The daughter atoms from nuclear fission are nearly always radioactive and nearly always have very short half lives decaying through chains of atoms of short half lives. There is a reason for this.
We do not know exactly what the daughter atoms from the fission of a given atom will be, but we do know they will contain all the protons of the parent. The number of neutrons is also preserved, though a few unbound neutrons are usually emitted from the fission. Since atoms with higher atomic numbers can have a greater proportion of protons to neutrons, the daughters usually have far too many neutrons to be stable, and will usually undergo negative beta decay. For example, the fission of
235U might look like this:
92235U --> 3692Kr + 56141Ba + 2n
The most massive stable isotope of krypton is
86Kr, so our daughter krypton atom has six too many neutrons to be stable. The decay chain of the
92Kr, given as isotopes and half lives, is as follows, with all decays by negative beta decay:
92Kr 1.8 seconds
92Rb 4.5 seconds
92Sr 2.71 hours
92Y 3.54 hours
92Zr stable
The most massive stable isotope of barium is
138Ba, so our daughter has three too many neutrons to be stable. The decay chain of the
141Ba similar to the above is as follows, again all by negative beta decay:
141Ba 18.27 minutes
141La 3.92 hours
141Ce 32.5 days
141Pr stable
Most of the daughter decay chains do not produce stable isotopes nearly as quickly as the above, with many having products with half lives of decades to millennia. By comparison, our parent atom,
235U, had a half life of 703,800,000 years.