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Compared to the half-life and decay mode of the nuclide (^{90}\text{Sr}), the nuclide (^{226}\text{Ra}) has a significantly longer half-life and a different decay mode. (^{90}\text{Sr}) has a half-life of about 28.8 years and primarily decays via beta decay to (^{90}\text{Y}). In contrast, (^{226}\text{Ra}) has a half-life of about 1,600 years and decays primarily through alpha decay to (^{222}\text{Rn}). This means that (^{226}\text{Ra}) is more stable and persists longer in the environment compared to (^{90}\text{Sr}).

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Since the atomic number of Sr is less than 90, Sr undergoes beta decay. Beta decay is when the element decays into another element and a neutron actually breaks apart (sort of) into an electron and proton; the proton attaches to the other element, but the electron stays alone. Thus: 90------>90 Y+e0-1 38 Sr--->39 Y+e *there should only be one e, and the 0 and -1 should be in front, just like with the elements, but the format deletes the extra spaces so i put it like that for clarity's sake. sorry!


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