The "main sequence" is the region (on the HR diagram) for stars which burn hydrogen-1. Once stars use up most of their hydrogen-1 (and have significant amounts of helium-4), they leave the main sequence.
Wiki User
∙ 8y agoWiki User
∙ 8y agoWhen it runs out of hydrogen.
red supergiant
A star stops being a main sequence star when it exhausts the hydrogen fuel in its core, leading to changes in its internal structure and a transition to a different phase of stellar evolution, such as becoming a red giant or a white dwarf. This change marks the end of the star's main sequence stage.
Our Sun is currently a main sequence star. It is not a supernova, as supernovae are massive explosions that occur at the end of a star's life cycle, and it is not a white dwarf, which is a type of star that has exhausted its nuclear fuel and collapsed to a very dense state.
Before a star becomes a red giant, it goes through the stage of being a main sequence star, where nuclear fusion in its core converts hydrogen into helium, releasing energy in the form of light and heat.
The main sequence of a black hole starts with a massive star collapsing under its own gravity to form a singularity, which is a point of infinite density and zero volume. This singularity is surrounded by an event horizon, beyond which not even light can escape, leading to the characteristic black appearance.
When a star "goes off the main-sequence" it generally means the star has run out of hydrogen fuel and is beginning the post-main-sequence or its end of life phase. The main sequence of a star is the time where it is no longer just a proto-star but is burning hydrogen as a primary source of fuel.
red supergiant
Alioth is a white star nearing the end of it's main sequence. Hope this helps! (:
Depending on how "low" on the chart it will either be a red dwarf or a PMS (Pre-main sequence) star.
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.
It's the size. A dwarf star has reached the end of the road and has collapsed. It's a little old star and people don't notice it, mostly.
A "main-sequence star" is one that fuses hydrogen into helium. Eventually, the star will run out of this specific type of fuel - in other words, it won't have enough hydrogen (at least, near its core) to continue this process.
Spica is a dual star system, with the two members too close for resolution by the best telescopes. The larger, primary star is a blue-white giant, and does have the potential to end it's life as a supernova. The primary is not a main sequence star. The secondary, about 70% the size of the primary, is a main sequence star, also blue white.
The final stage of a yellow star like our Sun is the formation of a planetary nebula. This occurs when the star sheds its outer layers into space, leaving behind a hot core called a white dwarf. Over time, the white dwarf will cool and fade away.
The main sequence is a map of star brightness against their temperature. Stars that lie on the main sequence in the top left are the high mass stars. Cooler, smaller stars lie near the line at the lower right.
Assuming you mean a "main sequence" yellow star, it's a white dwarf star. In the end that fades to a black dwarf.
Dear Wiki Questioner, When a Star is fusing hydrogen together to create energy, we call it a "Main Sequence" Star. Most stars tend to enter this main sequence phase shortly after they are formed, and they stay in this state until they either run out of hydrogen (in which case they usually end up as a white dwarf) or if they are big enough they become type II supernovae and explode... forming neutron stars or black holes. However, it is important to note that stars primarily don't "burn" hydrogen (no combustion takes place). Instead, stars fuse hydrogen into helium, which releases the titanic amount of energy that powers main sequence stars.