  To understand how best to use observations of Type Ia supernovae (SNe Ia) to
obtain precise and accurate distances, we investigate the relations between
spectra of SNe Ia and their intrinsic colors. Using a sample of 1630 optical
spectra of 255 SNe, based primarily on data from the CfA Supernova Program, we
examine how the velocity evolution and line strengths of Si II 6355 and Ca II
H&K are related to the B-V color at peak brightness. We find that the
maximum-light velocity of Si II 6355 and Ca II H&K and the maximum-light
pseudo-equivalent width of Si II 6355 are correlated with intrinsic color, with
intrinsic color having a linear relation with the Si II 6355 measurements. Ca
II H&K does not have a linear relation with intrinsic color, but lower-velocity
SNe tend to be intrinsically bluer. Combining the spectroscopic measurements
does not improve intrinsic color inference. The intrinsic color scatter is
larger for higher-velocity SNe Ia --- even after removing a linear trend with
velocity --- indicating that lower-velocity SNe Ia are more "standard crayons."
Employing information derived from SN Ia spectra has the potential to improve
the measurements of extragalactic distances and the cosmological properties
inferred from them.
