The atomic radius of main group elements exhibits a clear trend: it decreases from left to right across a period and also decreases as one moves up a group in the periodic table. This trend is primarily influenced by the increasing nuclear charge, which pulls the outermost electrons closer to the nucleus, thereby reducing the atomic size. In contrast, transition metals follow a similar trend, but the change in atomic radius is more gradual and less pronounced.
As we examine the atomic structure, the principal quantum number \( n \) represents the outermost shell of electrons. For transition metals, the outer shell typically consists of \( s \) orbitals, which can accommodate one or two electrons. For instance, in the case of technetium (Tc) with an electron configuration of \([Kr] 4d^5 5s^2\) and rhenium (Re) with \([Xe] 4f^{14} 5d^5 6s^2\), we observe that Tc has its outer electrons in the 5th shell while Re has its outer electrons in the 6th shell. Despite the addition of electrons, the outer shell remains constant in size, as the additional electrons are being added to the inner \( d \) or \( f \) orbitals.
This phenomenon explains why the atomic radius of transition metals does not decrease as significantly as that of main group elements. The outer shell's electron count remains stable, leading to only slight variations in atomic radius among transition metals, particularly in rows 5 and 6. The 7th row is often excluded from this discussion due to the unpredictable behavior of synthetic heavy elements.
In summary, while the atomic radius decreases more prominently among main group elements, the transition metals exhibit a more gradual change due to the constant outer shell size and the addition of electrons to inner orbitals. This understanding sets the stage for exploring further phenomena that influence atomic radius in different contexts.