We discuss a new class of exoplanets that appear to be emitting a tail of dusty effluents. These disintegrating planets are found close to their host stars and have very hot, and likely molten, surfaces. The properties of the dust should provide a direct probe of the constituent material of these rocky bodies.
CITATION STYLE
Lieshout, R. van, & Rappaport, S. (2018). Disintegrating Rocky Exoplanets. In Handbook of Exoplanets (pp. 1–19). Springer International Publishing. https://doi.org/10.1007/978-3-319-30648-3_15-2
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