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We present an analysis of high-resolution imaging of an exoplanet by ameter-class telescope positioned at a real image of the exoplanet created bythe solar gravity lens. We assume an exoplanet viewed in full phase and asimple deconvolution method to correct for the intrinsic blur caused byaberrations in the solar gravity lens, and account for the foreground light ofthe solar corona. We derive equations for the measurement times required forthe telescope to produce such a high-resolution image, and find that due toshot noise considerations these times are large compared to human lifespans. Wealso discuss how measurement times could potentially be significantly shorterfor exoplanets with special orbital and rotational parameters.

Photometric Limits on the High Resolution Imaging of Exoplanets Using the Solar Gravity Lens