The orbit of a small object around a significantly more massive object is, for all intents and purposes, entirely unrelated to the mass of the small object. The sun is massive enough, and Earth is small enough by comparison, that the orbital equations can be simplified to a direct relationship between the orbital speed and orbital distance: $v = \sqrt{\frac{GM}{r}}$, where $G$ is the gravitational constant, $M$ is the mass of the larger body, and $r$ is the distance between the two centers of mass.
A 1.3 kilogram CubeSat, at the same orbital distance from the sun as Earth (1 AU), would have the same orbital period (1 year). The mass doesn't matter, even if the mass is changing.
What WOULD change is the orbit of the moon (and anything else orbiting Earth, natural or artificial). As Earth loses mass, its gravity will decrease, and Luna would begin to spiral outward into a higher orbit, farther away from the center of mass. Depending on how much mass is lost, Luna might escape Earth orbit completely.