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Table 4
Maximal amplitude of the signature in the range and the Doppler observables of the relativistic variations in the rotation angles for a lander in Elysium Planitia and using the RISE timing.
| Contribution | Magnitude (mas) | Signature in range obs. (m) | Signature in (mm s−1) | Doppler obs. (mHz) |
|---|---|---|---|---|
| Periodic variations in ϕ (seasonal and relativistic) | 670 | 10 | 0.56 | 31 |
| [ϕ]GR(t) (periodic terms only) | 167 | 2.7 | 0.14 | 7.8 |
| [ϕ]GR(t) (linear and periodic terms) | 58 000 | 950 | 49 | 2800 |
| [ϕ]GR,this paper − [ϕ]GR, Yoder & Standish (1997) | 8.8 | 0.14 | 0.007 | 0.41 |
| Liquid core contribution to nutations | ~20–30 | ~0.3 | ~0.01 | ~0.5 |
| ψso (geodetic nutation only) | 0.6 | 0.001 | 0.0001 | 0.007 |
| ψso (geodetic nutation and linear term) | 150 | 0.44 | 0.03 | 1.7 |
| InSight/RISE noise level | 0.02 | 1.1 | ||
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