Yes. The larger or more massive a star is, the faster it has to "burn" hydrogen to stay in Hydrostatic equilibrium.
The largest stars, known as population III stars (Formed about 400 million years after the big bang) were massive and used up all of the available hydrogen in millions of years.
Our Sun, is not so massive, so will stay on the main sequence for about 10 billion years. Part of this, is not due to it's mass, but also because of the metallicity or the metals within it. This "slows" down the rate of nuclear fusion.
"main sequence" is the tern.
There are billions of stars that are not on the main sequence.
The smallest stars in the main sequence are the stars with cooler surface temperatures.
main sequence stars , our sun is also a main sequence star
About 90% of all stars are main sequence stars, including our Sun. These stars are in the stable phase of their lifecycle, where they fuse hydrogen into helium in their cores. Main sequence stars are the most common type of stars found in the universe.
main sequence stars
Main sequence stars.
Main sequence stars are found in all galaxies.
Approximately 90% of stars in the universe are categorized as main sequence stars. These stars, like our Sun, are in the stable phase of their lifecycle where they fuse hydrogen into helium in their cores. Main sequence stars vary in size and temperature, leading to differences in brightness and color.
No. They have the lowest temperatures on the main sequence. The hottest main sequence stars are blue.
No. Main sequence stars are simply stars that are fusing hydrogen into helium and have a specific relationship between color and luminosity. They range from red dwarfs to large O-type main sequence stars.
yes