Loose Leaf For Explorations:  Introduction To Astronomy
Loose Leaf For Explorations: Introduction To Astronomy
9th Edition
ISBN: 9781260432145
Author: Thomas T Arny, Stephen E Schneider Professor
Publisher: McGraw-Hill Education
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Chapter 9, Problem 10QFR
To determine

The characteristics that are seen on surface of Venus, whether the surface of Venus is young or not, and whether the youngest surfaces on Venus are from plate ridges or not.

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What evidence indicates that plate tectonics does not occur on Venus? On Mars?
If we moved Venus out to 1 AU from the Sun (same as Earth), Venus would probably   a. become more like Earth, with oceans and a temperate climate   b. remain hot, dry, and dead because it's permanently lost its oceans   c. become more like Mars, losing most of its atmosphere and freezing   d. become much less geologically active due to decreased solar heating
Assume that Venus has an isothermal atmosphere with a surface temperature of 750 K. The surface pressure of Venus is 90 times the Earth's surface pressure which is about 1013mb. Also assume that the carbon dioxide dominant atmosphere of Venus is photodissociated and oxygen atoms are produced. These oxygen atoms stop the solar wind at the ionopause distance where the atmospheric pressure of Venus and the dynamic pressure of the solar wind are in balance. Accordingly, calculate the lonopause distance of the planet Venus if the solar wind density is 7 #/cm² and solar wind speed is 410 km/sec.
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