View Document - OSTI
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22<br />
220 ppm relative to silicon equal to I8.5 percent by weight in<br />
primitive nonvolatile solar material. Ihis is one fourth of its<br />
reported abundance. We use this somewhat larger factor because<br />
Urey's (1955) calculations indicate that his choice of radioactive<br />
elements is somewhat too high for reasons which he<br />
discusses. Also, the somewhat lower abundance gives a somewhat<br />
smoother abundance curve. This gives 854 for its atomic abundance.<br />
The use of this abundance leads to the similarity in shape of the<br />
even and odd mass curves in the minimum region between oxygen<br />
and iron.<br />
As explained above, the choice of this lov;er value for<br />
potassium requires that other abundances by adjusted if we are to<br />
be consistent. It seems likely that the melting processes which<br />
produced the silicate minerals produced the fractionation of<br />
potassium, uranium and thorium, and in this case the abundances of<br />
all elements which are markedly concentrated by such processes<br />
must be appropriately adjusted as well. In order to Judge the<br />
direction and amount of such adjustments we have studied the<br />
relative abundances of the elements in the earth*s crust and in<br />
the meteorites. Potassium makes up 2.6 percent of the earth's<br />
surface rocks and only O.O9 percent of the meteorites. Also,<br />
analyses of ultramafic rocks show that potassium is very low in<br />
these rocks. Ross, Poster and Myers (1954) analysed olivine bombs<br />
from basaltic lava flows and found low values for sodium and<br />
potassium and Edwards (1955h) using an improved method of analysis