Counting every star in the universe is like measuring a beach

How Many Stars Are There? · 3:32 · Video: SciShow · Watch at the source

In short: You can see a few thousand stars with your naked eyes, but the true number of celestial bodies is so vast it defies simple counting. To grasp the scale of our universe, astronomers have to move from individual observation to complex mathematical estimation.

Because stars are not scattered randomly but gathered into galaxies, scientists cannot simply count them one by one. Instead, they use a method analogous to measuring sand on a beach: they determine the average 'depth' or density of a small representative volume and multiply it across the whole area. In this cosmic analogy, our galaxy serves as the representative volume, while the millions of other galaxies represent the rest of the beach. This approach allows researchers to bypass the impossibility of individual observation. Scientists rely on these integrated quantities because stars are clustered into vast groups rather than being distributed uniformly across space.

The Milky Way alone is estimated to contain more than 100 billion stars, with some estimates placing that number between 10^11 and 10^12. When these figures are multiplied by the estimated 10^11 to 10^12 galaxies in the universe, the resulting total is a staggering range of 10^22 to 10^24 stars. Some estimates suggest the universe could contain up to one septillion stars—a one followed by 24 zeros. Our own Sun is currently positioned roughly halfway through its main sequence life cycle. While massive stars burn fuel quickly and may only last a few million years, lower-mass stars can shine for trillions of years.

These numbers remain rough because galaxies vary significantly in size and luminosity. To improve accuracy, observatories like ESA's Herschel have measured integrated quantities, such as infrared luminosity and star formation rates throughout cosmic history. This allows astronomers to move beyond guesswork toward a more precise understanding of how many stars exist across the vast reaches of space. The Herschel observatory specifically provided data on how many galaxies exist in the infrared spectrum. These measurements help clarify the total count by accounting for different cosmic histories.

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