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Here is a list of observations that will be taken of Io by Galileo between December 2000 and October 2001. This covers Galileo orbits G29, C30, I31, and I32. Many of these are only preliminarily scheduled and are subject to change. The G29-I32 observation schedule is accurate as of November 2000.
| Orbit | Observation | Filters | Center Coordinates | Res (/pxl)* | Mode | Comments |
| G29 | 29ISGLOCOL01 2 1x2 OCMs global color mapping |
GRN, RED, VLT, 7560 | -0.3, 46.5 | 11.1 km | IM8 | low-phase global mapping complementary with Cassini mapping; synergistic with Cassini high-phase plume inventory |
| 29ISPROMTH01 1x1 + 1x2 OCM Prometheus plume |
CLR, VLT | -0.3, 64.2 | 11.1 km | IM8 | plume morphology and comparison with Cassini monitoring sequence and previous VGR and GLL images. | |
| 29ISGLOCOL02 2 1x2 OCMs global color mapping |
GRN, RED, VLT, 7560 | 0.0, 167.0 | 10.3 km | HIM |
low-phase global mapping complementary with Cassini mapping; synergistic with Cassini high-phase plume inventory Click here to view the observation (Galileo image on the right) |
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| 29ISGLOCOL03 2 1x2 OCMs global color mapping |
GRN, RED, VLT, 7560 | 0.2, 264.3 | 17.3 km | HIM |
low-phase global mapping complementary with Cassini mapping; synergistic with Cassini high-phase plume inventory Click here to view the observation (Galileo image on the left) |
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| 29ISECLIPS01 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 325.7 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS02 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 327.6 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS03 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 329.5 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS04 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 331.5 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS05 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 333.4 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS06 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 335.3 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS07 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 337.2 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| 29ISECLIPS08 2 1x2 OCMs eclipse |
CLR, VLT, 9680 | 0.2, 339.1 | HMA | Complementary to Cassini, significant new science on atmospheric emissions, plumes. and hot spots; better S/N ratio than in E15 | ||
| C30 | 30ISHSPOTS01 2 1x2 OCMs eclipse |
CLR, 9680 | IM8 | |||
| 30ISLEDHEM01 3 images |
GRN, VLT, 9680 | IM8 | ||||
| 30ISCHANGE01 3 images |
GRN, VLT, 9680 | IM8 | ||||
| I31 |
31ISMAXRES01 |
CLR | 2-3 m | IM8 | Highest resolution image taken by Galileo of Io | |
| 31ISTVASHT01 1x5 Tvashtar Catena |
CLR | 4-6 m | IM8 | Ultra-high resolution mosaic of Tvashtar Catena | ||
| 31ISPROMTH01 2x3 Prometheus |
CLR | 50-70 m | IM8 | High resolution mosaic of Prometheus | ||
| 31ISTVASHT02 1x5 Tvashtar Catena |
CLR | 90 m | IM8 | Context for 31ISTVASHT01 | ||
| 31ISPROMTH02 1x2 Prometheus |
CLR | 150 m | IM8 | Context for 31ISPROMTH01 | ||
| 31ISSAVITR01 2x3 Savitr Patera |
CLR | 160 m | IM8 | Mosaic of a large volcano bordering a mountain south of Tvashtar Catena | ||
| 31ISAMRANI01 2x3 Amirani-Maui |
CLR | 170 m | IM8 | Mosaic of Amirani-Maui lava flow | ||
| 31ISSUSANO01 5 color 1x1 Itzamna Patera |
GRN, RED, VLT, 7560, 9860 | 180 m | IM8 | Color mosaic of very colorful volcano SE of Emakong Patera | ||
| 31ISMASUBI01 1x5 Masubi |
CLR | 380 m | IM8 | Mosaic of long lava flow and Voyager and Galileo plume site | ||
| 31ISLEIZI_01 2x2 Lei Zi Fluctus |
CLR | 400 m | IM8 | Mosaic of large lava flow northwest of Kanehekili | ||
| 31ISKANEHE01 1x2 Kanehekili |
CLR | 410 m | IM8 | Mosaic of consistent hotspot and plume site | ||
| 31ISTERMIN01 1x4 |
CLR | 420 m | IM4 | Mosaic of mountains on Io | ||
| 31ISTERMIN02 1x5 |
CLR | 420 m | IM8 | Mosaic of mountains on Io | ||
| I32 |
32ISLOKI__01 |
CLR | 1.15 km | IM4 | Loki Patera near the terminator | |
| 32ISPELE__01 1x5 Pele |
CLR, 968 | IM8 | Pele at Night | |||
| 32ISTELGNS01 1x4 Telegonus Mensae |
CLR | 14 m | IM4 | Sapping Scarp at Telegonus Mensae | ||
| 32ISEMAKNG01 1x4 Emakong Patera |
CLR | 40 m | IM4 | |||
| 32ISTELGNS02 1x2 Telegonus Mensae |
CLR | 50 m | IM8 | Context for TELGNS01 | ||
| 32ISTOHIL_01 1x5 Tohil Mons |
CLR | 55 m | IM8 | High resolution context for previous images of Tohil Mons in low sun conditions | ||
| 32ISTUPAN_01 Tupan Patera |
GRN, VLT, 756 | 160 m | IM8 | Low sun color mosaic of Tupan Patera | ||
| 32ISTVASHT01 1x2 Tvashtar Catena |
CLR | 250 m | IM8 | |||
| 32ISGSHBAR01 1x2 Gish Bar Patera |
CLR | 320 m | IM4 | Mosaic of Gish Bar Patera and its associated mountain | ||
| 32ISSHMASH01 1x3 Shamash Patera |
GRN, VLT, 756 | 330 m | IM8 | Color Mosaic of Lava flows near southeastern edge of Tohil Mons | ||
| 32ISTERMIN01 6 image strip |
CLR | 410 m | IM8 | Strip along the terminator | ||
| 32ISTERMIN02 6 image strip |
CLR | 420 m | IM8 | Strip of the other terminator | ||
| 32ISEAAM__01 1x5 |
CLR | 440 m | IM8 | 5 image strip over Ekhi, Arusha, Altijirra, and Malik |
*All resolutions approximate
Last Updated March 28, 2001 .
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