You can look at your text book and look for the answer its on book
ok kid don't do that
ok
mass
On the main sequence.
The stages in a star's life cycle are: formation from a nebula, main sequence (where it fuses hydrogen into helium), red giant or supergiant phase, depending on the star's mass, and finally either collapse into a white dwarf, neutron star, or black hole. This life cycle is accurate for most stars, including our Sun.
A supernova occurs at the end of a massive star's life cycle.
Yes, all stars have a place on the Hertzsprung-Russell (HR) Diagram, which plots stars based on their luminosity and temperature. The diagram features distinct regions, including the main sequence, red giants, and white dwarfs, where different types of stars are categorized according to their evolutionary stages. While the exact position of a star on the diagram can change over time as it evolves, every star can be represented at some point in its life cycle.
What is capella star life cycle
The "star life cycle" refers to stars. Earth is not a star.
No, a protostar is basically the BEGINNING of a star's life cycle.
Stars in different stages of their life cycle appear in different regions of the H-R diagram. For example, main sequence stars, where our Sun is located, occupy a diagonal band. Red giants are located in the upper right of the diagram, while white dwarfs are in the bottom left. Supernovae and neutron stars are found in the upper left.
How does the life cycle of humans compare to the life cycle of a star? They both have stages where they are born and die which is in the main sequence and supernova and in a human they are born in a womb and die of old age.
Nobody "invented" it, the life cycle of stars happens naturally.
its mass
A dog.
Life cycle of a sun like star. A sun like star will start out as a nebula to a protostar to a main sequence star to a red giant and into a white dwarf and will simply fade out.
A white dwarf diagram typically shows the main features of a star in the final stage of its life cycle, including its small size, high density, and cooling temperature. It may also display the relationship between luminosity and temperature as the star evolves.
To estimate a star's age using the star life cycle, key information needed includes its mass, luminosity, and temperature. These properties help determine the star's position on the Hertzsprung-Russell diagram, which indicates its evolutionary stage. Additionally, knowledge of the star's chemical composition can provide insights into its formation history and age relative to other stars of similar types. By comparing these factors to theoretical models of stellar evolution, astronomers can estimate the star's age.
dust