Table D.2

Initial conditions for the secular eccentricity and inclination variables at time J2000 in the La2004 invariant reference frame (see Sec. D.2), derived from the full LaX13b solution. In the first column,k is the index of the planet, and in columns 2 and 3, and are the real and imaginary part of the eccentricity variables . In columns 4and 5, and are the same quantities for the inclination variables.

k
1	+ 5.6990505842292892e-2	+ 1.9872894591036927e-1	+ 4.6165713227763444e-2	+ 2.9410664010632515e-2
2	− 4.1735654068702976e-3	+ 5.3327342759766343e-3	+ 1.1928053604473932e-2	+ 1.4987173725293589e-2
3	− 2.7278550885769647e-3	+ 1.6484645103357756e-2	+ 3.3422496351974010e-3	− 1.3363750560862579e-2
4	+ 8.2969437680297631e-2	− 4.3116239799066092e-2	+ 1.4518563462960753e-2	− 1.7430317715928134e-3
5	+ 4.7651130651270288e-2	+ 9.0836135513906891e-3	+ 1.9689371814761709e-3	− 2.0725403616100885e-3
6	+ 4.7464039310316251e-4	+ 5.5529067938940795e-2	− 4.1232378462891421e-3	+ 7.0205383101661738e-3
7	− 4.5530988000471201e-2	+ 8.4408377405346107e-3	+ 5.5957559447492129e-3	− 7.0021269706505322e-3
8	+ 6.4028803643053234e-3	+ 6.3248118090214632e-3	− 6.2175356759488895e-3	− 1.2331754395710286e-3