The new face of Venus

Details The new face of Venus The new face of Venus

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993s%26t....86...22s&link_type=abstract

Sky & Telescope (ISSN 0037-6604), vol. 86, no. 2, p. 22-31.

Astronomy and Astrophysics

Astrophysics

Magellan Spacecraft (Nasa), Planetary Craters, Venus Surface, Volcanoes, Natural Satellites, Planetary Crusts, Planetary Structure, Venus, Surface, Features, Popular, Comparisons, Planetology, Volcanoes, Volcanism, Craters, Streaks, Lava Flows, Impact Craters, Description, Earth, Analogs, Channels, Domes, Origin, Formation, Mountains, Halos, Composition, Reflectivity, Tesserae, Topography, Gravity Effects, Heat, Relaxation, Distribution, Resurfacing, Hypotheses, Tectonism, Upwelling, Plate Tectonics, Water,

Scientific paper

The Magellan data on the Venus landscape which revealed volcanoes, shining mountains, relaxing plateaus, and craters on the surface of about 500 C, with an atmospheric pressure 90 times that of earth, are discussed. Venus is considered to be a planet that is both incredibly similar and dissimilar to earth. Venus might not exhibit plate tectonism but it might be dominated by catastrophes. The greenhouse around Venus has operated for at least the last 500 million years. The Magellan data revealed channels extending for thousands of kilometers, beautiful outflows surrounding impact craters, and odd volcanic constructs like the steep-sided domes.

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