
Age of meteorites and the earth
writt,en for a representative lead which is derived today from any system belonging
to the met’eoritic array:
Pb2”6/Pb2”4 = 9.50 + l-014 U238/Pb204
(4
Pb207/Pb204 = 10.36 + O-601 U23s/Pb204
(3)
If any two of the three ratios above can be independently measured in the earth’s
uranium-lead system, and they satisfy expressions (2) and (3). then this system
belongs to the meteoritic array and must have it’s age. Two of t,he ratios can be
measured in a sample of earth lead. but the problem of choosing such a sample is
complex because the ratio of uranium to lead varies widely in different rocks and
minerals whose ages are short compared to t’he age of the earth.
One approach is to partition the earth’s crust int,o separate chemical syst’ems
of uranium and lead and consider t’heir interactlions.
Such systems may range from
minerals t’o geochemical cycles.
Nearly all of the lead-isotope data concerns either
minerals in which the uranium-to-lead ratio is very high (uraninites, et,c.) or
minerals in which this ratio is essentially zero (galenas). The approsimat,e times of
formation of some galenas have been determined! and of these. two dozen or so
lately formed galenas may be used as a measure of earth lead (Suclea)
Qeobogy (lg.%). IV. Faul, Ed.). The isotopic compositions of lead in some recent
oceanic sediments have also been determined (PATTERSOK, GOLDBERG. and
IXGHRAM 1953), and these may be used as a measure of earth lead.
Any of these samples will be improper or biased if they are derived from a
system of uranium and lead which is only partially closed and is subject to slow
but appreciable transport from other systems with different I_?238/Pb204 ratios.
In this respect, the sample which may represent the system of largest mass is
probably t’he more reliable.
One sample of oceanic sediment lead probably
represents more material than a dozen galenas. The isotopic composition of t,his
sediment lead is Pb206/Pb204 = 19-O and Pb207/Pb20f = 15-5, which satisfies
expressions (2) and (3) surprisingly well. It is doubtful if these figures are grossly
biased, since a few measurements of uranium and the isotopes of lead in rocks
with widelv different
-CT238 Pb204
I
ratios indicate rather good mixing t,o be t,he
first-order effect on the isotopic composition of lead in the earth’s crust (PATTERSOS:
TILTOX, and ISGHRAM, 1955).
Independent of the absolute abundances of lead isotopes, a rough measure of
t’he rates of change of the lead-isotope abundances in the earth’s crust may be
obt,ained from the isotopic composit’ion of galenas of different ages. These rates
of change are defined by the ratios of uranium and thorium to lead in the material
from which the galenas are derir’ed. From t,he observed rate of change of Pb206,
the U23s/Pb204
ratio in the earth’s crust is found to be 10 (COLLINS, RUSSELL, and
FARQCHAR? 1953). This value satisfies expression (2) and (3) for sedimentary lead
with unexpectedly good agreement.
In Fig. 2
it is shown that oceanic sediment lead (open circle) falls on the
meteoritic lead isochron.
Most of the lately formed galenas fall within the dotted
outline, although a few are widely aberrant.
isochron is determined by t(he U23S/Pb204
The position of a lead along the
ratio in the system from which the lead
235