New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs

We present observations and analyses of eight white dwarf stars (WDs) that have accreted rocky material from their surrounding planetary systems. The spectra of these helium-atmosphere WDs contain detectable optical lines of all four major rock-forming elements (O, Mg, Si, and Fe). This work increases the sample of oxygen-bearing WDs with parent body composition analyses by roughly 33%. To first order, the parent bodies that have been accreted by the eight WDs are similar to those of chondritic meteorites in relative elemental abundances and oxidation states. Seventy-five percent of the WDs in this study have observed oxygen excesses implying volatiles in the parent bodies with abundances similar to those of chondritic meteorites. Three WDs have oxidation states that imply more reduced material than found in CI chondrites, indicating the possible detection of Mercury-like parent bodies, but are less constrained. These results contribute to the recurring conclusion that extrasolar rocky bodies closely resemble those in our solar system, and do not, as a whole, yield unusual or unique compositions.

Automated summary

We present observations and analyses of eight white dwarf stars that have accreted rocky material from planetary systems. The spectra of these stars contain detectable optical lines of major rock-forming elements. The composition of the accreted material is similar to that of chondritic meteorites. These results support the conclusion that extrasolar rocky bodies resemble those in our solar system.