How Long Will the Sun Continue to Burn

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Will our solar system survive the death of our sun?

An artist's depiction of the solar system as it appears today. (Image credit: NASA/Goddard Space Flight Center Conceptual Image Lab)

Our sun's death is a long way off — about 4.5 billion years, give or take — but someday it's going to happen, and what then for our solar system?

The trouble begins before the death proper: The first thing we have to contend with is the elderly sun itself. As the fusion of hydrogen continues inside the sun, the result of that reaction — helium — builds up in the core.

The ageing sun

With all the waste product hanging around, it gets harder for the sun to do its fusion dance. But the inward crushing weight of the sun's atmosphere doesn't change, so to maintain balance the sun has to increase the temperature of its fusion reactions, leading ironically to a hotter core.

This means that as the sun ages, it gets steadily brighter. The dinosaurs knew a dimmer sun than we see today, and in as little as a few hundred million years, Earth will get too hot to handle.

Our atmosphere will get stripped away. Our oceans will evaporate. For awhile, we'll look something like Venus, locked in a choking, carbon dioxide atmosphere.

And then it gets worse.

Related: 25 weird and wild solar system facts

The red giant

In the final stages of hydrogen fusion, our sun will swell and swell, becoming distorted and bloated — and red. The red giant sun will consume Mercury and Venus for sure. It might or might not spare Earth, depending on exactly how large it gets. If the sun's distended atmosphere does reach our world, Earth will dissolve in less than a day.

But even if the sun's expansion stops short, it won't be pretty for Earth. The extreme energies emitted by the sun will be intense enough to vaporize rocks, leaving behind nothing more than the dense iron core of our planet.

The outer planets won't enjoy the increased radiation output from the sun either. The rings of Saturn are made of almost pure water ice, and the future sun will simply be too hot for them to survive. The same goes for the ice-locked worlds orbiting those giants. Europa, Enceladus, and all the rest will lose their icy shells.

At first, the increased radiation will blast the four outer planets, stripping away their atmospheres, which are just as fragile as that of a terrestrial planet. But as the sun continues to swell, some of the outer tendrils of its atmosphere can find their way to the giants, traveling through funnels of gravity. Feeding on that material, the outer planets can gorge themselves, becoming far larger than they ever were before.

But the sun still won't be done. In its final stages, it will repeatedly swell and contract, pulsing for millions of years. This isn't the most stable situation, gravitationally speaking. The deranged sun will push and pull the outer planets in odd directions, potentially drawing them into a deadly embrace or kicking them entirely out of the system.

Can life survive sun's end?

For a few hundred million years, the outermost parts of our solar system will be a decent place to call home. With so much heat and radiation pouring from the red giant sun, the habitable zone — the region around a star where the temperatures are just right for liquid water — will shift outward.

As we saw above, at first the moons of the outer worlds will melt, losing their icy shells and potentially hosting liquid water oceans on their surfaces. Eventually, the Kuiper belt objects, including Pluto and its mysterious friends, will also lose their ices. The largest may transform into mini-Earths orbiting a distant, distorted red sun.

But eventually, our sun will give up the struggle, shrugging off its outer atmosphere in a series of outbursts that leave behind the star's core: a white-hot lump of carbon and oxygen.

This white dwarf will initially be staggeringly hot, blasting off X-ray radiation that can do brutal damage to life as we know it. But within a billion years or so, the white dwarf will settle down to more manageable temperatures and simply hang out for trillions upon trillions of years.

That dim white dwarf will host a new habitable zone, but because the former sun will be so cool, that zone would be incredibly close, much closer than Mercury orbits our sun today.

At that distance, any planet (or planetary core) would be vulnerable to tidal disruption — a pretty way of saying the gravity of the white dwarf could inadvertently rip a planet to shreds.

But that may be the best we'll get.

First evidence of a planet surviving a star's death

In October 2021, astronomers discovered the first-ever planet orbiting a white dwarf. The discovery, the scientists said, provides a glimpse into the possible future of the solar system.

The newfound planet is a gas giant about 40% larger than Jupiter, orbiting a dead star some 6,500 light-years away from Earth towards the center of our galaxy, the Milky Way.

Scientists don't know much about the planet, not even its distance from the star. The planet was discovered accidentally, during a "gravitational microlensing" event in 2010.

Gravitational microlensing occurs when two stars at different distances from Earth temporarily align from our perspective. The gravity of the star in the foreground acts like a lens and magnifies the light from the background star. If a planet orbits the foreground star, the magnified light briefly warps as the planet whizzes in front of the star.

"To detect an object through gravitational microlensing, you are only depending on the mass of the object; you don't need any light coming from it," Jean-Philippe Beaulieu, professor of astrophysics at the University of Tasmania in Australia and director of the Institute of Astrophysics in Paris, told Space.com. "We could see that there was an object about half the mass of the sun with a Jupiter-mass planet orbiting."

It was only during subsequent observations with one of the W. M. Keck telescopes in Hawaii that astronomers realized the star in the background was so dim it had to be a white dwarf.

Additional resources

Learn more by listening to the episode "Can planets survive the death of their star?" on the Ask A Spaceman podcast, available on iTunes (opens in new tab) and on the Web at http://www.askaspaceman.com.

Bibliography

Blackman, J.W. et al. A Jovian analogue orbiting a white dwarf star, Nature, October 13, 2021

https://www.nature.com/articles/s41586-021-03869-6

NASA, NASA Missions Spy First Possible 'Survivor' Planet Hugging White Dwarf Star, September 16, 2020

https://www.nasa.gov/press-release/nasa-missions-spy-first-possible-survivor-planet-hugging-white-dwarf-star

Join our Space Forums to keep talking space on the latest missions, night sky and more! And if you have a news tip, correction or comment, let us know at: community@space.com.

Paul M. Sutter is an astrophysicist at SUNY Stony Brook and the Flatiron Institute in New York City. Paul received his PhD in Physics from the University of Illinois at Urbana-Champaign in 2011, and spent three years at the Paris Institute of Astrophysics, followed by a research fellowship in Trieste, Italy, His research focuses on many diverse topics, from the emptiest regions of the universe to the earliest moments of the Big Bang to the hunt for the first stars. As an "Agent to the Stars," Paul has passionately engaged the public in science outreach for several years. He is the host of the popular "Ask a Spaceman!" podcast, author of "Your Place in the Universe" and "How to Die in Space" and he frequently appears on TV — including on The Weather Channel, for which he serves as Official Space Specialist.

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Source: https://www.space.com/solar-system-fate-when-sun-dies

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