Department of Geology - Portland State University
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Student Page for Dr. Alexander M. Ruzicka

 
Backscattered electron (BSE) image showing forsteritic olivine grains  (dark-grey, at center) with ferrous olivine overgrowths (light grey edges) in the Sahara-97210 (LL3.3) chondrite. 
Cathodoluminescence (CL) image showing same region as upper BSE image.  The most forsteritic olivine is rich in Ca and Al and luminesceses brightly. 
Students that have worked with Dr. Ruzicka:
  • Thomas Lindsay--  assisted in obtaining chemical data on the Miles (IIE) iron meteorite
  • Sean Greeney-- completed M.S. Thesis on diffusion modelling of chemical exchange between relict forsterite and overgrowth olivine to place constraints on chondrule thermal histories 
  • Karen Carroll-- completed Honors Thesis on the classification of three new meteorites from Northwest Africa
  • Randy Goosen-- obtained SEM data on possibly meteoritic igneous rocks obtained in Africa 
  • Chastelle Allegre-- obtained SEM data on Tatahouine diogenite for microbe project, to compare with terrestrial rocks 
  • Niina Jamsja-- obtained EMPA data on new chondrite with megachondrules and unusual overgrowths 
  • Thomas Schepker-- developed XRD technique for classifying ordinary chondrites & obtained EMPA data on new howardite
  • Doug McCarty, Karen Carroll, Julie Ryan, Robert McGown, Thomas Schepker--  Reading and Conference

 
 
 
 
 
 
 

 


 
Image above: Panorama obtained by the Spirit Mars Exploration Rover on Sols 814-932 at the Winter Haven site.  South Promontory is the hill at center.  Dark boulders are vesicular basalt and overlie lighter-colored thin bedrock layers in places.  Two candidate iron meteorites identified by distinctive thermal emission spectra, Zhong Shan and Allan Hills, are labeled. (Courtesy NASA.) 


Last Updated: 24 January 2008