NH at Jupiter, Planning the Jupiter encounter |
NH at Jupiter, Planning the Jupiter encounter |
Jan 22 2006, 10:57 PM
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#1
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Member Group: Members Posts: 706 Joined: 3-December 04 From: Boulder, Colorado, USA Member No.: 117 |
I think the Jupiter encounter deserves its own thread.
I've just been taking a first look at the Jupiter encounter geometry. You can do the same using Mark Showalter's excellent on-line ephemeris tools at the PDS rings node, which by good fortune happens to include a New Horizons ephemeris (calculated over a year ago) for our actual launch date, January 19th. We'll have an updated ephemeris soon, but this one's already good enough for planning. As Roby72 noted in the Star 48 thread, the satellites are (annoyingly) all on the opposite side of Jupiter at closest approach. We'll still get good views of all sides of Io because Io rotates in only 1.8 days and we'll be pretty close to Jupiter for that long. We'll get fairly good coverage on Europa too, for the same reason. But we won't get very close to Ganymede or Callisto. Luckily Io is our highest priority satellite target and Europa is next, so we'll do OK. |
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Jan 22 2006, 11:16 PM
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#2
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Member Group: Members Posts: 809 Joined: 11-March 04 Member No.: 56 |
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Jan 23 2006, 12:00 AM
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#3
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Member Group: Members Posts: 706 Joined: 3-December 04 From: Boulder, Colorado, USA Member No.: 117 |
QUOTE (David @ Jan 22 2006, 11:16 PM) Nah, IMHO New Horizons discussions should stay under the New Horizons topic. John. |
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Jan 23 2006, 12:28 AM
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#4
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Member Group: Members Posts: 122 Joined: 26-June 04 From: Austria Member No.: 89 |
John,
yes the day before (or after), Io must be on the right side of the planet, but I think the high speed of NH makes the distance about equal than on encounter day at the other side (about 2.5 Mio km). Resolution for LORRI (bw imager) should be about 12 km, for RALPH (color) about 50km) This would be nice for plume searching and is about 5 times more resolution in case of LORRI than Cassini had at its Jupiter encounter in Dec. 2000. Robert |
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Jan 23 2006, 12:44 AM
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#5
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Senior Member Group: Members Posts: 2454 Joined: 8-July 05 From: NGC 5907 Member No.: 430 |
Any chance NH could image Europa well enough to see if any surface features have changed/moved since Galileo?
-------------------- "After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance. I see that such intercourse long continued would make one thoroughly prosaic, hard, and coarse. But the longest intercourse with Nature, though in her rudest moods, does not thus harden and make coarse. A hard, sensible man whom we liken to a rock is indeed much harder than a rock. From hard, coarse, insensible men with whom I have no sympathy, I go to commune with the rocks, whose hearts are comparatively soft." - Henry David Thoreau, November 15, 1853 |
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Jan 23 2006, 01:40 AM
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#6
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Member Group: Members Posts: 706 Joined: 3-December 04 From: Boulder, Colorado, USA Member No.: 117 |
QUOTE (ljk4-1 @ Jan 23 2006, 12:44 AM) Any chance NH could image Europa well enough to see if any surface features have changed/moved since Galileo? We'll be looking at Europa but not specifically for that purpose- our images will be far lower resolution than Voyager's and no changes were seen between Voyager and Galileo even at Voyager resolution, and over a longer timespan than between Galileo and NH. Our main goal in imaging Europa will be to look at the peculiar large, shallow, depressions that were seen by Galileo near the terminator- it's one area where we can improve over Galileo. Plus we'll be observing Europa's auroral emissions in Jupiter eclipse. By the way, here's a table I just sent to the science team, showing the timing and geometry of various significant events during the encounter. Times are spacecraft times, and the numbers will change just a bit once we get a final ephemeris. I've only calculated the times of the eclipses of each satellite that occur closest to the spacecraft- there are many more at greater ranges. "UT" means Universal Time, "mrad" means the angular diameter in milliradians, and "Sub-S/C Lon" means the sub-spacecraft longitude. I couldn't figure out how to align the columns properly without replacing all the spaces with underscores... --------------------------------------------------------------------------- ____________________Range___Diam__Solar__Sub- ____Date_______UT___(km)___(mrad)_Phase_S/C_Lon__Event --------------------------------------------------------------------------- February_25__09:45_6334186__0.831___11____349____Ganymede eclipse ingress February_25__11:45_6222615__0.846___12____352____Ganymede eclipse egress February_27__10:46_3074450__1.021___40____315____Europa eclipse ingress February_27__13:18_3045261__1.030___45____321____Europa eclipse egress February_27__14:20_2734370__1.331___48____303____Io Eclipse ingress February_27__16:28_2758131__1.320___53____316____Io Eclipse egress February_28__02:00_2957815__1.061___72____347____Europa closest approach February_28__05:00_2304575_61.920___82___________Jupiter closest approach February_28__06:00_3029556__1.737__102_____41____Ganymede closestapproach February_28__06:30_4153289__1.156___81____353____Callisto closest approach February_28__22:00_2260221__1.610__118____141____Io_closest approach ___March__1__08:48_2748816__1.324__120____231____Io_eclipse ingress ___March__1__10:58_2951842__1.233__121____248____Io_eclipse ingress --------------------------------------------------------------------------- John. |
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Jan 23 2006, 05:16 PM
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#7
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Senior Member Group: Members Posts: 2454 Joined: 8-July 05 From: NGC 5907 Member No.: 430 |
QUOTE (john_s @ Jan 22 2006, 08:40 PM) We'll be looking at Europa but not specifically for that purpose- our images will be far lower resolution than Voyager's and no changes were seen between Voyager and Galileo even at Voyager resolution, and over a longer timespan than between Galileo and NH. Our main goal in imaging Europa will be to look at the peculiar large, shallow, depressions that were seen by Galileo near the terminator- it's one area where we can improve over Galileo. Plus we'll be observing Europa's auroral emissions in Jupiter eclipse. John. Thank you for the information, John. Would New Horizons be able to look for any possible geysers from Europa as well? Might be good practice for similar events in the Pluto system, too. -------------------- "After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance. I see that such intercourse long continued would make one thoroughly prosaic, hard, and coarse. But the longest intercourse with Nature, though in her rudest moods, does not thus harden and make coarse. A hard, sensible man whom we liken to a rock is indeed much harder than a rock. From hard, coarse, insensible men with whom I have no sympathy, I go to commune with the rocks, whose hearts are comparatively soft." - Henry David Thoreau, November 15, 1853 |
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Jan 23 2006, 10:56 PM
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#8
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Senior Member Group: Members Posts: 1592 Joined: 14-October 05 From: Vermont Member No.: 530 |
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Guest_Sunspot_* |
Jan 23 2006, 11:50 PM
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#9
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Guests |
How many days/weeks before closest approach will New Horizons start imaging Jupiter?
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Guest_AlexBlackwell_* |
Jan 23 2006, 11:55 PM
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#10
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Guests |
QUOTE (john_s @ Jan 22 2006, 10:57 PM) I think the Jupiter encounter deserves its own thread. Maybe I missed it in another thread (or website), John, but is there any possibility of getting imagery of any of the outer jovians (e.g., Himalia)?
I've just been taking a first look at the Jupiter encounter geometry. |
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Guest_BruceMoomaw_* |
Jan 24 2006, 02:11 AM
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#11
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Guests |
Judging from the NH Jupiter encounter planning meeting I attended back at the 2003 DPS meeting, the most interesting piece of new information that comes out of the NH Jupiter flyby may be its near-IR spectra of the surface composition of the Galilean moons -- especially Europa. Its spectrometer has much higher spectral resolution than Galileo's and will be considerably closer to the Galilean moons that Cassini's, implying that it may be able to nail down whether that stuff mixed with Europa's ice is Mg sulfate or sulfuric acid.
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Jan 24 2006, 09:45 PM
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#12
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Member Group: Members Posts: 706 Joined: 3-December 04 From: Boulder, Colorado, USA Member No.: 117 |
QUOTE (AlexBlackwell @ Jan 23 2006, 11:55 PM) Maybe I missed it in another thread (or website), John, but is there any possibility of getting imagery of any of the outer jovians (e.g., Himalia)? We typically get a couple of pixels on Himalia, similar to Cassini, though I haven't seen the geometry for the actual trajectory yet. Anyway, don't expect anything too dramatic on any outer satellties. |
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Jan 25 2006, 12:11 AM
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#13
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Junior Member Group: Members Posts: 48 Joined: 8-December 05 Member No.: 603 |
On an extremely amateur basis, I did some (very) back of the envelope calculations and came up with Himalia spanning about 9.5 pixels a week after Jupiter C/A - slightly better than Cassini.
Can't wait to hear real numbers from people who actually know in a couple of weeks. Bart |
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Jan 26 2006, 07:26 AM
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#14
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Junior Member Group: Members Posts: 72 Joined: 22-December 05 Member No.: 616 |
So New Horizons will take images of the Gas giant Jupiter and some of its moons?
Wondered if the lenses on the cameras are closed afterwards as some kind of protection and opened before Pluto encounter? |
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Jan 26 2006, 05:57 PM
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#15
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Senior Member Group: Members Posts: 2454 Joined: 8-July 05 From: NGC 5907 Member No.: 430 |
* ASTRONOTES: Derelict Booster to Beat Pluto Probe to Jupiter
http://www.space.com/astronotes/astronotes.html NASA's Pluto-bound New Horizons spacecraft now speeding through the Solar System is set to reach Jupiter on Feb. 28, 2007, but it will not be the first craft of its mission to reach the gas giant, mission officials said this week. -------------------- "After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance. I see that such intercourse long continued would make one thoroughly prosaic, hard, and coarse. But the longest intercourse with Nature, though in her rudest moods, does not thus harden and make coarse. A hard, sensible man whom we liken to a rock is indeed much harder than a rock. From hard, coarse, insensible men with whom I have no sympathy, I go to commune with the rocks, whose hearts are comparatively soft." - Henry David Thoreau, November 15, 1853 |
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