1. **Time** – Light travels at a finite speed and the universe has a finite age, meaning that beyond a certain distance, the starlight hasn’t had *time* to reach us yet.
2. **Space** – Space is really, really, really, really, REALLY, REALLY big. To get an idea of just how big space is, check out [this site](https://joshworth.com/dev/pixelspace/pixelspace_solarsystem.html), which is essentially the solar system (*just the solar system*) to scale. Interstellar space is much *sparser* than even this; intergalactic space sparser still.
3. **”Spreading out” of light** – A star emits from its surface a specific number of photons per unit of time (This is an oversimplification, and light also behaves as a wave, but this is ELI5). That number doesn’t change. (Well, it does, but not for our purposes.) What *does* change is the area of the sphere these photons cover – they have to “spread out” across the universe. The further they spread out, the dimmer the star is – the fewer photons hit your eye per unit of time, and once that number gets below a certain threshold, you just can’t see it. If you were to move the Sun out to where Sirius is now, it would still be a pretty bright star, but it would be less bright than Sirius, perfectly safe to look at. (Also, we’d all freeze, but that’s beside the point.)
4. **Redshift** – Almost all of the stars you can actually see without a powerful telescope are from the Milky Way. Because the universe is expanding, stars from distant galaxies are “redshifted” – their light gets pushed toward the red end of the EM spectrum, and eventually out of the visible-light range entirely. This effect is stronger the further away from Earth you get.
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