Abstract

The carbonaceous matrix of ureilite meteorites (C‐bearing olivine‐pigeonite achondrites) contain abundant minute phases that emit a multicolored fluorescence under electron bombardment. These phases include NaCl and KCl, found in all seven ureilites studied, high‐Si glass with pyroxene and chlorapatite quench crystals in North Haig, an unidentified high‐Ca‐Al‐Cl phase in Novo Urei, and possibly free SiO2 in Novo Urei and Dingo Pup Donga. The origin of these phases is uncertain but some, especially chlorides and glass, may represent residual postcumulus materials precipitated from a late‐stage interstitial liquid during the igneous phase of ureilite history.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.