1 Cosmology and the Earth
2 Journey to the Center of the Earth
3 Drifting Continents and Spreading Seas
4 The Way the Earth Works: Plate Tectonics
5 Patterns in Nature: Minerals
6 Up from the Inferno: Magma and Igneous Rocks
7 A Surface Veneer: Sediments, Soils, and Sedimentary Rocks
8 Metamorphism: A Process of Change
9 The Wrath of Vulcan: Volcanic Eruptions
10 A Violent Pulse: Earthquakes
11 Crags, Cracks, and Crumples: Crustal Deformations and Mountain Building
12 Deep Time: How Old Is Old?
13 A Biography of Earth
14 Squeezing Power from a Stone: Energy Resources
15 Riches in Rock: Mineral Resources
16 Unsafe Ground: Landslides and Other Mass Movements
17 Streams and Floods: The Geology of Running Water
18 Restless Realm: Oceans and Coasts
19 A Hidden Reserve: Groundwater
20 An Envelope of Gas: Earth’s Atmosphere and Climate
21 Dry Regions: The Geology of Deserts
22 Amazing Ice: Glaciers and Ice Ages
23 Global Change in the Earth System
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Chapter 17: Streams and Floods: The Geology of Running Water

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The Rest of the Story: Floods on Mars?

by Stephen Marshak

In the late nineteenth century, the Italian astronomer Giovanni Schiaparelli published sketches of linear features on Mars, which he called canali, meaning "channels." In the English press, these features came to be known as canals and were taken as evidence of a Martian civilization. Subsequently, astronomers determined that the canali were simply artifacts of color variations on Mar's surface, caused by seasonal winds. While no canals or civilizations exist on Mars, close-up images of the planet taken by spacecraft in the last few decades have revealed well-defined braided stream channels. Astronomers have little doubt that liquid water flowed on the surface of Mars at time in the past. They speculate that the water formed when heat from the planet's interior, caused by volcanic activity, melted the ice in near-surface permafrost. The water then flooded across the vegetation-free surface and quickly carved out river channels. And this all must have happened a long time ago, for meteor craters pockmark the channels. Nevertheless, the channels retain their fluvial character because of the lack of erosion on the planet.

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