Skip Navigation

Main Sequence Star Lives

Stars spend much of their lives on the main sequence, which classifies stars that are fusing hydrogen into helium.

Atoms Practice
This indicates how strong in your memory this concept is
Practice Now
Turn In
14.5Main Sequence Star Lives

What do most stars look like?

We have a main sequence star nearby. Our Sun is on the main sequence, classified as a yellow dwarf. Our Sun has been a main sequence star for about 5 billion years. As a medium-sized star, it will continue to shine for about 5 billion more years. Most stars are on the main sequence.

Main Sequence Stars

For most of a star’s life, hydrogen atoms fuse to form helium atoms. A star like this is a main sequence star. The hotter a main sequence star is, the brighter it is. A star remains on the main sequence as long as it is fusing hydrogen to form helium.

Classifying Stars by Color

The most common way of classifying main sequence stars is by color as shown, in Table below. Each class of star is given a letter, a color, and a range of temperatures. The letters don’t match the color names because stars were first grouped as A through O. It wasn't until later that their order was corrected to go by increasing temperature. When you try to remember the order, you can use this phrase: “Oh Be A Fine Good Kid, Man.”

Class Color Temperature range (degrees Kelvin) Sample Star
O Blue >30,000

An artist’s depiction of the O class star Zeta Puppis.

B Blue-white 10,000–30,000

Computer generated image of Rigel, a Class B star.

A White 7,500–10,000

Sirius A is the brightest star that we see in the night sky. The dot on the right, Sirius B, is a white dwarf.

F Yellowish-white 6,000–7,500

There are two F class stars in this image, the supergiant Polaris A and Polaris B. What we see in the night sky as the single star “Polaris,” we also know as the North Star.

G Yellow 5,500–6,000

Our sun: the most important G class star in the Universe, at least for humans.

K Orange 3,500–5,000

Arcturus is a Class K star that looks like the sun but is much larger.

M Red 2,000–3,500

There are two types of Class M stars: red dwarfs and red giants.

An artist’s concept of a red dwarf star. Most stars are red dwarfs.

The red supergiant Betelgeuse is seen near Orion’s belt. The blue star in the lower right is the Class B star Rigel.

The surface temperature of most stars is due to its size. Bigger stars produce more energy, so their surfaces are hotter. But some very small stars are very hot. Some very big stars are cool.

Large stars burn through their supply of hydrogen very quickly. These stars “live fast and die young!” A very large star may only be on the main sequence for 10 million years. A very small star may be on the main sequence for tens to hundreds of billions of years.


  • main sequence star: A star that is fusing hydrogen atoms to helium; a star in the main portion of its “life.”


  • Stars spend most of their lives on the main sequence. These stars fuse hydrogen into helium for energy.
  • Large main sequence stars may be hotter than small stars but not always.
  • Large stars are not on the main sequence as long as small stars.


Use this resource to answer the questions that follow.

Properties of Main Sequence Stars at http://www.youtube.com/watch?v=kQLU0gEI61k (0:51)

  1. What are main sequence stars converting?
  2. What process releases the energy in these stars?
  3. What keeps these stars stable?
  4. What is the mass range of main sequence stars?
  5. What is the mass of most main sequence stars?


  1. What characteristic do all main sequence stars have?
  2. What are the characteristics of our Sun compared with other stars?
  3. What are the characteristics of large stars?
  4. What are the characteristics of small stars?

Notes/Highlights Having trouble? Report an issue.

Color Highlighted Text Notes
Please to create your own Highlights / Notes
Show More

Image Attributions

Explore More

Sign in to explore more, including practice questions and solutions for Main Sequence Star Lives.
Please wait...
Please wait...