  We present a catalog of spectra and geometric albedos, representative of the
different types of Solar System bodies, from 0.45 to 2.5 microns. We analyzed
published calibrated, un-calibrated spectra, and albedos for Solar System
objects and derived a set of reference spectra and reference albedo for 19
objects that are representative of the diversity of bodies in our Solar System.
We also identified previously published data that appears contaminated. Our
catalog provides a baseline for comparison of exoplanet observations to 19
bodies in our own Solar System, which can assist in the prioritization of
exoplanets for time-intensive follow-up with next-generation Extremely Large
Telescopes (ELTs) and space-based direct observation missions. Using high and
low-resolution spectra of these Solar System objects, we also derive colors for
these bodies and explore how a color-color diagram could be used to initially
distinguish between rocky, icy, and gaseous exoplanets. We explore how the
colors of Solar System analog bodies would change when orbiting different host
stars. This catalog of Solar System reference spectra and albedos is available
for download through the Carl Sagan Institute.
