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Table 1 Model ages of mare deposits.
The formation ages of mare ridges are constrained by the depositional ages of mare basalts, which are either deformed or dammed by the ridges.
Graphical Abstract The formation ages of mare ridges are constrained by the depositional ages of mare basalts, which are either deformed (orange unit) or dammed (blue unit) by the ridge.
The model ages of mare basalts investigated in our study range from 3.7 to 2.7 Gyr ago (i.e., from the Late Imbrian Epoch to the Eratosthenian Period).
As presented by Haruyama et al. (2009), comparing model ages of mare basalts on the farside and those on the nearside indicates that the timing of the termination of mare volcanism differed between the farside (∼2.5 Ga) and the nearside (∼1.2 Ga).
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Data from the mission has helped to determine the approximate age of Mare Imbrium, suggesting that it is no more than about 4.25 billion years old.
The confounding variables "age of mare" (three levels), "stud", "year" and "stallion" were tested in the model as fixed effects.
The final model included the variables "age of mare", "stud" and "stallion" in addition to "method of semen handling" and the random mare-effect.
Many studies report the negative effect of ageing of mares on the rates of pregnancy and foaling and on the pregnancy loss [ 1, 3, 6, 8- 16, 16, 19- 21].
Fig. 4 The ages of the mare units in the study area.
The estimated model ages of the mare deposits range from 2.7 to 3.5 Ga.
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