  Within the context of a fractal paradigm that emphasizes nature's
well-stratified hierarchical organization, the delta Scuti class of variable
stars is investigated for evidence of discrete cosmological self-similarity.
Methods that were successfully applied to the RR Lyrae class of variable stars
are used to identify Atomic Scale analogues to delta Scuti stars and their
relevant range of energy levels. The mass, pulsation mode and fundamental
oscillation period of a well-studied delta Scuti star are shown to be
quantitatively self-similar to the counterpart parameters of a uniquely
identified Atomic Scale analogue. Several additional tests confirm the
specificity of the discrete fractal relationship.
