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#81
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On 2004-06-10, Henry Spencer wrote:
If you want to do anything with the outer planets (ie with RTGs)... It's not unthinkable to do non-RTG missions to Jupiter in particular. Or in the case of one conceptually elegant Discovery proposal - do it "conventionally", from the place we best know how to work "conventional" satellites... earth orbit. The mission, if memory serves, was to study Jovian (weather patterns?) by putting a tailored telescope in orbit and dedicating it to the task. Unsexy, but quite likely to work (at least from a technical standpoint). Looking at the 2000 proposals, since I have a summary to hand: http://www.space.com/news/discovery_sidebar000828.html (I keep meaning to dig out old press releases and write a little bit on each of these throughout the Discovery program; it's interesting what people choose to get excited over) * one lunar rover (south pole, looking for volatiles); * one sample return (ditto); * a Martian microlander net (24 of them, 13lb each!) to study the atmosphere (plus an orbiter thrown in); * a plan to run multiple (!) gliders through Valles Marineris to look at the geology; * a Martian roving balloon with magnetometer; * Kepler, an orbiting telescope to look for extrasolar transits; * a proposal to have a system which "cancels out" starlight to look for reflected light from their planets; * and one to look for orbital pertubations with gravitational lensing; * a mission to refly CRAF! Well, sort of. Nine-month mission to study the nucleus of Kopff, which was one of CRAFs targets, and a flyby of Themis thrown in; * one to study Vesta and Ceres; * one to study Vesta; * INSIDE Jupiter - " Interior Structure and Internal Dynamical Evolution of Jupiter", which does what it says on the tin; * one to study rhe abundance of water/ammonia in Jupiter's interior * a probe to study Venus regarding 'how it got that atmosphere, and how it evolved'; * a Venus orbiter to "undertake an investigation of the planet's global meteorology, chemistry and volcanism" - big plans for a small mission; * and the intriguingly named Venus Sounder for Planetary Exploration; 16 there, which means there's ten or so not listed. But you get the idea of the variety... -- -Andrew Gray |
#82
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Neil Gerace wrote:
"Christopher M. Jones" wrote in message ... Few members of the cabinet have the ability to dissolve the senate or congress. Neither does any member of the PM's cabinet, though. Only the PM himself through the head of state. Many European parliamentary republics work like that too. The comparison being made was between the unelected cabinet and the unelected PM. Both represent positions of power, both are nominally accountable to elected bodies. My comment was meant to imply that the PM has rather more power than cabinet members and thus greater power being held by persons less directly accountable to the electorate makes for a less direct and less populist democracy. |
#83
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#84
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In article ,
Duncan Young wrote: But there are lots of other low-hanging fruit remaining, as witness all the rejected Discovery proposals. There were reasons why those missions got rejected - some more than others. *Some* of them certainly had problems, or were pushing things too hard. Others were perfectly reasonable missions which simply didn't make the cut. The Moon remains poorly mapped in several important ways, e.g. we still do not have good topographic maps of the poles or gravity maps of the farside. True - but the moon now has its own entire Office outside of Discovery. And it could be back in Discovery a year from now. But what relevance has that to the topic? The issue at hand is that there is still significant work that could be done there at relatively low cost. Which office it's run from is irrelevant. I predict that we're going to find out that comets, like asteroids, are much more diverse than we'd thought. We've barely scratched the surface of what can be done with low-cost missions to them. And its a damn shame about CONTOUR. A tightly-proscribed program like Discovery might not be the best program for investigating diversity. The big problem with Discovery for that is that it's not really a "program", just a random grab-bag of missions, whoever did the best sales pitch last year. For properly investigating diverse objects, you want a series of similar spacecraft, and there's no home for that in Discovery. (In fact, there isn't really a comfortable home for that anywhere in NASA. Even the Mars program, which really is a *program* to some extent, finds it difficult to just repeat a successful mission, even when that would be scientifically a very interesting thing to do.) It's not unthinkable to do non-RTG missions to Jupiter in particular... It seems to me that propulsion requirements for entering Jupiter orbit and DSN support issues limit what you can do with non-nuclear power at Jupiter, especially when you include the mission duration constraints of Discovery. Some of this is a matter of artificial limitations of Discovery, rather than inherent difficulties of doing low-cost missions. The DSN issue definitely is a bad one, though. Cheaply landing on Mercury or Venus is pretty hard. But there are plenty of more-accessible unexplored bodies in the inner solar system. Again, Moon and Mars have their own offices. I wasn't thinking of either one. And again, I'm talking about missions, not about bureaucratic turf. Finally, let us not forget that if you're willing to limit yourself to carefully-chosen objectives in the inner solar system, there are people in several places who think they could give you a sizable program of unmanned missions for the cost of one Discovery mission. There's no inherent reason why planetary missions have to cost hundreds of millions each. Beagle 2 and Deep Space 2 remain counterpoints. Note the words "carefully-chosen objectives". If you insist that the objective has to be a Mars landing, and you have no tolerance for failure so the hardware has to work the first time, that does make for an expensive mission which can't be slimmed down below a certain point. -- "Think outside the box -- the box isn't our friend." | Henry Spencer -- George Herbert | |
#85
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Henry Spencer wrote:
In article , Duncan Young wrote: snip Finally, let us not forget that if you're willing to limit yourself to carefully-chosen objectives in the inner solar system, there are people in several places who think they could give you a sizable program of unmanned missions for the cost of one Discovery mission. There's no inherent reason why planetary missions have to cost hundreds of millions each. Beagle 2 and Deep Space 2 remain counterpoints. Note the words "carefully-chosen objectives". If you insist that the objective has to be a Mars landing, and you have no tolerance for failure so the hardware has to work the first time, that does make for an expensive mission which can't be slimmed down below a certain point. Even on the Mars landing side, the problem usually isn't scaling down, per se. The problem is usually in the scale in terms of what they want to load onto any given mission. It only gets expensive in the boundry conditions. One one side is the boundry condition of a working vehicle and no payload. Then, incremental discrete costs for payload packages. Then an upper limit where they try to cut back the core delivery vehicle (or its testing) for more payload. They never scale down. Only up. They would have had exactly the same results from the Beagle mission had they not tried to crowbar in the lander. |
#86
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#87
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"Henry Spencer" wrote in message ... The DSN issue definitely is a bad one, though. Somebody tell me why adding stations to the DSN isn't a top priority? I'd think that Japan, Diego Garcia, South Africa, Britain, Nova Scotia, Brazil, Kansas, Easter Island and others should be good candidates. In addition, a couple of satellites similar to the "Big Ear" spy sats should work AND have the advantage of being able to access far more sky without bothering about weather. If the DSN is the bottleneck, let's spend a little less adding to the bottleneck and a lot more relieving it. |
#88
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Christopher M. Jones wrote:
To date we have seen imagery from the surface or within the atmosphere of three plantary bodies which were not Earth (Moon, Mars, Venus). Huygens will raise that number to 4, the Rosetta Lander to 5, and Muses-C/Hayabusa to 6. I would count the NEAR on the surface of asteroid "433 Eros" too. These last images of NEAR Shoemaker: http://near.jhuapl.edu/iod/20010212f/index.html while it was descending, were *almost* surface images. Actually the very last image was taken from 120m (4000ft) height, but the resolution is good enough that you could (I think...) recognize human faces if they were there. And the spacecraft did descent and worked also after that for a while. Matti Anttila -- http://masa.net/ |
#89
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In article ,
Scott Hedrick wrote: The DSN issue definitely is a bad one, though. Somebody tell me why adding stations to the DSN isn't a top priority? Basically, because it's hard to get serious money for infrastructure upgrades like that. It doesn't help that (I'm told) DSN's management is bureaucratic and timid, and is reluctant to face the need for major growth. They are making improvements, but relatively modest ones that aren't going to keep up with demand. think that Japan, Diego Garcia, South Africa, Britain, Nova Scotia, Brazil, Kansas, Easter Island and others should be good candidates. There is no dire need for lots more sites, especially in places like Diego Garcia and Easter Island where overhead costs would be high. DSN *could* definitely use one more Southern Hemisphere site -- currently the Canberra site is often a bottleneck -- perhaps in Argentina or South Africa. And I'd think it would mildly benefit from a third, plus a third Northern Hemisphere site somewhere like Japan, so that both hemispheres could have round-the-clock coverage of most sky directions. But the big requirement is not more sites, but more antennas. There's no reason to spread the antennas out over a dozen sites, which will just run up operations costs. What you want to do is not to commission a bunch more sites, but to commission a bunch more big dishes at the same three or four sites. In addition, a couple of satellites similar to the "Big Ear" spy sats should work AND have the advantage of being able to access far more sky without bothering about weather. A space-based DSN has been studied repeatedly, but the extremely high costs of mass, power, and maintenance up there have always led to the conclusion that spending the same amount of money on the ground would give better results. The time when you really start thinking hard about orbital infrastructure is when you take the next big jump up the frequency scale and go laser. *Then* weather, even light cloud, bites hard. Still not a clear-cut win for orbital receiving stations, but it makes them much more competitive. -- "Think outside the box -- the box isn't our friend." | Henry Spencer -- George Herbert | |
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