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Stars on the main sequence have hydrogen-burning cores. A star's position on the H-R diagram tells you a great deal of information about it. ... When stars have exhausted all their hydrogen fuel, they evolve to red giants. Their outer layers of gas expand and cool; therefore, the stars move to the right on the H-R diagram.
In the HR diagram, total brightness (known as “Luminosity” or “Absolute Magnitude”) is plotted against the surface temperature of the star. As the star goes through its life cycle, it moves along the HR diagram from one place to another. ... These stars are “brown dwarfs” or “giant planets,” like Jupiter.
In the HR diagram, total brightness (known as “Luminosity” or “Absolute Magnitude”) is plotted against the surface temperature of the star. As the star goes through its life cycle, it moves along the HR diagram from one place to another. ... So a young star is cool but bright.
When stars have exhausted all their hydrogen fuel, they evolve to red giants. Their outer layers of gas expand and cool; therefore, the stars move to the right on the H-R diagram. Although a star cools when it becomes a red giant, it grows so large its luminosity (or total power emitted) increases.
Depending on its initial mass, every star goes through specific evolutionary stages dictated by its internal structure and how it produces energy. Each of these stages corresponds to a change in the temperature and luminosity of the star, which can be seen to move to different regions on the HR diagram as it evolves.
A star's life cycle is determined by its mass. The larger its mass, the shorter its life cycle. A star's mass is determined by the amount of matter that is available in its nebula, the giant cloud of gas and dust from which it was born. ... The outer shell of the star, which is still mostly hydrogen, starts to expand.
The Hertzsprung-Russell (H-R) diagram is simple. It plots two basic properties of stars: their luminosity (intrinsic brightness) and their surface temperature (as revealed by their color). In doing so, it anchors stellar astronomy just as the periodic table anchors chemistry.
However, the outer layers of this protostar are cooler than the Sun, so the point we plot on the HR diagram for this protostar is above and to the right of the Sun's current location in the diagram (temperature about 3,500 K).
The Hertzsprung Russell diagram, abbreviated as HR diagram, HR diagram or HRD, is a scatter plot of stars showing the relationship between the stars' absolute magnitudes or minorities versus their stellar classifications or effective temperatures.
Hertzsprung-Russell (HR) Diagram If all stars were alike, stars of the same temperature would give off the same amount of light. Hotter stars would be brighter that cooler stars. ... It is by convention reversed so that the hottest stars are located near the origin, and the coolest stars are to the right.
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