| G_RS_18G6 | | Working Group 2 |
| G_RS_17G5 | | 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_9C3 | | Working Group 2 |
| C_RS_8C2 | | Working Group 2 |
| E_RS_7E2 | | Working Group 2 |
| E_RS_6E1 | | Working Group 2 |
| C_RS_5C1 | | Working Group 2 |
| G_RS_4G4 | | Working Group 2 |
| G_RS_3G3 | HAA as per 3GM UM
IS considering NIM | Working Group 2 |
| G_RS_2G2 | | Working Group 2 |
| ASTRO_INNER | Astrometry inner moons | Working Group 2 |
| CHAR_IRR1 | Characterization irregular moons group 1 (see list below) | Working Group 2 |
| IO_RS | | Working Group 2 |
| J_RING | | Working Group 2 |
| EUROPA_FB_RS | Europa Flyby remote sensing | Working Group 2 |
| CALLISTO_FB_RS | Callisto Flyby remote sensing | Working Group 2 |
| GANYMEDE_FB_RS | Ganymede flyby remote sensing | Working Group 2 |
| FB_RS | | Working Group 2 |
| G_distant | | Working Group 2 |
| E_RS | | Working Group 2 |
| E_distant | | Working Group 2 |
| C_RS | | Working Group 2 |
| C_distant | | Working Group 2 |
| ASTRO_IRR2_PASIPHAE | astrometry measurement with inertial pointing to moon Pasiphae | Working Group 2 |
| ASTRO_IRR2_SINOPE | | Working Group 2 |
| ASTRO_IRR_ELARA | | Working Group 2 |
| CALLISTO_DISTANT | | Working Group 2 |
| CALLISTO_FLYBY_WG2 | | Working Group 2 |
| CHARACTERIZATION_IRR2_CARME | | Working Group 2 |
| CHARACTERIZATION_IRR2_PASIPHAE | characterization irregular moon Pasiphae | Working Group 2 |
| CHARACTERIZATION_IRR2_SINOPE | Characterization irregular moon Sinope | Working Group 2 |
| CHARACTERIZATION_IRR_ELARA | Characterization irregular moon Elara | Working Group 2 |
| EUROPA_FLYBY_WG2 | | Working Group 2 |
| GANYMEDE_DISTANT | | Working Group 2 |
| GANYMEDE_FLYBY_WG2 | | 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 |
| IO_TOR_DUST | Io torus dust | Working Group 2 |