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Home All issues Volume 707 (March 2026) A&A, 707 (2026) A224 Full HTML
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Table C.2

Expected tidal mode contributions to ∆C22 and ∆S22

ωlmpqs |ΔC, S2m|(ωlmpq0) ∑s≠0 |ΔC, S2m|(ωlmpqs)
Moon Phobos Moon Phobos
–6 n 2.59 ∙ 10−16 3.85 ∙ 10−18 2.52 ∙ 10−19 2.43 ∙ 10−18
–5 n 2.93 ∙ 10−15 1.87 ∙ 10−16 2.65 ∙ 10−18 1.04 ∙ 10−16
–4n 3.06 ∙ 10−14 8.38 ∙ 10−15 2.11 ∙ 10−17 3.01 ∙ 10−15
–3 n 2.42 ∙ 10−13 2.85 ∙ 10−13 7.99 ∙ 10−18 1.76 ∙ 10−12
–2n 0.0 0.0 1.25 ∙ 10−13 5.75 ∙ 10−10
-n 1.45 ∙ 10−9 3.18 ∙10−8 3.92 ∙ 10−12 4.56 ∙ 10−8
0 0.0 0.0 0.0 0.0
n 1.01 ∙ 10−8 2.22 ∙ 10−7 4.05 ∙ 10−12 4.57 ∙ 10−8
2n 1.55 ∙ 10−9 7.93 ∙ 10−9 8.84 ∙ 10−13 2.58 ∙ 10−9
3n 2.02 ∙ 10−10 2.41 ∙ 10−10 1.35 ∙ 10−13 9.59 ∙ 10−11
4n 2.41 ∙ 10−11 6.70 ∙ 10−12 1.76 ∙ 10−14 2.98 ∙ 10−12
5n 2.75 ∙ 10−12 1.76 ∙ 10−13 2.10 ∙ 10−15 8.40 ∙ 10−14
6n 2.97 ∙ 10−13 4.42 ∙ 10−15 2.36 ∙ 10−16 2.22 ∙ 10−15

Notes. We provide the tidal mode contributions both in the absence of librations (s = 0), and specifically caused by the once-per-orbit libration (s ≠ 0). Are reported the amplitudes of the ∆C22 and ∆S22 variations induced at each forcing mode ωlmpq following Eqs. 38 and 39.

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