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atmospheric-pressure-effects
The chapter explains how atmospheric pressure, alongside temperature, determines whether liquid water can exist on Mars' surface.
1 chapter across 1 book
Red Mars (1992)Kim Stanley Robinson
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In this chapter, the characters reflect on the fragile state of the Martian polar ice cap and the potential consequences of terraforming efforts. Ann explains the delicate balance of temperature, atmospheric pressure, and water distribution on Mars, emphasizing the possibility that the polar ice could sublime away entirely before significant melting occurs. The dialogue reveals both scientific insight and the emotional weight carried by the characters as they confront the planet's harsh realities and uncertain future.