Characterizing the Chemistry of Planetary Materials Around White Dwarf Stars
arXiv:1707.03064 · doi:10.1007/978-3-319-55333-7_14
Abstract
Planetary systems that orbit white dwarf stars can be studied via spectroscopic observations of the stars themselves. Numerous white dwarfs are seen to have accreted mostly rocky minor planets, the remnants of which are present in the stellar photospheres. The elemental abundances in the photospheres unveil the bulk compositions of the accreted parent bodies with a precision far greater than can be attained with any other technique currently available to astronomers. The most significant discovery, overall, is that rocky extrasolar planets have bulk elemental compositions similar to those of Earth and other rocky objects in our solar system. The white dwarf studies reveal that many extrasolar minor planets (asteroids) are differentiated, possessing analogs of terrestrial crust, mantle and core; this finding has important implications for the origin of our own solar system.
Updated and improved version of an invited review to appear in 'Handbook of Exoplanets,' Springer Reference Works, Juan Antonio Belmonte and Hans Deeg, Eds
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