The brightness is very similar to the temperature, the brightness relies on the temperature
By multiple observations it was noted that that correlation was true.
The temperature is displayed along the horizontal axis while the vertical axis is the star's absolute magnitude. So the HR diagram is a scatter diagram relating temperature and brightness, and eah star occupies one point.
Brightness tells you the temperature and mostly temperature would tell the brightness of the star that we are talking about.
The temperature is displayed along the horizontal axis while the vertical axis is the star's absolute magnitude. So the HR diagram is a scatter diagram relating temperature and brightness, and eah star occupies one point.
Stars' brightness and temperature are typically represented on a Hertzsprung-Russell (H-R) diagram. An average star like the Sun would be located on the "Main Sequence" portion of the graph, where brightness increases as temperature increases.
Hertzsprung and Russell.
Hertzsprung and Russell.
Distance from Earth, size of star, and temperature of star.
Distance from Earth, size of star, and temperature of star.
A main sequence star's temperature is most closely related to its color and brightness.
You find its size.
A decrease in a star's absolute brightness could be caused by the star moving farther away from Earth, interstellar dust blocking some of its light, or a decrease in the star's temperature. All of these factors would result in less light reaching Earth, causing a decrease in the star's apparent brightness.