Hubble Heritage imaging of Jupiter during the New Horizons encounter
WFPC2 images of Jupiter in Feb 2007 in support of New Horizons flyby of Jupiter. This Hubble Heritage DD program is working in concert with the existing GO programs by John Clarke (10862) and John Spencer (10871).
First Jupiter Heritage target goes along with visits 1-7, with same sequence of orbits to be repeated over a range of Jovian longitudes for global coverage. These 7 visits can be split if necessary, but should be as close in time as possible and cover a full range of Jovian CML values.
Later Jupiter Heritage target -- this is only the initial planning for later visits in Jupiter heritage program, these will be filled in to apt proposal at a later date, along with 5 more orbits for Jupiter spots. We will try to include filter F343N in at least one observation of this target. We expect 12 orbits for this target, giving a total of 19 orbits for this program.
SOLAR SYSTEM
0
false
0.0
false
false
false
false
false
false
SUPPORTED
SOLAR SYSTEM
PLANET
planet jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=95.78,REF=NORTH
SOLAR SYSTEM
PLANET
planet Jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=94.9,REF=NORTH
SEP OF IO JUPITER-HERITAGE-LATER FROM EARTH GT -11.0"
SOLAR SYSTEM
PLANET
Great Red Spot on Jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=94.9,REF=NORTH
CML OF JUPITER FROM EARTH BETWEEN 309.0 363.0
SOLAR SYSTEM
PLANET
Little Red Spot on Jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=94.9,REF=NORTH
CML OF JUPITER FROM EARTH BETWEEN 204.0 240.0
SOLAR SYSTEM
PLANET
planet Jupiter
STD=JUPITER
SEP OF JUPITER IO FROM EARTH LT 40.0",
SEP OF JUPITER GANYMEDE FROM EARTH LT 70.0"
SOLAR SYSTEM
PLANET
Great Red Spot on Jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=94.1,REF=NORTH
CML OF JUPITER FROM EARTH BETWEEN 316.0 10.0
SOLAR SYSTEM
For Visit 40 Io CML range choose so that Io is transiting Jupiter while the vent of the Pele plume is close to the limb.
PLANET
planet Jupiter
STD=JUPITER
TYPE=POS_ANGLE,RAD=1.0,ANG=94.9,REF=NORTH
TRANSIT OF IO ACROSS JUPITER FROM EARTH,
CML OF IO FROM EARTH BETWEEN 171.4 183.0,
SEP OF IO JUPITER FROM EARTH GT -14.0"
POS-TARG
DITHER
0.5566
LINE
0.5566
false
false
143.130005
4
26.565001
BOX
1
false
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The filter priority sequence is from highest priority to lowest: F410M, F673N, F255W, F160BN15, FQCH4P15, F953N, F218. We include as many filters as we can fit in each orbit, but schedulers may follow the above priority list to remove filters as needed to make this 7-orbit sequence scheduleable. The clipping could go all the way down to just the first two filters (F410M and F673N), and we'd still be able to get good science out of this sequence.
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false
7
0
A single-orbit visit to image the Little Red Spot (LRS) region simultaneously with the New Horizons LRS observations, preferably near 2/26 15:50 or 2/27 01:50 (Earth time).
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true
1
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Visits 11-14 are 4 single-orbit visits spaced ~10 hrs apart, to observe the Great Red Spot (GRS) at the same time NH is making it's IR image cube (2/26 19:30 - 2/28 12:00 Earth time).
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true
1
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Visits 11-14 are 4 single-orbit visits spaced ~10 hrs apart, to observe the Great Red Spot (GRS) at the same time NH is making it's IR image cube (2/26 19:30 - 2/28 12:00 Earth time).
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false
1
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Visits 11-14 are 4 single-orbit visits spaced ~10 hrs apart, to observe the Great Red Spot (GRS) at the same time NH is making it's IR image cube (2/26 19:30 - 2/28 12:00 Earth time).
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Visits 11-14 are 4 single-orbit visits spaced ~10 hrs apart, to observe the Great Red Spot (GRS) at the same time NH is making it's IR image cube (2/26 19:30 - 2/28 12:00 Earth time).
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true
1
0
A single-orbit visit to get the ful disk of Jupiter on one of the WF chips, along with any nearby moons. This is a "family portrait" near the time of New Horizons closest approach. We use a sub-sampling dither box to recover as much PC-like resolution as possible. We execute the dither pattern with one filter at a time, to minimize the undermining effect of the rotation of Jupiter. We include two iterations of the dither box for each of two filters. But the schedulers could remove the redundant iterations for each filter to shorten this orbit, if necessary to make it scheduleable.
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1
0
This visit is "Plan B" if the 7 consecutive orbits in visit 2 cannot get scheduled. It is a copy of just one of the 7 orbits in visit 2, and it is ON HOLD until we know that visit 2 cannot be executed. The filters in this orbit are in priority sequence. We include as many filters as we can fit in the orbit, but schedulers can keep removing filters off the tail end of the orbit, as needed to make this visit scheduleable. The clipping could go all the way down to just the first two filters (F410M and F673N), and we'd still be able to get good science out of this visit.
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false
1
0
This visit is an alternate for visit 20. Use this visit only if visit 20 cannot be scheduled.
This visit is ON HOLD and would be used 3 weeks after the New Horizons flyby, only if at least one of our earlier orbits was unscheduleable during the busy flyby week. This visit gets one last image of the Great Red Spot.
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false
1
0
This visit is an alternate for visit 20. Use this visit only if visit 20 cannot be scheduled.
on hold; to be used if need filler to reach 20 orbits total
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false
1
0
The filter priority sequence is from highest priority to lowest: F410M, F673N, F255W, F160BN15, FQCH4P15, F953N, F218. We include as many filters as we can fit in each orbit, but schedulers may follow the above priority list to remove filters as needed to make this 7-orbit sequence scheduleable. The clipping could go all the way down to just the first two filters (F410M and F673N), and we'd still be able to get good science out of this sequence.
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