This orange blob shows the nearby star Betelgeuse, as seen by the Atacama Large Millimeter/submillimeter Array (ALMA). This is the first time that ALMA has ever observed the surface of a star and this first attempt has resulted in the highest-resolution image of Betelgeuse available. Betelgeuse is one of the largest stars currently known — with a radius around 1400 times larger than the Sun’s in the millimeter continuum. About 600 light-years away in the constellation of Orion (The Hunter), the red supergiant burns brightly, causing it to have only a short life expectancy. The star is just about eight million years old, but is already on the verge of becoming a supernova. When that happens, the resulting explosion will be visible from Earth, even in broad daylight. The star has been observed in many other wavelengths, particularly in the visible, infrared, and ultraviolet. Using ESO’s Very Large Telescope astronomers discovered a vast plume of gas almost as large as our Solar System. Astronomers have also found a gigantic bubble that boils away on Betelgeuse’s surface. These features help to explain how the star is shedding gas and dust at tremendous rates (eso0927, eso1121). In this picture, ALMA observes the hot gas of the photosphere of Betelgeuse at sub-millimeter wavelengths — where localised increased temperatures explain why it is not symmetric. Scientifically, ALMA can help us to understand the extended atmospheres of these hot, blazing stars. Links: Size comparison: Betelgeuse and the Sun
Betelgeuse, the glowing red star in Orion’s shoulder, is one of the most captivating sights in the night sky—famous for its size, color, and dramatic behavior. As a red supergiant nearing the end of its life, it captivates astronomers and stargazers alike with its sheer size, violent surface activity, and impending doom—a supernova explosion that could light up Earth’s sky like a second Sun.
1. What Is Betelgeuse?
A Bright Star in Orion
Betelgeuse (pronounced “Beetle-juice”) is Orion’s second-brightest star and the 10th brightest in the entire night sky. Its reddish hue makes it easy to spot, marking Orion’s right shoulder (or left, from our perspective).
Key Facts About Betelgeuse
Distance from Earth: ~642 light-years
Age: ~8–8.5 million years (very young for a star!)
Type: Red supergiant (M1-2 spectral class)
Mass: ~16.5–19 times the Sun
Luminosity: ~100,000 times brighter than the Sun
Unlike our Sun, which will live for billions of years, Betelgeuse is already in its final stages of life—despite being just a cosmic toddler in stellar terms.
2. Why Is Betelgeuse Dying So Soon?
Massive Stars Burn Fast, Die Young
Stars like Betelgeuse are celestial giants, but their enormous size comes at a cost. The bigger a star is, the quicker it uses up its nuclear fuel—meaning massive stars live fast and die young.
Our Sun (a G-type star): Lives ~10 billion years
Betelgeuse (a red supergiant): Lives only ~8–10 million years
Betelgeuse has already exhausted its hydrogen fuel and is now fusing helium into carbon and oxygen. Once it runs out of usable fuel, its core will collapse—triggering a supernova explosion.
A Supernova Waiting to Happen
When Betelgeuse explodes, it will become a Type II supernova, one of the most energetic events in the universe.
What happens during a supernova?
The core collapses in less than a second.
A shockwave blasts outward, tearing the star apart.
For a few weeks, it will outshine entire galaxies.
What’s left after a massive star dies depends on its size—its core can collapse into either a dense neutron star or an even denser black hole.
3. How Big Is Betelgeuse? (Spoiler: It’s Unimaginably Huge!)
A Star That Could Swallow Jupiter
If we replaced our Sun with Betelgeuse:
Its surface would extend past Jupiter’s orbit.
Mercury, Venus, Earth, and Mars would be inside it.
Its diameter is ~1.4 billion km (about 1,000 times wider than the Sun).
Betelgeuse vs. The Sun: A Size Comparison
Feature
Betelgeuse
Our Sun
Diameter
~1.4 billion km
~1.4 million km
Volume
~1 billion Suns
1 (baseline)
Mass
~17x Sun
1 Solar Mass
Luminosity
~100,000x Sun
1 (baseline)
4. The Sharpest Image Ever of Betelgeuse
ALMA’s Stunning View of a Dying Star
In 2017, ALMA (the Atacama Large Millimeter/submillimeter Array) snapped the most detailed image ever taken of Betelgeuse’s surface, revealing never-before-seen features on this giant star. What they saw was astonishing:
A lopsided, boiling blob – Unlike the Sun’s relatively smooth surface, Betelgeuse is covered with enormous convection cells—giant bubbles of hot gas that rise and fall, making its surface look lumpy and turbulent.
An unstable atmosphere – The star’s outer layers are pulsating and ejecting material, creating a vast, irregularly shaped envelope.
Why Does Betelgeuse Look So Weird?
It’s losing mass rapidly—shedding material equivalent to one Earth mass every year.
Giant magnetic fields warp its surface.
It’s not a perfect sphere—more like a wobbly, unstable ball of plasma.
5. When Will Betelgeuse Explode?
Could It Happen in Our Lifetime?
The truth is: nobody knows for sure.
Some astronomers suggest it could explode within the next 100,000 years.
Others think it might take longer.
Signs Betelgeuse Is Nearing Its End:
Rapid dimming episodes (like the “Great Dimming” of 2019–2020)
Increased mass loss (ejecting huge amounts of gas and dust)
Unstable pulsations (brightness fluctuations)
What Will We See When It Explodes?
When Betelgeuse finally goes supernova:
One day, Betelgeuse will go supernova and blaze in the sky as brightly as the full Moon—for several weeks!
It could be visible even during the day.
The explosion will leave behind a neutron star or black hole.
6. Why Are Scientists So Obsessed with Betelgeuse?
A Rare Chance to Study a Dying Supergiant Up Close
It’s the closest red supergiant to Earth, giving us a unique look at stellar death.
Helps us understand supernovae—key to the creation of heavy elements like gold and uranium.
Could reveal secrets about black holes and neutron stars.
Could a Betelgeuse Supernova Be Dangerous?
Fortunately, no. Even though Betelgeuse will go supernova, it’s 642 light-years away—far enough that its radiation won’t harm Earth. The only risk? A spectacular light show and a new nebula in Orion.
7. The Great Dimming of 2019-2020: What Really Happened?
A Star That Suddenly Faded
In late 2019, astronomers noticed something strange—Betelgeuse had dramatically dimmed, losing about two-thirds of its brightness. This event, dubbed “The Great Dimming,” sparked worldwide speculation:
Was Betelgeuse about to explode?
Was this a precursor to a supernova?
Or was something else entirely going on?
The Surprising Truth Revealed
Using the Hubble Space Telescope and other observatories, scientists discovered the dimming was caused by:
A massive dust cloud – Betelgeuse had ejected a huge plume of stellar material that cooled into dust, partially blocking its light.
Surface cooling – Simultaneously, a large convective cell caused a temporary temperature drop on one side of the star.
Key Takeaway: While fascinating, the Great Dimming was not a sign of an imminent supernova—just another example of Betelgeuse’s turbulent nature.
8. How Betelgeuse Compares to Other Famous Stars
Betelgeuse vs. Other Supergiants
While Betelgeuse is huge, it’s not the largest known star. Let’s compare it to other stellar giants:
Star
Type
Size (Solar Radii)
Distance (Light-Years)
Betelgeuse
Red Supergiant
~1,000x Sun
~642
UY Scuti
Red Hypergiant
~1,700x Sun
~9,500
VY Canis Majoris
Red Hypergiant
~1,420x Sun
~3,900
Stephenson 2-18
Red Supergiant
~2,150x Sun
~20,000
Fun Fact: If Stephenson 2-18 took the Sun’s place, its sheer size would swallow all the inner planets—and even stretch past Saturn’s orbit!
Why Betelgeuse Stands Out
The closest red supergiant to Earth is Betelgeuse, making it easier for astronomers to study its size, brightness changes, and life cycle in detail.
Brighter than most giants – Visible to the naked eye.