Scientific American Supplement No. 822, October 3, 1891Various
Science
Scientific American Supplement No. 822, October 3, 1891
Various
Science -- Periodicals
The polariscopic reading may now be taken, an observation on the 90 deg.
control plate having been made immediately before as previously
described. Then without altering the position of the instrument
relative to the light, or changing the character of the latter in any
way, the tube filled with the sugar solution is substituted for the
control plate. The telescope is adjusted, if necessary, so as to give
a sharply defined field, which must appear round and clear. (This
condition must be fulfilled before the observation is performed, as it
is essential to accuracy.) The milled head is turned until the neutral
point is found, and the reading is taken exactly as previously
described, the operation repeated five or six times, the average taken
with the rejection of aberrant readings, the average figure corrected
for the deviation shown by the control observation from the sugar
value of the control plate at the temperature of observation as given
in the table, and the result taken as the polarization of the sugar.
When a series of successive polarizations is made under the same
conditions as regards temperature, position of the instrument with
relation to the high intensity, of the light, etc., the control
observation need not be made before each polarization, one such
observation being sufficient for the entire series. The control must
be repeated at least once an hour, however, and oftener when the
operator has reason to think that any of the factors indicated above
have been altered, for any such alteration of conditions may change
the zero point of the instrument.
In the polarization of the quartz plates, as also in the polarization
of very white sugars, difficulty may be experienced in obtaining a
complete correspondence of both halves of the field. With a little
practice this may be overcome and the neutral point found, but when it
cannot, the ordinary telescope of the instrument may be replaced by
another, which is furnished with the polariscope and which carries a
yellow plate. This removes the difficulty and renders it possible,
even for one not well accustomed to the instrument, to set it at the
exact point of neutrality.
SUMMARIZED SOURCES OF ERROR.
The following principal sources of error must be especially guarded
against:
1. Drying out of sample during weighing.
2. Excess of subacetate of lead solution in clarification.
3. Incomplete mixing of solution after making up to mark.
4. Imperfect clarification or filtration.
5. Concentration of solution by evaporation during filtration.
6. Undue compression of the cover glass.
7. Alteration of the temperature of room, position of instrument, or
intensity of light while the observation or control observation is
being performed.
8. Performances of polarization with a cloudy, dim, or not completely
round or sharply defined field.
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