Astronomen haben die ältesten Planetentrümmer in unserer Galaxie entdeckt – die Überreste des zerstörten Sonnensystems

Künstlerische Darstellung der alten Weißen Zwerge WDJ2147-4035 und WDJ1922+0233, umgeben von umkreisenden Planetentrümmern, die sich auf den Sternen ansammeln und ihre Atmosphäre verschmutzen würden. WDJ2147-4035 ist rot und sehr dunkel, während WDJ1922 + 0233 ungewöhnlich blau ist. Bildnachweis: University of Warwick/Dr. Markus Knoblauch

• Neue Studie stellt ein langweiliges Leben[{“ attribute=““>white dwarf star of over ten billion years
• Engulfed remains of recently orbiting planetesimals make this the oldest dead star with an evolved planetary system
• Provides insight into the formation and evolution of asteroids, icy moons, and Earth-like rocky planets in the early history of the universe

Astronomers have identified the oldest star in our galaxy that is accreting debris from orbiting planetesimals, making it one of the oldest rocky and icy planetary systems ever discovered in the Milky Way.

Their findings conclude that a faint white dwarf located just 90 light-years from Earth, as well as the remains of its orbiting planetary system, are over ten billion years old. Led by the University of Warwick, the study was published on November 5 in the Monthly Notices of the Royal Astronomical Society.

Most stars, including those like our Sun, will eventually turn into white dwarfs. A white dwarf is a star that has used up all of its fuel, lost its outer layers, and is now undergoing a process of contracting and cooling. Any planets in orbit will be disrupted and, in some circumstances, destroyed during this process, and their debris will be left behind to accrete onto the surface of the white dwarf.

For this study, the team of astronomers modeled two unusual white dwarfs that were detected by the GAIA space observatory of the European Space Agency. Both stars are polluted by planetary debris. One of them was found to be unusually blue, while the other is the faintest and reddest found to date in the local galactic neighborhood. Both were subjected to further analysis by the team of scientists.

The astronomers used spectroscopic and photometric data from GAIA, the Dark Energy Survey, and the X-Shooter instrument at the European Southern Observatory to calculate how long the stars have been cooling for. They found that the ‘red’ star WDJ2147-4035 is around 10.7 billion years old, of which 10.2 billion years have been spent cooling as a white dwarf.

Spectroscopy involves analyzing the light from the star at different wavelengths. This can detect when elements in the star’s atmosphere are absorbing light at different colors and helps determine what elements those are and how much is present. By analyzing the spectrum from WDJ2147-4035, the team found the presence of the metals sodium, lithium, and potassium and tentatively detected carbon accreting onto the star – making this the oldest metal-polluted white dwarf discovered so far.

The second ‘blue’ star WDJ1922+0233 is only slightly younger than WDJ2147-4035 and was polluted by planetary debris of a similar composition to the Earth’s continental crust. The science team concluded that the blue color of WDJ1922+0233, despite its cool surface temperature, is caused by its unusual mixed helium-hydrogen atmosphere.

The debris found in the otherwise nearly pure-helium and high-gravity atmosphere of the red star WDJ2147-4035 are from an old planetary system that survived the evolution of the star into a white dwarf, leading the astronomers to conclude that this is the oldest planetary system around a white dwarf discovered in the Milky Way.

Lead author Abbigail Elms, a PhD student in the University of Warwick Department of Physics, said: “These metal-polluted stars show that Earth isn’t unique, there are other planetary systems out there with planetary bodies similar to the Earth. 97% of all stars will become a white dwarf and they’re so ubiquitous around the universe that they are very important to understand, especially these extremely cool ones. Formed from the oldest stars in our galaxy, cool white dwarfs provide information on the formation and evolution of planetary systems around the oldest stars in the Milky Way.”

“We’re finding the oldest stellar remnants in the Milky Way that are polluted by once Earth-like planets. It’s amazing to think that this happened on the scale of ten billion years, and that those planets died way before the Earth was even formed.”

Astronomers can also use the star’s spectra to determine how quickly those metals are sinking into the star’s core, which allows them to look back in time and determine how abundant each of those metals was in the original planetary body. By comparing those abundances to astronomical bodies and planetary material found in our own solar system, we can guess at what those planets would have been like before the star died and became a white dwarf – but in the case of WDJ2147-4035, that has proven challenging.

Abbigail explains: “The red star WDJ2147-4035 is a mystery as the accreted planetary debris are very lithium and potassium-rich and unlike anything known in our own solar system. This is a very interesting white dwarf as its ultra-cool surface temperature, the metals polluting it, its old age, and the fact that it is magnetic, makes it extremely rare.”

Professor Pier-Emmanuel Tremblay of the Department of Physics at the University of Warwick said: “When these old stars formed more than 10 billion years ago, the universe was less metal-rich than it is now, since metals are formed in evolved stars and gigantic stellar explosions. The two observed white dwarfs provide an exciting window into planetary formation in a metal-poor and gas-rich environment that was different to the conditions when the solar system was formed.”

Reference: “Spectral analysis of ultra-cool white dwarfs polluted by planetary debris” by Abbigail K Elms, Pier-Emmanuel Tremblay, Boris T Gänsicke, Detlev Koester, Mark A Hollands, Nicola Pietro Gentile Fusillo, Tim Cunningham and Kevin Apps, 5 November 2022, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac2908

This research received funding from the European Research Council under the European Union’s Horizon 2020 research and innovation program, the Leverhulme Trust Grant and the UK STFC consolidated grant.