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. 2006 Nov 3;103(46):17184–17189. doi: 10.1073/pnas.0608163103

Fig. 1.

Fig. 1.

Shadowing geometry. (Left) Schematic. The L1 point and the common Earth–moon barycenter remain in-line as they both orbit the sun with a 1-year period (not to scale). (Right) Time-averaged view from Earth. The Earth wobbles with a 1-month period relative to the penumbral shadows cast from a sunshade at 1.5 and 2.4 Gm (dashed circles).