A black hole does not appear on an H-R diagram. An H-R diagram is a scatter plot of stars based on their luminosity and temperature. Black holes are objects with extreme gravitational forces, not visible light output.
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Neutron stars are not typically found on the H-R diagram because they are remnants of massive stars that have undergone supernova explosions. However, their progenitor stars could be located on the diagram based on their luminosity and temperature.
The Hertzsprung-Russell (H-R) diagram is a plot of stars' luminosity versus their temperature (or color). This diagram is a valuable tool in understanding the life cycle and evolution of stars, as it allows astronomers to classify stars according to their size, mass, and stage of stellar evolution.
Because there not that hot
Is a diagram with the same purpose as a Venn diagram, but shaped as an H. the differences go on the left and right of the diagram while the similarities go in the middle
H-H
The H-R diagram compares a star's surface temperature to its absolute brightness.
A black hole does not appear on an H-R diagram. An H-R diagram is a scatter plot of stars based on their luminosity and temperature. Black holes are objects with extreme gravitational forces, not visible light output.
The H-R diagram is a graphical tool used to classify stars according to color, temperature, spectral type, luminosity, and evolutionary stage. H-R stands for Hertzsprung-Russell.
The H-R diagram is a graphical tool used to classify stars according to color, temperature, spectral type, luminosity, and evolutionary stage. H-R stands for Hertzsprung-Russell.
An H-R diagram compares the luminosity (brightness) of stars with their surface temperature. It helps classify stars based on their temperature and luminosity, allowing astronomers to study their characteristics and evolution.
The Hertzsprung-Russell diagram (H-R diagram) shows the relationship between absolute magnitude, luminosity, classification, and effective temperature of stars. The diagram as originally conceived displayed the spectral type (effectively the surface temperature) of stars on the horizontal axis and the absolute magnitude (their intrinsic brightness) on the vertical axis.
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H-O- or just -OH
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The Hertzsprung-Russell diagram, or H-R diagram, was created in 1911 by Ejnar Hertzsprung and Henry Norris Russell. They plotted the luminosity of stars against their surface temperature to classify and study stellar populations. This diagram revolutionized our understanding of stars and their life cycles.