Bottom right
The colors of the HR Diagram are:BlueBlue-WhiteYellowOrangeRed-OrangeRed
Cool red giant stars are located in the upper right corner of the Hertzsprung-Russell diagram, where they are both cool (low temperature) and bright (high luminosity). These stars have evolved from main sequence stars and are in a late stage of stellar evolution.
The large, cool stars found at the upper right of the H-R diagram are red giants. These stars are in a later stage of their evolution, where they have exhausted their core hydrogen fuel and expanded in size. They are cooler in temperature but have a large luminosity due to their increased surface area.
Large cool stars are classified as either K or M type stars on the spectral classification scale, with M stars being cooler and redder than K stars. These stars are part of the main sequence on the Hertzsprung-Russell diagram and have surface temperatures lower than 5,000 K.
Stars in their giant and supergiant stages are located in the top right portion of the Hertzsprung-Russell diagram, also known as the "red giant branch." These stars are characterized by being large and cool compared to main sequence stars, and they represent later stages in stellar evolution.
Cool and luminous stars would be located in the top right corner of a Hertzsprung-Russell diagram, in the region known as the red giant branch.
The colors of the HR Diagram are:BlueBlue-WhiteYellowOrangeRed-OrangeRed
Cool red giant stars are located in the upper right corner of the Hertzsprung-Russell diagram, where they are both cool (low temperature) and bright (high luminosity). These stars have evolved from main sequence stars and are in a late stage of stellar evolution.
Hot stars are found in the left hand side of the diagram, cool stars the right, bright stars at the top, and lastly the faint stars are located at the bottom.
top,right
The large, cool stars found at the upper right of the H-R diagram are red giants. These stars are in a later stage of their evolution, where they have exhausted their core hydrogen fuel and expanded in size. They are cooler in temperature but have a large luminosity due to their increased surface area.
Large cool stars are classified as either K or M type stars on the spectral classification scale, with M stars being cooler and redder than K stars. These stars are part of the main sequence on the Hertzsprung-Russell diagram and have surface temperatures lower than 5,000 K.
The location on the Hertzsprung-Russell (H-R) diagram where most stars lie is known as the main sequence. This diagonal band extends from the upper left (hot, luminous stars) to the lower right (cool, dim stars) of the diagram. Main sequence stars, including our Sun, primarily fuse hydrogen into helium in their cores, which is the dominant phase of stellar evolution for the majority of stars.
Red dwarf stars are located in the lower right corner of the H-R diagram, which means they are cool and dim compared to other stars. They are low-mass stars that have a long lifespan and are the most common type of star in the universe.
The majority of stars in a Hertzsprung-Russell (HR) diagram are located along the main sequence, which runs diagonally from the upper left (hot, luminous stars) to the lower right (cool, dim stars). This area contains about 90% of all stars, including our Sun. Stars on the main sequence are in a stable phase of hydrogen fusion in their cores. Other regions of the HR diagram, such as the giant and white dwarf areas, contain significantly fewer stars.
Stars in their giant and supergiant stages are located in the top right portion of the Hertzsprung-Russell diagram, also known as the "red giant branch." These stars are characterized by being large and cool compared to main sequence stars, and they represent later stages in stellar evolution.
Most stars are plotted along the main sequence in the Hertzsprung-Russell (HR) diagram, which extends diagonally from the upper left (hot and luminous stars) to the lower right (cool and less luminous stars). This is because the majority of stars, including our Sun, spend the majority of their lives in the main sequence phase where they are fusing hydrogen into helium.