Concept:The apparent brightness of a star depends on both its intrinsic properties (size and temperature) and its distance from the observer.
Explanation:The power radiated by a star (its luminosity) is given by the Stefan‑Boltzmann law:
P=σAT4, where
A is the surface area and
T is the temperature.
For a spherical star,
A=4Ï€r2, so
P=4πr2σT4.
A larger radius
r (size) and higher temperature
T increase the radiated power, making the star intrinsically brighter.
However, the brightness we observe (apparent brightness) also depends on the distance from Earth.
For a given luminosity, a star appears dimmer if it is farther away.
Thus, the apparent brightness depends on size, temperature, and distance from the Earth.
Answer:size, temperature, and distance from the earth (Option D).