Step 1 — Stars always shine: All the stars, like our Sun, produce their own light all the time. So their light is always reaching the Earth.
Step 2 — Why are they visible at night? At night the side of Earth on which we stand is turned away from the Sun. The sky is therefore dark, so even the faint light coming from the very distant stars can enter our eyes without much brighter light competing with it. Hence we can see the stars clearly.
Step 3 — Dawn and dusk: • Dawn (early morning) begins as soon as the Sun is just below the horizon. Its light starts to spread through the atmosphere.
• Dusk (early evening) is the opposite situation, when the Sun has just set and its light is slowly disappearing from the sky.
Step 4 — Scattering of sunlight in the atmosphere: Molecules of air and tiny dust or water droplets act like millions of minute mirrors. They scatter the Sun’s light in all directions. As a result the whole sky becomes bright, even if the Sun itself is not yet above the horizon.
Step 5 — Brightness comparison: The Sun is enormously brighter than any single star. A simple way to state this is
\[ I_{\text{sun (day sky)}} \approx 10^{10}\, I_{\text{average star}} \]
where $$I$$ stands for light intensity. Because $$I_{\text{sun}}$$ is nearly ten billion times larger, the scattered sunlight floods the eye and the much weaker starlight is lost in the glare.
Step 6 — How the eye reacts: The human eye adjusts its pupil and retina to the brightest light that is present. In bright daylight the eye “closes down” so that the starlight, which is ten orders of magnitude weaker, no longer produces a signal big enough to be noticed.
Step 7 — Result: • At dawn the increasing brightness of the scattered sunlight overpowers the faint starlight, so the stars seem to fade and finally disappear.
• At dusk the brightness of the sky decreases after the Sun sets. When the scattered sunlight becomes weak enough, the same faint starlight once again becomes detectable, and the stars appear to “switch on.”
Step 8 — Why astronauts see stars even in daytime: Outside Earth’s atmosphere there is practically no air to scatter sunlight, so the sky looks black even on the day-side of a spacecraft. Under those conditions the stars remain visible all the time.
Therefore, we do not actually lose the stars during the day; their light is simply masked by the overwhelming brightness of the Sun’s scattered light in our atmosphere.