Table F.2
Quasi-periodic representation of the orbital dynamics of Venus.
| z | ζ | ||||
|---|---|---|---|---|---|
 |
Ej × 108 |  |
 |
Sj × 108 |  |
| 7.45592 | 2085594 | 200.24 | 0.00000 | 1377170 | 107.59 |
| 4.24882 | 1963621 | 30.67 | −18.85115 | 953835 | 60.43 |
| 17.91550 | 1346128 | 335.25 | −5.61755 | 671575 | 348.70 |
| 17.36469 | 1164633 | 123.95 | −17.74818 | 575205 | 123.28 |
| 5.59644 | 659312 | 110.35 | −7.07963 | 404368 | 93.77 |
| 17.08266 | 324058 | 179.38 | −18.30007 | 298364 | 89.80 |
| 5.47449 | 248173 | 275.01 | −5.50098 | 239467 | 342.89 |
| 16.81285 | 239435 | 274.43 | −6.84091 | 208804 | 286.39 |
| 6.93423 | 216696 | 169.77 | −7.19493 | 201837 | 285.16 |
| 17.63081 | 191660 | 193.67 | −6.96094 | 191673 | 277.95 |
| 5.71670 | 188411 | 120.52 | −19.40256 | 188959 | 209.10 |
| 7.05595 | 178786 | 358.98 | −7.33264 | 116984 | 16.75 |
| 7.34103 | 176112 | 207.85 | −3.00557 | 99208 | 140.33 |
| 17.81084 | 129713 | 58.56 | −19.13075 | 88217 | 305.90 |
| 7.57299 | 122891 | 11.47 | −5.85017 | 80983 | 165.47 |
| 18.18553 | 118540 | 57.28 | −0.69189 | 65885 | 23.96 |
| 19.01870 | 116085 | 219.75 | −5.21610 | 60616 | 18.91 |
| 17.15752 | 111520 | 325.02 | −5.37178 | 60304 | 35.48 |
| 18.46794 | 110955 | 6.95 | −5.10025 | 59016 | 195.38 |
| 5.35823 | 101244 | 94.89 | −18.01114 | 43620 | 242.09 |
| 17.72293 | 97999 | 48.46 | −17.66094 | 41358 | 138.93 |
| 18.01611 | 83405 | 44.83 | −6.73842 | 38337 | 224.50 |
| 16.52731 | 67232 | 131.91 | −18.97001 | 36654 | 73.36 |
| 17.47683 | 58638 | 260.26 | −7.40536 | 35440 | 53.35 |
| 16.26122 | 57777 | 58.89 | −5.96899 | 34592 | 350.64 |
| 6.82468 | 57706 | 194.53 | −17.83857 | 33636 | 289.13 |
| 3.08952 | 54138 | 121.36 | −7.48780 | 32924 | 227.95 |
| 18.08627 | 48156 | 356.17 | −6.56016 | 30942 | 123.47 |
| 17.55234 | 47190 | 197.65 | −17.54636 | 29977 | 246.71 |
| 5.99227 | 37236 | 113.56 | −8.42342 | 25773 | 31.21 |
| 7.20563 | 36013 | 143.91 | −6.15490 | 25048 | 89.77 |
| 5.65485 | 35915 | 39.22 | −17.94404 | 21099 | 212.26 |
| 5.23841 | 29809 | 272.97 | −18.59563 | 19361 | 98.11 |
| 7.71663 | 22441 | 93.52 | −18.69743 | 19259 | 221.70 |
| 4.36906 | 20218 | 220.79 | −18.77933 | 18879 | 222.83 |
| 28.22069 | 16949 | 308.38 | −18.22681 | 18853 | 46.30 |
| 5.40817 | 3036 | 120.48 | −19.06544 | 16888 | 50.21 |
| −19.72306 | 1161 | 113.24 | −17.19656 | 11902 | 171.81 |
| 0.66708 | 1088 | 73.98 | 18.14984 | 9063 | 111.19 |
| 27.06140 | 536 | 218.72 | −26.33023 | 5577 | 127.29 |
| 4.89647 | 470 | 291.97 | −2.35835 | 2677 | 44.72 |
| 29.37998 | 416 | 217.51 | −1.84625 | 2187 | 40.13 |
| 52.19257 | 339 | 225.73 | −4.16482 | 2022 | 51.60 |
| 28.86795 | 277 | 32.64 | −3.11725 | 663 | 326.97 |
| 27.57346 | 244 | 43.74 | −0.58033 | 641 | 17.33 |
| 3.60029 | 242 | 121.40 | −50.30212 | 215 | 29.83 |
| −56.90922 | 216 | 44.11 | 11.50319 | 212 | 281.02 |
| 2.97706 | 141 | 306.81 | −1.19906 | 194 | 133.77 |
| 1.93168 | 69 | 93.94 | 0.46547 | 184 | 286.88 |
| −20.88236 | 67 | 203.93 | −26.97744 | 128 | 44.89 |
| 76.16447 | 63 | 143.03 | 10.34389 | 98 | 191.39 |
| 1.82121 | 46 | 148.00 | 20.96631 | 82 | 57.78 |
| 51.03334 | 35 | 316.30 | 0.57829 | 64 | 103.72 |
| 0.77840 | 19 | 65.10 | 9.18847 | 36 | 1.15 |
| 53.35188 | 16 | 135.62 | 82.77163 | 24 | 128.95 |
| −0.49216 | 5 | 164.74 | 58.80017 | 14 | 212.90 |
| 34.82788 | 11 | 294.12 | |||
| −27.48935 | 7 | 218.53 | |||
| −25.17116 | 7 | 215.94 | |||
| −28.13656 | 5 | 314.08 | |||
Notes. This representation is used in Fig. 3. It has been directly obtained from Laskar (1990), see text.
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