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 detection of cerium in a mixture of earths is a comparatively simple
matter, as it has several distinctive reactions. The brown colour of the
peroxy-compounds has been suggested as a convenient test by several
authors. This may be observed when ammonia is added to a cerous salt in
presence of hydrogen peroxide. In the presence of a large excess of
foreign earths, very dilute ammonia should be added, drop by drop, with
continuous shaking, until a small permanent precipitate remains; this
will be rich in the weakly basic ceric hydroxide, and on addition of the
peroxide solution will show the colour clearly.[226] For very small
quantities of cerium, the neutral solution is added to warm concentrated
potassium carbonate solution, and one or two drops of dilute hydrogen
peroxide added to the clear liquid; the yellow colour is then very
characteristic.[227]
[226] Marc, _Ber._ 1902, ~35~, 2370.
[227] Meyer, _Zeitsch. anorg. Chem._ 1904, ~41~, 94.
Biltz and Zimmerman[228] employ the reducing powers of cerous hydroxide;
ammoniacal silver nitrate is added to the neutral solution of the cerous
salt, and the mixture warmed. Dilute solutions (1-2 mgms. per litre)
give a brown colour, concentrated solutions a black precipitate. The
oxidation of an ammoniacal solution of the tartrate by air or hydrogen
peroxide, by which an intense yellowish brown colour is developed, has
been recently suggested by Wirth[229] as a very delicate test for the
element.
[228] _Ber._ 1907, ~40~, 4979.
[229] _Abstr. Chem. Soc._ 1913, ~104~, ii. 712.
_Spectrum analysis._--Cerous salts show no absorption, ceric salts
general absorption of the violet end of the spectrum. Arc spectrum--see
Exner and Haschek,[230] Eder and Valenta,[231] and Cooper.[232] The
emission spectrum of cerium is especially rich in lines; for
identification, the following may be used:
[230] _Die Spektren der Elemente, etc._, Leipzig and Vienna, 1911.
[231] _Sitzungsber. kaiserl. Akad. Wiss. Wien_, 1910, ~119~, II_a_,
531.
[232] _Astrophys. J._ 1909, ~29~, 352.
4150·11
4186·78
4222·78
4296·88
4337·96
4382·32
4386·95
4460·40
4479·52
4487·06
4527·51
4528·64
4539·90
4562·52
4572·45
4594·11
4628·33
5512·72
The _estimation_ of cerium cannot be carried out accurately by
gravimetric methods in the presence of other earths; volumetric methods,
however, will give reasonably accurate results, if the necessary
precautions are taken. In Bunsen’s method the ignited oxides are treated
with hydrochloric acid in presence of potassium iodide, the iodine set
free from the hydriodic acid by reduction of the cerium dioxide being
estimated by means of sodium thiosulphate, in the usual way. This method
gives very inaccurate results, since in the presence of cerium dioxide,
other oxides of the group can be converted into higher oxides which will
also liberate iodine under these conditions.
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