The optical constants n(r) + in(i) of liquid methane and phase I solid
methane were determined over the entire spectral range by the use of
various data sources published in the literature. Kramers-Kronig analy
ses were performed on the absorption spectra of liquid methane at the
boiling point (111 K) and the melting point (90 K) and on the absorpti
on spectra of phase I solid methane at the melting point and at 30 K.
Measurements of the static dielectric constant at these temperatures a
nd refractive indices determined over limited spectral ranges were use
d as constraints in the analyses. Applications of methane optical prop
erties to studies of outer solar system bodies are described.