Here are 66 false-color images from the 1400 orbit range.

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PSP_001406_2680 looks like the higher relief was saturated (too bright for the camera settings), possibly due to CO2 frost cover.

PSP_001432_2015 is really cool; it’s on the edge of Olympus Mons, on the steep scarp leading to the much more gradual rise of the shield volcano. The rippled rolling dunes in PSP_001432_2610 are in striking contrast to the rocky floors between them. Check out the amazing slot canyons fractures along the left side in PSP_001440_2175.

The atmospheric haze in PSP_001444_2610 is incredible, though it does screw up the color registration on the bottom half of the image. This is 30 degrees East of the aforementioned dune location, but the same type of terrain. On some of these images, there will be CTX (Context camera) images. With similar haze conditions, over on UnmannedSpaceflight.com, Nirgal shows a colorized CTX image from MRO orbit 3624 for which there is a HiRISE view.

There are so many other great images in this set. The Holden Crater image deserves special mention. This area is on the candidate list for MSL, as mentioned in a previous post. A stereo print was made of this region at about the same resolution you see here; it was amazingly sharp, like looking into a scale model or diorama.

Again, feel free to post your favorites here in the comments.

Updated (2008-Apr-10)

Today a press release went out about a forthcoming paper in the journal Geology (click here for full text online or here to download a PDF). John Grant, a Co-Investigator on the HiRISE science team, is the lead author, and most of the co-authors are also on our science team.

What is a megabreccia? A breccia is a jumbled-up mixture of broken rocks, cemented together by a finer-grained material. We see them in impact craters and volcanoes on the Earth, places where there was a lot of violent energy to break up rocks. A megabreccia is just a larger version of that – something we can see with HiRISE resolution, as opposed to something you’d have to pick up in your hand to identify. The megabreccia in Holden formed when the explosion that opened the crater shattered rocks, mixed them up, and then the fragmented ejecta collapsed back down into the crater. Before HiRISE, we didn’t have the resolution to detect these textures.

This is a cutout of an image taken in Holden Crater, showing the megabreccia texture, in false color as usual. A context map is shown to the right, showing where in the crater rim this image is located (click these images to enlarge). The blocks here are mostly darker, and they’re embedded in a lighter-toned material. The dark chunks are kind of “scooped out,” which means they’re more easily eroded than the surrounding light-colored rock. Scientists think this may be because they’re sedimentary rocks, formed at the bottom of a lake or river. The stripey dark blobs on top are sand dunes that are slowly covering up the area again.

This megabreccia is located in an area scientists find fascinating for other reasons, too: there are clays that were laid down over a long period of time when it had to be wet. This implies there was once a lake in this crater – perhaps more than once over its history. At one point, the lake broke through the rim of the crater, releasing a huge flood of liquid water. You can see the channel this formed in the context map above. This flood eroded away material that was covering the megabreccia, exposing it for HiRISE to see.

The HiRISE image PSP_003077_1530 shows another part of Holden Crater, and the caption includes more information about the geologic history of the area.

You may have read that, late last year, the list of candidate landing sites for the next mission to be launched to Mars (the Mars Science Laboratory) was narrowed to six. HiRISE and other MRO instruments play a critical part in the selection process. MRO scientists at JPL put together a short presentation to show these six sites for outreach purposes (thanks!). I’m putting it up here in online form (i.e. blame me if it doesn’t work).

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