El Qasia and Um Naggat granites are relatively small Late-Proterozoic
plutons, located north of Idfu-Marsa Alam asphaltic road in the Eastern
Desert of Egypt. Ratioing enhancement techniques of Landsat TM images
were used for lithological discrimination of different rock types and
to distinguish the mineralized from the barren granites in the studied
areas. Also, the airborne radiometric data of the same areas were
processed to show the distribution and intensities of uranium (U),
thorium (Th) and potassium (K40). The colour composite images of U, Th,
and K40 (in B,G,R) reveal the presence of significant U-anomalies in
blue color, confiding with the peripheries of the studied plutons,
forming zonal structure. The resulted data were correlated with
geological and structural maps prepared by using Landsat TM images, to
show the distribution of the mineralized granites. The applied
techniques distinguished two granitic types: barren granites occupying
the core of both plutons and mineralized granites occurring at the
peripheries of these plutons, forming zonal structure. The geochemical
studies favored that the barren one is calc-alkaline to alkaline rocks
of the I-type, equivalent to G-2 granites and probably were formed by
suturing at plate boundaries in compressional environment. The
mineralized granites are characterized by relatively higher contents of
SiO2, Rb, Zr, Nb,Y, Hf, Ga, U and Th and lesser contents of Al2O3,
Fe2O3, Sr, Ba and Zn compared to the barren biotite granites. The high
REE content in these granites, and the pronounced negative Eu anomaly
in the mineralized granites point to their bearing mineralization. The
obtained results demonstrate the suitability of both Landsat TM imagery
and airborne radiometric data in exploration for the radioactive-REE
bearing granites in the Eastern Desert of Egypt.