How will the solar system die? It’s a hugely important question that researchers have speculated a lot about, using our knowledge of physics to create complex theoretical models. We know that the sun will eventually become a “white dwarf,” a burnt stellar remnant whose dim light gradually fades into darkness. This transformation will involve a violent process that will destroy an unknown number of its planets. So which planets will survive the death of the sun? One way to seek the answer is to look at the fates of other similar planetary systems. This has proven difficult, however. The feeble radiation from white dwarfs makes it difficult to spot exoplanets (planets around stars other than our sun) which have survived this stellar transformation; they are literally in the dark. In fact, of the over 4,500 exoplanets that are currently known, just a handful have been found around white dwarfs, and the location of these planets suggests they arrived there after the death of the star. This lack of data paints an incomplete picture of our own planetary fate. Fortunately, we are now filling in the gaps. In our new paper, published in Nature, we report the discovery of the first known exoplanet to survive the death of its star without having its orbit altered by other planets moving around, circling a distance comparable to those between the sun and the solar system planets. A Jupiter-Like Planet This new exoplanet, which we discovered with the Keck Observatory in Hawaii, is particularly similar to Jupiter in both mass and orbital separation, and provides us with a crucial snapshot into planetary survivors around dying stars. A star’s transformation into a white dwarf involves a violent phase in which it becomes a bloated “red giant,” also known as a “giant branch” star, hundreds of times bigger than before. We believe that this exoplanet only just survived; if it was initially closer to its parent star, it would have been engulfed by the star’s expansion. When the sun eventually becomes a red giant, its radius will actually reach outwards to Earth’s current orbit. That means the sun will (probably) engulf Mercury and Venus, and possibly the Earth, but we are not sure. Jupiter, and its moons, have been expected to survive, although we previously didn’t know for sure. But with our discovery of this new exoplanet, we can now be more certain that Jupiter really will make it. Moreover, the margin of error in the position of this exoplanet could mean that it is almost half as close to the white dwarf as Jupiter currently is to the sun. If so, that is additional evidence for assuming that Jupiter and Mars will make it. So could any life survive this transformation? A white dwarf could power life on moons or planets that end up being very close to it (about one-tenth the distance between the sun and Mercury) for the first few billion years. After that, there wouldn’t be enough radiation to sustain anything. Asteroids and White Dwarfs Although planets orbiting white dwarfs have been difficult to find, what has been much easier to detect are asteroids breaking up close to the white dwarf’s surface. For exoasteroids to get so close to a white dwarf, they need to have enough momentum imparted to them by surviving exoplanets. Hence, exoasteroids have been long assumed to be evidence that exoplanets are there too. Our discovery finally provides confirmation of this. Although in the system being discussed in the paper, current technology does not allow us to see any exoasteroids, at least now we can piece together different parts of the puzzle of planetary fate by merging the evidence from different white dwarf systems. The link between exoasteroids and exoplanets also applies to our own solar system. Individual objects in the asteroid main belt and Kuiper belt (a disc in the outer solar system) are likely to survive the sun’s demise, but some will be moved by gravity by one of the surviving planets towards the white dwarf’s surface. Future Dis...