Stars' Luminosity Classes & Stellar Classifications

An error occurred trying to load this video.

Try refreshing the page, or contact customer support.

Coming up next: How to Find the Size of a Star

You're on a roll. Keep up the good work!

Take Quiz Watch Next Lesson
Your next lesson will play in 10 seconds
  • 0:01 How Stars Can Be Classified
  • 0:39 Atoms and Spectral Lines
  • 1:44 Luminosity Classes
  • 3:10 Lesson Summary
Save Save Save

Want to watch this again later?

Log in or sign up to add this lesson to a Custom Course.

Log in or Sign up

Speed Speed
Lesson Transcript
Instructor: Artem Cheprasov
Astronomers have a neat trick up their sleeves when it comes to approximating the size of a star. This lesson will tell you how they do it and how the sizes are grouped.

How Stars Can Be Classified

The spectra of stars are like a product barcode. I used to work at a place where I had to scan barcodes. When I did, it would tell me what the product was, where it had come from, and where it needed to go.

Like a barcode told me about the product I was scanning, a star's spectrum can tell an astronomer different things as well. It can tell them about the chemical composition of the star, what its temperature is, as well as what kind of star it is. The former two are covered in other lessons, as we talk about how stellar spectra help astronomers classify the different kinds of stars and what luminosity classes have to do with it.

Atoms and Spectral Lines

When I scanned different products, I noticed that not all barcode lines were created equal. Some lines were really thin and others were really broad. All of that signified something to the computer analyzing those lines.

When an astronomer analyzes a star's spectrum and finds broad spectral lines, it tells them something important. In a dense gas, atoms collide more frequently. This distorts their energy levels in such a way as to produce broader spectral lines. Main-sequence stars, adult stars lying on the main sequence of the HR diagram, have broad spectral lines because their atmospheres are dense.

Giant stars are less dense. Their atoms collide less frequently and the spectral lines are narrower. Supergiants are even less dense and their spectral lines are very narrow.

You get the idea. Lower density equals narrower spectral lines.

Luminosity Classes

Unfortunately, I never figured out the meaning of what broad or narrow lines on the barcodes I scanned meant and was subsequently fired as a result. I'm only kidding. I quit.

You can actually eyeball a star's spectrum and be able to tell how big it is. The size of a star as derived from a star's spectrum is known as a luminosity class. The word 'luminosity' is used because the more luminous a star is, the larger its size has to be. Luminosity is the total energy a star radiates in one second. Like a big fire pushes you away with all the hot energy it radiates, a bigger star will have a larger luminosity.

The luminosity classes can be simplified into the following:

To unlock this lesson you must be a Member.
Create your account

Register to view this lesson

Are you a student or a teacher?

Unlock Your Education

See for yourself why 30 million people use

Become a member and start learning now.
Become a Member  Back
What teachers are saying about
Try it risk-free for 30 days

Earning College Credit

Did you know… We have over 200 college courses that prepare you to earn credit by exam that is accepted by over 1,500 colleges and universities. You can test out of the first two years of college and save thousands off your degree. Anyone can earn credit-by-exam regardless of age or education level.

To learn more, visit our Earning Credit Page

Transferring credit to the school of your choice

Not sure what college you want to attend yet? has thousands of articles about every imaginable degree, area of study and career path that can help you find the school that's right for you.

Create an account to start this course today
Try it risk-free for 30 days!
Create an account