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Table 1
Parameter values used for computing the relativistic contributions to the Mars BCRS rotation model, in the frame of analytical and toy model developments of Sects. 2.2 and 3.1, where the orbit of the planets are assumed to be Keplerian.
| Parameter | Value | Reference |
|---|---|---|
| GM⊙ | 1.3271244 × 1020 m3 s−2 | Simon et al. (2013) |
| GMJ | 1.2671 × 1017 m3 s−2 | ibid |
| GMS | 3.794 × 1016 m3 s−2 | ibid |
| a | 2.27939 × 1011 m | ibid |
| aJ | 7.78298 × 1011 m | ibid |
| aS | 1.42939 × 1012 m | ibid |
| e | 0.09340 | ibid, as  |
| c | 299792458 ms−1 | ibid |
| n | 1.058576 × 10−7 rad s−1 | ibid |
| nJ | 1.678489 × 10−8 rad s−1 | ibid |
| nS | 6.759040 × 10−9 rad s−1 | ibid |
 |
350°.891985339 day−1 | Le Maistre et al. (in prep.) |
| ε0 | 25°.18940927 | Le Maistre et al. (in prep.) |
| 35°.437639 | adapted from Le Maistre et al. (in prep.) | |
| S ⊙ | 1 .909 × 1041 kg m2 s−1 | Pijpers (1998) |
| α⊙ | 304°.414 | Adapted from Archinal et al. (2018) |
| δ⊙ | 84°.351 | Adapted from Archinal et al. (2018) |
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