Cosmochemistry Group

Articles that made the journal cover

 

MAPS 1998

 

 

 

Meteoritics and Planetary Science

January 1998.  Vol. 33, no. 1.

Cover: A cathodoluminescence photomosaic of a thin section of Apollo 14 lunar highland regolith breccia (14318,6). The section is -2 cm across. The sample's brecciated texture is readily apparent in CL, with clasts being light blue and the matrix dark but containing a variety of smaller lumi­nescent objects. Among the small objects in the matrix are crystalline lunar spherules (CLS) that are the subject of a paper by Symes et al. in the pres­ent issue. The CLS, often referred to as "lunar chondrules" or "chondrule-like objects," are the ubiquitous, generally circular objects in the matrix with distinctive yellow CL. Steve Symes and his colleagues at Arkansas obtained data on the size and abundance of the CLS and the ballistics of their formation by impact; and with colleagues at the Johnson Space Center, he obtained compositional data for the CLS and their phases. Symes et al. conclude that the CLS are crystallized melt spherules from the impact that produced the Imbrium Basin. They argue that meteoritic chondrules are also crystallized impact melt spherules from impacts on their much smaller asteroidal parent bodies.

 

Symes S. J. K., Sears D. W. G., Taunton A., Akridge D. G., Yanghong Zhang and Benoit P. H. (1998)  The crystalline lunar spherules:  Their formation and implications for the origin of meteoritic chondrules.  Meteorit. Planet. Sci. 33, 13-29. Click here for article.