

15.2 Required Conditions for the Origin of Life: Necessity of Rapid-Frequency Oscillations of Parameters

15.3 Parameters of the Environment for the Origin of Life

15.4 Formation of Prebiotic Microsystem Clusters and Their Conversion into Primary Communities of Thermophilic Extremophiles

15.5 Theoretical and Experimental Verification of the Proposed Approach

15.6 Conclusion

References

16. Extremophiles and Horizontal Gene Transfer: Clues to the Emergence of Life

16.1 Introduction

16.2 T-LUCAs, LUCAs and Progenotes

16.3 Prebiotic World and T-LUCA

16.4 Emergence of LUCA

16.5 Chemical Composition of LUCA

16.6 Emergence of Cellular Life Forms

16.7 Evidence for the Earliest Cellular Life Forms

16.8 The Hypotheses: Genetic First vs. Metabolism First

16.9 Extremophiles

16.10 The Viral Connection to the Origin of Life

16.11 Horizontal Gene Transfer (HGT)

16.12 Mechanisms of HGT

16.13 Clues to the Origins of Life and a Phylogenetic Tree

16.14 Conclusion

Acknowledgment

References

17. What Do the DPANN Archaea and the CPR Bacteria Tell Us about the Last Universal Common Ancestors?

17.1 Introduction

17.2 The Discovery of DPANN and CPR

17.3 Common Features of CPR and DPANN

17.4 LUCA and the Deep-Rootedness of CPR and DPANN

17.5 Short Branches, Deep Branches and Multiple LUCAs

17.6 Viruses: LUCA without ‘Cellular’

References

18. Can Biogeochemistry Give Reliable Biomarkers in the Solar System?

Abbreviations

18.1 Evidence of Life in the Solar System

18.2 Extremophiles on Earth

18.3 Extremophiles in Low Orbits Around the Earth

18.4 Have There Been Extremophiles on the Moon?

18.5 Have There Been Extremophiles on Mars?

18.6 Europa is a Likely Location for an Extremophilic Ecosystem

18.7 Are There Other Environments for Extremophiles in the Solar System? 18.7.1 Titan

18.7.2 Enceladus

18.7.3 Triton, Icy Moons, Pluto and Charon

18.8 Are There Environments for Extremophiles on Exoplanets?

References

Index

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2.21. Chapelle, F.H., O´Nelly, K., Bradley, P.M., Methé, B.A., Ciufo, S.A., Knobel, L.L., Lovley, D.R., A hydrogen-based subsurface microbial community dominated by methanogens. Nature, 415, 312–314, 2002.

2.22. Colín-García, M., Kanawati, B., Harir, M., Schmidt-Kopplin, P., Amils, R., Parro, V., García, M., Fernández-Remolar, D., Detection of peptidic sequences in the ancient acidic sediments of Río Tinto, Spain. Orig. Life Evol. Biosph., 41, 523–527, 2011.

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