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Chapter 6 - Venus

Published online by Cambridge University Press:  05 February 2013

Ronald Greeley
Affiliation:
Arizona State University
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Summary

Introduction

After the Sun and the Moon, Venus is the brightest object in the sky, a consequence of sunlight being reflected from its dense clouds. The planet’s diameter, mass, and gravity are nearly the same as those of Earth (Table 1.1). Along with the presence of an atmosphere, these characteristics led some observers to refer to Venus as Earth’s sister planet. Even as late as the 1960s, some serious researchers thought that the surface of Venus was a wet, tropical environment, possibly teaming with life.

With the dawn of the Space Age, Venus was revealed to be substantially different from Earth. The surface temperature is a hellish 480 °C and exceeds the melting point of lead, while the dense carbon dioxide atmosphere is laced with droplets of sulfuric acid that form dense clouds and exerts a surface pressure of 95 bars, comparable to being underwater on the sea floor of Earth at a depth of 900 m. This leads some wags to refer to Venus as Earth’s evil sister. On the other hand, the geomorphology of Venus displays features indicative of extensive tectonic and volcanic processes (Fig. 6.1), some of which are similar to those on Earth and could be active today, and a surface age of no older than about 750 Ma, much like most of the surface of Earth.

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Publisher: Cambridge University Press
Print publication year: 2013

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  • Venus
  • Ronald Greeley, Arizona State University
  • Book: Introduction to Planetary Geomorphology
  • Online publication: 05 February 2013
  • Chapter DOI: https://doi.org/10.1017/CBO9781139020961.008
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  • Venus
  • Ronald Greeley, Arizona State University
  • Book: Introduction to Planetary Geomorphology
  • Online publication: 05 February 2013
  • Chapter DOI: https://doi.org/10.1017/CBO9781139020961.008
Available formats
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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.

  • Venus
  • Ronald Greeley, Arizona State University
  • Book: Introduction to Planetary Geomorphology
  • Online publication: 05 February 2013
  • Chapter DOI: https://doi.org/10.1017/CBO9781139020961.008
Available formats
×