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#23 |
(loop (#_fork))
Feb 2006
Cambridge, England
11000111011112 Posts |
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I'd like to put three small satellites 120 degrees apart around Callisto's orbit, to get real-time full-planet-scale imagery of the Jovian atmosphere. Jupiter is about two degrees wide as seen from Callisto-orbit, so a well-corrected six-inch telescope onto a large CCD (e2v offers a 9Mx9M device with 10um pixels) gets you adequate imagery, 20km pixels are about the same as the closest flyby missions have produced to date but this would give coverage comparable to Earth's meteosat network.
(hmm, yes, you'd also want IR imaging since Jupiter is strongly self-luminous and that would mean you didn't waste the time when one and a half of the satellites are looking at the unilluminated side of Jupiter) Callisto orbit is well outside the radiation belts; I don't know what the gravitational stable points in the Galilean system look like so this may need prohibitively much fuel for orbit control. |
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#24 |
Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
299816 Posts |
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I'd like to put something useful in the solar focal sphere but although it just about might be within budget, it would take far too long to get there. Increase both constraints by a factor of a few and it would become possible.
Closer to home, it would be nice to land a technology prototype on Mars which converts atmospheric carbon dioxide into carbon monoxide and oxygen. The products are used as rocket fuel for sample return to earth. Once again, budgetary constraints are likely to be the limiting factor. |
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#25 | |
"Forget I exist"
Jul 2009
Dumbassville
26·131 Posts |
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#26 | |
Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
246308 Posts |
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In particular, where does that "60"? come from? 19G miles is 30G km in more conventional units and 20 AU is even more conventional in this area. It's about the right order of magnitude in that Uranus is about that distance from us and the Voyager probes took about that length of time to get there, though not in a straight line of course. The distance they actually travelled to reach Uranus was significantly greater. If you want to go as far as possible outwards you should be able to do significantly better by bouncing off at least two of the Moon, Venus, the Earth, Jupiter and Saturn en route, especially if you use a long-duration low-thrust ion engine during the cruise phases. Voyager was constrained by having to visit Uranus after its earlier and compulsory gravity assists from Jupiter and Saturn. A long distance mission to the middle of nowhere doesn't have that limitation. The science from such a package would, in my view, best be devoted to observing charged particles, magnetic fields and ultra low frequency radio. Put cameras on board if you wish for the planetary fly-bys, but heading out into interstellar space is likely to be better served by using a significant fraction of the payload for electrical power, reaction mass (presumably Xe or Hg0, a very large comms antenna and even longer ULF radio antennae. If the comms antenna is large enough, in the 20 to 100m class, it could do double duty for radio astronomy and, in particular, enable mult-AU baseline interferometry. I haven't yet worked out the numbers but it may be possible to detect parallax shifts for the nearest quasars which would get the cosmologists excited. |
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#27 | ||||
6809 > 6502
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Aug 2003
101Γ103 Posts
11·863 Posts |
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#28 | |
Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
101001100110002 Posts |
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An attractive proposition is to send it significantly out of the plane of the solar system but that can only be done at the final planetary encounter, for obvious reasons. If the interferometry idea pans out, a vector at right angles to (the maximum number of) the interesting point sources would also be indicated. I don't yet know what that might be. |
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#29 |
Bamboozled!
"πΊππ·π·π"
May 2003
Down not across
1064810 Posts |
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Another mission: fly a soft-gamma ray observatory with a high-resolution (arcsec or better) telescope optimized for the 1.809MeV gammas emitted by the decay of 26Al. This isotope is created a few earth-masses at a time in supernovae explosions and has a half live approaching a million years. Current observations have an angular resolution measured in degrees so it's possible to say that there have been quite a lot of SN towards the galactic centre (big surprise!) and a clump out Cygnus way, but not much more than that can be deduce.
Being able to map the locations, ages, distribution and velocities of supernovae and, especially, their ejecta would be rather useful. This one could fly in relatively low earth orbit and wouldn't need excessive fuel and comms requirements, so several tonnes could be used for the telescope if desired.. It could even be designed to be user-serviceable. Do you yet get the idea that I could propose missions at the rate of a few a week for a significant length of time if I set my mind to it? There's no shortage of ideas, only a shortage of cash. |
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#30 |
6809 > 6502
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Aug 2003
101Γ103 Posts
11×863 Posts |
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Indeed. The pair of scopes that NASA received from the NRO. Those would be fun to play with. Put them out near one of the Lagrange points. Tie them together as far apart as practical to make a full time space based optical interferometer.
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#31 |
(loop (#_fork))
Feb 2006
Cambridge, England
638310 Posts |
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I'm afraid I do get a bit annoyed by the way that, whenever someone mentions space telescopes in quantities greater than one, someone else mentions interferometry. Particularly with the NRO telescopes, which are short focal length and optimised for very-wide-field work in the visual in almost exactly not the way that you'd want for interferometer elements.
NASA put about a billion dollars into space interferometry development, to discover that building an exciting space interferometer cost more than they would be prepared to spend ... planet-hunting by interferometric astrometry is so much more expensive than Kepler. VLBI with an actually-long baseline is more interestingly practical - big deployable antenna are off-the-shelf, JAXA has launched a test comsat with a 17-metre one. Regrettably the very biggest ones are off the NSA's shelf and so you probably have to pay for the development again. With current 10,000km baselines you can get 10-microarcsecond precision, which allows pretty good parallax measurements out to 10kpc within the Milky Way, and direct measurements of Keplerian motion of water masers to 60Mpc - there are admittedly issues of getting enough signal for those fairly weak sources. So you probably do need a billion-kilometre baseline for direct parallax to quasars, but the water-maser work might well be possible with sufficiently large dishes at Earth-Sun L4 and L5. |
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#32 |
"Marv"
May 2009
near the TannhΓ€user Gate
2·313 Posts |
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EUROPA !! We must go to this moon of Jupiter for the obvious reason that it may harbor life in its oceans. Even if not, it is one of the most interesting places in the solar system. Anyway, we've got to check it out to see if one of A.C. Clarke's monoliths stands guard there !
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#33 |
6809 > 6502
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Aug 2003
101Γ103 Posts
11×863 Posts |
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