Inferring and Interpreting the Visual Geometric Albedo and Phase Function of Earth
Tyler D. Robinson

TL;DR
This paper accurately determines Earth's visual geometric albedo and phase function using ground and spacecraft data, revealing a lower albedo than previously thought and analyzing the effects of clouds, aerosols, and ocean glint on planetary brightness.
Contribution
It introduces a physical-statistical model for interpreting Earth's phase curves, providing a definitive albedo value and insights into scattering processes affecting planetary reflectance.
Findings
Earth's geometric albedo is approximately 0.242, 30-40% lower than earlier estimates.
Aerosol forward scattering can mimic ocean glint, affecting habitability assessments.
Phase curve analysis can disentangle surface and atmospheric contributions at different wavelengths.
Abstract
Understanding reflectance-related quantities for worlds enables effective comparative planetology and strengthens mission planning and execution. Measurements of these properties for Earth, especially its geometric albedo and phase function, have been difficult to achieve due to our Terrestrial situation -- it is challenging to obtain planetary-scale brightness measurements for the world we stand on. Using a curated dataset of visual (0.4--0.7 um) phase-dependent, disk-averaged observations of Earth taken from the ground and spacecraft, alongside a physical-statistical model, this work arrives at a definitive value for the visual geometric albedo of our planet: . This albedo constraint is up 30--40% smaller than earlier, widely-quoted values. The physical-statistical model enables retrieval-like inferences to be performed on phase curves, and includes…
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