Planetary Debris Disk Detected around White Dwarf-Brown Dwarf System
Evidence of planetary debris surrounding a white dwarf and its substellar companion has been found by a University College London-led international team of astronomers. The discovery is remarkable because the debris appears to be rocky and suggests that terrestrial planets might exist in this exotic system.

A disc of rocky debris from a disrupted planetesimal surrounds the white dwarf-brown dwarf binary system SDSS 1557. Image credit: Mark Garlick, University College London, University of Warwick and University of Sheffield.
The binary system in question is called SDSS J155720.77+091624.6 (hereafter SDSS 1557).
It is 1,592 light-years away from Earth and consists of a low-mass white dwarf (0.45 solar masses) and a brown dwarf (66 Jupiter’s masses).
To date, all exoplanets discovered in orbit around binary stars are gas giants and are thought to form in the icy regions of their systems.
In contrast to the carbon-rich icy material found in other binaries, the planetary material identified in SDSS 1557 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 white dwarf, polluting it temporarily with at least 1017 g (or 1.1 trillion US tons) of matter, equating it to an asteroid at least 4 km in size.
“Building rocky planets around two suns is a challenge because the gravity of both stars can push and pull tremendously, preventing bits of rock and dust from sticking together and growing into full-fledged planets,” said lead author Dr. Jay Farihi, a researcher in the Department of Physics and Astronomy at the University College London.








