| RING_PHASECURV_90 | | Working Group 2 |
| RING_PHASECURV_80 | | Working Group 2 |
| RING_PHASECURV_70 | | Working Group 2 |
| RING_PHASECURV_60 | | Working Group 2 |
| RING_PHASECURV_50 | | Working Group 2 |
| RING_PHASECURV_40 | | Working Group 2 |
| RING_PHASECURV_30 | | Working Group 2 |
| RING_PHASECURV_20 | | Working Group 2 |
| RING_PHASECURV_170 | | Working Group 2 |
| RING_PHASECURV_160 | | Working Group 2 |
| RING_PHASECURV_150 | | Working Group 2 |
| RING_PHASECURV_140 | | Working Group 2 |
| RING_PHASECURV_130 | | Working Group 2 |
| RING_PHASECURV_120 | | Working Group 2 |
| RING_PHASECURV_110 | | Working Group 2 |
| RING_PHASECURV_100 | | Working Group 2 |
| J_SAT_VALETUDO | | Working Group 2 |
| J_SAT_THEMISTO | | Working Group 2 |
| J_SAT_TAYGETE | | Working Group 2 |
| J_SAT_SINOPE | | Working Group 2 |
| J_SAT_PRAXIDIKE | | Working Group 2 |
| J_SAT_PASITHEE | | Working Group 2 |
| J_SAT_PASIPHAE | | Working Group 2 |
| J_SAT_PANDIA | | Working Group 2 |
| J_SAT_MEGACLITE | | Working Group 2 |
| J_SAT_LYSITHEA | | Working Group 2 |
| J_SAT_LEDA | | Working Group 2 |
| J_SAT_KALLICHORE | | Working Group 2 |
| J_SAT_ISONOE | | Working Group 2 |
| J_SAT_IRR_CHAR_E | | Working Group 2 |
| J_SAT_IRR_AST_E | | Working Group 2 |
| J_SAT_IOCASTE | | Working Group 2 |
| J_SAT_INN_CHAR_A | | Working Group 2 |
| J_SAT_INN_AST_T | | Working Group 2 |
| J_SAT_INN_AST_A | | Working Group 2 |
| J_SAT_HIMALIA | | Working Group 2 |
| J_SAT_HERSE | | Working Group 2 |
| J_SAT_HERMIPPE | | Working Group 2 |
| J_SAT_HELIKE | | Working Group 2 |
| J_SAT_HEGEMONE | | Working Group 2 |
| J_SAT_HARPALYKE | | Working Group 2 |
| J_SAT_ERSA | | Working Group 2 |
| J_SAT_ERINOME | | Working Group 2 |
| J_SAT_ELARA | | Working Group 2 |
| J_SAT_CHALDENE | | Working Group 2 |
| J_SAT_CARME | | Working Group 2 |
| J_SAT_CALLIRRHOE | | Working Group 2 |
| J_SAT_AUTONOE | | Working Group 2 |
| J_SAT_ARCHE | | Working Group 2 |
| J_SAT_AOEDE | | Working Group 2 |
| J_SAT_ANANKE | | Working Group 2 |
| J_RING | | Working Group 2 |
| IO_RS | | Working Group 2 |
| GANYMEDE_FLYBY_WG2 | | Working Group 2 |
| GANYMEDE_DISTANT | | Working Group 2 |
| G_RS_5G5 | | Working Group 2 |
| G_RS_4G4 | | Working Group 2 |
| G_RS_2G2 | | Working Group 2 |
| G_RS_26G11 | | Working Group 2 |
| G_RS_25G10 | | Working Group 2 |
| G_RS_24G9 | | Working Group 2 |
| G_RS_23G8 | | Working Group 2 |
| G_RS_22G7 | | Working Group 2 |
| G_RS_1G1 | | Working Group 2 |
| G_RS_18G6 | | Working Group 2 |
| G_RS_17G5 | | Working Group 2 |
| G_distant | | Working Group 2 |
| FB_RS | | Working Group 2 |
| EUROPA_FLYBY_WG2 | | Working Group 2 |
| EUROPA_DISTANT | | Working Group 2 |
| E_RS_7E2 | | Working Group 2 |
| E_RS_6E1 | | Working Group 2 |
| E_RS | | Working Group 2 |
| E_distant | | Working Group 2 |
| CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
| CALLISTO_FLYBY_WG2 | | Working Group 2 |
| CALLISTO_DISTANT | | Working Group 2 |
| C_RS_9C3 | | Working Group 2 |
| C_RS_8C2 | | Working Group 2 |
| C_RS_5C1 | | Working Group 2 |
| C_RS_21C13 | | Working Group 2 |
| C_RS_20C12 | | Working Group 2 |
| C_RS_19C11 | | Working Group 2 |
| C_RS_16C10 | | Working Group 2 |
| C_RS_15C9 | | Working Group 2 |
| C_RS_14C8 | | Working Group 2 |
| C_RS_13C7 | | Working Group 2 |
| C_RS_12C6 | | Working Group 2 |
| C_RS_11C5 | | Working Group 2 |
| C_RS_10C4 | | Working Group 2 |
| C_RS | | Working Group 2 |
| C_distant | | Working Group 2 |
| ASTRO_IRR2_SINOPE | | Working Group 2 |
| ASTRO_IRR_ELARA | | Working Group 2 |
| IO_MONITORING | - JANUS minimum distance = 7.00e+05 km
- MAJIS minimum distance = 8.00e+05 km
- SWI minimum distance = 6.00e+05 km (able to resolve target when angular size is > 1 mrad)
| Working Group 2 |
| ASTRO_INNER | Astrometry inner moons | Working Group 2 |
| ASTRO_IRR2_ANANKE | Astrometry irregular moon Ananke | Working Group 2 |
| ASTRO_IRR2_CARME | Astrometry irregular moon Carme | Working Group 2 |
| ASTRO_IRR1_CARPO | Astrometry irregular moon CARPO | Working Group 2 |
| ASTRO_IRR1_CHALDENE | Astrometry irregular moon CHALDENE | Working Group 2 |