The Amazonis Quadrangle on Mars

The Amazonis quadrangle (MC-08) is one of the 30 distinct regions of Mars defined by the United States Geological Survey for systematic planetary mapping.

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Amazonis quadrangle

Amazonis quadrangle

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History

The geological history of the region is dominated by the Amazonian period, characterized by widespread volcanic activity that deposited thick layers of lava, effectively resurfacing the area and obscuring ancient cratering.

Examples

Key features include the Amazonis Planitia, which contains evidence of complex geological interactions between volcanic flows and potential subsurface ice.

Overview

The Amazonis quadrangle spans the coordinates 0° to 30° north latitude and 135° to 180° west longitude. It is primarily defined by its extensive, low-lying plains.

Importance

The quadrangle serves as a primary site for studying the Amazonian epoch, the most recent geological period on Mars, providing insights into the planet's late-stage volcanic and tectonic evolution.

How It Works

The surface morphology is the result of flood volcanism. Low-viscosity lava flows traveled great distances, filling topographic depressions and creating the characteristic flat plains of the Amazonis Planitia.

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Frequently Asked Questions

What is the Amazonis quadrangle?+
It is one of 30 distinct regions of Mars defined by the United States Geological Survey for systematic planetary mapping.
How many regions are there on Mars?+
There are 30 distinct regions on Mars.
Who defined the Amazonis quadrangle?+
The United States Geological Survey defined the Amazonis quadrangle.
What does MC-08 mean?+
MC-08 is the designation used by the USGS for the Amazonis quadrangle.
Why is the Amazonis quadrangle important?+
It helps scientists map and study Mars in a systematic way.
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