Advanced Technology Paths to Global Climate Stability: Energy for a Greenhouse Planet

Author:

Hoffert Martin I.1,Caldeira Ken2,Benford Gregory3,Criswell David R.4,Green Christopher5,Herzog Howard6,Jain Atul K.7,Kheshgi Haroon S.8,Lackner Klaus S.9,Lewis John S.10,Lightfoot H. Douglas11,Manheimer Wallace12,Mankins John C.13,Mauel Michael E.14,Perkins L. John2,Schlesinger Michael E.7,Volk Tyler15,Wigley Tom M. L.16

Affiliation:

1. Department of Physics,

2. Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.

3. Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA.

4. Institute of Space Systems Operations, University of Houston, Houston, TX 77204, USA.

5. Department of Economics, McGill University, Montreal, Quebec H3A 2T7, Canada.

6. MIT Laboratory for Energy and the Environment, Cambridge, MA 02139, USA.

7. Department of Atmospheric Sciences, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA.

8. ExxonMobil Research and Engineering Company, Annandale, NJ 08801, USA.

9. Department of Earth and Environmental Engineering,

10. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.

11. Centre for Climate and Global Change Research, McGill University, Montreal, Quebec H3A 2K6, Canada.

12. Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375, USA.

13. NASA Headquarters, Washington, DC 20546, USA.

14. Department of Applied Physics and Applied Mathematics, Columbia University, New York, NY 10027, USA.

15. Department of Biology, New York University, New York, NY 10003, USA.

16. National Center for Atmospheric Research, Boulder, CO 80307, USA.

Abstract

Stabilizing the carbon dioxide–induced component of climate change is an energy problem. Establishment of a course toward such stabilization will require the development within the coming decades of primary energy sources that do not emit carbon dioxide to the atmosphere, in addition to efforts to reduce end-use energy demand. Mid-century primary power requirements that are free of carbon dioxide emissions could be several times what we now derive from fossil fuels (∼10 13 watts), even with improvements in energy efficiency. Here we survey possible future energy sources, evaluated for their capability to supply massive amounts of carbon emission–free energy and for their potential for large-scale commercialization. Possible candidates for primary energy sources include terrestrial solar and wind energy, solar power satellites, biomass, nuclear fission, nuclear fusion, fission-fusion hybrids, and fossil fuels from which carbon has been sequestered. Non–primary power technologies that could contribute to climate stabilization include efficiency improvements, hydrogen production, storage and transport, superconducting global electric grids, and geoengineering. All of these approaches currently have severe deficiencies that limit their ability to stabilize global climate. We conclude that a broad range of intensive research and development is urgently needed to produce technological options that can allow both climate stabilization and economic development.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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