2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Ephemerides/mimas-orb-all Mimas 2023-03-08T16:41:53Z A number of features in Saturn's rings are related to resonances with Mimas. Mimas is responsible for clearing the material from the Cassini Division, the gap between Saturn's two widest rings, the A Ring and B Ring. Particles in the Huygens Gap at the inner edge of the Cassini division are in a 2:1 resonance with Mimas. They orbit twice for each orbit of Mimas. The repeated pulls by Mimas on the Cassini division particles, always in the same direction in space, force them into new orbits outside the gap. The boundary between the C and B ring is in a 3:1 resonance with Mimas. Recently, the G Ring was found to be in a 7:6 co-rotation eccentricity resonance[clarification needed] with Mimas; the ring's inner edge is about 15,000 km (9,300 mi) inside Mimas's orbit. Mimas is also in a 2:1 mean-motion resonance with the larger moon Tethys, and in a 2:3 resonance with the outer F Ring shepherd moonlet, Pandora. spase://CNES/Person/CDPP-AMDA/NAIF PrincipalInvestigator sat-moons-orb PartOf Saturn Moons spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi mimas-orb-all Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. SPICE spase://CNES/Instrument/CDPP-AMDA/Ephemerides Ephemeris 1970-01-01T00:00:00Z 2035-01-19T23:19:31Z PT20M Saturn Saturn.Mimas distance mimas-saturn mim_sat_r Rs TimeSeries Positional xyz_ksm mim_sat_ksm Rs Cartesian KSM TimeSeries 3 x 1 mim_sat_ksm(0) y 2 mim_sat_ksm(1) z 3 mim_sat_ksm(2) Positional xyz_kso mim_sat_kso Rs Cartesian KSO TimeSeries 3 x 1 mim_sat_kso(0) y 2 mim_sat_kso(1) z 3 mim_sat_kso(2) Positional xyz_IAU_saturn mim_sat_xyz Rs TimeSeries 3 x 1 mim_sat_xyz(0) y 2 mim_sat_xyz(1) z 3 mim_sat_xyz(2) Positional latitude IAU_saturn mim_sat_lat deg Positional longitude IAU_saturn mim_sat_lon deg Positional