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We present the science results from the first two years of the Solar-Stellar Spectrograph (SSS) project. These results will include (1) representative observations from our current database of $\approx 1500$ spectra of about 200 solarlike stars, (2) a discussion of their calibration to flux, (3) our initial detections of cyclic as well as shorter-term variability, (4) variability correlations between various diagnostic lines, (5) the unification of our flux-calibrated data to all extant datasets, in particular the Mt.\ Wilson $S$ index, and (6) the consistent placement of the Sun among the stellar sample.
