THE AGE OF THE EARTH 

 

 

Clarence L. Dulaney          and  Patrick L. Dulaney

2226 Fairgreen Drive                            1091 S. Corona St.

Missouri City, TX 77489                      Denver, CO 80209

e-mail cldtx1@sbcglobal.net              e-mail dulaneyp@comcast.com

 

 

ABSTRACT: Finding the age of the earth and of historical artifacts such as fossils, and of archaeological specimens has long been of interest.  Because some radioactive elements have very long lived species, attempts to use the decay of these elements to measure age has been accepted as the “benchmark”.  This paper discusses why such methods, except for “radiocarbon” dating, have questionable accuracy for measuring the age of the earth.

 

                                                                                                                                    

 

ORIGIN OF THE EARTH

 

Note: references are given as [a.xxx], where a is the reference number and xxx is the page number.

 

Probably the most cogent theory of the origin of the earth is that it was formed, along with the rest of the solar system by aggregation of particles of a “cosmic dust cloud”.  [1.12-37].

 

It is here proposed that the “cosmic dust cloud” was a result of the disintegration of a large star, which became a supernova.  It would be hard to otherwise explain the local concentration of enough total elements to make up the solar system.  It is further postulated that all of the elements present on earth are resultant from and were formed in the precursor star.

 

The chemical composition of the large precursor star varied from Hydrogen to Uranium, with all the “stable” isotopes in between, with stable indicating those that have half lives greater than 108 years.  This includes K40 and U238.  All these isotopes had to have been built up by fusion of various isotopes with hydrogen [2.251].  In the buildup of elements in a star, the fusion to form isotopes is exothermic up to 26Fe [2.254].  Once a core of iron builds up, the star becomes hotter, and the endothermic production of the higher elements proceeds.   Elements higher than U have very short half lives.  Roughly equal numbers of atoms of the stable elements with higher atomic numbers than iron are produced, with those of even atomic number generally being of larger concentration than those of odd atomic numbers [1.19,22].

 

Note that, in the solar system, only the sun has ever been hot enough to support fusion reactions, so that all the elements in the planets came from the precursor star, (including those from meteorites)..

 

As the solid earth formed, it almost undoubtedly was molten, with temperatures of 1500-3000K being proposed [1.54].  There was not enough Oxygen to oxidize all the metals present, particularly the Fe, Co, and Ni.  These metals, being molten, and heavier than the oxides sank to the center of the mass, and became the core of the earth.  Those elements with higher heats of formation of oxides than that of FeO were oxidized and became “lithophiles”, which later became the earth’s crust when sufficient cooling occurred. 

 

All the alkali metals, alkaline earths, rare earths, silicon, Al, Sc and particularly U and Th (among others)are lithophiles [1.51].

When the “original”, molten earth cooled enough, the composition of the lithosphere was “frozen”.  There was almost undoubtedly some inclusion of atmospheric gasses in the very viscous magma.  Estimates of the time the primordial earth was entirely molten until the crust was formed vary from a minimum of several thousand of years up to hundreds of thousands of years [1.56]. 

Once the crust was “frozen”, the composition of various radioactive systems were fixed, as far as a basis for radioactive dating of the earth was concerned.

This paper is particularly interested in two decay cycles, that of K40-Ar40, and U238-Pb206.  The latter cycle goes through several steps, with an overall half-life of 4.5 x 109 years. Note that one of the intermediates is the gas Rn [3.285].  That of the K40 system has a half-life of 1.25 x 109 years.  

Particularly in the case of the K40 system, for “dating” purposes, it is assumed that there was no Ar40 in the rock initially, and that any that is found came from decay of the K40.  It is also assumed that the system was ‘closed” throughout, that there is no loss or gain of K or Ar throughout the history of the rock. (Note that virtually all K compounds are water soluble.)  If there was no loss or gain, the general formula for the age of the rock A is:   A = (t½/ln2) (ln(1+(D/P))) where ln indicates logarithm to the base e.  A is in the same units as t½.  D is the number of atoms of the daughter element (Ar40) and P is the number of atoms of the parent isotope (K40) at the time of analysis.  Thus, in a closed system not subjected to any outside forces, where there is absolutely no loss of any of the “daughter elements” age can be relatively accurately estimated.

ANOMALOUS K40-Ar40 DATES

Lava samples obtained from Mount Nguruhoe in New Zealand from known eruptions dating back to 1949 were sent to a commercial dating laboratory, Geochron Laboratories in Cambridge, MA, with the notation that they were “probably young, with little Ar in them” [4].  The measured ages were reported to be from 0.27 to 3.5 million years.  This indicated that there must have been some Ar in the hot lava, and it must have remained there after the lava solidified.

These results cast serious doubts on dates obtained on older, unknown history, samples.  Either the Ar was present in the lava and not evolved while it was molten, or was included from atmospheric contamination with the 0.9% Ar of the air.

It is here proposed that some Ar could have been included in the primordial magma, and that there may have been “reaction” between the very electropositive alkali metals and the “inert” Ar in the high temperature melt.  There may have also been the same sort of inclusion in the molten lava.

THE U238-Pb206 SYSTEM

In this system there would definitely be some Pb206 present in the primordial system.  To determine the age of this system, it would be necessary to know the amount of Pb206 initially present.  One method of determining this amount would be to use the concentration of the stable, non-radiogenic isotope Pb204 in the present sample, along with an estimate of the Pb206/Pb204 initially present.  This ratio has been determined on an ancient sample of galena, PbS, and was found to be 16.25 [3.290].  (This is fairly close to the ratio in current Pb, with a Pb204 content of 1.48% and a Pb206 content of 23.6%, for an atomic ratio of  16.10 [5.B481].)

Thus, the age A of a U238-Pb206 sample would be: [3.287ff]   A = (1/1.55125 x 10-10) x (ln(1+((Pb206/Pb204) – (16.25))/(U238/Pb204))).   The 16.25 is the initial lead isotope ratio, and all the other concentrations are the number of atoms in the current sample

There are several doubtful assumptions tacitly made in this analysis.  As Faure himself pointed out, (We give a paraphrased quote applying only to this system),  For the formula to hold,  1.  The mineral has remained closed to U, and Pb, and to the intermediate daughters throughout history.  2. Correct values are used for the Pb isotope ratios.  3. The decay constant for U238 is known accurately. , and 4.  All analytical results are accurate and free from systematic error”.

In regard to closed systems, it is known that the U in the lithosphere is close enough to the surface that it is impossible to date samples by amount of He in the rocks, because of loss of He by evaporation [3.283].  (Note also that the gas Rn is a daughter product, and might also be lost in the same manner.)

Secondly, in most cases, at least some of the U is oxidized to the uranyl ion (UO22+), for which most salts are water soluble.  This could lead to loss (or gain) of U in samples,

Concerning the Pb isotope ratio, it would seem that the initial concentration of Pb204 would at least be equal to that of the Pb206, at least in the star where both were made only by fusion.  If the star were old enough that a considerable amount of U238 had decayed, then the Pb206 would be higher.

The reason that the Pb206/Pb204 ratio is 16.25 may be that all the daughter elements of U238 have fairly short half lives, with the longest being 2.5 x 105 years, and many having half lives less than a year.  In the large stars, fusion builds up these daughters, which in turn rapidly, (compared to the life of the life of the star), decay to Pb206, while the number of atoms of Pb204 remains virtually the same.  Of course, the fusion goes on to U238, which builds up at slightly less rate than the Pb204.  (There are 18 daughters, as shown by Figure 18.1 by Faure [3.285]).  This again indicates that the radiometric agers are measuring something pertaining to the age of the large precursor star.

Other samples that are used in dating are U235-Pb207, t½ = 7.04 x 106 years, Th238-Pb238, t½ = 14 x 109 years, Rb87- Sr87, t½ = 48.8 x 109 years, and Sm147-Nd143, t½ = 106 x 109 years.  In any of these systems, the analytical problems are formidable, and there are the same sort of questions about “closed systems” and initial daughter concentrations.

 

The age of the original star may actually be what is measured rather than that of any system on earth.  It is interesting that many of the estimates of the age of the oldest earth rocks by different methods all give around 4 x 109 years, which is believed by us to be that of  the precursor star..

 

CARBON14 DATING

 

In measuring ages less than 50,000 years, the decay of isotope C14 is usually measured, following the work of W. F. Libby in 1949 [6].

There is roughly a constant amount of C14 in the atmosphere in the form of  C14O2.  1 x 10-10 % of the total atmospheric CO2.  The generally accepted mechanism for generation of C14 is high altitude absorption of a neutron by N14 which then becomes C14 by emission of a proton.  Then the C14 is oxidized to CO2.  It is here proposed that a more plausible scenario is that the isotope is made at any altitude by striking of a C13O2   molecule by a high speed H atom (from  cosmic rays”).  C13 amounts to about 1.1% of ordinary Carbon and is a stable isotope. 

At any rate, C14O2 is present in the atmosphere and is metabolized by plants in a proportional amount with the normal CO2.  Animals eat the plants and thus also acquire an amount of the radioactive isotope. 

When the plants and animals die, the C14 begins to decay with a half-life of 5730 years.  By measuring the amount of isotope remaining in the sample, the time since the sample was alive can be estimated.

Not all organic samples give meaningful results, particularly samples that came from, or have been covered by water, because the carbon dioxide makeup in seawater is significantly different from that of the atmosphere.  For example, it would be impossible to correctly determine the date of coral beds.

Also, after about 10 half-life periods, the radioactive isotope content falls so low as to be essentially non-measurable.  Thus C14 dating does not work at all for samples over about 50,000 years old.

Several methods are used to measure the C14 content of a sample.  The sample is generally burnt to produce CO2, and the CO2 recovered by absorption.  Then the radioactivity can be counted directly.  Other methods include converting the carbon dioxide to acetylene, and measuring the amount of C14 directly by mass spectrometry. Since the C14 content of even recent samples is very low, analytical techniques must be very sophisticated.

Carbon dating has been compared with known historical dates with some success.  In particular, the carbon age of acacia wood from Pharaoh Djoser’s tomb gave results within 10% of the historical date[7].

Dates obtained by C14 measurements are probably good up to 40,000 to 50,000 years, but this assumes the atmospheric content of C14O2 has been constant over this period of time.

Basically the only thing that can be said about the age of the earth is that it is between 40,000 and about 4 billion years.  

Since the age of the precursor star is probably about 4 billion years, the  universe must be at least this old.

 

CONCLUSIONS

Measurement of the age of ancient rocks by radiometry is questionable, because it is not known how large a concentration of “daughter” atoms was present in the primordial rock, and because it cannot be guaranteed that the rock has remained a “closed system” throughout its entire history.  The oldest ages being measured are likely that of the precursor star.

It is possible to estimate the age of organic matter that is less than about 40,000 years old by means of  C14 analysis.

The age of the earth cannot be estimated more accurately than between 40,000 and  about 4 billion years.

 

REFERENCES

1.   B. Mason, “Principles of Geochemistry”, John Wiley & Sons, NY, (1952)

2.   E. Novotny, “Introduction to Stellar Atmospheres and Interiors”, Oxford U. Press, Oxford, (1973)

3.   G. Faure, “Principles of Isotope Geology”, 2nd Ed., John Wiley & Sons, NY, (1986)

4.   A. Snelling, Creation Ex Nihilo. 22, (1), 18, December 1999, February 2000

5.   “Handbook of Chemistry and Physics”, 35th Ed., R. Weast, Ed., Chemical Rubber Co., Cleveland, (1972)

      6.W. Libby, E. Anderson and J. Arnold, Science, 109, 227 (1949)

      7. W. Libby, “Radiocarbon Dating”, U. of Chicago Press, Chicago, (1955)

     

 

© 1/26/03

Clarence L. Dulaney

Patrick L. Dulaney