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One of the more interesting results of the various NASA space engineering projects.
Designed by a team from the University of Auburn, this Saturn V launched probe, which would have been launched sometime between 1975 -1980 had it been built.
Upon arrival at Jupiter (After an 800-900 day trip, see the attached mission profile.) the 3.6 metric tonne orbiter would have entered an initial eliptical polar orbit with a perijove of no less than 7 Jupiter radii that following checkout would have been lowered to one with a perijove of around 4 Jupiter radii.
Keeping with the view at the time that the Jovian moons would be uninteresting 'dead' worlds the instrumentation fit (See below) was biased towards particle and fields detection. While cameras were fitted they were intended primarily to photograph Jupiter itself. Power was to be supplied by eight RTGs supplying a total of 640w.
Instruments
1. Solar Wind/Flare detectors
2. Cosmic Ray detectors
3. Micrometeorite detectors
4. Magnetometers
5. Trapped radiation detectors
6. Radiometers & photometers
7. UV/Visible/IR Spectrographs
8. Wide (10º) & Narrow (1º) angle television cameras. (Resolution at 7 Jupiter Radii Wide angle (150km), Narrow Angle (35km), at 4 Jupiter Radii. 70km & 18km respectively.)
The full two volume report can be downloaded below:
https://app.box.com/s/7wd95p24t97ru6dvwdw0
Designed by a team from the University of Auburn, this Saturn V launched probe, which would have been launched sometime between 1975 -1980 had it been built.
Upon arrival at Jupiter (After an 800-900 day trip, see the attached mission profile.) the 3.6 metric tonne orbiter would have entered an initial eliptical polar orbit with a perijove of no less than 7 Jupiter radii that following checkout would have been lowered to one with a perijove of around 4 Jupiter radii.
Keeping with the view at the time that the Jovian moons would be uninteresting 'dead' worlds the instrumentation fit (See below) was biased towards particle and fields detection. While cameras were fitted they were intended primarily to photograph Jupiter itself. Power was to be supplied by eight RTGs supplying a total of 640w.
Instruments
1. Solar Wind/Flare detectors
2. Cosmic Ray detectors
3. Micrometeorite detectors
4. Magnetometers
5. Trapped radiation detectors
6. Radiometers & photometers
7. UV/Visible/IR Spectrographs
8. Wide (10º) & Narrow (1º) angle television cameras. (Resolution at 7 Jupiter Radii Wide angle (150km), Narrow Angle (35km), at 4 Jupiter Radii. 70km & 18km respectively.)
The full two volume report can be downloaded below:
https://app.box.com/s/7wd95p24t97ru6dvwdw0