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tivity on the carmel faul

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3.3.2 Single sample dating<br />

Single sample dating was d<strong>on</strong>e using equati<strong>on</strong> [1] according to Broecker and<br />

Kaufman (1965):<br />

[1] [ 230 Th/ 234 U] = [ 238 U/ 234 U]*(1-e -λ230t ) + {1-[ 238 U/ 234 U]}*{λ 230 /(λ 230 -λ 234 )}*[1-e (-λ230-λ234)t ]<br />

As menti<strong>on</strong>ed above (ch. 1.3- Dating of speleo<strong>the</strong>ms), this equati<strong>on</strong> is based <strong>on</strong> <strong>the</strong><br />

assumpti<strong>on</strong> that no initial 230 Th is present in <strong>the</strong> sample. Any initial 230 Th is always<br />

accompanied by a much larger amount of 232 Th, <strong>the</strong>refore 232 Th is routinely m<strong>on</strong>itored<br />

during analysis, and samples c<strong>on</strong>taining less than an acceptable threshold of 230 Th/ 232 Th<br />

can be identified (Hellstrom, 2007). According to Kaufman et al. (1998) a sample is<br />

c<strong>on</strong>sidered to have a high detrital c<strong>on</strong>tent, which requires a correcti<strong>on</strong> for <strong>the</strong> c<strong>on</strong>tributi<strong>on</strong><br />

of 230 Th by <strong>the</strong> decay of 232 Th, if this ratio is less than ~30, since for larger ratios <strong>the</strong><br />

correcti<strong>on</strong> becomes negligible compared to <strong>the</strong> analytical uncertainty. Richards and<br />

Dorale (2003) and Li et al. (1989) argued that thresholds of between 100 and 300 for <strong>the</strong><br />

case of mass spectrometric dating, due to <strong>the</strong> high-precisi<strong>on</strong> analysis of initial 230 Th.<br />

Hellstrom (2007) argued that even a value of 230 Th/ 232 Th=300 requires a correcti<strong>on</strong> for<br />

<strong>the</strong> derital fracti<strong>on</strong>.<br />

C<strong>on</strong>sidering <strong>the</strong>se higher values, most ages obtained for Denya Cave seismite samples<br />

need to be corrected for initial 230 Th, using as a correcti<strong>on</strong> factor <strong>the</strong> detrital molar ratio of<br />

232 Th/ 238 U. The most comm<strong>on</strong> correcti<strong>on</strong> factor for crust value rocks is 3.8 (Wedepohl,<br />

1995). Even higher values of 4.2 were determined (e.g. Kuperman, 2005). Haase-<br />

Schramm et al. (2003) reported a single sample correcti<strong>on</strong> factor for Lake Lisan<br />

arag<strong>on</strong>ites detritus of 232 Th/ 238 U atomic ratio=0.85 (i.e. 232 Th/ 238 U detrital molar ratio of<br />

0.83=0.27 ac<str<strong>on</strong>g>tivity</str<strong>on</strong>g> ratio*3.05). They also suggested that some initial 230 Th found in those<br />

samples was c<strong>on</strong>tributed by hydrogenous Th. In a carb<strong>on</strong>ate terrain <strong>the</strong> correcti<strong>on</strong> factor<br />

was calculated by Kaufman et al. (1998), using an isochr<strong>on</strong> method, yielding a value of<br />

1.8±0.25=detrital molar ratio (Soreq cave). In <strong>the</strong>ir study Kaufman et al. (1998) showed<br />

that all <strong>the</strong> Th in <strong>the</strong> speleo<strong>the</strong>ms from Soreq cave was associated with detrital material.<br />

In <strong>the</strong>ir method <strong>the</strong> slopes of isochr<strong>on</strong>s in a plot of ( 232 Th/ 234 U) vs. ( 230 Th/ 234 U) were used<br />

in order to calculate <strong>the</strong> detrital molar ratio of 232 Th/ 238 U. Those isochr<strong>on</strong> lines are<br />

essentially mixing lines between a clean sample (low detrital comp<strong>on</strong>ent) and <strong>the</strong> DEM<br />

within <strong>the</strong> lamina, since stalagmites often have observable differences in <strong>the</strong> quantity of<br />

detrital material al<strong>on</strong>g growth layers (Richards and Dorale, 2003). Following Kaufman et<br />

al. (1998) isochr<strong>on</strong> slopes and <strong>the</strong>ir intersects with <strong>the</strong> Y axis ( 230 Th/ 234 U) enables a<br />

calculati<strong>on</strong> of a correcti<strong>on</strong> factor as follows:<br />

36

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