Fig. 12
Jupiter geometric albedo from PlanetCam VIS observations (blue dots) compared to reference values from ground-based observations in July 1995 (Karkoschka 1998; black line) and February 2016 HST-OPAL data (Simon et al. 2015; red dots). Horizontal error bars account for the width (FWHM) of each filter, while vertical error bars indicate the uncertainty in the photometric calibration.
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