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 _bromate_, Sa(BrO₃)₃,9H₂O, melts at 75°, and closely resembles the
corresponding compounds of the didymium metals. The _sulphate_
crystallises with 8, and the _nitrate_ with 6 molecules of water. The
_carbonate_, Sa₂(CO₃)₃,3H₂O, can be obtained only by passing carbon
dioxide through an aqueous suspension of the hydroxide; addition of
alkali carbonate to a solution of a samarium salt precipitates hydrated
double carbonates.
The _acetylacetone compound_ melts at 146°-147°C.
Many organic salts have been prepared by James, Hoben, and Robinson
(_loc. cit._).
~Atomic Weight.~--The earlier determinations of this constant were
carried out with material not entirely free from europium. Demarçay[296]
carried out a synthetic sulphate operation with the material which he
obtained free from europium in 1900, and found values between the limits
147·2 and 148·0. The International Committee has adopted the value
150·4, which is based on the work of Urbain and Lacombe[297] in 1904.
These authors made determinations of three series of ratios, obtained by
(_a_) conversion of sulphate octohydrate to anhydrous sulphate, (_b_)
conversion of anhydrous sulphate to oxide, and (_c_) conversion of
sulphate octohydrate to oxide; these gave the values 150·314, 150·533,
and 150·484 respectively, from which the mean atomic weight is
150·44.[298]
[296] _Loc. cit._
[297] _Compt. rend._ 1904, ~138~, 1166.
[298] These numbers are calculated by Brauner (Abegg’s _Handbuch_,
III. i. p. 285) on the basis O = 16, S = 32·06, H = 1·0076, and are
somewhat higher than those given by Urbain and Lacombe, who used the
round numbers O = 16, S = 32, and H = 1.
~Detection.~--The absorption spectrum of samarium compounds is only
visible in fairly concentrated solutions, so that the element cannot
usually be detected in a mixture by this means. The position of the
maxima of the strongest bands (Demarçay, _loc. cit._) are:
476
463
417
402
These are all in the blue and violet regions; the first and second are
in the neighbourhood of neodymium and europium bands (_q.v._), and in
concentrated solutions the bands would partially coincide. Since these
are the two elements from which the separation is most difficult, and
are moreover the most constant in their occurrence with samarium, the
absorption spectrum is of very little use as a test.
The arc spectrum is very rich in lines,[299] of which the most intense
are:
3739·30
4152·38
4203·18
4225·48
4229·83
4236·88
4256·54
4319·12
4329·21
4334·32
4347·95
4391·03
4420·72
4421·32
4424·55
4434·07
4434·52
4452·92
4454·84
4458·70
4467·50
4519·80
4524·08
4544·12
4566·38
4577·88
4642·41
4674·79
[299] Exner and Haschek; Eder and Valenta; Rütten and Mersch,
_Zeitsch. wiss. Photochem._ 1905, ~3~, 181.
CHAPTER XIII
THE TERBIUM GROUP
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