The Sun: Our Source of Light and Heat - First Grade Science

Every morning, a brilliant golden light fills our world, waking up sleeping animals, warming the chilly morning air, and inviting plants to open their leaves. That light comes from the sun, the giant glowing star located at the absolute center of our solar system. The sun is by far the most important celestial body for life on Earth. Without the sun's tremendous output of radiant light and thermal heat, planet Earth would be a frozen, pitch-black sphere of solid ice drifting lifelessly through deep space.

What is the Sun?

Although the sun looks like a warm golden disc in our daytime sky, it is not a solid planet made of rock or soil like Earth. The sun is a colossal ball of super-hot, glowing gases.

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|                           FACTS ABOUT OUR SUN                         |
|                                                                       |
|   CLASSIFICATION    A yellow dwarf star (medium-sized star).          |
|   COMPOSITION       74% Hydrogen gas and 24% Helium gas.              |
|   SURFACE TEMP      About 5,500 degrees Celsius (9,932 Fahrenheit)!   |
|   CORE TEMP         Over 15 million degrees Celsius!                  |
|   DISTANCE TO EARTH Roughly 93 million miles (150 million km) away.   |
|   SIZE COMPARISON   Over 1 MILLION Earths could fit inside the Sun!   |
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The Nearest Star

The sun is actually an ordinary star, just like the millions of tiny stars that twinkle in the night sky. The only reason the sun looks so big, bright, and warm compared to nighttime stars is that it is much closer to us! The next closest star to Earth is trillions of miles farther away, making it look like a tiny pinpoint of light.

Nuclear Fusion: The Sun's Engine

Deep inside the sun's core, intense gravity and crushing pressure cause hydrogen gas atoms to fuse together into helium gas. This powerful reaction, called nuclear fusion, releases incomprehensible amounts of energy that travel through space in the form of electromagnetic waves, including visible light, infrared heat, and ultraviolet rays.

The Sun's Gifts to Planet Earth

Life on Earth exists because our planet orbits at the perfect distance from the sun—an area astronomers call the habitable "Goldilocks Zone" where it is not too hot and not too cold for liquid water to exist.

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|                    HOW THE SUN SUPPORTS LIFE ON EARTH                 |
|                                                                       |
|   LIGHT FOR PLANTS    Powers photosynthesis; plants make food and     |
|                       produce clean oxygen for all living things.     |
|   HEAT AND WARMTH     Keeps Earth's oceans liquid; warms the air and  |
|                       soil so life can thrive.                        |
|   THE WATER CYCLE     Heats lake and ocean water to create clouds,    |
|                       rain, and fresh water for drinking.             |
|   DRIVES WEATHER      Uneven solar heating creates winds and seasons. |
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Sun Safety: Protecting Yourself

The sun is magnificent and powerful, but its radiant energy requires caution and respect.

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|                          SUN SAFETY RULES                             |
|                                                                       |
|   NEVER LOOK AT SUN   Looking directly at the sun can permanently     |
|                       damage your retina and cause blindness!        |
|   WEAR SUNSCREEN      Protects your skin from ultraviolet (UV) rays   |
|                       that cause painful sunburns.                    |
|   WEAR A HAT & SHADES Wide brim hats shade your face and neck; UV-    |
|                       blocking sunglasses protect your eyes.          |
|   STAY HYDRATED       Drink plenty of fresh water on hot sunny days.  |
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Shadows: Playing with Sunlight

Because light travels in perfectly straight lines, when an object blocks the sun's rays, a dark area called a shadow forms on the ground directly behind the object.

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|                      HOW SHADOWS CHANGE WITH THE SUN                  |
|                                                                       |
|   MORNING (Sun Low in East)    ---> LONG shadow pointing West.        |
|   NOON (Sun High Overhead)     ---> VERY SHORT shadow right under feet|
|   LATE AFTERNOON (Sun Low West)---> LONG shadow pointing East.        |
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By observing how your shadow changes length and direction throughout the day, you can track the position of the sun just like an ancient sundial!

Chapter Review Exercises

Question 1: What is the sun, and why does it look so much larger and brighter than other stars in the sky?

Question 2: List three vital ways that the sun supports living organisms on planet Earth.

Question 3: Describe how the length of your shadow changes from early morning to midday noon.

Question 4: What is the number one safety rule regarding looking at the sun with your eyes?

Solutions and Explanations

Solution 1: The sun is a medium-sized star made of glowing, super-hot hydrogen and helium gases. It looks much larger and brighter than other stars because it is located much closer to Earth (about 93 million miles away) than any other star.

Solution 2: The sun supports life by providing light for green plants to make food and oxygen through photosynthesis, providing heat to keep Earth's water liquid and temperatures habitable, and powering the water cycle and weather patterns.

Solution 3: In the early morning, when the sun is low on the eastern horizon, your shadow stretches out very long toward the west. At midday noon, when the sun is directly overhead, your shadow shrinks and becomes very short right beneath your feet.

Solution 4: The number one safety rule is to never look directly at the sun, as the intense solar radiation can permanently burn your retinas and cause blindness.