The cooler a star is, the less luminous it is. That's assuming the star stays about the same size. "Red giant" stars for example are relatively cool, but very luminous because of their size. However, red giants are not main sequence stars.
For a main sequence star, a lower temperature means it is LESS bright.
That means it has a higher number on the "magnitude" scale.
So the answer is: "the magnitude increases"
Our Sun is putting out more energy than it did a billion years ago. It is expected to get even hotter before it leaves the main sequence and becomes a red giant.
In the main sequence, as the temperature of a star decreases, its luminosity also decreases. This relationship is explained by the Stefan-Boltzmann Law, which states that a star's luminosity is proportional to the fourth power of its temperature. Therefore, cooler stars emit less energy and light compared to their hotter counterparts. As a result, lower temperature main sequence stars, such as red dwarfs, are significantly less luminous than hotter stars like blue giants.
When temperature decreases, a fluid will eventually freeze and become solid
The temperature decreases
The temperature decreases
decreases
In every liquid (with the exception of water) the molecules, when the temperature decreases, contract.
the temperature decreases
The temperature decreases.
What happens to a stars nuclear energy generation change if the core decreases in temperature?
Thermal Contraction
It decreases.
As the temperature is lowered, the movement of the molecules decreases.