The phenomenon of the Sun appearing red during sunrise and sunset is a fascinating interplay of atmospheric physics and human perception. This effect is commonly referred to as the “red Sun” or “Sunset/Sunrise effect” and results from the scattering of sunlight by the Earth’s atmosphere. Understanding why the Sun appears red during these times involves delving into the science of light scattering, atmospheric conditions, and the way our eyes perceive color.
The Science of Light Scattering
Light scattering is a fundamental concept that explains why the Sun looks red at certain times of the day. The Sun emits light across the visible spectrum, which includes all colors from violet to red. This light, however, doesn’t reach our eyes directly from the Sun; instead, it passes through the Earth’s atmosphere, which can significantly alter its appearance.

The scattering of light occurs due to interactions between light waves and particles or molecules in the atmosphere. There are two primary types of scattering that are relevant to this phenomenon:
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Rayleigh Scattering: This type of scattering occurs when light interacts with particles that are much smaller than the wavelength of the light, such as molecules of air. Rayleigh scattering is more effective at shorter wavelengths, which are the blues and violets of the spectrum. Therefore, when sunlight passes through the atmosphere, shorter wavelengths are scattered in all directions, making the sky appear blue during the day.
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Mie Scattering: This occurs when the particles causing the scattering are closer in size to the wavelength of light, such as dust or water droplets. Mie scattering is less wavelength-dependent and affects all colors more equally compared to Rayleigh scattering.
Why the Sun Appears Red During Sunrise and Sunset
During sunrise and sunset, the Sun’s light has to travel through a much thicker layer of the Earth’s atmosphere compared to when it is overhead. This extended path length means that the light encounters more air molecules, dust, and other particulates, leading to increased scattering of shorter wavelengths. Here’s a step-by-step explanation of why this results in the Sun appearing red:
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Increased Path Length: As the Sun is low on the horizon, its light must pass through a greater thickness of the Earth’s atmosphere. This longer journey increases the amount of scattering that occurs.
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Scattering of Shorter Wavelengths: The increased scattering affects the shorter wavelengths (blue and violet light) more than the longer wavelengths (red and orange light). The blue and violet light is scattered out of the direct path of sight, leaving the longer wavelengths to dominate.
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Remaining Red Light: The light that reaches our eyes from the Sun at sunrise and sunset is thus predominantly composed of the longer wavelengths. This is why the Sun can appear a deep red or orange color during these times.
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Atmospheric Conditions: Various atmospheric conditions can also influence the color of the Sun. For example, the presence of dust, pollution, or water droplets can enhance the scattering effect, leading to even more vivid reds and oranges.
Perception and Human Vision
The way our eyes perceive color also plays a role in how we see the red Sun. Human vision is adapted to perceive a range of colors based on the intensity and distribution of light reaching the retina. During sunrise and sunset, the Sun’s light is less intense and more scattered, which can make the red hues more noticeable and striking against the usually cooler and dimmer background.
Conclusion
The red appearance of the Sun during sunrise and sunset is a beautiful example of atmospheric science and light behavior. It is primarily caused by the scattering of sunlight by the Earth’s atmosphere, with longer wavelengths dominating the view due to the scattering of shorter wavelengths. This effect is influenced by the increased path length of sunlight through the atmosphere and various atmospheric conditions. Understanding this phenomenon not only highlights the complexities of light and atmosphere but also enhances our appreciation of the natural world’s beauty.