About 90 percent of stars are classified as main sequence stars, which means they are in the stable phase of their lifecycle where they are fusing hydrogen into helium in their cores. These stars follow a pattern on the Hertzsprung-Russell diagram known as the main sequence.
Main sequence stars are bigger.
Red Giants - although they can be branch main sequence for a while.Brown DwarfsBlack dwarfsWhite dwarfsT-Tauri starsProtostarsNeutron starsPre-main sequence stars (PMS stars)
"main sequence" is the tern.
Yes, the majority of stars in our galaxy, including our Sun, are found in the main sequence stage of their life cycle. The main sequence is a phase where stars are fusing hydrogen into helium in their cores, which is the most common stage of stellar evolution.
main sequence stars , our sun is also a main sequence star
The diagonal pattern on an H-R diagram where most stars lie is called the main sequence. This is where stars are fusing hydrogen into helium in their cores, representing the stable phase of a star's life cycle. The main sequence is a fundamental feature of stellar evolution and provides insight into a star's mass, luminosity, and temperature.
I assume the different points on the main sequence represent a kind of balance for the case of hydrogen-to-helium fusion.
This pattern is a sequence of shapes -- circle, square, circle, square, circle
Main sequence WIMP burners look much like protostars link the paradoxically young OB stars found at the galactic centre with WIMP burners.
Main Sequence
its to the right of the middle of the main sequence.
There are billions of stars that are not on the main sequence.
No. They have the lowest temperatures on the main sequence. The hottest main sequence stars are blue.
That's more or less the description of the so-called "main sequence". Those are the stars that get their energy by fusing hydrogen into helium.
About 90 percent of stars are classified as main sequence stars, which means they are in the stable phase of their lifecycle where they are fusing hydrogen into helium in their cores. These stars follow a pattern on the Hertzsprung-Russell diagram known as the main sequence.
The temperature of main sequence stars can vary quite a bit.