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Erythraea

Planets of the Erythraea class are desert rocky bodies with a thin carbon dioxide atmosphere, subjected to strong erosion and sharp thermal contrasts.

Definition

A planet of the Erythraea class is a desert rocky world, with vast plains, dunes, and a thin atmosphere mainly composed of carbon dioxide. The surface is shaped by dry winds carrying particles, creating erosional formations, valleys, and plateaus.

Structure

The atmosphere, due to its low density, prevents heat retention and causes large temperature variations between day and night. The lack of protection against radiation intensifies the slow disintegration of exposed rocks. Metallic oxides in the regolith layers give the surface a reddish color.

Hydrology

Liquid water cannot exist under current conditions. Traces of channels and dry basins indicate wetter phases in the past. Today, water exists mainly as subsurface ice or trapped in stable mineral layers.

Surface dynamics

The winds, although infrequent, raise dust clouds and move sediments. They contribute to the formation of dunes, sedimentary layers, and the slow change of topography.

Constraints

The conditions include very low atmospheric pressure, dust storms, and extreme temperature variations. These factors require specific technical adaptations for exploration or infrastructure construction.


KODO: D2