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On a logarithmic scale for luminosity, it is quite close to a negative linear relationship.
To determine a star's luminosity is from size and temperature.
The scatter plot of the relationship between a star's temperature and luminosity is represented by the Hertzsprung-Russell diagram. In a standard H-R diagram the horizontal axis shows the [surface] temperature, increasing from right to left, while the vertical axis shows luminosity increasing from bottom to top. When both axis are on a logarithmic scale, the main sequence stars from a diagonal belt stretching from top right (very hot and very luminous) to bottom left (not so hot and not so luminous).
It shows the relationship between stars luminosity versus their classifications and effective temperatures
Yes.
as surface temperature increases, luminosity increases
The star that is hotter will have a higher luminosity.
The star that is hotter will have a higher luminosity.
On a logarithmic scale for luminosity, it is quite close to a negative linear relationship.
To determine a star's luminosity is from size and temperature.
The scatter plot of the relationship between a star's temperature and luminosity is represented by the Hertzsprung-Russell diagram. In a standard H-R diagram the horizontal axis shows the [surface] temperature, increasing from right to left, while the vertical axis shows luminosity increasing from bottom to top. When both axis are on a logarithmic scale, the main sequence stars from a diagonal belt stretching from top right (very hot and very luminous) to bottom left (not so hot and not so luminous).
It is a chart showing a scatter chart of stars according to their temperature and their luminosity (or absolute magnitude).
It shows the relationship between stars luminosity versus their classifications and effective temperatures
Generally speaking, the apparent luminosity would be an inverse square relationship, which is to say, if the same star was at twice the distance, a quarter of the light would be reaching the observer. But absolute luminosity can of course vary without regard to distance from Earth - dim stars can be close, or bright stars distant, or vice-versa.
The temperature and luminosity of stars.
Yes.
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.