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Chapter 10 - Atmosphere and ocean

from Part II - The motivation to continue the quest

Published online by Cambridge University Press:  05 September 2014

Fredric W. Taylor
Affiliation:
University of Oxford
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Summary

The pre-space age planetary astronomers knew that the albedo (reflectivity) of Venus is higher than that of Earth, which must partially offset the extra heating that comes from being closer to the Sun. It was widely expected that Venus would turn out to be a more tropical version of the Earth, but no one pictured a climate as extreme as the reality that was first detected by ground-based radio astronomers and confirmed by Mariner 2 and Venera 9. This was a big surprise at the time.

In fact, the modern value for the albedo, integrated over wavelength, is more than two and a half times that of Earth, at about 76 per cent rather than 30 per cent, so that Venus actually absorbs less radiative energy than Earth, despite the Sun appearing twice as large in the sky. Thus, it could be argued that Venus should be not warmer but actually cooler overall. This, however, does not take into account the huge difference in atmospheric thickness. On Venus the surface temperature enhancement through the blanketing ‘greenhouse’ effect is similar to, but more than ten times larger, than the corresponding effect on Earth.

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Publisher: Cambridge University Press
Print publication year: 2014

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References

Elementary Climate Physics (Oxford University Press, 2005), for details.
Velikovsky, Immanuel, who maintained in Worlds in Collision (1950)

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  • Atmosphere and ocean
  • Fredric W. Taylor, University of Oxford
  • Book: The Scientific Exploration of Venus
  • Online publication: 05 September 2014
  • Chapter DOI: https://doi.org/10.1017/CBO9781139151245.015
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  • Atmosphere and ocean
  • Fredric W. Taylor, University of Oxford
  • Book: The Scientific Exploration of Venus
  • Online publication: 05 September 2014
  • Chapter DOI: https://doi.org/10.1017/CBO9781139151245.015
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Atmosphere and ocean
  • Fredric W. Taylor, University of Oxford
  • Book: The Scientific Exploration of Venus
  • Online publication: 05 September 2014
  • Chapter DOI: https://doi.org/10.1017/CBO9781139151245.015
Available formats
×