CO 2 release due to impact devolatilization of carbonate: Results of shock experiments

• Published in: Meteoritics & Planetary Science
• Main Author: Bell, Mary Sue
• Other Authors: Jacobs and NASA's Planetary Geology and Geophysics Program
• Format: Article in Journal/Newspaper
• Language: English
• Published: Wiley 2016
• Subjects: Iceland
• Online Access: http://dx.doi.org/10.1111/maps.12613; https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fmaps.12613; https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.12613

Abstract A study of pure, single crystal calcite shocked to pressures from 9.0 to 60.8 GPa was conducted to address contradictory data for carbonate shock behavior. The recovered materials were analyzed optically and by transmission electron microscopy (TEM), as well as by thermogravimetry (TGA), X‐ray diffraction (XRD), and Raman‐spectroscopy. In thin section, progressive comminution of calcite is observed although grains remain birefringent to at least 60.8 GPa. TGA analysis reveals a positive correlation between percent of mass loss due to shock and increasing shock pressure ( R = 0.77) and suggests that shock loading leads to the modest removal of structural volatiles in this pressure range. XRD patterns of shocked Iceland spar samples produce peaks that are qualitatively and quantitatively less intense, more diffuse, and shift to lower o 2θ. However, the regularity observed in these shocked powder patterns suggests that structures with very uniform unit cell separations persist to shock pressures as high as 60.8 GPa. Raman spectral analyses indicate no band asymmetry and no systematic peak shifting or broadening. TEM micrographs display progressively diminishing crystallite domain sizes. Selected area electron diffraction (SAED) patterns reveal no signatures of amorphous material. These data show that essentially intact calcite is recovered at shock pressures up to 60.8 GPa with only slight mass loss (~7%). This work suggests that the amount of CO 2 gas derived from shock devolatilization of carbonate by large meteorite impacts into carbonate targets has been (substantially) overestimated.