A disintegration series is the pathway of a radioactively unstable element into a stable element. The pathway alters the atomic number of the element and converts the element into another element. A common one is the uranium disintegration series.
The name for the emissions of rays and particles by a radioactive material are called radioactive decay. There are many different types of radioactive decay that emit different rays and particles.
Minerals like uraninite and carnotite are highly radioactive ores of uranium.
The heaviest element that is highly radioactive is Ununoctium, which has an atomic number of 118.
You can just put something in the sentence that is going to be radioactive that's all.
Stars seem to be, but they don't have big and/or unstable atoms such as most radioactive elements have. They release sub atomic units when their atoms fuse, along with rays such as gamma rays, which is why they can seem to be similar to other radioactive things. Some planets with atmostpheres that are ionised by ionising rays can also be similar to radioactive things perhaps.
The radioactive decay of americium 241 is by alpha disintegration; the disintegration of radioactive krypton isotopes is by beta particles emission.
No. It is a nuclear reaction - radioactive disintegration.
After disintegration all radioactive elements are transformed in other elements.
Francium is a radioactive element supporting radioactive disintegration.
This phenomenon is called radioactive disintegration.
This the decay (disintegration) rate.
Polonium (Po) is the only Group 16 element that undergoes natural radioactive disintegration.
Atomic nuclei are changed by nuclear reactions or radioactive disintegration.
It is smaller than the original atom and is possibly radioactive.
Francium don't explode instantly; probably a confusion with the radioactive disintegration.
Yes; helium appear from radioactive disintegration of uranium or thorium.
The disintegration constant is the fraction of the number of atoms of a radioactive nuclide which decay in unit time; is the symbol for the decay constant in the equation N = Noe^-t, where No is the initial number of atoms present, and N is the number of atoms present after some time (t).