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What is the Sun's Corona?

Visual representation of the sun with its corona visible as a glowing halo
The sun's corona extends millions of kilometers into space

The corona is the sun's outer atmosphere! It's the glowing halo of super-hot gas that surrounds our star. Even though the sun's surface is about 10,000°F (5,500°C), the corona is much hotter—over 1 million degrees! This is one of the biggest mysteries in solar science.

Definition: The corona is the outermost part of the sun's atmosphere, made of plasma (superheated gas) that extends millions of kilometers into space. It's visible during a total solar eclipse as a beautiful, pearly-white crown around the darkened sun.

Amazing Corona Features

Diagram showing different features of the sun's corona
Features of the sun's corona

The corona isn't just a smooth halo—it has fascinating structures that scientists study:

1

Coronal Holes

Dark, cooler areas where solar wind escapes into space

2

Streamers

Long, wispy structures that follow magnetic fields

3

Loops & Arches

Bright curves formed by magnetic fields trapping hot gas

4

Solar Wind

Constant stream of charged particles flowing from corona

5

Temperature Mystery

Why is the corona hotter than the sun's surface?

Scientists use special telescopes called coronagraphs to study the corona. These instruments create an artificial eclipse by blocking the bright face of the sun, allowing us to see the fainter corona any time!

Solar Eclipses & The Corona

Illustration of a total solar eclipse showing the moon covering the sun with the corona visible around it
Total solar eclipse showing the sun's corona

The best time to see the corona is during a total solar eclipse when the moon completely covers the sun's bright face. This creates temporary darkness on Earth and reveals the beautiful corona!

During a total solar eclipse:
• The moon perfectly aligns between Earth and sun
• The sun's bright surface is completely blocked
• The fainter corona becomes visible
• This lasts only a few minutes at any location

Coronal Mass Ejections (CMEs)

Illustration showing a massive coronal mass ejection
A coronal mass ejection erupting from the sun

Sometimes the sun releases enormous bubbles of plasma and magnetic fields called Coronal Mass Ejections (CMEs). These solar storms travel through space at millions of miles per hour!

When a CME reaches Earth:
• It can create beautiful auroras (northern lights)
• It might disrupt satellites and power grids
• Astronauts in space need special protection
• Scientists monitor CMEs to predict space weather

Solar Quiz

Test your solar knowledge with this quiz about the sun's corona! Answer all 5 questions to see how much you've learned.

1. What is the sun's corona?
2. When can we see the corona without special instruments?
3. What is a Coronal Mass Ejection (CME)?
4. How hot is the sun's corona?
5. What causes the beautiful northern lights (auroras)?

Frequently Asked Questions

Here are answers to some common questions about the sun's corona:

Solar Trivia

Discover some amazing facts about the sun's corona:

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