This is a re-submission which still contains two variations of our one orbit (one visit will be deleted in the final version). We have decided to go with the 1k x 1k subarray which doesn't quite fit the full disk of Jupiter but gives us many more "movie" frames with no discontinuity (buffer dumps). The nominal roll on Jan 24 is very close to ideal, aligning Jupiter's equator to the subarray diagonal. But I specify a slight;y off-nominal roll for better allignment, which is essential for making the 1k aperture work. Please very this intended alignment with MOSS/Percy. -- Max Mutchler -1348454802 ----- Attempting Submission 1 (Thu Dec 11 12:15:44 GMT 2014) ----- ----- Attempting Submission 2 (Thu Dec 18 03:30:10 GMT 2014) ----- OK Io, Callisto, and Europa will simultaneously be in transit on the disk of Jupiter on 24 January 2015. Smaller moons Amalthea, Thebe, and Adrastea will also be transiting at this time. We will conduct Hubble WFC3 imaging to capture these moons, and their shadow play, across the disk of Jupiter. The most critical transit moment occurs on 24 Jan 2015 at 7:10 UT, when Io, Callisto, and Europa will all be on the disk of Jupiter at the same brief moment. Smaller moons Amalthea, Thebe, and Adrastea will also be transiting at this time, and Metis will be just off the disk. The shadows of these objects will also be evident on the disk of Jupiter. Unfortunately, the HST orbit available at this time is impacted by the South Atlantic Anomaly (SAA) near the end. We use the 1k x 1k WFC3 subarray which allows us to obtain many monochromatic "movie mode" frames as rapidly as possible to capture all the relative motions involved in the unfolding event. At the end of the orbit, and during the brief moment of triple-transit, we obtain one full-color image of Jupiter. Default false false false false false AVAILABLE SOLAR SYSTEM PLANET Jupiter moon transits STD=JUPITER EARTH 1418871645345 Using ephemeris for target 14042-10-JUPITER ephemeris data for target 14042-10-JUPITER does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 14.213 to 16.090. ephemeris interval: 14.334 to 16.336 The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1422080287000 286.0 (Tic-Visit :proposal-id 14042 :visit-id "10" :proposal-version -1 :trans-version "20140605" :date "17-Dec-2014 22:00:44.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 499088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14042 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14042 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2751 :al-overhead-at-end 0 :internal-dur-at-end 582 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0