We report the discovery and confirmation of two sub-Saturn planets orbiting a bright (V = 11.3), metal-rich ([Fe/H] = 0.42 $pm$ 0.04 dex) G3 dwarf in the K2 Campaign 2 field. The planets are 5.68 $pm$ 0.56 Earth-radii and 7.82 $pm$ 0.72 Earth-radii and have orbital periods of 20.8851 $pm$ 0.0003 d and 42.3633$pm$0.0006 d, near to the 2:1 mean-motion resonance. We obtained 32 radial velocities (RVs) with Keck/HIRES and detected the reflex motion due to EPIC-203771098b and c. These planets have masses of 21.0 $pm$ 5.4 Earth-masses and 27.0 $pm$ 6.9 Earth-masses, respectively. With low densities of 0.63 $pm$ 0.25 g/cc and 0.31 $pm$ 0.12 g/cc, respectively, the planets require thick envelopes of H/He to explain their large sizes and low masses. Interior structure models predict that the planets have fairly massive cores of 17.6 $pm$ 4.3 Earth-masses and 16.1 $pm$ 4.2 Earth-masses, respectively. They may have formed exterior to their present locations, accreted their H/He envelopes at large orbital distances, and migrated in as a resonant pair. The proximity to resonance, large transit depths, and host star brightness offer rich opportunities for TTV follow-up. Finally, the low surface gravities of the EPIC-203771098 planets make them favorable targets for transmission spectroscopy by HST, Spitzer, and JWST.
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