Fig. 2
Differences in the eccentricity of the Earth-Moon barycenter over 1 Myr for various solutions as follows: a1 = La2004-INPOP08; a2 = La2010d-INPOP08; a3 =b3= La2010a – INPOP08; a4=INPOP06-INPOP08; b1 = La2010b – INPOP08; b2 = La2010c -INPOP06. We note that the vertical scale is enlarged ten times in the bottom plot. All solutions are compared to INPOP08. In the top figure, La2010d (a2) and INPOP06 (a4) are almost superimposed. This is because La2010d was adjusted over INPOP06.
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