How will our Sun look after it dies? Scientists have made predictions about what the final days of our Solar System will look like, and when it will happen. And we humans won't be around to see the Sun's curtain call.
Previously, astronomers thought the Sun would turn into a planetary nebula – a luminous bubble of gas and cosmic dust – until evidence suggested it would have to be a smidge more massive.
An international team of astronomers flipped it again in 2018 and found that a planetary nebula is indeed the most likely solar corpse.
The Sun is about 4.6 billion years old – gauged on the age of other objects in the Solar System that formed around the same time. Based on observations of other stars, astronomers predict it will reach the end of its life in about another 10 billion years.
There are other things that will happen along the way, of course. In about 5 billion years, the Sun is due to turn into a red giant. The core of the star will shrink, but its outer layers will expand out to the orbit of Mars, engulfing our planet in the process. If it's even still there.
One thing is certain: By that time, we won't be around. In fact, humanity only has about 1 billion years left unless we find a way off this rock. That's because the Sun is increasing in brightness by about 10 percent every billion years.
That doesn't sound like much, but that increase in brightness will end life on Earth. Our oceans will evaporate, and the surface will become too hot for water to form. We'll be about as kaput as you can get.
It's what comes after the red giant that has proven difficult to pin down. Several previous studies have found that, in order for a bright planetary nebula to form, the initial star needs to have been up to twice as massive as the Sun.
However, the 2018 study used computer modeling to determine that, like 90 percent of other stars, our Sun is most likely to shrink down from a red giant to become a white dwarf and then end as a planetary nebula.
"When a star dies it ejects a mass of gas and dust – known as its envelope – into space. The envelope can be as much as half the star's mass. This reveals the star's core, which by this point in the star's life is running out of fuel, eventually turning off and before finally dying," explained astrophysicist Albert Zijlstra from the University of Manchester in the UK, one of the authors of the paper.
"It is only then the hot core makes the ejected envelope shine brightly for around 10,000 years – a brief period in astronomy. This is what makes the planetary nebula visible. Some are so bright that they can be seen from extremely large distances measuring tens of millions of light years, where the star itself would have been much too faint to see."
The data model that the team created actually predicts the life cycle of different kinds of stars, to figure out the brightness of the planetary nebula associated with different star masses.
Planetary nebulae are relatively common throughout the observable Universe, with famous ones including the Helix Nebula, the Cat's Eye Nebula, the Ring Nebula, and the Bubble Nebula.
They're named planetary nebulae not because they actually have anything to do with planets, but because, when the first ones were discovered by William Herschel in the late 18th century, they were similar in appearance to planets through the telescopes of the time.
Almost 30 years ago, astronomers noticed something peculiar: The brightest planetary nebulae in other galaxies all have about the same level of brightness. This means that, theoretically at least, by looking at the planetary nebulae in other galaxies, astronomers can calculate how far away they are.
The data showed that this was correct, but the models contradicted it, which has been vexing scientists ever since the discovery was made.
"Old, low mass stars should make much fainter planetary nebulae than young, more massive stars. This has become a source of conflict for the past 25 years," said Zijlstra
"The data said you could get bright planetary nebulae from low mass stars like the Sun, the models said that was not possible, anything less than about twice the mass of the Sun would give a planetary nebula too faint to see."
The 2018 models have solved this problem by showing that the Sun is about the lower limit of mass for a star that can produce a visible nebula.
Even a star with a mass less than 1.1 times that of the Sun won't produce a visible nebula. Bigger stars up to 3 times more massive than the Sun, on the other hand, will produce the brighter nebulae.
For all the other stars in between, the predicted brightness is very close to what has been observed.
"This is a nice result," Zijlstra said. "Not only do we now have a way to measure the presence of stars of ages a few billion years in distant galaxies, which is a range that is remarkably difficult to measure, we even have found out what the Sun will do when it dies!"
The research was published in the journal Nature Astronomy.
An earlier version of this article was first published in May 2018.