Why Is The Sky Lighter Closer To The Horizon?

Table of Contents (click to expand)

The sky looks lighter near the horizon because your line of sight is travelling through much more atmosphere than when you look straight up — roughly twelve times more air, plus water vapour, dust and pollutants concentrated near the ground. Repeated Rayleigh scattering washes the blue light out across all directions, while Mie scattering from larger particles adds whitish, evenly scattered light. The result is a pale, washed-out band where the sky meets the Earth.

Imagine the last time you were walking outside on a sunny day with clear skies. Looking directly above you, the sky would have likely been a bright and vibrant blue. This should come as no surprise, since we have been taught since childhood that grass is green and the sky is blue. Of course, even those with a rudimentary understanding of optics know that color is merely a construct based on the reflection and refraction of light.

Now, think back to that same sunny stroll; if you continued up a hill, and then to the top of the mountain, and looked towards the horizon, you may be surprised by the colors you see. The rich and vibrant blue present directly above your head does not remain uniform as your gaze stretches miles in the distance. In fact, near the horizon, the sky may appear nearly white. What causes this disparity of color in our stereotypically blue sky? Why is the sky so light near the horizon?


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Blue-Sky Science

When people think about the sunlight that bathes our planet in life-giving warmth, it is common to imagine it as warm yellow light, as that is the color we closely associate with the sun. However, visible light is a combination of all the colors in varying wavelengths. When rays from the sun enter Earth’s atmosphere, they begin to interact with all the molecules present there, including nitrogen, oxygen, hydrogen, carbon dioxide and others, along with particulate matter and pollutants in the air.

a picture of the sky
The characteristic blue color of the sky (Photo Credit : ESB Professional/Shutterstock)

Scattering

As sunlight strikes atmospheric particles, it makes their electrons oscillate rapidly up and down. The accelerating electrons re-emit radiation at the same frequency as the incoming light, but spread out in all directions. (The much heavier protons in the nucleus barely budge, so they make a negligible contribution.) This process of redirecting sunlight is known as scattering. When you look at the visible light portion of the electromagnetic spectrum, you’ll see that the blue side has a higher frequency and shorter wavelength than the red side.

Rayleigh Scattering

When sunlight strikes nitrogen and oxygen molecules in the atmosphere (the two most abundant components of air), short-wavelength blue light is scattered much more than long-wavelength red light. The Rayleigh formula goes as 1/λ⁴, which means blue light (~450 nm) is scattered roughly four to five times more strongly than red light (~650 nm). This type of unequal scattering of light through a medium of particles much smaller than the wavelength of the light is called Rayleigh scattering. This blue light is scattered in all directions at a high concentration, making the sky appear blue.

The less amount of atmosphere the light must pass through, the more blue it will appear, so when you look straight up on a clear day, you will see a “pure” blue color. However, the atmosphere does not evenly scatter light, so the effect of Rayleigh scattering is variable depending on what point in the sky you’re viewing. Further away from the mountaintop, for example, the sky will look like a paler blue, as the light must pass through far more of the atmosphere before reaching your eyes. This allows for a greater mixture of colors being scattered, so the “blue” is not as pure.

Mie Scattering

The example above was good for a clear sunny day, but we don’t always enjoy blue skies. Sometimes the sky appears grey or white, particularly on cloudy days. When light interacts with small air molecules like nitrogen and oxygen, Rayleigh scattering dominates, but in the case of larger particulate matter, such as pollutants, aerosols, water vapour, dust or smoke, light scatters more uniformly across wavelengths (though it tends to be peaked in the forward direction, not equal in every direction). The particles need to be roughly the same size as — or larger than — the wavelength of the incoming visible light for this effect to dominate. Because all colours scatter together, the result looks white — a combination of all the colors on the visible spectrum. This is why clouds are generally white, yet the sky is blue! This scattering of light in all directions by large particles is called Mie Scattering.

portrait of a man and his mie scattering meme

As mentioned above, as you look further away from you, the blue of the sky will begin to look somewhat paler, because the Rayleigh scattering effect is being “watered down” by the excess atmosphere you are looking through. Above your head is roughly 8 miles of atmosphere, but when looking at the horizon, the light must travel through 100 miles or more of the atmosphere before reaching your eye.

Therefore, viewing the horizon is like looking at the “bottom” of the atmosphere, where there is a higher concentration of aerosols, pollutants, smoke and dust (i.e., closer to the ground and human activity). These larger particles are heavier than air molecules like nitrogen and oxygen, which means that they will sit lower in the atmosphere. Therefore, looking out towards the horizon, the light will interact with more of these particles, causing a greater amount of Mie Scattering than if you were looking straight up!

A Final Word

Staring up into the endless blue has been a pastime since time immemorial, but don’t let anyone try to tell you that the whole sky is always blue! The color that we see in the world is merely a product of light interacting with different surfaces and substances, bouncing around the atmosphere and morphing depending on distance, intensity and any particulate obstacles in its way. And next time you’re gazing out from a mountain vista at the band of whiteness above the horizon, you can casually explain to your companions what causes this blue-sky anomaly—Mie scattering!

References (click to expand)
  1. What Determines Sky's Colors At Sunrise And Sunset?. Science Daily
  2. DW Hahn. Light Scattering Theory Introduction - plaza. The University of Florida
  3. Lilienfeld, P. (2004, June 3). A Blue Sky History. Optics and Photonics News. The Optical Society.
  4. Caruthers, J. W. (2011). On Rayleigh and Mie scattering. Proceedings of Meetings on Acoustics. Acoustical Society of America.