he_who_is_nobody
Well-Known Member
Inferno said:he_who_is_nobody said:That age came about from Ca-Al dating, not U-Pb dating.
I'm not very knowledgeable about this subject so correct me if I'm wrong, but I am not familiar with Ca-Al dating. I think you got a wrong idea when you read "Ca-Al-rich inclusions" on Wikipedia.
Now just to be clear, the only Calcium isotope that has a long enough half life is Ca-48, but that half-life is long enough that "for all practical purposes it can be considered stable". All other isotopes have a half-life of mere seconds at most, only one has a half-life of over a hundred thousand years. None of these is suitable for radiometric dating. However, even if we consider that there might be one that has a suitable half-life (only Ca-48 remains), it immediately stops at Se-76 after double-beta decay. During no point does an isotope of Calcium with a long enough half-life to consider it for dating actually decay into aluminium.
So that being said, what are these Ca-Al-rich inclusions we're talking about and how can they be measured? They are inclusions in the actual meteor, so both elements are available in their stable form. It's the atoms of lead (Pb) inside them that are dated.
[url=http://www.ncbi.nlm.nih.gov/pubmed/12215641 said:Paper 1[/url]"]The lead-lead isochron age of chondrules in the CR chondrite Acfer 059 is 4564.7 +/- 0.6 million years ago (Ma), whereas the lead isotopic age of calcium-aluminum-rich inclusions (CAIs) in the CV chondrite Efremovka is 4567.2 +/- 0.6 Ma.
However, you're still correct that they can be dated differently, though not by this invented Ca-Al method.
Looking at either Paper 2 or the Wikipedia page, we can see that the alternative ways are either Magnesium-Chromium or Magnesium-Aluminium dating.
So since I'm a complete and utter n00b at this: Am I correct or not?
You are correct. I am in-error.