Why Is Technetium Radioactive?

Technetium (Tc), element 43, is the lightest element in the periodic table with absolutely no stable isotopes. Every form of Technetium is radioactive, meaning its nucleus will eventually decay. This silvery-grey metal was the first element to be produced artificially in a laboratory in 1937. Trace amounts are now known to occur naturally in the Earth’s crust as a spontaneous fission product of uranium.

The Physics Governing Nuclear Stability

A nucleus’s stability is a delicate balance between the strong nuclear force, which binds protons and neutrons (nucleons) together, and the repulsive electromagnetic force between protons. The strong force is powerful but only operates over extremely short distances. As a nucleus gets larger, the repulsive electromagnetic force gains a significant advantage. To maintain stability, a nucleus requires a specific ratio of neutrons to protons (the N/Z ratio). Stable nuclei fall within a narrow band on a chart of all known isotopes, often called the “Valley of Stability,” while those outside this zone must undergo radioactive decay.

Why Element 43 Has No Stable Isotopes

Technetium’s inherent instability is a direct consequence of its odd atomic number, Z=43. Nuclei with an even number of protons or neutrons are generally more stable because the nucleons can pair up, lowering the overall energy. Elements with an odd number of protons, like Technetium, have far fewer stable isotopes than their even-numbered neighbors, Molybdenum (Z=42) and Ruthenium (Z=44).

The absence of stable Technetium isotopes is due to an energetic “gap” in the Valley of Stability. For every possible Technetium isotope, a neighboring element (Molybdenum or Ruthenium) exists that has a more energetically favorable, stable nucleus with the same total mass number. This systematic energetic preference means that any Technetium isotope is primed to decay into one of these more stable neighbors.

For instance, Technetium-97, -98, and -99 are the longest-lived isotopes. Isotopes with a proton deficiency, like Technetium-97, decay into Molybdenum via electron capture. Those with a neutron excess, such as Technetium-99, decay into Ruthenium via beta decay.

How Technetium Isotopes Undergo Radioactive Decay

The instability of Technetium results in several distinct decay pathways, primarily involving Technetium-99 (\(\text{Tc-99}\)) and its isomer, Technetium-99m (\(\text{Tc-99m}\)).

Technetium-99 Decay

\(\text{Tc-99}\) undergoes beta decay, where a neutron converts into a proton, emitting an electron and an antineutrino. This process transforms the atom into the stable isotope Ruthenium-99 (\(\text{Ru-99}\)). \(\text{Tc-99}\) has a very long half-life of approximately 211,000 years, making it a low-activity, long-lasting radioisotope.

Technetium-99m Decay

\(\text{Tc-99m}\) is a metastable nuclear isomer, meaning it is an excited, higher-energy state of the \(\text{Tc-99}\) nucleus. This excited state relaxes to its lower-energy ground state through isomeric transition, shedding excess energy by emitting a gamma ray photon. \(\text{Tc-99m}\) has a short half-life of about six hours, which is desirable for its widespread use in medical diagnostic procedures.