Conformational Mobility of (-)-α-Phellandrene, Deduced from its Optical Rotatory Dispersion
Conformational Mobility of (-)-α-Phellandrene, Deduced from its Optical Rotatory Dispersion
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(-)-α-水芹烯的构象迁移率,由其旋光色散推导
DOI:
10.1021/ja00874a024
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发表时间:
1962
影响因子:
15
通讯作者:
U. Weiss
中科院分区:
文献类型:
--
作者:
H. Ziffer;E. Charney;U. Weiss
The optical rotations of (—)-a-phellandrene (I) and 3, 5-cholestadiene (III) have been measured at 11, 23, and 82. The observed temperature-dependence of the rotation of I, but not of III, is interpreted as indicating the existence of a mobile equilibrium between two conformations of I. The populations and relative stabilities of these conformers are discussed. It is concluded that one of these conformers la has the larger rotational strength, but it is present in smaller concentrations than lb, at least at room temperature.In a recent communication from this Laboratory1 it was deduced from the rotatory dispersion curve of (—)-a-phellandrene that the preferred conforma-tion of this molecule is that in which the isopropyl group is quasi-axial (IA). This conclusion was based on the “skewed diene’’rule2 which allows the sign of the optical rotation of a molecule con-taining a non-planar cisoiddiene to be predicted from the skew sense or helicity of the diene: if the four carbon atoms of the conjugated system form a left-handed helix, its contribution on the long-wave length side of the diene absorption band produces levorotation, whereas a right-handed helix produces dextrorotation. Furthermore, the contribution to the optical activity produced by the skewed diene is much greaterthan that associated with, eg, an asymmetric carbon atom. Conse-quently, the rotatory dispersion in the vicinity of the diene absorption will largely reflect the relative orientation of the double bonds of the chromophore. By this reasoning, in the case of (—)-a-phellan-drene of known absolute configuration, the observed negative rotation suggested that the predominant conformer at room temperature was the quasi-axial (IA) rather than the quasi-equatorial