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High-mass stars emit more energy and are hotter than low-mass stars on the main sequence. Main-sequence stars derive their energy from the fusion of protons to helium. About 90% of the stars lie on the main sequence.
The HertzsprungRussell diagram (abbreviated as HR diagram, HR diagram or HRD) is a scatter plot of stars showing the relationship between the stars absolute magnitudes or luminosities and their stellar classifications or effective temperatures.
This stage is called the main sequence. Main-sequence stars are fusing hydrogen into helium. This nuclear fusion take place deep in the cores of stars. Stars spend about 90% of their lives in this stage.
Main sequence stars make up around 90% of the universes stellar population. They range in luminosity, color, and size from a tenth to 200 times the Suns mass and live for millions to billions of years.
Schematic HR Diagram for Many Stars: Ninety percent of all stars on such a diagram fall along a narrow band called the main sequence. A minority of stars are found in the upper right; they are both cool (and hence red) and bright, and must be giants.

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The most surprising thing about the H-R diagram was that the stars were not randomly scattered on it, but clustered in certain regions and along certain lines. The band that stretches across the diagram includes 90% of the stars in the night sky. This band is called the main sequence stars.
WHAT IS A HERTZSPRUNG-RUSSELL DIAGRAM? A diagram that shows the relationship or differences between SURFACE TEMPERATURE and LUMINOSITY of STARS.
Plot the luminosity on the y-axis with brighter stars going toward the top. Since brighter stars have lower magnitudes, if you choose to plot magnitude on the y-axis, the values will decrease as you go up! Thats OK - just remember that the luminosity of the star is increasing. Plot temperature on the x-axis.

hr diagram worksheet answer key