Voyager and Galileo Images of Ganymede, The Ganymede images and mosaics thread |
Voyager and Galileo Images of Ganymede, The Ganymede images and mosaics thread |
May 18 2007, 09:43 PM
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IMG to PNG GOD Group: Moderator Posts: 2256 Joined: 19-February 04 From: Near fire and ice Member No.: 38 |
I've been processing some of the high resolution Galileo Ganymede images recently. As far as I know the two mosaics below have not appeared at the official websites (at least not in this form) so in a sense they are 'new'.
The first one was obtained during the G1 flyby in 1996. It covers a part of Memphis Facula which is centered at roughly 15°N, 132°W. The images were obtained at a distance of approximately 5000 km from Ganymede's center. The second one was obtained during the G28 flyby in May 2000. It is centered near 14.5°S, 319.7°W. The images making up the mosaic were obtained at a distance of roughly 4500 km from Ganymede's center. I will probably post more Ganymede mosaics later this month or next month. |
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May 19 2007, 03:56 AM
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Merciless Robot Group: Admin Posts: 8789 Joined: 8-December 05 From: Los Angeles Member No.: 602 |
Bjorn, honored to be the first to complement you on this remarkable work!
Interesting that Ganymede seems to have its own 'look' on this scale. The crater rims seem to be quite rounded, almost eroded in appearance...I'm at a loss to explain this, unless they are truly ancient and this is the result of micrometeoroid action over the ages as we see on the Moon. However, this conflicts with the existence of very prominent fracture/faulting features...odd indeed. -------------------- A few will take this knowledge and use this power of a dream realized as a force for change, an impetus for further discovery to make less ancient dreams real.
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May 19 2007, 08:51 AM
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#3
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Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
One of the things that seems to happen on Ganymede and even more so on Callisto is the sublimation of ice by "dirty" regolith. Icy dirt gets hot enough in the afternoon to sublimate ice and darken itself. That accelerates the process. At the same time it can tend to creap downslope, tending to thin and expose more ice on elevations and slopes, lightening those surfaces and slowing the ice evaporation process. That seems to be very important in the highest resolution images, from what I've read (and also speculated myself). Callisto high-rez images show the resulting topography best.
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May 19 2007, 03:49 PM
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#4
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Interplanetary Dumpster Diver Group: Admin Posts: 4405 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
Great work! It really is amazing how many good Galileo mosaics/images never became public release products. Here is one from G-2 (use the link for a higher resolution version).
http://www.strykfoto.org/g2-1a.jpg -------------------- |
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May 19 2007, 04:26 PM
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#5
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Senior Member Group: Admin Posts: 4763 Joined: 15-March 05 From: Glendale, AZ Member No.: 197 |
Thank you Bjorn. That was a real treat.
Too bad it's such a cliche now, but the term "alien landscape" would be most appropriate here. -------------------- If Occam had heard my theory, things would be very different now.
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May 20 2007, 01:58 AM
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#6
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IMG to PNG GOD Group: Moderator Posts: 2256 Joined: 19-February 04 From: Near fire and ice Member No.: 38 |
Great work! It really is amazing how many good Galileo mosaics/images never became public release products. Here is one from G-2 (use the link for a higher resolution version). From the G2GSPLMPST01 imaging sequence it seems. Interesting that Ganymede seems to have its own 'look' on this scale. The crater rims seem to be quite rounded, almost eroded in appearance... I have noticed this too. Sublimation is probably significant. However, in some cases the very high contrast between the bright and dark material plays tricks on one's eyes and makes the relief appear greater than it really is. Finally, here's a new one. This is a mosaic of 16 images from the Ganymede 2 G2GSLTDKBD01 imaging sequence obtained on September 6, 1996. The images show an area at ~61°N, ~170°W and were obtained at a distance of ~4300 km from Ganymede's center. North is up and a bit to the left. Many of the images were heavily compressed aboard the spacecraft (several by a factor of more than 20) so compression artifacts are clearly visible. This also significantly reduces the resolution (by a factor of roughly 2-4). This is also apparent in Ted's mosaic above. |
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May 20 2007, 05:38 AM
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#7
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Merciless Robot Group: Admin Posts: 8789 Joined: 8-December 05 From: Los Angeles Member No.: 602 |
Wow! Thanks yet again, Bjorn!
Temperature-dependent selective erosion aside as Ed correctly mentioned...this is odd. The 'hummocks' clearly are more recent than the craters, and actually seem to be destroying them over geologically recent time scales. Ganymede seems to be far more active than I thought.... -------------------- A few will take this knowledge and use this power of a dream realized as a force for change, an impetus for further discovery to make less ancient dreams real.
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May 20 2007, 09:40 AM
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#8
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SewingMachine Group: Members Posts: 316 Joined: 27-September 05 From: Seattle Member No.: 510 |
Can't help but toss my hat in the ring with this obscure observation from the E12 orbit in December 1997. Galileo passed within 20,000km of Ganymede and took this hard-to-decipher oblique pan across the floor of the giant Gilgamesh basin. The fractures scale all the way down to the limit of resolution in the right-hand portion of the mosaic.
-------------------- ...if you don't like my melody, i'll sing it in a major key, i'll sing it very happily. heavens! everybody's all aboard? let's take it back to that minor chord...
Exploitcorporations on Flickr (in progress) : https://www.flickr.com/photos/135024395@N07/ |
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May 20 2007, 09:43 AM
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#9
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Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
Apparently we're seeing similar temp controlled sublimation at Iapetus and Hyperion. There's very un-intuitive feedbacks going on in the processes, I suspect, and quick-and-dirty arm-waving analysis can only go so far. These terrains will look *STRANGE* when we finally get some hard lander down on these objects. The fractured and faulted ice terrains of Europa and volcanic terrains of Io (not the S02/Sulfer etched terrains and the like) will look positively familiar, I suspect.
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May 20 2007, 12:15 PM
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#10
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Member Group: Members Posts: 241 Joined: 16-May 06 From: Geneva, Switzerland Member No.: 773 |
Thanks a lot to all of you for these great mosaics !
These pictures were taken 10 years ago, and there is still a lot to do with them. Did anybody try to assemble the very high resolution pictures taken during G1 over Xibalba Sulcus ? Due to their "bad" quality, it might be difficult. I even don't know if they really overlap ! I also did not find any mention about the G29 images. What about the regional and color polar cap boundary mosaic near Perrine Regio ? Finally, there were these pictures taken when Ganymede was in Jupiter shadow in order to look for aurora events : http://pdsimg.jpl.nasa.gov/outdir/4846r.img.gif I never heard about them in any publication. As you can see, my "frustration" is still quiet high ten years later, and that's why I really enjoy your posts. Marc. |
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May 20 2007, 06:57 PM
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#11
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Interplanetary Dumpster Diver Group: Admin Posts: 4405 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
Well, I have this color mosaic I put together a few years ago from G29. I will say that because I made it years ago, I used relatively crude methods compared with what I use now, but at any rate, here it is.
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May 20 2007, 07:02 PM
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#12
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Senior Member Group: Moderator Posts: 3242 Joined: 11-February 04 From: Tucson, AZ Member No.: 23 |
I might as well join the fray too:
Both of these are from a non-targeted encounter during orbit C9. C9GSSULCUS01 Distance to planet center: 84379 km This four-image mosaic covers portions of Xibalba Sulcus (roughly N-S set of grooves and ridges at the center of the mosaic) and Nineveh Sulcus (the roughly E-W set of grooves and ridges on the right-hand side of mosaic). This mosaic is roughly centered near 28 N, 82 W. Xibalba Sulcus seperates Galileo Regio on the left and Perrine Regio on the right. C9GSGLOBAL01 Distance to planet center: 201468 km This seven-image global mosaic is centered on Ganymede's leading hemisphere, with Galileo Region on the limb at upper left, Perrine Regio near the terminator at upper right. The bright ray crater Cisti can be seen near the bottom. -------------------- &@^^!% Jim! I'm a geologist, not a physicist!
The Gish Bar Times - A Blog all about Jupiter's Moon Io |
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May 20 2007, 09:01 PM
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#13
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Interplanetary Dumpster Diver Group: Admin Posts: 4405 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
Here is a montage of Galileo Callisto and Ganymede views I did. I could swear I have a version of the Ganymede image somewhere without the horribly saturated whites, but I am not sure (it was a victim of my crash a few years ago, but I could swear it was backed up). In both cases, the color data is filled in from other orbits and Voyager.
Click the link for full resolution (keep in mind that full resolution is keyed to the Callisto image, which is much smaller). http://www.strykfoto.org/calgan.jpg -------------------- |
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May 20 2007, 11:16 PM
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#14
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Senior Member Group: Admin Posts: 4763 Joined: 15-March 05 From: Glendale, AZ Member No.: 197 |
I will say that because I made it years ago, I used relatively crude methods compared with what I use now Me too. Since the advent of Photoshop I have saved a fortune on tape and razor blades. You can hardly see the scars on my fingertips any more. -------------------- If Occam had heard my theory, things would be very different now.
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May 21 2007, 03:11 AM
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#15
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Interplanetary Dumpster Diver Group: Admin Posts: 4405 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
I have now completed my earlier post with an improved Ganymede and added Europa and Io.
http://www.strykfoto.org/calgalileans.jpg -------------------- |
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