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The Sun shines continually at the North Pole for 6 months, from the spring equinox until the fall equinox, yet temperatures never get very warm. Explain why this is the case.

Short Answer

Expert verified
Low solar angle and high reflectivity of ice prevent significant warming at the North Pole.

Step by step solution

01

Understanding the Position of the Sun

At the North Pole, during the six months when the Sun is continually above the horizon, it never rises high in the sky. The Sun remains low, near the horizon, resulting in its light coming in at a very shallow angle.
02

Analyzing the Angle of Sunlight

Sunlight hitting the Earth at a shallow angle spreads over a larger area compared to when it hits directly overhead. This dispersion reduces the intensity of solar energy received per unit area at the North Pole.
03

Considering the Reflectivity of Ice and Snow

The ice and snow covering the Arctic have a high albedo, meaning they reflect a significant portion of the solar radiation back into space. This reflection further reduces the amount of solar energy absorbed, keeping temperatures lower.
04

Evaluating the Energy Balance

Despite continuous sunlight during these months, the combination of low solar angle, high reflectivity, and the Earth's energy balance (including outgoing long-wave radiation) results in little net energy gain, preventing significant warming.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Solar Angle
The solar angle is crucial in determining the amount of solar energy an area receives. At the North Pole, during the months when the sun is visible in the sky, it remains low and near the horizon. This means that the solar angle is quite shallow.
When sunlight arrives at a shallow angle, it spreads over a larger area compared to when it strikes directly overhead. Because of this spread, the intensity of sunlight - or the energy per unit area - is greatly reduced.
Hence, even if the sun shines for 24 hours a day, the shallow solar angle prevents the North Pole from heating up significantly. In simple terms, the light is stretched thin over the surface, resulting in less warmth.
Albedo Effect
Albedo refers to the reflectivity of a surface. Surfaces with high albedo reflect a large portion of incoming solar radiation back into space.
Ice and snow, which cover much of the Arctic region, have very high albedo values. They can reflect up to 85% of the sunlight that hits them.
This high reflectivity adds another layer of cooling at the North Pole. Instead of absorbing the sun's warmth, the snow and ice bounce it away, further reducing the potential for significant warming even with continuous daylight.
Energy Balance
Energy balance is about the equilibrium between incoming solar energy and outgoing energy from the Earth. For an area to warm up, it must retain more energy than it loses.
At the North Pole, despite perpetual sunlight for half the year, the combination of factors such as low solar angle and high albedo means less solar energy absorption. Additionally, the Earth emits long-wave radiation - energy from the Earth's surface radiating back into space.
These processes - especially the emission of long-wave radiation - play a crucial role in maintaining the energy balance. The Arctic region often experiences a near-zero or even negative energy balance, preventing the environment from accumulating a net energy gain that would lead to warming.
North Pole
The North Pole provides a unique environment with extreme seasonal variations. During its summer months, the sun never sets, creating a phenomenon known as the "midnight sun."
However, due to factors like the solar angle, the albedo effect, and the region’s overall energy balance, temperatures remain frigid. These factors all work together to prevent temperatures from rising drastically.
Understanding these concepts helps explain why even with the sun's presence for half the year, the North Pole stays cold. It's a remarkable demonstration of nature's balancing act, where even continuous daylight has limited impact due to a combination of natural laws and surface characteristics.

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Most popular questions from this chapter

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