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. 2021 Dec 1;126(12):e2021JE006875. doi: 10.1029/2021JE006875

Table 6.

Present‐Day Secular Rates of Change of Earth Rotation Rate ωE, Obliquity ε, and Earth‐Moon Orbital Parameters a (Semi‐Major Axis), e (Eccentricity), and i (Inclination), due to Tides on Earth, Tides Within the Moon, and Lunar Core‐Mantle Boundary Effects (CMB) a , b

Constituent
dadt(mmyear)
dedt(1012year)
didt(μasyear)
dεdt(μasyear)
dωEdtcentury2
Long‐period tides
Mf
−0.161 0.0057 0.0019 −0.528 0
Mm
−0.0178 −0.416 0 0 0
Diurnal tides
K1
0 0 0 −9.51 −93.7
O1
4.98 −0.176 −0.0596 8.83 −73.8
P1
0 0 0 1.36 −11.4
Q1
0.283 2.20 −0.0023 0.335 −2.80
Ω (K1 nodal) 0 0 −0.172 0.0154 −1.72
L+F (O1 nodal) 0.181 −0.0064 0.266 0.0241 −2.68
Semi‐diurnal tides
K2
0 0 0 −1.10 −10.9
M2
31.3 −1.11 −0.375 8.37 −930
S2
0 0 0 1.32 −147
N2
2.23 17.4 −0.0178 0.397 −44.2
Ω (K2 nodal) 0 0 −0.0489 −0.0452 −0.978
L+F (M2 nodal) 0.0429 −0.0015 0.0633 −0.0590 −1.27
Tides within the Moon c
−0.387 (−0.471) −5.49 (−6.9) −0.459 (−0.51)
Lunar core‐mantle boundary (CMB) c
−0.0143 (−0.015) 0 (0) −0.0429 (−0.04)
a

Shown are results for 14 constituents of tides on Earth, as included in our orbital dynamics model.

b

Effects of lunar tides and lunar core‐mantle boundary (CMB) computed respectively from Equations (40), (41), (42) and (46), (47), (48), and parameter values used in this study.

c

DE440 values are given in parentheses.