Stars spend the majority of their life span in the main sequence phase, which is a stable period of nuclear fusion where they convert hydrogen into helium. This phase can last for billions of years for stars like the sun.
A majority of visible stars are in the main sequence but it is likely that there are a lot more brown dwarfs than are recorded. This is because they are stars that almost did not quite make it. They are not very luminous at visible wavelengths and so may be under-represented.
Yes Star spend most of their life span as a main sequence star. A star end will depend on its size in life the end of a start can be a red giant to supernova, a white dwarf, pulsar, or black hole.
The majority of visible stars in the sky are main sequence stars, like our own Sun. These stars are in the stable phase of their life cycle where they are fusing hydrogen into helium in their cores.
Stars spend most of their life in the main sequence phase, where nuclear fusion of hydrogen into helium occurs in their cores, producing energy that counteracts gravitational collapse. This phase can last billions of years for stars like our Sun.
Stars spend most of their life span in the main sequence phase, where they are fusing hydrogen into helium in their cores. After exhausting their hydrogen fuel, they will expand and cool down to become red giants before eventually evolving into white dwarfs or other stellar remnants.
The main sequence.
All stars spend the majority of their lives on the main sequence. Once high mass stars have exhausted the hydrogen fuel in their cores they expand into much larger red or blue supergiant stars.
A majority of visible stars are in the main sequence but it is likely that there are a lot more brown dwarfs than are recorded. This is because they are stars that almost did not quite make it. They are not very luminous at visible wavelengths and so may be under-represented.
Manhattan, New York City.
Yes Star spend most of their life span as a main sequence star. A star end will depend on its size in life the end of a start can be a red giant to supernova, a white dwarf, pulsar, or black hole.
The majority of visible stars in the sky are main sequence stars, like our own Sun. These stars are in the stable phase of their life cycle where they are fusing hydrogen into helium in their cores.
Stars spend most of their life in the main sequence phase, where nuclear fusion of hydrogen into helium occurs in their cores, producing energy that counteracts gravitational collapse. This phase can last billions of years for stars like our Sun.
Bahgdad,Iraq
Stars spend most of their life span in the main sequence phase, where they are fusing hydrogen into helium in their cores. After exhausting their hydrogen fuel, they will expand and cool down to become red giants before eventually evolving into white dwarfs or other stellar remnants.
The portion of a star's life cycle when it is using hydrogen for fuel is called the main sequence phase. This is when a star fuses hydrogen in its core to produce energy and maintain stability. Stars spend the majority of their lives in this phase.
White dwarf stars are theorized to be the final evolutionary state of all stars that did not become neutron stars. This stage is the longest in a stars life outside of black dwarfs which are white dwarfs that have cooled dramatically.
well he was born in akron Ohio but i am not sure where he spent the majority of his life. oh and another thing admiral Peary was born in cresson Pennsylvania. Admiral peary is the guy who discovered the north pole!