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. 2000 Mar 21;97(8):3814–3819. doi: 10.1073/pnas.070047197

Table 2.

Computation of angular velocity of moon at syzygy, γ

To compute γ we employ the expression:
graphic file with name M1.gif
where, for full moon and new moon, respectively:
 γm = 17.1650, 17.1489 deg⋅day−1
a1 = 0.002326, 0.001663 deg⋅day−1⋅hr−1
a2 = 0.007372, 0.006742 deg⋅day−1
a3 = 0.09323, 0.08706 deg⋅day−1
f1 = 0.4508 ΔTperig − 1.4505 − 0.0254 ΔTperih
f2 = 4.8254 sin (2π ΔTnode/(24.)(27.212220)) − 0.06545
f3 = (1 − cos(2π ΔTperih/365.))
where ΔTperig (in hours), ΔTnode (in hours), and ΔTperih (in days) are,  respectively, the separation-intervals of syzygy from perigee,  lunar node, and perihelion.