Latest http://www.ciclops.org/view/7206/Rev166 article is available.
I've been looking forward to this one for a while as we get our first decent look at Methone Closest ISS activity is from 4,500km, which should yield images comparable to the best views we have so far of Atlas.
There are also images planned of Tethys' trailing hemisphere from mid-ranges, and of course a close (955km) Titan flyby with specular-reflection searches, and radar swaths at C/A. This is the flyby whereby Titan bends Cassini's orbit 'down' and out of the ring plane for the next couple of years.
I know we can't have it all, but I was hoping for another decent look at Telesto on this rev (Cassini buzzes past at around 11,000km) which would have given us images at high phases and from almost the same range as the flyby in 2005. Never mind, there's another similar-range pass to Telesto in 2015.
Lots to look forward to.
Jase
Re: Methone, Emily's wish came true....(from 6 years ago on this forum):
"Although I wouldn't call this a "main focus," I would like to see the trajectory studied hard for the opportunity to do a pretty close flyby (say around 2,000 km) of one of the itty bitty moons, and to give the flyby a resonably dense set of observations. The closest Cassini will get to any of those things during the primary mission is 10,000 km from Telesto, which happened on October 11. Hyperion looked so bizarre up close, I'd like to see what one or two of the itty bitty ones -- Methone, Pallene, Calypso, Polydeuces, or Helene looks like from that kind of perspective."
--Emily
Does anyone know why is imaging from 4,500 km and not from ~2,000 km (closest distance to Methone)?
I'm guessing that the relative motion at closest approach might be too high for a target with such a small angular diameter.
Or maybe the closest view direction would be very high phase angle? (mostly shadow)
Phil
According to great PS site http://www.planetary.org/explore/space-topics/space-missions/cassinis-tour.html ,
Methone flyby is at modest speed 5.1 km/s, but relatively high phase angle 126°, so I think, that Phil can be right.
But on other side, even high phase angle images are very useful, not only because Methone will be much closer in this case (1861 km), but because of photometric investigations of Methone's surface (regolit roughness etc).
My guess is that there is perhaps still sufficient uncertainty about perturbations to Methone's orbit, that the further distance ensures Methone falls within frame. (remember the Helene flyby where some the closest NAC frames missed Helene altogether)
Jase
Titan's south polar haze layer is certainly starting to look interesting. Judging by these http://saturn.jpl.nasa.gov/photos/raw/rawimagedetails/index.cfm?imageID=261529 and http://saturn.jpl.nasa.gov/photos/raw/rawimagedetails/index.cfm?imageID=261532 images, it would appear larger particles (judging by the prominent visibility in the infrared CB2 filter as well) are piling on top of the detched haze layer (!?).
Interesting indeed. A bright portion is visible even in the CL1 CB3 images. Using the filters' depth penetration one can build a nice visual analysis of the S Polar haze from Cassini's most recent Rev 166 images.
Methone and Tethys images are here:
Methone - wow!? Smmooth....
http://saturn.jpl.nasa.gov/multimedia/images/raw/casJPGFullS73/N00189072.jpg
Tethys
http://saturn.jpl.nasa.gov/photos/raw/rawimagedetails/index.cfm?imageID=261595
Craig
Wow. At this resolution Methone seems completely free of craters. Coated with a thick layer of dust or could this small body simply be a 'clump' of dust?
Probably getting coated by a lot of ice particles from Enceladian plumes? Cool little worldlet.
Spectacular! Here's a cleaned-up and contract-enhanced image of Methone. There are real albedo variations across it.
Phil
Wow! This must be the biggest egg in the Universe!
Methone is very reminiscent of Pallene - peanut-shaped and very smooth. Interesting.
That's interesting. The smooth shape says it's a snowdrift with a young surface, but the albedo differences can't be accounted for that way. How would the lighter and darker patches perpetuate themselves? Maybe there's a postive feedback loop (like Iapetus) that is sufficiently vigorous to keep up with the 'snowfall'.
Submitted for your derision: my first attempt at processing Cassini data, an approach movie for Methone. The noise algorithm clearly needs some work...
Would the presumed particles coating the surface (if it isn't that way all the way through) be charged and discharged by Saturn's magnetic field and 'sorted' somehow by size (or something) and that is making the albedo variations? Or maybe the particles are not spherical, and their orientation is aligned that way and that makes them look different in different regions.
Good job. I tried something similar, painting out the cosmic ray hits, but there were so many that I realized I wasn't so much painting things out as I was painting a picture of Methone, so I quit. I think it probably is better to leave them in, for now. Once we can get our hands on data that's not been JPEG-compressed, it'll be substantially easier to remove them.
Very pleased indeed that they got these good shots of Methone.
Albedo variations?!?
As usual, I had no idea what to expect. But whatever it was that I was not expecting, this wasn't it.
I get the feeling that Methone is not unlike Atlas: it probably has a solid core and a smooth cover of ring dust, as dense as freshly fallen snow, filling its minuscule Roche "sphere of gravitational influence". don't forget that Methone has its own ringlet from which to collect dust. too bad we don't have a reliable estimate for its mass, otherwise it would be easy to compute the size of its sphere of influence. I bet it's of the order of 6 km across...
Fascinating object. Cometary size and incredible smoothness like some parts of comets visited by spacecraft in the last decade (see below). Could methone be a captured comet, its passage around the sun vaporizing the volatiles on/in its surface, smoothing its crust and perhaps passing too close to Saturn (in or outbound) and thus captured in its altered state???
What hemisphere are we looking at here, trailing or leading (or a combination of both)?
In passing, a milestone of distance travelled for Cassini on this last revolution - see attached...
I never cared much for the "total distance travelled" number. Isn't it really pretty meaningless when you think about it? What frame of reference was used? Cassini was cruising through the solar system for 7 years so one can assume the trajectory length centered around the Sun was what was measured. What happened when it entered the Saturnian system, did the statistic switch (and at which point?) to measuring the length of all the ellipses centered around the Saturn or still the heliocentric path?
It's also much easier to clock in billions of km if you're in the inner solar system. Speaking of which, how "far" did MESSENGER travel?
And how far have I travelled, sitting on my butt reading UMSF ?
John,
No need to apologize. To each his own.
What is the orientation of Methone? Is the long axis pointed towards Saturn (similar to a gravity-gradient stabilized spacecraft)? If this is in fact a loose dust pile, is this the expected type of deformation?
North is down in the raw images.
I think we would have noticed if Methone was as irregular as a bowling pin (like that dog-bone asteroid, Kleopatra?)
Or we can go with eggs, those are universal, right?
Actually, when you said Skittle' this UK resident thought you were referring to the small, coloured-shell chewy sweet ('candy' in US usage...)
Probably not the best descriptors, the geometrical ones are better... compared to other forums this is not a lay audience nor a US-centric one.
To the point though, and not trying to be repetitive - I'd be interested if anyone can tell if it is prolate or oblate.
One of the last datasets from this Rev: a wide-angle view of Saturn, rendered in CB2 / Synthetic Green / Blue:
"I'd be interested if anyone can tell if it is prolate or oblate."
I'm fairly sure it is prolate, elongated on one of its equatorial axes. But we will need more views to get a good shape model.
Phil
Is that Mimas?
Taken on 23rd May from around a million km from Saturn.
If my surname began with Hoag- and ended with -land I would be beside myself.
Edit: it is Mimas - that's Herschel to the left.
A little play-around with the best Methone image - processed to within an inch of its life. Is that a tantalising hint of detail in the darker area, or am I enhancing artifacts?
--edit---
There is real detail in the darker area, in the form of slightly darker smudges. Real because it shows up in all the images, not just one. I don't see any obvious topographic expression of it, but the sun is nearly overhead at that location.
Phil
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