Astronomers have found four nearby white dwarf stars surrounded by disks of material that could be the remains of rocky planets much like Earth — and one star in particular appears to be in the act of swallowing up what’s left of an Earthlike planet’s core.
The research, announced on Thursday by the Royal Astronomical Society, gives a chilling look at the eventual fate that may await our own planet.
Astronomers from the University of Warwick used Hubble to identify the composition of four white dwarfs’ atmospheres, found during a survey of more than 80 such stars located within 100 light-years of the sun. What they found was a majority of the material was composed of elements found in our own solar system: oxygen, magnesium, silicon and iron. Together these elements make up 93 percent of our planet.
In addition, a curiously low ratio of carbon was identified, indicating that rocky planets were at one time in orbit around the stars.
Since white dwarfs are the leftover cores of stellar-mass stars that have burnt through all their fuel, the material in their atmosphere is likely the leftover bits of planets. These worlds may have once been held in safe, stable orbits. But when their stars neared the ends of their lives, the stars may have expanded, possibly engulfing the innermost planets and disrupting the orbits of others. This could have triggering a runaway collision effect that eventually shattered all the planets, forming an orbiting cloud of debris.
This could very well be what will happens to our solar system in 4 billion or 5 billion years.
“What we are seeing today in these white dwarfs several hundred light years away could well be a snapshot of the very distant future of the Earth,” said Professor Boris Gänsicke of the Department of Physics at the University of Warwick, who led the study. "During the transformation of the sun into a white dwarf, it will lose a large amount of mass, and all the planets will move further out. This may destabilize the orbits and lead to collisions between planetary bodies as happened in the unstable early days of our solar systems."
One of the white dwarfs studied, labeled PG0843+516, may be in the midst of eating the remains of an once-Earthlike world’s core.
The researchers identified an abundance of heavier elements such as iron, nickel and sulfur in the atmosphere surrounding PG0843+516. These elements are found in the cores of terrestrial planets, having sunk into their interiors during the early stages of planetary formation. Finding them out in the open attests to the destruction of a rocky world like ours.
Of course, being heavier elements, they will be the first to be accreted by their star.
“It is entirely feasible that in PG0843+516 we see the accretion of such fragments made from the core material of what was once a terrestrial exoplanet,” Gänsicke said.
It’s an eerie look into a distant future, when Earth and the inner planets could become just some elements in a cloud.
Jason Major is a graphic designer living in Dallas. He writes about astronomy and space exploration on Universe Today and also on his blog , Discovery News and National Geographic News. This report was originally published on Universe Today as