Figure 2 from Planetary Phase Variations of the 55 Cancri System

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Planetary Phase Variations of the 55 Cancri System

Authors: Stephen R. Kane, Dawn M. Gelino, David R. Ciardi, Diana Dragomir, and Kaspar von Braun

Kane et al. 2011 The Astrophysical Journal 740 61.

Caption: Figure 2.

As for the top two panels of Figure 1, but the e planet is now assumed to have a molten surface with a geometric albedo of 0.6 (see Section 4.2).