Special alpha-proton-X-ray spectrometric complexes (APXS) have been develop
ed in order to perform chemical analyses of the Mars atmosphere and rock su
rface compounds by alpha back-scattering, alpha-proton measurements, and X-
ray fluorescence. The sources were prepared by high temperature condensatio
n of metal curium vapour onto silicon substrates. They are silicon disks wi
th curium-244 fixed on their surfaces as a silicide. The sources have overa
ll dimensions as follows: disk diameter 8 mm; thickness 0.3 mm; and 6 mm di
ameter active spot. The source activities are 5 +/- 1 mCi and the alpha-lin
e half-widths are equal to (1.7-2.5) and (2.9-4.5)% of full width at 10% of
Maximum (Maximum is equal to 5.8 MeV). Thermovacuum (from 196 to 1000 degr
ees C), mechanical, and resource tests were performed and demonstrated that
the sources maintained their characteristics. The applicability of the sou
rces for the above-mentioned analytical purposes was confirmed during NASA
Mars Pathfinder mission. (C) 2000 Published by Elsevier Science Ltd.