How many stars in our galaxy? Learn why astronomers estimate 100–400 billion stars in the Milky Way, and how they calculate this number.
How many stars in our galaxy? Podcast:
Key Takeaways
- The Milky Way contains an estimated 100–400 billion stars.
- Astronomers cannot directly count stars; they rely on mass estimates and statistical models.
- Red dwarfs make up ~70% of all stars, but they are faint and hard to detect.
- The Gaia mission has mapped 1+ billion stars, only ~1% of the total.
- Compared with the Andromeda Galaxy (~1 trillion stars), the Milky Way is mid-sized.
- The observable universe may hold 200 sextillion to 1 septillion stars, more than grains of sand on Earth.
What Does “How Many Stars in Our Galaxy” Mean?

When people ask “how many stars in our galaxy?”, they expect a neat number.
In reality, the answer is an estimate based on complex science.
The Milky Way’s stellar population lies between 100 billion and 400 billion stars.
This wide range exists because scientists must account for:
- Our limited view from inside the galaxy
- Dust blocking starlight
- Billions of faint, undetectable red dwarfs
- Uncertainty in star formation models
Why Can’t Astronomers Count Every Star?

Our Vantage Point in the Milky Way
We live inside the galactic disk, about 27,000 light-years from the center.
From this perspective, mapping the Milky Way is like trying to map a city while standing on one street corner.
Interstellar Dust and Gas
The disk is filled with gas clouds and dust.
These absorb starlight and create a “Zone of Avoidance” where billions of stars are hidden from view in visible light.
Faint Red Dwarfs Dominate
The majority of stars are red dwarfs.
They are tiny, cool, and faint—making them almost invisible across large distances.
Limits of Technology
Even with advanced missions like Gaia, which has mapped 1+ billion stars, that’s only about 1% of the Milky Way’s population.
How Do Astronomers Estimate the Number of Stars?
The basic equation:
Number of Stars = Total Stellar Mass ÷ Average Stellar Mass
- If the average star is similar to the Sun → ~100 billion stars.
- If dominated by red dwarfs → closer to ~400 billion stars.
This relies on the Initial Mass Function (IMF), a model describing how many stars form at different masses.
The Role of Galactic Mass and Dark Matter
Galactic Rotation Curves
Astronomers measure how fast stars orbit the galactic center.
They expected outer stars to move slower—but instead, the curve is flat.
Discovery of Dark Matter
This mystery led to the discovery of dark matter, which makes up most of the Milky Way’s mass.
Current Estimates
- Total mass of Milky Way: ~1.5 trillion solar masses
- Stellar mass: 100–200 billion solar masses
- When divided by average star mass, this gives the 100–400 billion range.
What Types of Stars Fill the Milky Way?
- Red Dwarfs (M-type): ~70%, small, cool, and long-lived.
- Sun-like Stars (G-type): ~7%, including our Sun.
- Blue Giants (O & B types): Rare but extremely luminous.
- White Dwarfs: Dead stars’ remnants.
- Neutron Stars & Black Holes: Exotic and rare.
👉 Because red dwarfs dominate, the star count heavily depends on their numbers.
How Many Planets Are in the Milky Way?
- The Kepler mission found that most stars have at least one planet.
- That means 100–400 billion planets may exist in our galaxy.
- Many orbit in the habitable zone, raising hopes for alien life.
How Does the Milky Way Compare to Other Galaxies?

- Milky Way: 100–400 billion stars, 100,000 light-years wide.
- Andromeda Galaxy (M31): ~1 trillion stars, >200,000 light-years wide.
- Large Magellanic Cloud (LMC): ~30 billion stars, a dwarf galaxy.
👉 The Milky Way is not the largest galaxy, but a fairly typical large spiral galaxy.
What Will Happen When the Milky Way and Andromeda Collide?
- In ~4.5 billion years, the Milky Way and Andromeda will merge.
- Stars won’t collide directly (too far apart).
- Gravitational reshuffling will create a giant elliptical galaxy.
- New bursts of star formation will occur.
This future event shows galaxies are dynamic, ever-evolving systems.
How Many Stars Exist in the Universe?
Counting Galaxies
Deep-field images (Hubble, JWST) show billions of galaxies.
Estimates range from 2 trillion to 20 trillion galaxies.
Multiplying by Stars per Galaxy
- If each has ~100 billion stars → 200 sextillion stars.
- NASA suggests as high as 1 septillion stars.
That’s 10^24 stars—more than all the grains of sand on Earth.
Firsthand Perspective: Seeing the Stars From Earth
When I take people outside on a clear night, they often ask:
“How many stars can we see?”
The answer: only about 5,000 with the naked eye.
This gap—between what we see and what exists—shows why astronomy is so inspiring.
The Milky Way holds hundreds of billions of hidden suns, waiting to be revealed by science.
Frequently Asked Questions
Can astronomers count every star in the Milky Way?
No. Dust, faint red dwarfs, and our position inside the galaxy make it impossible.
How accurate is the 100–400 billion estimate?
It’s based on the galaxy’s mass and the Initial Mass Function. The wide range reflects small-star uncertainty.
Which type of star is most common in our galaxy?
Red dwarfs, making up about 70% of all stars.
Is the Milky Way bigger than Andromeda?
No. Andromeda is larger, with ~1 trillion stars compared to our 100–400 billion.
How many stars exist in the universe?
Between 200 sextillion and 1 septillion stars.