What causes the seasonal change in size of the Martian polar caps? During what season would the largest amount of dry ice be present at the polar cap?
Similar to Earth, we see condensation at the poles because they are typically colder than the area surrounding the Martian equator.
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The seasonal change in size of the Martian polar caps is primarily caused by the sublimation and deposition of carbon dioxide (CO2) ice, commonly known as dry ice. During Mars' winter, carbon dioxide freezes out of the atmosphere, forming a polar cap. In the spring and summer, sunlight causes the ice to sublimate directly into gas, reducing the size of the polar cap. The largest amount of dry ice would be present at the polar cap during Mars' winter season when the CO2 freezes out of the atmosphere.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

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