How many transition elements are there?

The transition elements, also known as transition metals, are a group of elements found in the d-block of the periodic table. They are characterized by their partially filled d orbitals and exhibit a wide range of chemical properties. There are a total of 38 transition elements in the periodic table.

These transition elements include:

Scandium (Sc)
Titanium (Ti)
Vanadium (V)
Chromium (Cr)
Manganese (Mn)
Iron (Fe)
Cobalt (Co)
Nickel (Ni)
Copper (Cu)
Zinc (Zn)
Yttrium (Y)
Zirconium (Zr)
Niobium (Nb)
Molybdenum (Mo)
Technetium (Tc)
Ruthenium (Ru)
Rhodium (Rh)
Palladium (Pd)
Silver (Ag)
Cadmium (Cd)
Hafnium (Hf)
Tantalum (Ta)
Tungsten (W)
Rhenium (Re)
Osmium (Os)
Iridium (Ir)
Platinum (Pt)
Gold (Au)
Mercury (Hg)
Rutherfordium (Rf)
Dubnium (Db)
Seaborgium (Sg)
Bohrium (Bh)
Hassium (Hs)
Meitnerium (Mt)
Darmstadtium (Ds)
Roentgenium (Rg)
Copernicium (Cn)
These elements are known for their ability to form multiple oxidation states and their various applications in chemistry and industry.