Appendix: Radiohalos in a Radiochronological and Cosmological Perspective
Secondary Radiohalos in Coalified Wood
All the various types of halos discussed thus far are termed primary halos
because they developed from alpha radioactivity emanating from small accessory
inclusions that were present when the mineral crystallized. But secondary halos
also exist in pieces of coalified wood taken from highly uraniferous deposits
in the Colorado Plateau. There is abundant evidence that U solutions infiltrated
much of the sedimentary material in the geological formations of that region
when the wood was still in a gel-like condition (17). When
U-bearing solutions passed through pieces of wood, certain active sites within
these specimens preferentially collected U, other sites collected rare earth
type elements, and still others Se, Po, and Pb. It is quite significant that the
U halos, which developed around the tiny U-rich sites, are all underdeveloped,
which, on the [p. 275] basis of a uniform decay rate (the rationale for using this assumption
for these specimens will be explained subsequently), suggests only a relatively
short time since U infiltration. Ion microprobe mass scans of these U halo centers
have shown extremely high 238U/206Pb ratios, which, again on
the assumption of a uniform decay rate, is consistent with a U infiltration within
the last several thousand years (17).
Figure 4. Elliptical (compressed) 210Po halos in coalified
wood from the Colorado Plateau. Reproduced from ref. (17)
by permission of the AAAS. (× 250) [on p. 274]
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Figure 5. Circular 210Po halos in Colorado Plateau coalified wood.
(× 250) [on p. 274]
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Figure 6. Circular and elliptical 210Po halo in Colorado
Plateau coalified wood. Reproduced from ref. (17) with AAAS
permission. (× 250) [on p. 274]
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Similar underdeveloped U halos have been found in the coalified wood from
the Chattanooga Shale, and in fact recent ion microprobe analyses show, in
agreement with earlier results (17), that the
238U/206Pb ratios of the U halos in the Colorado
Plateau samples (Eocene, Triassic, and Jurassic) and the Chattanooga Shale
(Devonian) are virtually indistinguishable. These results suggest that
U-infiltration occurred concurrently in all these formations.
Another class of more sharply defined halos was also discovered in the
Colorado Plateau coalified wood specimens (17). The centers
of these halos exhibit a distinct metallic-like reflectance when viewed with
reflected light. Three different varieties of this halo exist: one with a
circular cross section, another with an elliptical cross section with variable
major and minor axes, and a third most unusual one that is actually a dual halo,
being a composite of a circular and an elliptical halo around exactly the same
radio-center (see Figs. 4-6).
Although the elliptical halos differ radically from the circular halos in
minerals, the circular type resembles the 210Po halo in minerals
and variations in the radii of circular halos approximate the calculated
penetrated distances (26 to 31 μm) of the 210Po
alpha particle (energy E = 5.3 MeV) in this coalified wood (17).
Henderson (18) theorized that Po halos might form in
minerals when U-daughter Po isotopes or their alpha precursors were
preferentially accumulated into small inclusions from some nearby U source.
This hypothesis has not been confirmed for the origin of three distinct types
of Po halos in U-poor minerals (1,2,11),
but it does seem to provide a reasonable explanation for the origin of
210Po halos in U-rich coalified wood specimens.
Electron microscope x-ray fluorescence analyses showed these halo centers
were mainly Pb and Se. This composition fits well into the secondary accumulation
hypothesis for both of the U-daughters, 210Po (half-life, t½
= 138 days) and its beta precursor 210Pb (t½ = 22 y),
possess the two characteristics that are vitally essential for the hypothesis:
(i) chemical similarity with the elements in the inclusion and (ii) half-lives
sufficiently long to permit accumulation prior to decay, a requirement related
to the nuclide transport rate.
What is the meaning of the 210Po halos in Figs. 4-6? Clearly, the
variations in shape can be attributed to plastic deformation which occurred prior to
coalification. Since the model for 210Po formation thus envisions that
both 210Po and 210Pb were accumulating simultaneously in
the Pb-Se inclusion, a spherical 210Po halo could develop in 0.5 to
1 year from the 210Po atoms initially present and a second similar
210Po halo could develop in 25 to 50 years as the 210Pb
atoms more slowly beta decayed to produce another crop of 210Po atoms.
If there was no deformation of the matrix between these periods, the two
210Po halos would simply coincide. If, however, the matrix was deformed
between the two periods of halo formation, then the first halo would have been
compressed into an ellipsoid, and the second would be a normal sphere. The result
would be a dual "halo" (Fig. 6). The widespread occurrence of these dual halos
in both Triassic and Jurassic specimens can actually be considered corroborative [p. 276]
evidence for a one-time introduction of U into these formations, because it is
then possible to account for their structure on the basis of a single specifically
timed tectonic event (17).
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