top of page
Inaugurated by IN-SPACe
ISRO Registered Space Tutor

S6-SA3-0342

What is the Reddening of Sun at Sunrise/Sunset?

Grade Level:

Class 10

AI/ML, Physics, Biotechnology, Space Technology, Chemistry, Engineering, Medicine

Definition
What is it?

The reddening of the Sun at sunrise and sunset is a phenomenon where the Sun appears orange or red due to the scattering of sunlight by tiny particles in Earth's atmosphere. This happens because blue light scatters much more easily than red light.

Simple Example
Quick Example

Imagine you are watching a cricket match on TV. If the signal is weak, you might see some colours clearly but others might look faded or disappear. Similarly, when sunlight travels a long distance through the atmosphere, some colours (like blue) get 'lost' or scattered away, leaving behind the stronger colours (like red and orange) for us to see.

Worked Example
Step-by-Step

Let's understand why blue light scatters more:

1. **Sunlight is White Light:** Sunlight is made up of all colours of the rainbow (VIBGYOR - Violet, Indigo, Blue, Green, Yellow, Orange, Red).
2. **Atmosphere has Tiny Particles:** Earth's atmosphere contains tiny air molecules and dust particles, much smaller than the wavelength of visible light.
3. **Rayleigh Scattering:** These tiny particles scatter light. The amount of scattering is inversely proportional to the fourth power of the wavelength (1/wavelength^4). This means shorter wavelengths (like blue and violet) scatter much more intensely than longer wavelengths (like red and orange).
4. **Sun Overhead (Midday):** When the Sun is directly overhead, its light travels a shorter path through the atmosphere. Most colours reach our eyes, making the Sun appear white or yellowish.
5. **Sunrise/Sunset:** When the Sun is near the horizon, its light has to travel a much longer path through the atmosphere.
6. **Blue Light Scatters Away:** Over this long path, most of the blue and violet light is scattered away in different directions and does not reach our eyes directly.
7. **Red Light Reaches Us:** The longer wavelength red and orange light, which scatters less, travels through the atmosphere more directly and reaches our eyes. This makes the Sun appear red or orange.

ANSWER: The longer path of sunlight through the atmosphere at sunrise/sunset causes most blue light to scatter away, leaving red and orange light to reach our eyes.

Why It Matters

Understanding light scattering is crucial in fields like Biotechnology for developing new imaging techniques, in Space Technology for studying planetary atmospheres, and in Physics for designing optical instruments. Careers in atmospheric science, optical engineering, and even cinematography use this knowledge daily.

Common Mistakes

MISTAKE: Thinking the Sun itself changes colour. | CORRECTION: The Sun always emits white light. Its apparent colour change is due to how our atmosphere interacts with its light.

MISTAKE: Believing dust particles are the only reason for scattering. | CORRECTION: While dust contributes, tiny air molecules (like nitrogen and oxygen) are the primary cause of Rayleigh scattering, which makes the sky blue and the Sun red.

MISTAKE: Confusing reflection with scattering. | CORRECTION: Reflection is when light bounces off a surface at an angle. Scattering is when light is redirected in many random directions by tiny particles.

Practice Questions
Try It Yourself

QUESTION: Why does the sky usually appear blue during the day? | ANSWER: The sky appears blue because blue light, having a shorter wavelength, is scattered more effectively by the tiny air molecules in the atmosphere in all directions.

QUESTION: If Earth had no atmosphere, what colour would the Sun appear at sunrise/sunset? | ANSWER: If Earth had no atmosphere, there would be no scattering. The Sun would appear white at all times, and the sky would be black, even during the day.

QUESTION: A planet has an atmosphere that scatters red light more than blue light. What colour would its sky likely appear during the day, and what colour would its sun appear at sunset? | ANSWER: If red light scatters more, the sky would likely appear reddish/orange during the day. At sunset, the blue light would be scattered less and reach the observer, so the sun might appear bluish or greenish.

MCQ
Quick Quiz

What is the main reason for the reddening of the Sun at sunrise and sunset?

The Sun emits more red light during these times.

The Earth's atmosphere scatters blue light more effectively than red light, especially over long distances.

Clouds reflect red light towards us at these times.

Pollution in the air absorbs all other colours except red.

The Correct Answer Is:

B

Option B is correct because blue light scatters much more than red light due to Rayleigh scattering. At sunrise/sunset, sunlight travels a longer path, causing most blue light to scatter away, leaving red light to reach our eyes. The Sun's emission doesn't change, clouds reflect all colors, and while pollution can affect color, the primary reason is atmospheric scattering of blue light.

Real World Connection
In the Real World

This concept helps meteorologists predict visibility and atmospheric conditions, especially useful for pilots flying during dawn or dusk. It's also used by photographers to capture stunning 'golden hour' photos, understanding how light behaves to create beautiful, warm-toned pictures.

Key Vocabulary
Key Terms

SCATTERING: The process where light is redirected in various directions by particles in its path | WAVELENGTH: The distance between two consecutive crests or troughs of a wave, determining its color in visible light | RAYLEIGH SCATTERING: The scattering of electromagnetic radiation by particles of a much smaller wavelength, explaining blue sky and red sunsets | ATMOSPHERE: The layer of gases surrounding Earth or another planet

What's Next
What to Learn Next

Now that you understand light scattering, you can explore other light phenomena like 'Refraction of Light' and 'Dispersion of Light'. These concepts will help you understand how lenses work and why rainbows form!

bottom of page