Ab initio geometry optimizations at the RHF/3-2tG basis set level were calculated for equatorial and axial N-methyl diastereomers of O-formyltropine and O-formylscopine esters and other model compounds. These optimized geometries were then utilized as input for single-point energy calculations using the higher level RHF/6-31G* basis set to afford a more precise estimation of the total energies and atomic charges. Ethano bridge "pinching" of the N-protonated tropanyl piperidine moiety pushes the smaller axial N-proton closer toward the neighboring two axial C--H bonds compared with the analogous case for a bulky axial N-methyl. Increased cisl,3-diaxial interactions in the axial N-methyl diastereomer destabilize this epimer in favor of the equatorial N-methyl counterpart [e.g., 2.121 kcal/mol lower energy for the equatorial N-methyl O-formyltropine N-protonated diastereomer (12) than for the axial epimer (13)]. Lower pyramidality at nitrogen in the free base maintains the relative stability of the equatorial N-methyl free base diastereomer (14) (1.120 kcal/mol more stable than the axial free base 15). A nonprotonated carbon atom at the apex of a three-membered ring fused to the 6,7-positions of the O-formyltropine skeleton results in severe transannular nonbonding steric interactions involving the neighboring equatorial N-methyl group in N-protonated 16 (3.335 kcal/mol less stable than the axial N-methyl epimer 17, where these transannular interactions are reduced due to the smaller equatorial N--H proton). Oxygen atom occupation of the apex of a similar fused three-membered ring retains the same severe transannular nonbonding steric interactions involving the neighboring equatorial N-methyl group in N-protonated 18. These transannular interactions now become electrostatically attractive in the N-protonated axial N-methyl epimer 19 (2.031 kcal/mol more stable than the equatorial epimer). Reduced pyramidality at nitrogen in the O-formylscopine free base reduces the repulsive transannular interaction with the neighboring equatorial N-methyl group compared to that in the N-protonated form. Lowered pyramidality also reduces the cis-l,3-diaxial interactions in the axial N-methyl epimer, but the nitrogen lone pair is pushed close to the transannular oxygen lone pair as a result (the equatorial N-methyl free base 20 is 3.870 kcal/mol more stable than the axial epimer 21). These ab initio-calculated models of O-formyltropines and O-formylscopine N-methyl diastereomeric protonated cations and free bases provide stereochemical insight into the relative stabilities of solution-state atropine and scopolamine N-methyl species previously observed by NMR spectroscopic methods.KEY WORDS: Scopolamine; atropine; scopine; tropine; ab initio; X-ray crystallography; NMR. . It was reasoned that the root of this confusion resulted from a very broadened low-intensity 6 33 N-CH 3 signal (width at half-height W1/2 = 55 Hz) in D20 which could be buried in the baseline noise of a low-S/N spectrum [12]. The relatively low 7.55 pK~ value of pro...