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. Author manuscript; available in PMC: 2019 Apr 22.
Published in final edited form as: Astrophys J. 2017 Feb 13;836(1):109. doi: 10.3847/1538-4357/836/1/109

Table 7.

Data for all 4 Sets at t = 109 years.

Set A Set B Set C Set D
< Mring/MMET > 0.12 ± 0.02 0.12 ± 0.01 0.12 ± 0.02 0.11 ± 0.02
< Lring/LMET > 0.07 ± 0.01 0.07 ± 0.01 0.07 ± 0.01 0.06 ± 0.01
< Msats/MMET > 2.12 ± 1.02 2.62 ± 1.66 2.13 ± 1.02 1.95 ± 1.01
< Msats/Mring,0 > 0.22 ± 0.01 0.25 ± 0.05 0.22 ± 0.01 0.2 ± 0.01
< Lsats/LMET > 2.18 ± 1.1 2.67 ± 1.78 2.2 ± 1.13 1.87 ± 1.03
< ΔLDR//LMET > N/A N/A 0.09 ± 0.1 0.11 ± 0.08

Note—Average values at 109 for the 4 sets of simulations. Mring is the rings’ mass, MMET is the total mass of Mimas, Enceladus and Tethys, Lring is the rings’ angular momentum, Msats is the total mass of the spawned satellites in a given Run (excluding Dione and Rhea), Mring,0 is the rings’ initial mass, Lsats is the angular momentum of the spawned satellites in a given Run (excluding Dione and Rhea), LMET is the total angular momentum of Mimas, Enceladus and Tethys, and < ΔLDR/LMET > is the variation of angular momentum of Dione and Rhea.