Stephenson 2-18: the largest known star – and what is uncertain about it

By · Published on · Details checked on 29 October 2026

Stephenson 2-18 is a red supergiant in the constellation Scutum and is considered the largest known star of all. Its radius is estimated at around 2,150 solar radii – if it stood in place of our Sun, its surface would reach out beyond the orbit of Saturn.

More in our overview: Stars.

⭐ In short: Stephenson 2-18 is the record holder among known stars – with one big caveat: its size depends on a distance estimate that is disputed. You can’t see it anyway: it lies around 19,000 light-years away behind dense dust and only shines brightly in the infrared.
Size comparison: Stephenson 2-18, VY Canis Majoris, UY Scuti and Betelgeuse on the scale of the planetary orbits
If these stars stood in place of the Sun, this is how far they would reach. UY Scuti after Healy et al. 2023 (Gaia DR3). Own graphic, sterngucker.de

Stephenson 2-18 in numbers

TypeRed supergiant (hypergiant)
ConstellationScutum (the Shield)
Distancearound 19,000 light-years
Radiusaround 2,150 solar radii ≈ 1.5 billion km
Diameter in AUaround 20 astronomical units
Luminosityabout 440,000 times the Sun’s luminosity
Surface temperaturearound 3,200 kelvin
Apparent magnitudeabout 15 mag in visible light
Membershipstar cluster Stephenson 2
The radius assumes that the star belongs to the cluster Stephenson 2.

What 2,150 solar radii mean

Numbers of this size only mean something once you convert them. The diameter of Stephenson 2-18 is about 20 astronomical units – twenty times the distance between Earth and the Sun.

In place of the Sun it would swallow Mercury, Venus, Earth, Mars, Jupiter and Saturn. Only somewhere between Saturn and Uranus would you reach its surface.

To take away: Light travels around the Sun in about 15 seconds. To go once around Stephenson 2-18, the same light would need almost nine hours. Nearly ten billion Suns would fit inside the star.

Even so, it is no heavyweight. Red supergiants are bloated stars with an extremely thin envelope – their outer layers are thinner than any vacuum we can create on Earth.

Why the record is shaky

This is where it gets uncomfortable, and that is why it is here: a star’s radius cannot be measured directly, only calculated from brightness, temperature and distance. Of these three, the distance is the least certain.

The record figure assumes that Stephenson 2-18 belongs to the star cluster of the same name and therefore shares its distance. Several studies doubt exactly that – the star’s velocity does not fit neatly with the other cluster members.

If it were actually closer, it would be considerably smaller and the record would fall. Until the distance is confirmed independently, “the largest known star” remains a well-founded assumption and not an established fact.

Careful with rankings: Lists of the largest stars change their top spot every few years – not because the stars change, but because the distance measurements change. If you read a number without error bars, you are reading half the information.

The competition for first place

StarRadius (solar radii)DistanceConstellation
Stephenson 2-18around 2,150around 19,000 lyScutum
VY Canis Majorisaround 1,420around 3,900 lyCanis Major
UY Scutiaround 900around 5,900 lyScutum
Betelgeusearound 760around 550 lyOrion
All figures carry considerable uncertainty – the farther away, the larger the margin.

The pattern is striking: the less certain the distance, the larger the estimate tends to be. UY Scuti is the best example: for years it was listed as the largest known star at around 1,700 solar radii – until the Gaia distance (around 5,900 instead of 9,500 light-years) shrank it to roughly 900 (Healy et al. 2023). A reason to read the top of the list with caution.

That is why the best-studied one is the neighbour: Betelgeuse in Orion. It is much smaller, but close enough that its surface can actually be imaged.

Can you observe Stephenson 2-18?

Honest answer: no, at least not visually. At about 15 mag in visible light it is theoretically within reach of larger amateur telescopes – but it sits in a region of the Milky Way packed with stars and dust.

In practice that means an inconspicuous reddish point of light among thousands, identifiable only by its catalogue coordinates. The star is a target for infrared telescopes, not for the eyepiece.

If you want to see giant stars with your own eyes, start with Betelgeuse instead. It stands high in the winter sky and is visible to the naked eye – and you can follow its changes in brightness yourself over weeks.

Our beginner recommendation: Skywatcher Dobson Telescope N 130/650 Heritage FlexTube

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If you want more: the next step
With the Apertura AD8 8" Dobsonian TelescopeSkywatcher Dobson Telescope N 200/1200 Skyliner Classic and its 200 mm aperture you reach roughly 14 mag – that is what first brings distant red giants in the winter Milky Way within range. The extra cost pays off if you want to seek out faint objects specifically; for bright stars like Betelgeuse you don’t need it.

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Stephenson 2-18: FAQ

How big is Stephenson 2-18?

Its radius is estimated at around 2,150 solar radii, which is about 1.5 billion kilometres. Its diameter is therefore around 20 astronomical units – in place of the Sun it would extend beyond the orbit of Saturn.

Is Stephenson 2-18 really the biggest star?

The biggest known one, yes – but with a caveat. Its size follows from the assumed distance, and whether the star really belongs to the cluster Stephenson 2 is disputed. If it were closer, it would be smaller.

Where is Stephenson 2-18 in the sky?

In the constellation Scutum, a small constellation in the southern summer Milky Way between Aquila and Sagittarius. From mid-northern latitudes this region stands low in the south in summer.

What will happen to Stephenson 2-18?

Red supergiants of this mass end as a supernova. When that will happen cannot be predicted – astronomically speaking it is at the end of its life, which can mean tens of thousands to hundreds of thousands of years.

How can a star be bigger than a planetary orbit?

Because a red supergiant is almost empty. At the end of its life a massive star swells enormously, while most of its mass stays concentrated in the core. The outer envelope is extremely thin – huge, but barely there.

Further reading