The Grand Finale, Proximal orbits |
The Grand Finale, Proximal orbits |
Oct 27 2016, 01:34 PM
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Member Group: Members Posts: 655 Joined: 22-January 06 Member No.: 655 |
With a month to go before the F-ring orbits commence, I thought it would be good to open a discussion about what exactly to expect, and the challenges and risks associated with the final months of Cassini's mission.
The final phase has been described as a mission in itself - one that might have attracted funding if it were stand-alone rather than one planned for the end of an already phenomenally successful enterprise. We will no doubt continue to get regular updates at ciclops a resource which has been invaluable to followers of the mission, and which have provided a brilliant insight into upcoming science activities during each orbit, since early 2007 (Thanks Jason). I'm hoping too that perhaps Emily may post one of her excellent articles on the TPS blog that give more of an inside track on the science that is planned for the final months. To summarise, the F-ring orbits commence on November 30th and comprise 20 orbits of the spacecraft with periapses just a few thousand kilometres outside the F-ring - this will allow the opportunity to image the dynamism of the F-ring as never before, as well as (imaging opportunities willing) our best views of the rings and ring-moons - Atlas, Pan, Daphnis, Pandora, Epimetheus and Janus (Prometheus has already had it's closeup) There may be opportunities to get images of some of the known ring clumps (S/2004/S6 if still extant) and/or the known propellers/clumps in the outer A-ring such as S/2009/S1 and Bleriot/Earhart. The rings are simply gigantic though, and many of the orbits of the ring-embedded moons are chaotic so probably I'm hoping for a bit too much. From what I can gather, there seems to be less risk with the F-ring orbits than with the proximal orbits as Cassini has sampled this environment to a degree already, and I believe it is intrinsically less dusty than the D-ring, and with relatively low radiation exposure to Cassini. The 23 proximal orbits commence on 23rd April next year following the penultimate Titan flyby, and will thread between the inner rings and Saturn's cloud tops. This is slated as the opportunity to pin down Saturn's rotation, measure the mass of the rings and obtain unparalleled data on Saturn's atmosphere. This is where the spirits of adventure and exploration reach their zenith, as the environment between the rings and the planet is not fully understood. The attached article gives an insight into the enormous planning challenges that these orbits present. It's fairly technical, but in summary: The dust and radiation hazards present unknown risks to not only Cassini's science instruments but also the ability of the spacecraft to maintain it's optimal orientation whilst preventing any safing events. As I understand it, it's not possible to prevent the glare of Saturn's atmosphere and rings blinding the sun sensor and star trackers, as they are located on the HGA which is facing forward to minimise risk of damage to the science instruments, so it's planned to command Cassini to 'suspend' star identification for 5 hours either side of each periapsis - thus flying blind during the 'hairy' part of the orbit. Mission controllers also have to deal with the not-fully constrained effects of aeroheating during periapses which may affect the instruments, and there is also a risk of safing due to radiation constrained within Saturn's magnetic field. The article states that the first proximal orbits will 'test the water' as regards the environment in that region, with periapse being lower on the final five orbits. It seems that many of the 'safing' protocols/thresholds will be relaxed during periapses, hopefully preventing Cassini entering safe mode - perhaps one of the worst-case scenarios - each orbit at this stage is only seven days, which doesn't allow a huge amount of time to upload new commands should that happen. I can only marvel at the technical brilliance of people involved in Cassini-Huygens and all they do, and have no doubt the final months of the mission will be a fitting end to this generation's exploration of Saturn. |
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Sep 15 2017, 07:39 PM
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Member Group: Members Posts: 356 Joined: 12-March 05 Member No.: 190 |
Followed the charmed mission since listening to the launch on the radio in '97. Sad to see it go but it's been one hell of a ride. I remember the first 7 years of the journey to Saturn being painfully long, though the past 10 or so of its presence there have now gone by terrifyingly fast. The Huygens landing remains the pinnacle of planetary science excitement for me, and I fear its fantastic wonder may never be equaled in my lifetime. Even though I post like once every 3 years now, glad to see this site still going, albeit not nearly with the level of activity of its heyday 8 years or so ago. I do not see many missions in progress or on the horizon having nearly the level of grandeur of our now largely complete initial survey of the solar system, but will stop by here from time to time nonetheless and hope to see that things are still marching along. till then...
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Sep 15 2017, 09:27 PM
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Senior Member Group: Members Posts: 2530 Joined: 20-April 05 Member No.: 321 |
In reference to past missions, and what we've lived through, it is perhaps obvious but must be stated in respect to the greatness of this board and those who run it…
The first big mission I was old enough to remember was Viking. And Viking was a masterpiece – four craft exploring the heck out of the most interesting planet and one really can't imagine the technology of the time doing it any better. But my main source of Viking info was National Geographic and "year books" that supplemented encyclopedias. Occasionally, something would make the print or TV news, but the information cycle for me was more typically one year. Then a book summarizing the main mission might make it into my hands. Viking happened "while" I was alive and waiting for the results, but it wasn't all that different from reading about something that had happened in the 18th century. There was a before and an after, but no during. Likewise Pioneer Venus and Voyager at Jupiter. By the time of Voyager at Saturn, I was subscribed to publications that shortened the news cycle considerably, but it was rarely under a week. In sharp contrast to that, I remember chatting live here about the first ISS pictures of Titan and manipulating them in Photoshop and having the real sense that I might be seeing something before anyone else ever had… and if I weren't first, I was certainly no more than minutes behind whoever was. Then, when Huygens arrived, a day when I shamelessly did no work at work, the fact that the first image was one of drainage channels in the headlands – unbelievable! And the descent more or less happened here in real time (plus some speed-of-light, downlink, etc. delay), with commentary (and sometimes it's well that interested amateurs are game to speculate more than a publishing scientist should). Viking happened in my lifetime, but Cassini and Huygens happened and were experienced here. And for the life that this provides the flow of information, I am tremendously grateful. |
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