I updated my site with a page with images of the moons of Uranus and Neptune. I will develop individual pages with more imagery, including color stuff eventually.
http://www.strykfoto.org/outericymoons/icymoons.htm
Also, http://www.strykfoto.org/proteus.htm is a link to the Proteus page, the only indivudual page that is already up.
By the way, at the bottom of the index page, I have a new shot of Neptune and Triton from WFPC 1 from before the repair mission.
Beautiful!
I knew Miranda was battered and resurfaced, but I didn't realise how 'out of round' it actually was. That white crater on Umbriel has always intruiged me - I assume its excavated to fresh ice below? I wonder if we will get better images that this of the Uranian system in our lifetimes...
P
Maybe this is an OK place to put this. I just made this for one of my students, and I might as well get more use out of it. It was hard to find in a quick google search or via Photojournal.
This is the clearest image of one of the plumes on Tritn, and I have labelled it to show the vent site, the vertical column, and the wind-transported plume.
Phil
Thanks, Phil! I've tossed it into the planetary.org image database -- should come in handy someday.
--Emily
Calvin Hamilton's excellent SolarViews website has an "animation" of one of the plumes:
http://www.solarviews.com/raw/nep/geyser.mov
http://www.solarviews.com/eng/triton.htm
I don't think the plume is moving per se, but rather the angle of the photo is changing causing the plume to parallax (Is that a verb? ) over the surface.
Here's an interesting video on the subject of Triton's plumes:
http://video.google.com/videoplay?docid=-2361275885502809184
Yeah, the white crater on Umbriel is neat -- note there is also another crater with a white peak. That moon's a bit of a chocolate-dip-cone, I guess.
Umbriel isn't one of my favorite moons, but I've wondered occasionally if it mightn't have some similarities with Iapetus --- sort of a "global Cassini Regio". However, since we don't see craters "punching through" Cassini Regio, the comparison's not very appropriate. It's fun speculation, though.
I tried to draw the best most I could out of the Voyager Umbriel set. The problem is that not only are the images distant and scarce, but because Umbriel has such a dark surface, they are either badly underexposed or smeared, for the most part.
Hello everyone,
A friend of mine is also experimenting with outer moons these days :-) I thought I could share a link to his latest creation - does THIS Proteus hang out of your screen?
http://ksiezyce.republika.pl/mapy/3-d/proteus-mapa_3-d.html
I have created a montage of the images from the flybys of the six largest Uranian moons (Puck, Miranda, Ariel, Umbriel, Titania, and Oberon). The images are to scale (not to the size of the worlds, but to their apparent size from Voyager. The exceptions are the closest views of Ariel and Miranda, which were scaled down. I have posted a small version below, and a link to the full version.
http://www.strykfoto.org/outericymoons/urcombo.jpg
To add a bit of perspective, here are some color images with similar illumation shown to scale (in the case of Puck, since there is no Voyager color, I gave it a reddish hue to conform to groundbased data).
Also, I animated the Titania approach. I haven't corrected the set for the fact that some images are just colorized because there was only one image at that point, and the other individual images vary between OGV, GBUV, and other such combinations. Also, the first image was taken quite a while before the others.
I like the presentation. Good work!
I am thinking I might have arranged the Miranda images wrong. The thing spins so quickly and liked a pinwheel that it gets confusing. Phil, you might know if this is right.
Sorry, Ted, it's not clear to me what you're trying to do. It looks like you want to arrange them so that we see the changing spacecraft geometry rather than the rotation - obviously they could be arranged either way. The chevron is the best clue. If so, then in your trio, the left one should be rotated 180 degrees. The dark patch from 1 o'clock to 3 o'clock in that view is the big dark patch on the left side of the other two views. Arden Corona, if I recall correctly. The other (non-chevron) corona is not dark, and in your little view it hardly shows up, but it's at 9 o'clock.
Phil
Thanks Phil. By the way, I have assembled the Proteus sequence into a movie.
Also, for good measure, here is the current version I have of the ~1.5 km pixel image (which is badly impacted by severe underexposure).
Wow great work!
Here is a new version of the Uranian combo with larger images.
Edit: See Below
On what principles did you scale those images? Titania is bigger than Oberon, but not that much bigger. Your Oberon is about 90% Titania's size or less, whereas the real Oberon is more like 96-97% Titania's size.
I used what I call "brain flatulence theory (BTT)." I was using the radius of Triton as the Diameter of Oberon...not sure quite how I did that. Here is a corrected version. It still looks a bit disproportionate due to the fact that more of Titania's disk is illuminated.
I have completed a global color Triton image from the best color set before Triton fully filled the narrow angle camera. Some versions of this are available, but I have tried to improve the level of detail.
That's marvellous Ted.
Speaking of Triton, have you considered recreating the view of an ancient Tritonian crater I mentioned in this thread:
http://www.unmannedspaceflight.com/index.php?s=&showtopic=4286&view=findpost&p=92193
I can't quite see what image that is. I hadn't considered it, but wasn't really aware of it either...This looks interesting...
This may have been the image you were thinking of (this is my version, with a normal terminator). It is multiframe, requiring reprojecting and of better quality in some areas than others. I did this a long time ago. I could probably make the coverage areas run together better now. The earlier image I posted was from the last set before triton filled the frame.
Sweet! I've added that one to my list of desktop backgrounds.
Here are the closest global views, excluding the receding sequence, in order.
Nice work, Ted.
It always amazes me how accurate a descriptor "cantaloupe terrain" is for Triton. I wonder if Triton is orange on the inside.
--Emily
All of the following polar projections were generated using the cylindrical maps created by Steve Albers (unless otherwise credited):
MIRANDA (southern hemisphere) (JPL):
UMBRIEL (southern hemipshere) (Philip Stooke):
TRITON (southern hemipshere) (JPL / William Johnston / A. Tayfun Oner / Steve Albers):
TRITON (northern hemipshere) (JPL / William Johnston / A. Tayfun Oner / Steve Albers)
No, no, no, Ted -- what we really need is Deep Rap - Triton, in which a huge *knuckle* is sent to Neptune's largest moon and used to rap on the rind. Extremely sensitive microphones aboard the flyby craft will then listen for the "exact right thunking sound" to determine the ripeness of the interior...
-the other Doug
I have improved my Proteus set. I have always thought there were features in the "Bad Tooth" image. After reprocessing these images, there is clear correlation between them. The highest resolution image has a resolution of 1.35 km/pixel. For context, that is somewhat better than the best pictures of Ariel (2.4 km/pixel). However, it was so severely underexposed that it is usually blurred to hide the effects of underexposure, making it appear to be an enlarged but distant image.
That's AMAZING Ted - I am ASTONISHED at the level of detail you've pulled out of the raws. What type of processing are you using here????
I used Photoshop. After calibrating the images, I compiled the pixels of some of the empty space from the images in the vertical direction (minus rows that contained moire) and subtracted this from the image. I used several noise reduction methods so as to minimize the loss of detail. I also used a high pass filter to bring out detail, which I merged with other versions of the images so as to bring back the low frequency features. Here is my complete Proteus set (the image in the upper left corner is Larissa, and next to it is a crescent Nereid, but the rest are Proteus).
Unbelievable, Ted. That's the first time I've ever seen a resolved image of Nereid...always wondered what it looked like. Thank you so much for this gift!!!
Now I can visualize how the terrain around the Outsider's base looked when Speaker-To-Animals tried to steal the Long Shot from the Puppeteers...
That odd texture on Proteus has got me scratching my head. It's too distinct to be a processing artifact. Does anyone know if any other solar system body exhibits half-swirls and brush-stroke features like that?
Yeah, I noticed that too, Dan. (I was also struck by the apparent low cratering rate, but it seems logical that the inner Solar System was/is much more prone to this; Neptune's orbit may sweep out a lot more volume of space, but there's also probably been a lot less debris out there since well before the LHB.) However, I do recall seeing things like the "brush strokes" in other enhanced imagery of other objects, so my money's on image processing artifacts.
Many of the "brush strokes" are cracks that radiate from the large impact craters. As for the unusual features in the lower portion of the high resolution image, I always interpreted them as artifacts until the same features showed up in the second closest image. I have heard the theory that Proteus is the reconstituted remains of an old Neptunian moon that was destroyed by Triton's arrival. That may have something to do with it.
One things that helps is that although the closest frame is a single, underexposed frame, the next closest set has four images, and the more distant shots are made using two images. This allows for much more effective noise reduction when compared to the lone Voyager image of Puck. It's dimensions are 440×416×404 km, compared to about 502 km for Enceladus, 480×468.4×465.8 for Miranda, and is a bit larger than Mimas (414.8×394.4×381.4). Ceres also falls in that range (487 km at the equator, 455 km at the poles). Nereid is only ~340 km in diameter, and Larissa comes in at 216×204×164.
I think you mentioned the diameter values for all the bodies except for Ceres, for which the numbers correspond to the radius. I' m almost sure Ceres has twice the size of Proteus, Miranda or Enceladus.
Marc.
Oops, you are right. I remembered an asteroid was in that range, but it is Vesta (578×560×458).
Think I need to give myself a photoshop tutorial.
Very nice work with the enhancements - great to see even a tiny bit of detail on Nereid (especially since we probably won't be out this way again for 30 or 40 years)
I noticed Steve Albers updated his Ariel map, he improved a bit of Uranus-shine part of Ariel
Yes, those are the images I reprocessed for my LPSC presentation.
Here are three of the main views.
Wonderful stuff. Especially like the Ariel work.
Dragons...now that would be a neat discovery!
Here is my guest blog about it that I wrote during the conference.
http://planetary.org/blog/article/00001362/
Cool. Are those two more moons to the left of Uranus? Where'd you get the data? Links, please!
--Emily
The inner one definitely is. The outer one may be a moon and may be a star (I am basing this on image to image motion). I will add that these were taken using the ACS wide field camera. High Resolution Channel images were taken during the transit, but they all missed the planet.
These images are from a large set http://archive.stsci.edu/proposal_search.php?mission=hst&id=10805. The datasets involved are:
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j9q307lhq
Here are some other sets of HST Uranus data from the same time period (and some Neptune stuff as well, since some of the proposals were mixed). Also, there were a lot of WFPC/2 images taken last year, but those are still proprietary.
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10870
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10534
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10473
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10502
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10170
http://archive.stsci.edu/proposal_search.php?mission=hst&id=10102
http://archive.stsci.edu/proposal_search.php?mission=hst&id=9823
http://archive.stsci.edu/proposal_search.php?mission=hst&id=9725
http://archive.stsci.edu/proposal_search.php?mission=hst&id=9035
http://archive.stsci.edu/proposal_search.php?mission=hst&id=9344
Here's the http://space.jpl.nasa.gov/cgi-bin/wspace?tbody=799&vbody=399&month=7&day=26&year=2006&hour=13&minute=20&rfov=2&fovmul=-1&bfov=30&porbs=1&showsc=1. Looks like the inner dot is Miranda; the outer one must be a star as there's no other moon that's close.
--Emily
Even including smaller moons, no moon matches the location of the outer dot. It would have to be exterior to Miranda (if in the ring plane).
I should also add that this was created using red-near IR filters, as there is no data available any "bluer" than red in this set.
Here is the Oberon sequence. It is hard to believe that this is the best sequence we have for Oberon, but it is.
Here is Tayfun Oner's map, which is labeled with some of the few names. http://www.solarviews.com/raw/uranus/obermap2.jpg
Also, comparison between these two images show that the peak on the limb is associated with a large basin. Also, there is a large basin next to Coriolanus on the terminator, which can be seen clearly in the distant image.
Here is my first Oberon map revision in nearly 3 years - thanks to the updated imagery from Ted Stryk. In addition to an earlier color image from Ted, the two largest ones are included from the new set:
http://laps.noaa.gov/albers/sos/sos.html#OBERON
I think the other smaller images may cover much of the same territory, though it is hard to be sure.
That's the latest,
Steve
I posted a short blog entry on poor Umbriel.
http://planetimages.blogspot.com/2009/10/murky-views-of-umbriel.html
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