Atjaunināt sīkdatņu piekrišanu

E-grāmata: Surviving 1000 Centuries: Can We Do It?

4.50/5 (15 ratings by Goodreads)
  • Formāts: PDF+DRM
  • Sērija : Springer Praxis Books
  • Izdošanas datums: 02-Apr-2010
  • Izdevniecība: Springer-Verlag New York Inc.
  • Valoda: eng
  • ISBN-13: 9780387746357
  • Formāts - PDF+DRM
  • Cena: 41,62 €*
  • * ši ir gala cena, t.i., netiek piemērotas nekādas papildus atlaides
  • Ielikt grozā
  • Pievienot vēlmju sarakstam
  • Šī e-grāmata paredzēta tikai personīgai lietošanai. E-grāmatas nav iespējams atgriezt un nauda par iegādātajām e-grāmatām netiek atmaksāta.
  • Formāts: PDF+DRM
  • Sērija : Springer Praxis Books
  • Izdošanas datums: 02-Apr-2010
  • Izdevniecība: Springer-Verlag New York Inc.
  • Valoda: eng
  • ISBN-13: 9780387746357

DRM restrictions

  • Kopēšana (kopēt/ievietot):

    nav atļauts

  • Drukāšana:

    nav atļauts

  • Lietošana:

    Digitālo tiesību pārvaldība (Digital Rights Management (DRM))
    Izdevējs ir piegādājis šo grāmatu šifrētā veidā, kas nozīmē, ka jums ir jāinstalē bezmaksas programmatūra, lai to atbloķētu un lasītu. Lai lasītu šo e-grāmatu, jums ir jāizveido Adobe ID. Vairāk informācijas šeit. E-grāmatu var lasīt un lejupielādēt līdz 6 ierīcēm (vienam lietotājam ar vienu un to pašu Adobe ID).

    Nepieciešamā programmatūra
    Lai lasītu šo e-grāmatu mobilajā ierīcē (tālrunī vai planšetdatorā), jums būs jāinstalē šī bezmaksas lietotne: PocketBook Reader (iOS / Android)

    Lai lejupielādētu un lasītu šo e-grāmatu datorā vai Mac datorā, jums ir nepieciešamid Adobe Digital Editions (šī ir bezmaksas lietotne, kas īpaši izstrādāta e-grāmatām. Tā nav tas pats, kas Adobe Reader, kas, iespējams, jau ir jūsu datorā.)

    Jūs nevarat lasīt šo e-grāmatu, izmantojot Amazon Kindle.

The circumstances that will shape the long-term future of our planet will be constrained by what is physically possible and what is not. This book provides a quantitative view of our civilization over the next 100,000 years, in comparison to the 40-60,000 years it took for modern humans to emerge from Africa, on the basis of contemporary scientific and technological knowledge. The first 5 chapters provide the general scientific background, starting with a brief history of our planet, from its formation 4.5 billion years ago until the present day. The evolution of the Earth's atmosphere and the origin of water are highlighted as being the most important factors for the emergence and the development of life, especially in comparison to Earth's neighbours, Venus and Mars. The authors then consider both cosmic and natural hazards, pointing out that scientific information provided by satellites and communication systems on the ground could prevent many unnecessary casualties by forward planning and the installation of elementary precautions.The changing climate in the past and in the future is considered, showing how atmospheric greenhouse gases CO2 and methane played an important role in past climates, whereas future human industrial and agricultural emissions of greenhouse gases largely determine the future climate. The authors highlight the importance of long term monitoring and control of the atmospheric composition. Chapter 7 looks at future energy and inorganic resources, the needs for which in the year 100,000 will be five times larger than the present ones. The most likely sources will be from fusion, solar and wind energy, and storage facilities will be needed for the latter two. Water, agriculture and forests are considered in the following chapter: although adequate food and water should be available worldwide, inadequate management may cause some densely populated areas to experience shortages. The colonization of other planets, in particular Mars and Venus, and the possibility of extracting resources from the Moon or asteroids are discussed in Chapter 9. The final chapters stress the importance of international collaboration to manage Earth's future, together with the crucial role of space for its monitoring, surveillance and management. Cooperative world governance and global laws should be undertaken by the political, scientific and space worlds and encompass both the rich and poorer countries.

This book provides a quantitative view of our civilization over the next 100,000 years, in comparison to the 40-60,000 years it took for modern humans to emerge from Africa, on the basis of contemporary scientific and technological knowledge. The opening chapters provide the general scientific background. The evolution of the Earth's atmosphere and the origin of water are highlighted. The authors then consider both cosmic and natural hazards. The changing climate in the past and in the future is considered, along with future energy and inorganic resources. The colonization of other planets, and the possibility of extracting resources from the Moon or asteroids are discussed. The final chapters stress the importance of international collaboration to manage Earth's future, together with the crucial role of space for its monitoring, surveillance and management.

Recenzijas

From the reviews:









"A good initial feeling for the thesis of the book can be obtained simply by reading the chapters. the authors turn to threats to survival from outside (from nearby supernovae to asteroid impact) and from inside (disease, seismic events, and climatic hazards), before turning to the current burning issue of climate change, both past and future. This is a fascinating and challenging book which is published at just the right moment. It should be required reading for all politicians ." (Robert Connon Smith, The Observatory, Vol. 129 (1210), June, 2009)

List of Illustrations
xi
Foreword xv
Preface xvii
Acknowledgments xix
Introduction
1(12)
Why a hundred thousand years?
1(4)
People and resources
5(2)
Management and cooperation
7(2)
The overall plan of the book
9(2)
Notes and references
11(2)
A Brief History of the Earth
13(40)
The age of the Earth
13(3)
Geological timescales
16(2)
The formation of the Moon and the Late Heavy Bombardment
18(5)
Continents and plate tectonics
23(8)
Continents
23(1)
Plate tectonics
24(4)
The Earth's magnetic field
28(3)
Evolution of the Earth's atmosphere
31(4)
Life and evolution
35(13)
The early fossils in the Archean
35(2)
The Proterozoic and the apparition of oxygen
37(1)
The Neo-Proterozoic: the Ediacarans and the `snowball earth'
38(5)
The Phanerozoic, life extinctions
43(5)
Conclusion
48(1)
Notes and references
48(5)
Cosmic Menaces
53(40)
Introduction
53(1)
Galactic hazards
54(8)
The death of the Sun
57(1)
Encounters with interstellar clouds and stars
57(2)
Supernovae explosions, UV radiation and cosmic rays
59(1)
Gamma-ray bursts and magnetars
60(2)
Solar System hazards
62(27)
Past tracks of violence
62(4)
The nature of the impactors: asteroids and comets
66(7)
Estimating the danger
73(3)
The bombardment continues
76(4)
Mitigation measures
80(1)
Deviation from the dangerous path
80(4)
Decision making
84(1)
Space debris
85(4)
Conclusion
89(1)
Notes and references
89(4)
Terrestrial Hazards
93(60)
Introduction
93(2)
Diseases
95(7)
How old shall we be in 1,000 centuries?
98(2)
How tall shall we be in 1,000 centuries?
100(2)
Seismic hazards: the threat of volcanoes
102(13)
Volcanoes and tectonic activity
102(4)
The destructive power of volcanoes
106(3)
Volcanoes and climate change
109(3)
Forecasting eruptions
112(3)
Seismic hazards: the threat of earthquakes
115(10)
Measuring the power of earthquakes
119(1)
Earthquake forecasting
120(5)
Mitigation against earthquakes
125(1)
Tsunamis
125(7)
What are they?
125(2)
The 26 December 2004 Sumatra tsunami
127(1)
Forecasting tsunamis and mitigation approaches
128(4)
Climatic hazards
132(14)
Storms: cyclones, hurricanes, typhoons, etc.
132(5)
Floods
137(5)
Droughts
142(4)
Conclusion
146(2)
Notes and references
148(5)
The Changing Climate
153(34)
Miscellaneous evidence of climate change
153(3)
The global climate system
156(4)
Climates in the distant past
160(3)
The recent ice ages
163(8)
Recent climate
171(3)
Changes in the Sun
174(2)
Volcanic eruptions
176(1)
Anthropogenic CO2
177(1)
Interpretation of the recent record
178(1)
The ozone hole
179(3)
Notes and references
182(5)
Climate Futures
187(26)
Scenarios for future climates
188(6)
Geographic distribution of warming
194(3)
Sea level
197(4)
The 100,000-year climate future
201(4)
Doubts
205(1)
Consequences of climate change
206(1)
Appendix
207(2)
The four main SRES scenarios
207(2)
Notes and references
209(4)
The Future of Survivability: Energy and Inorganic Resources
213(40)
Energy for 100,000 years
213(19)
Energy requirements for the 100,000-year world
215(2)
Minor energy sources for the long-term future
217(2)
Wind energy
219(2)
Solar energy
221(2)
Biofuels
223(2)
Nuclear energy
225(3)
Fusion energy
228(4)
Energy for the present century
232(6)
Fossil carbon fuels
232(4)
Electricity and renewables
236(1)
From now to then
236(2)
Elements and minerals
238(12)
Abundances and formation of the elements
238(3)
The composition of the Earth
241(1)
Mineral resources
242(2)
The present outlook
244(1)
Mineral resources for 100,000 years
245(5)
From now to then
250(1)
Conclusion
250(1)
Notes and references
250(3)
The Future of Survivability: Water and Organic Resources
253(28)
Water
253(10)
The water cycle
254(1)
Water use and water stress
255(2)
Remedial measures
257(3)
Water for 100,000 years
260(2)
From now to then: water and climate change
262(1)
Agriculture
263(8)
Increasing productivity
263(2)
Present and past land use
265(1)
Population
266(1)
Agricultural land and production
266(1)
Irrigation
267(1)
Fertilizers and pesticides
267(1)
Top soil
267(2)
Agriculture for 100,000 years
269(2)
From now to then
271(1)
Forests and wilderness
271(5)
Deforestation
273(3)
Conclusion
276(1)
Notes and references
276(5)
Leaving Earth: From Dreams to Reality?
281(34)
Introduction
281(1)
Where to go?
282(18)
The case of Venus
284(4)
The case of Mars
288(6)
Other worlds
294(3)
Interstellar travel
297(2)
Space cities?
299(1)
What to do with the Moon?
300(8)
The Lunar Space Station
301(2)
The Moon as a scientific base
303(1)
The Moon for non-scientific exploitation
303(3)
Resources from outside the Earth-Moon system: planets and asteroids
306(2)
Terraforming the Earth
308(3)
Absorbing or storing CO2
308(1)
Cooling down the Earth
309(2)
Conclusion
311(1)
Notes and references
311(4)
Managing the Planet's Future: The Crucial Role of Space
315(52)
Introduction
315(1)
The specific needs for space observations of the Earth
316(13)
The Earth's interior
316(3)
Water: the hydrosphere and the cryosphere
319(4)
The atmosphere
323(4)
The biosphere
327(2)
The tools and methods of space
329(33)
The best orbits for Earth observation
330(1)
Geodesy and altimetry satellites: measuring the shapes of the Earth
331(6)
Global Positioning Systems
337(2)
Synthetic Aperture Radars
339(8)
Optical imaging
347(3)
Remote-sensing spectroscopy
350(4)
Radiometry
354(3)
Monitoring astronomical and solar influences
357(5)
Conclusion
362(1)
Notes and references
363(4)
Managing the Planet's Future: Setting-Up the Structures
367(36)
Introduction
367(1)
The alert phase: need for a systematic scientific approach
368(13)
Forecasting the weather: the `easy' case
368(4)
The scientific alert phase: the example of the IPCC
372(4)
Organizing the space tools
376(5)
The indispensable political involvement
381(16)
The crucial role of the United States, China and India
381(3)
A perspective view on the political perception
384(9)
The emotional perception: the scene is moving
393(4)
Conclusion: towards world ecological governance?
397(2)
Notes and references
399(4)
Conclusion
403(12)
Limiting population growth
403(2)
Stabilizing global warming
405(1)
The limits of vessel-Earth
406(1)
The crucial role of education and science
407(1)
New governance required
408(2)
The difficult and urgent transition phase
410(1)
Adapting to a static society
411(2)
Notes and references
413(2)
Index 415
Dr R M Bonnet and Dr L Woltjer are outstanding, internationally renowned scientists. During his long tenure at the European Space Agency, Dr Bonnet has directed the launch of 17 artificial scientific satellites, initiating the development of the Huygens probe placed on the NASA Cassini Saturn Orbiter which landed on Titan on 14 January 2005, developing the successful Mars Express mission and directing the SMART-1 European lunar mission. He is President of COSPAR and Executive Director of ISSI and has acquired a world reputation in the field of space politics. After 11 years at Columbia University, NY, Dr Woltjer returned to Europe as Director General of ESO for 13 years. Since then he has worked closely with the Observatories de Haute Provence in France and the University of Florence in Italy, was President of the International Astronomical Union and Chairman of the Space Science Advisory Committee of ESA for 4 years.