Activity Description: Scouts learn how Scientists classify stars.
- Fulfills Step 3 of GSUSA Daisy Space Science Explorer badge requirements.
- Fulfills Step 2 or 4 of GSUSA Brownie Space Science Adventurer badge requirements.
- Fulfills Step 3 or 4 of GSUSA Junior Space Science Investigator badge requirements.
- Fulfills Step 3 or 4 of GSUSA Cadette Space Science Researcher badge requirements.
- Leaders – please be aware of double dipping and make your own informed choice.
Info Needed: Stars are big balls of hot gas that shine in the sky, even though they look tiny from Earth. We see stars at night because the sun’s light doesn’t block them. Stars form patterns called constellations, which people have named and imagined stories about for thousands of years. Telescopes help us see stars better.
Instructions: Explain the following.
When you look up at the night sky, it might seem like all stars are just tiny white dots. But in reality, stars come in many colors, sizes, and temperatures and scientists have a system to classify them based on these differences.
Color and Temperature
The color of a star tells us how hot it is. Even though it might sound backwards, blue stars are the hottest, and red stars are the coolest. Here’s the order from hottest to coolest:
- O – Blue (over 30,000°C)
- B – Blue-white
- A – White
- F – Yellow-white
- G – Yellow (like our Sun!)
- K – Orange
- M – Red (around 2,000°C)
Scientists use these letters to group stars by temperature. So if you hear someone say a star is a “G-type,” that means it’s yellow and medium-hot, just like the Sun!
Size and Brightness
Stars also come in different sizes, from tiny white dwarfs to massive supergiants. Scientists use Roman numerals to describe a star’s size and stage of life:
- I – Supergiants
- III – Giants
- V – Main sequence stars (most stars, including the Sun)
- D – White dwarfs
So the Sun’s full classification is G2V (a yellow star), slightly hotter than average, and in the main part of its life cycle.
Spectra: Light Fingerprints
Stars give off light that can be split into a spectrum (like a rainbow). Scientists use special tools to look at this light and find dark lines called absorption lines. These lines act like fingerprints, showing what elements are inside the star.
By studying a star’s spectrum, scientists can learn:
- What the star is made of
- How old it is
- How fast it’s moving
- Whether it’s part of a group or galaxy
Why It Matters
Classifying stars helps scientists understand how stars are born, live, and die. It also helps us learn more about our own Sun and how it compares to other stars in the universe. You don’t need a telescope to start learning. Just curiosity and a few good resources.
Where to Learn More?
Here are some great places to explore star classification and astronomy:
- Astronomical Society of the Pacific – Explore careers in astronomy and space science
- CK-12: Star Classification – Easy-to-read lessons with diagrams
- K20 LEARN: Classifying Stars With Spectra – Classroom activity with teacher tips
- NASA Science: Astrophysics – Learn how NASA studies stars and galaxies
- WikiHow: How to Classify Stars – Step-by-step guide with examples