Calibrating astronomical spectrographs to discover Earth-like planets

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This project aims to develop a robust, ultra-precise calibration system that improves the precision of Doppler spectrographs by a factor of ten –sufficient to discover rocky planets. The holy grail of exoplanet research is the discovery of an Earth-like planet in the habitable zone of a Sun-like star. The planet’s tug on its host star causes a periodic Doppler shift of the star’s spectrum which precision astronomical spectrographs record. Detecting minute shifts from rocky planets needs better precision than the best spectrographs provide. This project expects to help to discover Earth twins, habitable worlds outside the Solar system.