A.J. Locke et al. / Thermochimica Acta 459 (2007) 64–72
71
of jarosite on Mars, thus providing evidence for the existence or
pre-existence of water on Mars. Interest in evaporite minerals
and their thermal stability rests with the possible identification
of these minerals and related dehydrated paragenetically related
minerals on planets. The existence of these minerals on planets
would give a positive indication of the existence or at least pre-
existence of water on Mars. Further such minerals are formed
through crystallization from solutions.
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4. Conclusions
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hydrometallurgy, 2000, p. 405.
Thermogravimetric and differential analysis of mineral
known as pseudoalums including halotrichites, apjohnite,
pickeringite and wupatkiite. EDX analysis shows the chem-
ical formula of the minerals to be (Fe0.752+,Mg0.25)SO4·Al2
(SO4)3·22H2O,(Mn0.642+,Mg0.28,Zn0.08)SO4·Al2(SO4)3·22H2O,
(Fe0.222+,Mg0.78)SO4·Al2(SO4)3·22H2O, (Co0.45,Fe0.552+)SO4
·Al2(SO4)3·22H2O, respectively. X-ray diffraction showed the
minerals to be phase pure except for pickingerite which showed
the presence of gypsum.
The halotrichite minerals showed in general three low tem-
perature thermal decomposition steps attributed to dehydration.
A fourth dehydration step at around 317 ◦C was observed and
was assigned to water trapped within the halotrichite structure.
Depending on the halotrichite 2, 3 or 4 higher temperature ther-
mal decomposition steps are observed. For halotrichite thermal
decomposition steps are observed at 546, 625, 697 and 738 ◦C
and are attributed to the decomposition of sulphate anions to SO3
and consequentially to SO2 and 1/2O2. A comparison with the
thermal decomposition of jarosites shows that the halotrichites
decompose at higher temperatures.
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Therm. Anal. Calorim. 72 (2003) 769.
[29] R.L. Frost, K.L. Erickson, J. Therm. Anal. Calorim. 76 (2004) 217.
[30] R.L. Frost, K. Erickson, M. Weier, J. Therm. Anal. Calorim. 77 (2004)
851.
[31] R.L. Frost, M.L. Weier, K.L. Erickson, J. Therm. Anal. Calorim. 76 (2004)
1025.
[32] R.L. Frost, M.L. Weier, J. Therm. Anal. Calorim. 75 (2004) 277.
[33] R.L. Frost, W. Martens, Z. Ding, J.T. Kloprogge, J. Therm. Anal. Calorim.
71 (2003) 429.
[34] R.L. Frost, Z. Ding, H.D. Ruan, J. Therm. Anal. Calorim. 71 (2003)
783.
[35] R.L. Frost, S.J. Palmer, J.M. Bouzaid, B.J. Reddy, J. Raman Spectrosc. 38
(2007) 68.
[36] R.L. Frost, D.A. Henry, M.L. Weier, W. Martens, J. Raman Spectrosc. 37
(2006) 722.
Acknowledgments
[37] R.L. Frost, A.W. Musumeci, J.T. Kloprogge, M.O. Adebajo, W.N. Martens,
J. Raman Spectrosc. 37 (2006) 733.
[38] R.L. Frost, J. Cejka, M. Weier, W.N. Martens, J. Raman Spectrosc. 37
(2006) 879.
[39] R.L. Frost, M.L. Weier, J. Cejka, J.T. Kloprogge, J. Raman Spectrosc. 37
(2006) 585.
[40] R.L. Frost, J. Cejka, M.L. Weier, W. Martens, J. Raman Spectrosc. 37
(2006) 538.
The financial and infrastructure support of the Queens-
land University of Technology Inorganic Materials Research
Program of the School of Physical and Chemical Sciences
is gratefully acknowledged. The Australian Research Council
(ARC) is thanked for funding Thermal Analysis Facilty.
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