About: Lucinta Cal-Meg   Sponge Permalink

An Entity of Type : owl:Thing, within Data Space : 134.155.108.49:8890 associated with source dataset(s)

Lucinta Cal-Meg was the Physics Professor and Student Adviser at the Academy of Carida when Han Solo and Mako Spince were cadets training to become officers. Cal-Meg noted Cadet Solo's innate intelligence and the fact that he had attempted to improve his grades. Cal-Meg was present at Spince's expulsion proceedings after the cadet used antimatter stolen from the professor's own physics laboratory to blow up the Academy's Mascot Moon. Cal-Meg reported on the prognosis of the planetoid fragments, and the lack of stability in the orbital debris.

AttributesValues
rdfs:label
  • Lucinta Cal-Meg
rdfs:comment
  • Lucinta Cal-Meg was the Physics Professor and Student Adviser at the Academy of Carida when Han Solo and Mako Spince were cadets training to become officers. Cal-Meg noted Cadet Solo's innate intelligence and the fact that he had attempted to improve his grades. Cal-Meg was present at Spince's expulsion proceedings after the cadet used antimatter stolen from the professor's own physics laboratory to blow up the Academy's Mascot Moon. Cal-Meg reported on the prognosis of the planetoid fragments, and the lack of stability in the orbital debris.
Era
dcterms:subject
dbkwik:starwars/pr...iPageUsesTemplate
Story
  • The Hearing
Affiliation
Name
  • Lucinta Cal-Meg
Text
  • Dark Empire Sourcebook
Type
  • Galactic Empire
Book
  • Dark Empire Sourcebook
abstract
  • Lucinta Cal-Meg was the Physics Professor and Student Adviser at the Academy of Carida when Han Solo and Mako Spince were cadets training to become officers. Cal-Meg noted Cadet Solo's innate intelligence and the fact that he had attempted to improve his grades. Cal-Meg was present at Spince's expulsion proceedings after the cadet used antimatter stolen from the professor's own physics laboratory to blow up the Academy's Mascot Moon. Cal-Meg reported on the prognosis of the planetoid fragments, and the lack of stability in the orbital debris.
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