Presentation #500.04 in the session Plenary 7.
We have recently made the first direct detection of planetary material accreting onto a white dwarf using X-ray observations. This discovery, recently published in Nature, confirms G29–38 — the prototype of all metal-polluted white dwarfs with detected debris disks — as a significant source of soft X-rays. Our detection relied upon a 106 ks exposure with the Chandra X-ray Observatory and provides the first direct evidence of ongoing accretion of planetary material onto a white dwarf. From the measured low-energy X-ray emission and modelled X-ray luminosity, we provide the first independent constraint on the accretion rate at such a system, finding an instantaneous accretion rate consistent with modelling of observed photospheric abundances. We measure a relatively low plasma temperature of kT ≈ 0.5 keV, corroborating the predicted bombardment solution for white dwarfs accreting at low accretion rates. I will present this recent discovery and its implications for the study of evolved planetary systems, including the accretion rates and bulk elemental compositions.