The Sun: Our Special Star — Passage and Quiz

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Grades
4
5
Standards
RI.4.4
RI.4.2
PRINT+DIGITAL RESOURCE
This learning resource is available in interactive and printable formats. The interactive worksshet can be played online and assigned to students. The Printable PDF version can be downloaded and printed for completion by hand.
ABOUT THIS READER
The Sun is the closest star to Earth and the center of our solar system.
Publisher: Workybooks
|
Written by:Neha Goel Tripathi
|
Illustrated by:
CONTENT PREVIEW

The Sun: Our Special Star

At the center of our solar system is a very special star - the Sun. It's the closest star to Earth and the most important object in our solar system. The Sun is so big that it makes up more than 99% of all the mass in our solar system. That means it's much, much bigger than all the planets, moons, asteroids, and comets combined!

 

The Sun is a ball of hot gas, mostly hydrogen and helium. It's so hot that these gases are in a special state called plasma. The center of the Sun is incredibly hot - about 27 million degrees Fahrenheit! This extreme heat causes nuclear reactions that create the Sun's energy. This energy travels outward from the Sun's core and eventually reaches us as light and heat.

 

The Sun's energy is what makes life on Earth possible. It warms our planet, drives our weather, and helps plants grow through a process called photosynthesis. Without the Sun, our planet would be a frozen, dark world where life as we know it couldn't exist.

 

The Sun doesn't just sit still in space. It rotates, or spins, just like Earth does. It takes about 25-35 days for the Sun to complete one rotation. The Sun also has some interesting features on its surface. Sunspots are dark areas that appear on the Sun's surface. They're cooler than the areas around them, but they're still incredibly hot!

 

Sometimes, the Sun releases huge bursts of energy and particles into space. These are called solar flares and coronal mass ejections. When these reach Earth, they can cause beautiful light shows in the sky called auroras. They can also interfere with satellites and power grids on Earth.

 

The Sun has been shining for about 4.6 billion years, and scientists estimate it will continue to shine for another 5 billion years. After that, it will run out of fuel and change into a different type of star. But don't worry - that's a very, very long time from now!

 

Studying the Sun helps us understand other stars in the universe. It also helps us protect our technology from solar storms and learn more about how stars affect the planets around them. The Sun may be just one star among billions in our galaxy, but to us, it's the most important star of all!

Quiz

1. What is the main idea of this passage?

A
The Sun is a planet
B
The Sun is the center of our solar system and crucial for life on Earth
C
The Sun is made of solid rock
D
The Sun will explode soon

2. Which of the following is a supporting detail about the Sun's composition?

A
It's made mostly of hydrogen and helium
B
It's made of water and ice
C
It's composed of rock and metal
D
It's filled with air like Earth's atmosphere

3. What is the temperature at the center of the Sun?

A
100 degrees Fahrenheit
B
1,000 degrees Fahrenheit
C
1 million degrees Fahrenheit
D
27 million degrees Fahrenheit

4. How does the Sun's energy reach Earth?

A
Through sound waves
B
Through gravity
C
As light and heat
D
As radio waves

5. What are sunspots?

A
Bright spots on the Sun's surface
B
Dark areas that appear on the Sun's surface
C
Holes in the Sun
D
Small planets orbiting the Sun

6. According to the passage, how long will the Sun continue to shine?

A
For about 100 years
B
For about 1,000 years
C
For about 1 million years
D
For about 5 billion years

Common core standards covered

RI.4.2
Determine the main idea of a text and explain how it is supported by key details; summarize the text.
RI.4.4
Determine the meaning of general academic and domain-specific words or phrases in a text relevant to a grade 4 topic or subject area.

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