We propose a new scenario for early cosmology, where aninflationary de Sitter phase is obtained with a ghost condensate.The transition to radiation dominance is triggered by the ghostitself, without any slow-roll potential. Density perturbations aregenerated by fluctuations around the ghost condensate and can bereliably computed in the effective field theory. The fluctuationsare scale invariant as a consequence of the de Sitter symmetries;however, the size of the perturbations are parametricallydifferent from conventional slow-roll inflation, and the inflationhappens at far lower energy scales. The model makes definitepredictions that distinguish it from standard inflation, and canbe sharply excluded or confirmed by experiments in the nearfuture. The tilt in the scalar spectrum is predicted to vanish(ns = 1), and the gravity wave signal is negligible. Thenon-Gaussianities in the spectrum are predicted to be observable:the 3-point function is determined up to an overall \U0001d4aa(1)constant, and its magnitude is much bigger than in conventionalinflation, with an equivalent fNL≃100, not far fromthe present WMAP bounds.