The Rare Earths: Their Occurrence, Chemistry, and TechnologyLevy, Stanley Isaac
Science
The Rare Earths: Their Occurrence, Chemistry, and Technology
Levy, Stanley Isaac
Rare earths
The Euxenite-Polycrase series was studied by Hauser and Wirth in
1909,[71] in an endeavour to establish their theory that the proportions
in which the various earths and acids occur in this group of minerals is
subject to definite laws beyond the ordinary laws of combination. Thus
of the erbia earths they state that the proportion of holmia and
dysprosia increases relatively to erbia as titanium dioxide increases,
_i.e._ as we pass from the euxenites to the polycrases; at the same time
scandia and yttria increase relatively to the other yttria earths (the
terbia group), whilst in the ceria group samaria and praseodymia
decrease relatively to the others. Thus samaria is found in appreciable
quantities only when the titanium content is low. The original paper
must be consulted for full details.
[71] _Ber._ 1909, ~42~, 4443.
It was stated above that zirconium was found in euxenite in 1879. In
1901 Hofmann and Prandtl[72] declared that zirconia was an unfailing
constituent of the mineral, and that it was always accompanied by a new
oxide, which they named Euxenia (‘Euxenerde’). This was characterised by
the solubility of its oxalate in acid solutions, the insolubility of
the precipitated hydroxide in excess of alkali, and the gradual
precipitation by hydrogen peroxide from a slightly acid solution of its
salts. In their paper quoted above, Hauser and Wirth state that zirconia
is never present in typical euxenites. In a second paper[73] they state
that after exhaustive treatment of every known zirconia mineral, they
can find no trace whatever of the ‘new earth,’ and conclude that Hofmann
and Prandtl must have made some experimental error. During this
examination, they observed radioactivity in some minerals which
contained no traces of uranium or thorium.
[72] _Ibid._ 1901, ~34~, 1064.
[73] _Ber._ 1910, ~43~, 1807.
~Risörite.~[74]--A columbate of yttria earths, with titanium; ferric
oxide, alumina, lime and lead monoxide are present in small quantities.
It resembles fergusonite in composition, but differs in the almost
complete absence of uranium, the high loss on ignition, and the amount
of titanium present, which is here considerable (TiO₂ = 6·5 per cent.).
Hauser regards it as an orthocolumbate, R´´´(Cb,Ta)O₄, with an
isomorphous admixture of metatitanate, R´´´₂(TiO₃)₃.
[74] Hauser, _Ber._ 1907, ~40~, 3118; _Zeitsch. anorg. Chem._ 1908,
~60~, 230.
The rare earths are chiefly yttria, with some erbia earths and a little
terbia; ceria, lanthana and didymia are also present. The mineral
contains a considerable amount of helium, which is remarkable in view of
the very small content of uranium and thorium (cf. Thalenite). It is
radioactive, the active constituent being precipitated with the lead
(and to a very small extent with the rare earths).
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