78
R. L. Frost et al.
The controlling level of 0.1 mg min-1 was reached in both
steps resulting in a quasi-isothermal pattern of water evo-
lution at 80 and 150 °C. Above 400 min, dehydroxylation
took place in four steps at 200, 249, 325 and 452 °C under
the slow heating (the rate of decomposition did not reached
the controlling level of 0.1 mg min-1). This experiment
revealed the subtle nature of dehydroxylation which was
not observed in the dynamic experiment.
References
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The thermal decomposition of the silver-lead mixed
jarosites (Figs. 9 and 10) under CRTA conditions results in
dehydration occurring in a series of non-isothermal steps up
to 300 °C. A quasi-isothermal steps is observed at 562 °C,
attributed to desulphation. For the Ag075(Pb0.5 0.25Fe3
)
(SO4)2(OH)6 xH2O jarosite two dehydroxylation steps are
observed similar to the two dehydroxylation steps observed
in the dynamic experiment. A pseudo-isothermal desulph-
ation step at 566 °C is observed (Fig. 10).
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Synthetic jarosites show characteristic thermogravimetric
patterns with thermal decomposition steps: (a) dehydration,
(b) well defined dehydroxylation and (c) desulphation.
While the patterns of dehydration and dehydroxylation (as
well as the amounts of crystallisation water) differ signif-
icantly depending on the nature of the cation, desulphation
is a rather homogeneous process (the DTG peak tempera-
tures fall in the range between 760 and 800 °C for all the
five samples).
CRTA offers a better resolution and a more detailed
interpretation of the decomposition processes via
approaching equilibrium conditions of decomposition
through the elimination of the slow transfer of heat to the
sample as a controlling parameter on the process of
decomposition. With this technique differences in the
dehydration and decomposition patterns can be revealed
suspecting a more complex pattern of decomposition as
revealed under dynamic hating.
It is very important to be able to thermally characterise
minerals such as jarosites which may be found on planets
such as Mars. The existence of jarosites on Mars would
confirm the presence of water at some time in the past as
such minerals are only formed from solution. The thermal
stability of jarosites is most important as there is a need to
find the temperature range over which the minerals are
stable, since wide temperature ranges are likely on planets.
22. Thomas PS, Hirschausen D, White RE, Guerbois JP, Ray AS.
Characterization of the oxidation products of pyrite by thermo-
gravimetric and evolved gas analysis. J Therm Anal Calorim.
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23. Frost RL, Hales MC, Martens WN. Thermogravimetric analysis
of selected group (II) carbonate minerals—implication for the
Acknowledgements This research was supported by the Hungarian
Scientific Research Fund (OTKA) under grant No. K62175. The
financial and infra-structure support of the Queensland University of
Technology Inorganic Materials Research Program is gratefully
acknowledged.
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