 Lead author of the study, Dr. Jay Farihi from UCL's Department of Physics and Astronomy, said: "With the discovery of asteroid debris in the SDSS 1557 system, we see clear signatures of rocky planet assembly via large asteroids that formed, helping us understand how rocky exoplanets are made in double star systems." (illustration only) |
Evidence of planetary debris surrounding a double sun in a Star Wars-like system has been found by a team of researchers including scientists from the University of Sheffield.
The study, published in the journal Nature Astronomy, has found the remains of shattered asteroids orbiting a double sun consisting of a white dwarf star and a brown dwarf star roughly 1,000 light-years away in a system called SDSS 1557.
The debris appears to be rocky and suggesting that terrestrial planets, such as Tatooine, the home planet of Luke Skywalker in the film series Star Wars, might exist in the system.
To date, all exoplanets discovered in orbit around double stars are gas giants, similar to Jupiter, and are thought to form in the icy regions of their systems.
In contrast to the carbon-rich icy material found in other double star systems, the planetary material identified in the SDSS 1557 system has a high metal content, including silicon and magnesium.
These elements were identified as the debris flowed from its orbit onto the surface of the star, polluting it temporarily with at least 10^17 g (or 1.1 trillion US tons) of matter, equating it to an asteroid at least 4 km in size.
The discovery came as a complete surprise, as the team assumed the dusty white dwarf was a single star, but co-author Dr. Steven Parsons from the University of Sheffield, who is an expert in double star (or binary) systems and co-author of the study, noticed the telltale signs.
"We know of thousands of binaries similar to SDSS 1557 but this is the first time we've seen asteroid debris and pollution.
"The brown dwarf was effectively hidden by the dust until we looked with the right instrument but when we observed SDSS 1557 in detail we recognised the brown dwarf's subtle gravitational pull on the white dwarf."
Lead author of the study, Dr. Jay Farihi from UCL's Department of Physics and Astronomy, said: "With the discovery of asteroid debris in the SDSS 1557 system, we see clear signatures of rocky planet assembly via large asteroids that formed, helping us understand how rocky exoplanets are made in double star systems."
In the solar system, the asteroid belt contains the leftover building blocks for the terrestrial planets Mercury, Venus, Earth, and Mars, so planetary scientists study the asteroids to gain a better understanding of how rocky, and potentially habitable planets are formed. The same approach was used by the team to study the SDSS 1557 system as any planets within it cannot yet be detected directly, but the debris is spread in a large belt around the double stars, which is a much larger target for analysis.
The team studied the binary system and the chemical composition of the debris by measuring the absorption of different wavelengths of light or 'spectra,' using the Gemini Observatory South telescope and the European Southern Observatory Very Large Telescope, both located in Chile.
Co-author Professor Boris Gansicke from the University of Warwick analysed these data and found they all told a consistent and compelling story. "Any metals we see in the white dwarf will disappear within a few weeks, and sink down into the interior, unless the debris is continuously flowing onto the star.
"We'll be looking at SDSS 1557 next with Hubble, to conclusively show the dust is made of rock rather than ice."
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Prediction: More gas-giants will be found orbiting Sun-like stars
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