This is something I've been thinking about over the last few days and I'd like to post it here for discussion.
I got an idea for a Jupiter probe, which I term the Jupiter Distant Orbiter.
The instrument fit is primarily particles and fields, with the objective being to map the radiation belts/magnetic field from outside the orbit of Callisto. The probe would also be fitted with a 'HiRISE - style' camera to enable photography of the moons/Jupiter.
The orbit used would be one that is highly inclined so that the probe is never occluded by Jupiter itself.
Comments?
Umm - http://newfrontiers.nasa.gov/missions_juno.html ?
A HiRISE type camera doesn't work too well if you're not in a regular low orbit - a normal framing camera would make a lot more sense.
Doug
I see one obvious problem with your approach: orbit insertion burn cost. If you do the JOI burn outside of Callisto's orbit, you expend much more fuel than a close periapsis burn would. It's not very economic.
A spacecraft with a camera with the focal capabilities of the HiRise camera (you would want it to be framing) would be able to do considerable monitoring of Jupiter and Io as well as many flybies of Ganymede and Callisto. Such a spacecraft could use solar power; see the ESA mission study on a two craft mission to Jupiter. One would be a distant orbiter (although without a HiRISE-like camera) and the other a Europa orbiter.
Such a mission plan could be adopted to an international mission. The Europeans, for example, could do the distant orbiter and a larger camera could be put on the spacecraft. Then a simpler and less expensive Europa orbiter could do the close up Europa studies. If the Americans built the latter, it could be powered by RTGs.
One of the key advantages of the split mission according to the European mission is that the distant orbiter could be a relay for the Europa orbiter, simplifying its design and power requirements.
I don't recall how difficult this orbit would be for a spacecraft to achieve (eccentricity is quite high and no Jupiter flyby for orbit shaping) but a craft launched from earth to pass Jupiter roughly 60 degrees ahead in it's orbit, with 4 years of flight exterior to Jupiter's orbit would then cross 60 degrees behind Jupiter as it headed sunward. Such an orbit could encounter a mainbelt asteroid and a leading Jupiter Trojan out bound, and a trailing Jupiter Trojan and another mainbelt asteroid in bound. Time this right and maybe you get to go past Chiron, too.
Set up the orbit to return to the vicinity of earth in a multiple of 365 days, and you can flyby earth closely, mod the orbit some, and maybe go somewhere else interesting. (maybe pump up the orbit and go check out some possible Saturnian Trojans, or a comet far from the sun)
If studying asteroids is desired, a Jupiter Distant Orbiter with HiRISE resolution imaging could look at some of the outer satellites of Jupiter (read: captured asteroids). I realize these are WAY out from Jupiter, but there are several ways to approach the problem. One, design your Jupiter approach (pre-orbit insertion) to pass at least one outer satellite. Two, if I remember correctly, some of these satellites are in very loose clusters or at least constitute families of satellites, so may allow orbits to be designed that could pass more than one in a reasonable length of time. Three, a HiRISE-class imager would allow improvements over earth-based or Hubble imaging from a fairly large distance, so close flybys might not be necessary to get good science.
Any chance the Jupiter L1 or L2 positions are tantalyzingly close to the outer satellites?
Any halo orbits about L1 that interesected the outer Jupiter satellite 'cloud' might give us a low delta vee chance to look at some of them . . . .
Halo orbits around L1 apparently can be largish, but maybe not large enough . . .
http://solar-center.stanford.edu/FAQ/QL1.html
Somethings to keep in mind...
A camera (any camera), especially a high-end one like HiRISE, will be very difficult to deploy in the Jovian environment. The radiation would make much more difficult to build, and HiRISE was not exactly easy (or cheap ) to build in the first place.
Why a camera? What will you learn? Instruments are deployed on spacecraft to answer scientific questions. What questions will a camera answer?
The ESA mission study is pretty aggressive. The level of radiation shielding they assume for the instruments is paltry compared to the 5mrad assumption of radiation dosage. It is difficult to make digital electronics that can take 50-100 krad... let alone 5mrad with minimal shielding.
I also find the masses/power of the instruments to be very suspect... I usually check http://nssdc.gsfc.nasa.gov/ and look for similar instruments. You will probably be able to build lighter more capable instruments in the future... but not by factors of 2 or more... especially since you will have to use older, lower performing parts to withstand the radiation.
There was an interesting Jupiter Distant Orbiter-esque proposal at OPAG earlier in the year. It was called the Ganymede Observer I believe, and its main feature was the MIDAS (Multiple Instrument, Distributed Aperture?) platform - which (apparently) enabled considerably more science return for equivalent volume/mass. Looked like an impressive innovation, that MIDAS, despite the potential integration problems, ITAR etc.
I wonder if it could be part of an New Frontiers 3 "Galileo 2" type proposal. Or as part of the Europa Explorer for better than MRO resolution of interesting regions (especially repeat coverage over time).
Incidentally, does ICER compression still work properly at Europa? I presume it is durable enough with the radiation environment, given that ICT worked (I'd love to know the full story behind that, the few papers I saw, one from 1991, and the snippets on how hard it was to implement on the AACS processor is terrifying.)
Roly
ICER is just a compression algorithm. If you can manage to build a processor hardened enough to reliably execute instructions I don't see why it wouldn't work. I don't know about those snippets about Galileo (would love to find out more!), but I assume an AACS processor just wasn't general purpose "enough" to readily support heavy trigonometry calculations.
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