The graph that shows the relationship between a star's absolute magnitude and temperature is called the Hertzsprung-Russell (H-R) diagram. In this diagram, stars are plotted according to their absolute magnitude (or luminosity) on the vertical axis and their surface temperature on the horizontal axis. Typically, the temperature decreases from left to right, and the diagram reveals distinct regions for different types of stars, including main sequence stars, giants, and white dwarfs. This allows astronomers to classify stars and understand their evolutionary stages.
It is a chart showing a scatter chart of stars according to their temperature and their luminosity (or absolute magnitude).
its located somewhere
A Hertzsprung-Russell diagram is a scatter graph that can be used to plot the relationship between the absolute magnitude (i.e. luminosity) of a star versus it's spectral type / classification and effective temperature. Since a black hole does not have an absolute magnitude, spectral type, or an effective temperature, it cannot be located on an H-R diagram.
A star's absolute magnitude must be used when plotting it on the Hertzsprung-Russell (HR) diagram because it provides a standardized measure of a star's intrinsic brightness, independent of its distance from Earth. This allows for an accurate comparison of stars' luminosities and evolutionary stages. Using apparent magnitude, which varies with distance and interstellar absorption, would lead to misleading interpretations of a star's true properties and position on the diagram. Thus, absolute magnitude ensures a consistent framework for analyzing stellar characteristics.
The answer to this question is Hertzsprung-Russell diagram
Its called an HR diagram or a Hertzsprung-Russell diagram.
The HR diagram, also known as the Hertzsprung-Russell diagram, depicts the relationship between the luminosity and temperature of stars. It shows how stars are distributed in terms of their brightness and temperature, allowing astronomers to classify stars based on these characteristics.
It is a chart showing a scatter chart of stars according to their temperature and their luminosity (or absolute magnitude).
its located somewhere
That is called the Hertzsprung-Russell or HR diagram and each star occupies a point. The horizontal axis is temperature and the vertical axis is the absolute magnitude.
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.
The Hertzsprung-Russell diagram is a scatter graph of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their spectral types or classifications and effective temperatures.
That is called the HR diagram (Hertzsprung Russell) and the temperature is along the horizontal axis while the vertical axis is the star's absolute magnitude. Each star has a fixed point in this diagram, and it shows that most stars belong in a broad band on the left called the Main Sequence.
The Hertzsprung-Russell diagram predicts the relationship between a star's luminosity (brightness) and temperature, allowing astronomers to classify stars based on their properties. It shows the correlation between a star's temperature and its absolute magnitude, helping to understand their evolutionary stage and lifecycle.
The Hertzsprung-Russell (HR) diagram is a graph that shows the relationship between a star's magnitude (luminosity) and temperature. It plots stars based on their color (temperature) and brightness (magnitude), allowing astronomers to classify stars and understand their evolutionary stage.
Surface temperature and Absolute magnitude