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How will the universe end?

How will the universe end?

  • The universe will likely continue to exist for billions of years, but its future is uncertain and subject to change.
  • In a few billion years, the Milky Way and Andromeda galaxies might collide, resulting in a spectacular view for future observers.
  • Star formation will eventually shut down, leading to galaxies filled with old, red, dim stars that will gradually cool into darkness over trillions of years.
  • The universe’s expansion is expected to continue, potentially making it impossible to observe other galaxies beyond the local group in trillions of years.
  • Despite the uncertainty and potential for dramatic changes, scientists believe that humanity has plenty of time to explore and search for answers about the universe’s future, with billions of years of cosmic evolution ahead.

In a few billion years, the Milky Way and Andromeda, the nearest spiral galaxy, might collide. Future observers could be treated to fantastic views. NASA; ESA; Z. Levay and R. van der Marel, STScI; T. Hallas; and A. Mellinger

Curious Kids is a series for children of all ages. If you have a question you’d like an expert to answer, send it to CuriousKidsUS@theconversation.com.


How will the universe end? – Iez M., age 9, Rochester, New York


Whether the universe will “end” at all is not certain, but all evidence suggests it will continue being humanity’s cosmic home for a very, very long time.

The universe – all of space and time, and all matter and energy – began about 14 billion years ago in a rapid expansion called the Big Bang, but since then it has been in a state of continuous change. First, it was full of a diffuse gas of the particles that now make up atoms: protons, neutrons and electrons. Then, that gas collapsed into stars and galaxies.

A graphic timeline of the history of the universe, from the Big Bang on the left to accelerated expansion today on the right.

Our current theory for the history of the universe. On the left is the Big Bang roughly 14 billion years ago. The structure and makeup of the universe have changed over time.
NASA/WMAP Science Team

Our understanding of the future of the universe is informed by the objects and processes we observe today. As an astrophysicist, I observe objects like distant galaxies, which lets me study how stars and galaxies change over time. By doing so, I develop theories that predict how the universe will change in the future.

Predicting the future by studying the past?

Predicting the future of the universe by extending what we see today is extrapolation. It’s risky, because something unexpected could happen.

Interpolation – connecting the dots within a dataset – is much safer. Imagine you have a picture of yourself when you were 5 years old, and then another when you were 7 years old. Someone could probably guess what you looked like when you were 6. That’s interpolation.

A picture explaining interpolation vs extrapolation using pictures of the author at different ages

Using a picture of the author when he was 5 years old and 7 years old, you could interpolate what he looked like when he was 6 years old, but you couldn’t predict what he would look like at 29.
Stephen DiKerby

Maybe they could extrapolate from the two pictures to what you’d look like when you are 8 or 9 years old, but no one can accurately predict too far into the future. Maybe in a few years you get glasses or suddenly get really tall.

Scientists can predict what the universe will probably look like a few billion years into the future by extrapolating how stars and galaxies change over time, but eventually things could get weird. The universe and the stuff within might once again change, like it has in the past.

How will stars change in the future?

Good news: The Sun, our medium-sized yellow star, is going to continue shining for billions of years. It’s about halfway through its 10 billion-year lifetime. The lifetime of a star depends on its size. Big, hot, blue stars live shorter lives, while tiny, cool, red stars live for much longer.

Today, some galaxies are still producing new stars, but others have depleted their star-forming gas. When a galaxy stops forming stars, the blue stars quickly go “supernova” and disappear, exploding after only a few million years. Then, billions of years later, the yellow stars like the Sun eject their outer layers into a nebula, leaving only the red stars puttering along. Eventually, all galaxies throughout the universe will stop producing new stars, and the starlight filling the universe will gradually redden and dim.

An illustration of a red dwarf star and a nearby planet

Red dwarf stars are the longest-lived type of stars. Once star formation shuts down throughout the universe, eventually only red stars will be left, gradually fading away over trillions of years.
NASA/ESA/STScI/G. Bacon

In trillions of years – hundreds of times longer than the universe’s current age – these red stars will also fade away into darkness. But until then, there will be lots of stars providing light and warmth.

How will galaxies change in the future?

Think of building a sand castle on the beach. Each bucket of sand makes the castle bigger and bigger. Galaxies grow over time in a similar way by eating up smaller galaxies. These galactic mergers will continue into the future.

In galaxy clusters, hundreds of galaxies fall inward toward their shared center, often resulting in messy collisions. In these mergers, spiral galaxies, which are orderly disks, combine in chaotic ways into disordered blob-shaped clouds of stars. Think of how easy it is to turn a well-constructed sand castle into a big mess by kicking it over.

For this reason, the universe over time will have fewer spiral galaxies and more elliptical galaxies because the spiral galaxies combine into elliptical galaxies.

The Milky Way galaxy and the neighboring Andromeda galaxy might combine in this way in a few billion years. Don’t worry: The stars in each galaxy would whiz past each other totally unharmed, and future stargazers would get a fantastic view of the two galaxies merging.

How will the universe itself change in the future?

The Big Bang kick-started an expansion that probably will continue in the future. The gravity of all the stuff in the universe – stars, galaxies, gas, dark matter – pulls inward and slows down the expansion, and some theories suggest that the universe’s expansion will coast along or slow to a halt.

However, some evidence suggests that some unknown force is starting to exert a repulsive force, causing expansion to speed up. Scientists call this outward force dark energy, but very little is known about it. Like raisins in a baking cookie, galaxies will zoom away from each other faster and faster. If this continues into the future, other galaxies might be too far apart to observe from the Milky Way.

A simulated view of the night sky from a planet in a huge elliptical galaxy

After star formation shuts down and galaxies merge into huge ellipticals, the expansion of the universe might mean that other galaxies are impossible to observe. For trillions of years, this might be the view of the unchanging night sky: a single red elliptical galaxy.
NASA; ESA; Z. Levay and R. van der Marel, STScI; T. Hallas; and A. Mellinger

To summarize the best current prediction of the future: Star formation will shut down, so galaxies will be full of old, red, dim stars gradually cooling into darkness. Each group or cluster of galaxies will merge into a single, massive, elliptical galaxy. The accelerated expansion of the universe will make it impossible to observe other galaxies beyond the local group.

This scenario eventually winds down into a dark eternity, lasting trillions of years. New data might come to light that changes this story, and the next stage in the universe’s history might be something totally different and unexpectedly beautiful. Depending on how you look at it, the universe might not have an “end,” after all. Even if what exists is very different from how the universe is now, it’s hard to envision a distant future where the universe is entirely gone.

How does this scenario make you feel? It sometimes makes me feel wistful, which is a type of sadness, but then I remember we live at a very exciting time in the story of the universe: right at the start, in an era full of exciting stars and galaxies to observe! The cosmos can support human society and curiosity for billions of years into the future, so there’s lots of time to keep exploring and searching for answers.


Hello, curious kids! Do you have a question you’d like an expert to answer? Ask an adult to send your question to CuriousKidsUS@theconversation.com. Please tell us your name, age and the city where you live.

And since curiosity has no age limit – adults, let us know what you’re wondering, too. We won’t be able to answer every question, but we will do our best.

The Conversation

Stephen DiKerby receives funding from the National Science Foundation.

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Q. How will the universe end?
A. The universe’s fate is not certain, but all evidence suggests it will continue being humanity’s cosmic home for a very long time.

Q. What is the Big Bang and how did it affect the universe?
A. The Big Bang was a rapid expansion that occurred about 14 billion years ago, marking the beginning of the universe as we know it today.

Q. How do scientists predict the future of the universe?
A. Scientists use extrapolation to predict the future by studying the past, but they acknowledge that there is always a risk of unexpected events occurring.

Q. What will happen to stars in the future?
A. The Sun, our medium-sized yellow star, will continue shining for billions of years, while other stars like red dwarfs will live for trillions of years before fading away into darkness.

Q. How will galaxies change in the future?
A. Galaxies will grow and merge with each other over time, eventually forming a single massive elliptical galaxy, which may make it impossible to observe other galaxies beyond the local group.

Q. What is dark energy and how does it affect the universe?
A. Dark energy is an unknown force that causes expansion to speed up, potentially making it impossible to observe other galaxies beyond the local group in trillions of years.

Q. Will the universe have an “end”?
A. Depending on how one looks at it, the universe might not have an “end,” as new data could change our understanding of its future, and there may be a distant future where the universe is entirely different from what we know today.

Q. How will the Milky Way and Andromeda galaxies collide in the future?
A. The two galaxies are expected to collide in a few billion years, resulting in a spectacular view for future stargazers as their stars whiz past each other unharmed.

Q. What is the current understanding of the universe’s fate?
A. Based on current predictions, star formation will shut down, galaxies will be full of old, red, dim stars gradually cooling into darkness, and the expansion of the universe may make it impossible to observe other galaxies beyond the local group.

Q. Why should we feel hopeful about the future of the universe?
A. Despite the uncertainty of the universe’s fate, there is still plenty of time for human society and curiosity to thrive, making the present moment an exciting time in the story of the universe.