Time for a new thread... we should be starting up right about now after conjunction, and if no other targets have popped up our plucky rover should be heading south within days. This should be quite a scenic trip, so sit back and enjoy the fun.
Phil
Good timing, Phil - the first post-conjuction pics are coming in now:
http://qt.exploratorium.edu/mars/opportunity/pancam/2013-04-27/1P419822192ESFBY00P2651R8M1.JPG?sol3285
Now we know the sun's still shining on Mars!
Technically we haven't seen any images from the last 6 sols or so yet, but I'm going to take a leap of faith and assume those will be coming soon.
http://solarsystem.nasa.gov/news/display.cfm?News_ID=43484
Adding: @mikeseibert on Twitter says "Oppy should be back to regular operations after tomorrow's uplink. #knockonwood" So let's knock on wood.
If that's the case I'm off to listen to Tony Orlando...
As they say on the Internet: "Squee!"
Oh well, any is good
This is being widely reported right now:
http://www.nasa.gov/mission_pages/mer/news/mer20130429.html
So is Oppy up and running, or was that premature optimism and they're still trying to regain control?
tl;dr - or ?
I don't think there is any reason to be worried at this point.
I know we're all in withdrawal but hang in there folks, I'm sure we'll get our fix soon.
http://solarsystem.nasa.gov/news/display.cfm?News_ID=43484 has been updated today to confirm that Opportunity has resumed normal operations.
Our beloved Rover Driver was featured in a http://www.bbc.com/future/story/20130501-getting-stuck-in-a-rut-on-mars today
From the http://www.planetary.org/explore/space-topics/space-missions/mer-updates/2013/04-mer-update-opportunity-emerges-from-conjunction.html, some more details about plans:
And, per the more immediate plan, Opportunity bumped slightly to the right today (3296). Lots of good info in the Update, as usual.
Tau has jumped a lot in the past week or so, from around the 0.7 level where it's been for a long time up to 1.5 on 3301, as http://www.lpl.arizona.edu/~lemmon/mars-tau-b.html shows. This is the highest it's been this Martian year, although as you can see from the chart, we've had very similar jumps at the same solar longitude in previous years. So hopefully it will drop back down quickly (within a couple of weeks), as it has in the past.
The increased dust is very obvious in both the lightness of the shadows and the haziness of the far rim of Endeavour by comparing these views from 3296 and 3301:
http://qt.exploratorium.edu/mars/opportunity/forward_hazcam/2013-05-02/1F420797168EFFBY08P1201R0M1.JPG?sol3296
http://qt.exploratorium.edu/mars/opportunity/forward_hazcam/2013-05-07/1F421239422EFFBY08P1148R0M1.JPG?sol3301
I was reading again the http://www.planetary.org/explore/space-topics/space-missions/mer-updates/2013/04-mer-update-opportunity-emerges-from-conjunction.html this morning. If the plan is still the same, the above FHAZ image may be one of the last ones from this site.
From the http://www.msss.com/msss_images/2013/05/08/
Here's an MI mosaic from the images taken during sol 3301.
thanks for the nice mosaic, for a second it carried me back to the other thread looking at an orbital view of Gale..!
It looks like we're on our way:
http://qt.exploratorium.edu/mars/opportunity/forward_hazcam/2013-05-15/1F421864208EFFBYAEP1211R0M1.JPG?sol3308
Yeah!!
Looking at the "telemetry" I read something like 24m due south. A proper map update will have to wait 'til tomorrow when I'm back home.
We hit the road, Jake!
(thanks for everything)
And a further 80m tosol (3309)
So, we're now about 140 mere meters from Apollo 17th rover record. I'll expect Oppy will be n°2 quite soon, still 1.1 km short to pass Lunakhod 2. GoOppy, go
http://en.wikipedia.org/wiki/Lunokhod_2
The Lunokhod 2 achieved its distance record in about 6 months.
Contributing to this, the top speed of the rover was about 1.2 MPH compared to the MER and MSL rover speeds of about 0.1 MPH.
Opportunity may break the distance record, but I think it will be some time before the speed record is broken!
The beginning of a new journey is for me the occasion to going back to some imagery That was a long time not stitching and coloring these picture from our old little girl .
Sol 3303 - Dusty atmosphere this sol :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3303_pancam.jpg
And a last Navcam pan before the move :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3308_pano.jpg
(And also, a new gallery with a timeline, just like Curiosity http://www.db-prods.net/marsroversimages/opportunity-2013.html )
And ~95m more tosol (3310)
Quick look at some features just ahead in a stretched view of the Navcam frame.
Phil
James tweeted: "Oppy sol 3310 - Took pancam images of Karratha & Corunna Downs. Then drove 95m SW along Cape York. "
Do we know yet which features these are?
Phil
(always hungry for feature names)
Looks like there's another drive coming up for sol 3312.
Sol 3308 panoramic updated :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3308_pano.jpg
And the Pancam drive direction
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3308_pancam.jpg
Thanks, Ant. Isn't it great to see drive-direction pancams again?
Based on the drives so far, it looks like the plan may be to hug the "coast" of CY, just inland, rather than driving straight for Solander Point.
Actually, I'm wondering if she will do a quick stop near Odissey to image those old tracks around it.
According to the last http://www.planetary.org/explore/space-topics/space-missions/mer-updates/2013/04-mer-update-opportunity-emerges-from-conjunction.html
"We calculated a rapid transit... " Arvidson informed. "....This route allows for a short stop at Nobby's Head so that the rover can take some stereo images of the northern side of hill for engineering characterization of slopes, just in case we need a possible bail-out location for winter, but other than that it's a path that will take Opportunity to Solander as quickly as possible..."
Illustrated in the March 1, 2013 entry http://www.nmnaturalhistory.org/rover-field-reports-from-mars.html
Just bck to Opportunity's driving record, there's a nice little poster on vehicle driving distances (Moon and Mars) over on i09.
http://io9.com/the-records-for-the-greatest-distances-driven-on-mars-a-508328297
Back to the drive south
This looks like a good place to add a note of caution about Lunokhod driving distances. They will have to be recalculated based on the LROC images. When the actual Lunokhod 2 tracks are compared with the original Soviet-era map, it looks to me like they landed slightly north of the expected location, drove a bit further south than they thought, then east, and finally ended up further north than they thought. Some extra distance will probably come out of a recalibration of the drives (maybe they allowed for more wheel slip than actually occurred). A new mapping effort is under way at MIIGAiK - they already did Lunokhod 1 and are working on Lunokhod 2. Maybe by LPSC next year we will have a result. Just a caution - we might break the record and then have to break it again!
Phil
Don't just read that great site by Larry Crumpler - those images, especially the maps, can stand a considerable amount of enlargement. Lots of good stuff! Too bad there doesn't seem to be an archive of past reports like these.
Phil
Another drive...
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-19/1N422223111EFFBY%23%23P0713L0M1.JPG
Phil
Did you also notice that we (I on the Spirit & Oppy Statistics) used to get 35890 for Apollo 17 rover and this is also used on the New Mexico Museum's but Nasa says 35744...and tthey can't be wrong
Phil, do you think all Moon driving distances will have to be reevaluated?
Thanks
Apollo should be much better than Lunokhod because they had high resolution orbital images and lots of backup position data. I would not have expected much change for Apollo distances. I will look into the difference in those numbers.
Phil
Yes, they zeroed the nav system several times during the EVAs. And the system only told you the range and bearing back to the LM. Total odometry was calculable from this (it was calculated on wheel turns), but was considered somewhat of a "dead reckoning" system. Wheel slippage and meander to avoid rocks and craters meant that the nav system would get you back to where you could see the LM and drive back to it by eye. No one ever pretended that it could tell you within a few meters *exactly* where you were or how far you had driven.
On the LRV, the range and bearing were more often used in finding the planned station stops, and due to the various small detours and wheel slips these readings usually varied from the pre-mission calculated values, even when the slight variations in landing point were taken into account.
All this is to say that you'd have to do the kind of detailed wheel-track analysis they're now doing with the Lunakhods to get the absolute exact distance traveled by any of the LRVs. There is a "wander factor" in the LRV nav data that makes all calculations based on them somewhat approximate.
-the other Doug
Interesting stats would be long distance targets like Endurance or Victoria or Endeavor and what was the average drive length when heading towards these goals. Before embarking on the trek to Endeavor folks were doing some math about how long it would take.
btw, didn't we have a pool guessing the arrival date at Endeavor?
We had one long-running poll here years back and the back-and-forth arguing both during the drive and after the goal was reached became so annoyingly dull that polls have been banned here ever since.
Sol 3312 panoramas :
Navcam
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3312_pano.jpg
Pancam, drive "yes it's good to read drive " direction :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3312_pancam.jpg
I think I may have equated 'margin' with 'over engineering'.
I still think though the team was staying with the 90/180 day thing, as the costs for a 10 year mission would not have been at the time favorably looked at by the beancounters...... . There was even conjecture at one time one rover would be turned off to save said beans .
Here's an "enhanced version" of a FHAZ image taken during sol 3314.
I don't intend to be as precise as you are Eduardo, but Lunokhod 2's mark will be around there pending we detour to Nobby's Head as "scheduled", right?
This is to show how close we are.
There are some bumps on the horizon to the right. Is that Nobby head, Sutherland point or neither? What are we looking at?
We're now just starting to see Nobby's Head peeking around the side of CY. We had good views of it and Sutherland Point when we arrived at CY, but once we arrive at the south end of CY we should have a different view, since we'll be below Spirit Point/Odyssey, so Nobby/Sutherland may stick above the horizon.
Right on the edge of Cape York now, Nobby's Head/Sutherland Point ahead.
http://www.midnightplanets.com/web/MERB/image/03315/1N422477356EFFBZCUP0723R0M1.html
Fasten your seatbelts and take your gravol - the drive may get a little bumpy as we cross the choppy seas of Botany Bay!
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-23/1N422571856EFFBZJVP0733L0M1.JPG
Yes, a bit bumpy - now we have a clear view of Sutherland Point up ahead.
Phil
This navcam shot is a treat. Level horizon with interesting destination, sundial in the foreground and dramatic lighting: it has everything. Worthy of some artistic treatment in my view.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-24/1N422664439EFFBZW8P0733L0M1.JPG
This pancam mosaic was taken right after that navcam shot. The view of Sutherland Point is improving.
It's been a while since I did one of these vertical stretches - but here I think it helps to relate the horizon detail with the HiRISE image and see where we are and what's coming up. Nobby's Head is still partly hidden from view.
Phil
Sol 3317 panoramas The view to Sutherland Point is very good !
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3317_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3317_pancam.jpg
Artefact or something real ?
Sol 3314, local time between 02:03 and 02:21 pm. 12 images with 1 min separation between the single images.
Cheers, Udo
I assume the automatic routine that makes a small window around the sun is following the sun across the frame (rather than the camera trying to track the sun), so one hot pixel in the detector will appear to move.
Phil
Phil's got it. The solar neutral density filter used in those images absorbs so much light that any star/planet/meteor/satellite would be completely invisible.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-28/1N422650186EFFBZJVP1637R0M1.JPG
Very close to the new 'island' in Botany Bay now!
(oops! Mike just told me that one's looking backwards at Cape York just after leaving it - sorry about that, folks!)
Phil
Nice geologic contact, there...
--Bill
Yes, there's a bunch of Pancam images that should come down eventually mostly have come down.
Today we're treated to a lovely Navcam look back at Cape York, amongst other things. Odyssey Crater is just left of the North marker in this view.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-28/1N422650674EFFBZJVP1637R0M1.JPG
Big dust devil on the slope below Cape Tribulation - or wind gust.
Phil
Ooh, nice. Sol 3317.
I have noticed hints of wind activity on those slopes in the last two weeks or so, but not so obvious. Now we need to get one a bit further north!
This is a very faint DD lower down the hill on sol 3308.
http://marsrovers.jpl.nasa.gov/gallery/all/1/n/3308/1N421855083EFFBYAEP0713L0M1.JPG
Phil
Nice catch, Phil. Since the navcam imagery is only momentary, we're probably missing many gusts/dds. We had a cleaning event between 3311 and 3315 - let's hope for more.
Can you post any of those tentative gust images, Phil?
Edit - thanks!
Nice catch! Are we going to get this view in pancams?
I just want to see that "marvelous goodbye cross-section view"...or that "lovely lookback" in pancams.
Leaving Cape York, the "big picture" (Sols 3317 & 3318)
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3317-3318_pano.jpg
And Sol 3317 view of Endeavour.
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3317_pano2.jpg
Maybe it's Postcard time ?
http://www.db-prods.net/blog/2013/05/29/opportunity-dit-adieu-a-cape-york/
I'm wondering about making a colorized version…
Really nice mosaics! One thing they show clearly is how the hills all sit on a slope so the western side of the hill is nearly level and the eastern side is steeper. Remember when we approached Cape York and it was so hard to see it from a distance. For that reason it was easy to get 'up' onto the ridge of Cape York. But looking further south suggests the same will be true at Solander and even Cape Tribulation. They are steeper than Cape York, certainly, but it certainly looks like we can get all the way to the top of any of those hills from the west side.
I have been looking at the hills in HiRISE to see if the range of features visible at Cape York is also available further south. I especially hope to see networks of large filled cracks like we saw on Shoemaker Ridge but did not investigate at the time. So far I have not noticed anything like that, but maybe I have not looked at the best images yet.
Phil
This site seems to be the most comprehensive resource out there as far as I'm aware.
http://www.planetology.ru/panoramas/lunokhod2.php
The TV images used for driving ('hazcams') were recorded on tape. When the Soviet Union fell apart the tapes were taken home by one of the participants who probably hoped to sell them at some point. That never happened and the tapes were recovered a few years ago. So far they have not been read and the images recovered, as far as I know - if they have nothing much has been done with them. But a lot of work is going on in this area now. I have had this from the people involved, especially Kira Shingareva.
Phil
Yes, third from the left.
Phil
OK... Shirley they moved today.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-05-30/1N423192800EFFC000P0722R0M1.JPG
Phil
Yes; approximately 75m SW toward Sutherland Point on sol 3323. And stop calling us Shirley.
Adding: Here's an http://www.flickr.com/photos/marscat/8892256669/ from the sol 3323 location. We should be right next to that small crater along the way on the route map, so the next couple Navcam images to come down might be interesting.
And there it is: the small crater to the west on sol 3323. For a minute I thought it was not there. Very hard to make it out except in stereo; not what I was expecting to see!
http://www.flickr.com/photos/marscat/8893906947/
http://www.flickr.com/photos/marscat/8893906947/ on Flickr
A bit clearer if we perspectivize it (is that even a word?)
Phil
Sols 3317 & 3318 panoramic is getting full circular
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3317-3318_pano.jpg
A small crater met at Sol 3314 :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3314_pancam.jpg
And the last panoramas, Navcam and Pancam, from Sol 3323. Clearer view on Sutherland
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3323_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3323_pancam.jpg
This is Ant103's Sol 3317-3318 panorama in circular format.
Phil
And here she is at "Sutherland Point" - or pretty close to it anyway - on sol 3324. The drive was about 79m southwest, more or less - probably more, since she didn't go in an exact straight line.
This is like ve have Mars in live from Endeavour thes days
Today's pan, Sol 3324 :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3324_pancam.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3324_pano.jpg
The ground at our feet is trying to tell us something. What do you suppose it is?
http://qt.exploratorium.edu/mars/opportunity/pancam/2013-05-31/1P422652753EFFBZJVP2372L2M5.JPG
--Bill
That's the ground that was at our feet, back on 3317 when we had just left CY...
Not quite. Botany Bay sulphates are supposed to be well hydrated in comparison to the plain. Perhaps it is just my ageing eyes but despite the lag of big juicy berries, embedded berries seem extremely sparse. - almost as though the lag originated external to the crater.
Looks like we have now hopped up onto the bench surrounding Sutherland Point. More to follow.
Phil
There's those gypsum veins again:
http://www.midnightplanets.com/web/MERB/image/03325/1P423369085EFFC0NSP2378R2M1.html
Phil
A nice view of Solander Point & Cape Tribulation down thissol. Details becoming clearer.
http://qt.exploratorium.edu/mars/opportunity/pancam/2013-06-02/1P423362467EFFC0GHP2585L5M1.JPG
http://www.midnightplanets.com/web/MERB/image/03325/1P423369085EFFC0NSP2378R2M1.html
Any relation to MMB?
>Gypsum veins
May be, but it's a stretch with this/these views-- I see a few light-toned flakes which may be arranged linearly.
Given the genesis of these filled fractures, it's not surprising.
--Bill
"it's a stretch "
Yes, it is. But I think that's what they are. We'll see, as we get further on. This is quite a cute little mini-Cape York.
Phil
I'm on the hopeful lookout more examples of the "gypsum veins". They are the remnant of some wonderful geochemistry. Clays are weathering byproducts but fracture fills are (or can be) the fingerprints of the weathering processes.
> Yes: successor!
And wonderful, too !! I spent the last couple of hours twiddling with it. I'm a traditionalist, and like to go into Exploratorium and "shop", but when the relay comms get a bit spotty and we don't get all the images in neat packages the manual browse can be tedious. I just got caught up on my missing L 2, 5, and/or 7 post-conjunction images.
Kudos.
--Bill
I attempted an 'ad hoc' long-baseline stereo pair 'a la fredk'. It's composed of two views toward Solander Point taken on Sol 3325, before and after drive. Since the drive wasn't really lined up to produce stereo, view this image at your own risk - it may induce nausea.
It actually came out a lot better than I was expecting. Once again, I find I was misinterpreting the monoscopic views, and now I can see where Solander Point actually is - which is not exactly where I thought it was! For those without red-cyan glasses, I'm including a 'freeviewing' version, plus separate left and right frames if you'd like to do a blink comparison.
Also: quick http://makeagif.com/i/4UGQsu a la Gerald.
Many images on this Sol 3325
Begin with the drive "pancam" direction :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3325_pancam.jpg
The color view of Cape Tribulation & Solander Point :
http://www.db-prods.net/marsroversimages/Opportunity/2013/1P423362445EFFC0GHP2585LCoul.jpg
Two Navcam panoramics. One before moving, and one after :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3325_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3325_pano2_b.jpg
http://qt.exploratorium.edu/mars/opportunity/forward_hazcam/2013-06-04/1F423640407EFFC01NP1211L0M1.JPG
Looking back, with Sutherland Point at the left, quite far behind already. Just had a good drive!
Phil
About 100m S-SW according to the metadata.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-06-05/1N423717320EFFC01NP1952R0M1.JPG
Those white lines have just got to be gypsum veins again! It would be nice if a really good wide example was waiting for us on Solander Point, because a vein wide enough to brush and analyze properly was never found at Cape York. Homestake and Monte Cristo were too small, if I'm remembering correctly - sure we got some data from them, but not enough. But they only seem to show up on the outer apron, not up on top of Cape York so probably not up too high on Solander either. Oh well, keep looking...
Phil
My thoughts exactly. These look more probable.
Here is an X-eyed Stereo view looking due East from Sutherland Point over the Overlap/Bench area on Sol-3329. Note the probable light-toned veins in the foreground and the wonderful stratigraphy in the midground. The interior dunes and central mound of Endeavour Crater are on the horizon.
--Bill
Heading Nobbys Head, at Sol 3328 :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3328_pano.jpg
And a closer look with Pancam :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3328_pancam.jpg
An Opportunity telecon is coming up on Friday
http://www.jpl.nasa.gov/news/news.php?release=2013-192
It would be nice to get an update on findings... but maybe there will also be some news about distance records. There is some news but let's see if it gets mentioned tomorrow.
Phil
Planetary Society report:
http://www.planetary.org/explore/space-topics/space-missions/mer-updates/2013/05-mer-update-opportunity-departs-cape-york.html
Now that I'm getting caught up with the recent imagery, I'd like to share an image of part of the Ringtail outcrop in the Meridiani Onlap/Cape York, an L257 taken on Sol-3317. Nice colors, nice sedimentary structure-- our old friends, the Fine Laminations and Burple Strata.
--Bill
OK.. last question touched on Lunokhod 2. Steve was non-committal in his answer. Let me point interested parties to this Russian presentation from last year:
http://meetingorganizer.copernicus.org/EPSC2012/EPSC2012-464.pdf
In it you may find a surprise. A much longer distance, 42 km. And I can say that the more refined answer now is thought to be 42.1 km.
Why is this? The old value was based purely on engineering data, wheel turns and drive times etc. There was no chance to compare locations after each drive as we do now for Opportunity and Curiosity, because the available orbital imagery was inadequate. The engineering data are good for short drives but drift away from the correct value quite rapidly because of wheel slip and maybe sensor errors. Now we can check the actual distance using LRO images of tracks, and that's what the people at the mapping lab at MIIGAiK in Moscow are doing. They are not quite finished because they don't yet have high resolution DEMs for the whole traverse.
The old value was quite short, 5 km shorter than the new value. I think it is because they assumed a lot more slip than actually experienced, but it might also be a sensor problem. For Lunokhod 1 the new drive distance from LRO track mapping is 9.5 km, shorter than the old estimate - so you can see it's not very straightforward.
This is not really unique to Lunokhod 2. See this paper:
http://www-robotics.jpl.nasa.gov/publications/Mark_Maimone/05pers_mer.pdf
or this one:
http://www.lsgi.polyu.edu.hk/staff/Bo.Wu/publications/li&wu08_jgr_characterization_of_traverse_slippage.pdf
MER also has its issues with this, but we can fix the problem with the method called Bundle Adjustment in that paper. The Lunokhod team could not. Final result of all this - we have quite a way to go before we can be confident of beating that old record.
Phil
And then the actual ground distance traveled may be greater than the simple map distance due to the effect of rolling over the topography. Complex situation.
--Bill
Complex and interesting since, just for the record, a Marathon is 42195m. Don't tell me that Lunokhod 2 stopped 95m short to complete the task! Serriously, you're right, we have to wait to exceed and be sure.
Going through archives and looking at images of the Meridiani Onlap during the approach of Cape York around Sols-2676-2681 I came across this: a Navcam pano with 3x vertical exaggeration taken from the Meridiani Onlap on Sol-2679 showing Cape York on the left, Odyssey Crater in the center with Cape Tribulation above center on the right and Sutherland Point/Knobby's Head in the area just below right center.
It's deja'vu all over again...
--Bill
Note-- updated the attached image to a "slightly improved", wider version.
That is such a killer image on so many levels.
It even makes me feel seasick!
Phil
Takes me back to the old Spirit route map days, with the valley between Husband and McCool hills, and Home Plate....
It gives me a touch of vertigo seeing and thinking about the Central Mound and the Eastern Rim of Endeavour off in the distance behind Cape York...
Ideally, it would be nice to have a similar treatment of a similar Pancam panorama, but in reality Oppy was zipping along on the fast-track to get to Cape York ASAP, so I'm thinking that this Navcam sequence will be all we've got.
Aye, It reminds me of the heady days of Sputnik and Gagarin when the world trembled at the sound of our (rovers)...
--Bill
Note-- updated the attached image in Post#131 to a "slightly improved", wider version.
In case anyone's confused by the recent http://www.nasa.gov/mission_pages/mer/multimedia/pia17078.html that shows the sol 3325 view towards Solander and Tribulation, they've mislabelled those two features. Solander and Tribulation (and Byron behind it) are very closely aligned now, as you can see from this orbital view:
Interesting. That did puzzle me, but I think you're right.
Adding: Earlier I did this ID of Solander Point, which I think matches up with what you've labelled. (When they posted that slide, I figured I'd got it wrong again.)
http://www.flickr.com/photos/marscat/8960884717/
http://www.flickr.com/photos/marscat/8960884717/ on Flickr
Yes indeed, Fredk is right.
Phil
I don't think it was an error as much as it was sloppy graphics-- the annotations were in their correct locations, they just needed arrows drawn down to the hills.
I've always looked at Tribulation as "that big hill over thar" and Solander as "them foothills"...
--Bill
But the caption says
Well, I guess the caption does shred their cred...
--Bill
I just noticed all the frames of "Esperance" post-RAT on Opportunity sol 3308 are down. Here's the stretched L456. Beautiful.
That is beautiful. What a gallery of rocks we could put together now!
Phil
I'm think of the "Burple Rocks" being associated with Santa Maria Crater (Sol 2450-2546) and consequently the lower units of the Burns Fm, as was that Brown-Toned rock type, and others. I think of Erebus as being more about the Festooned Beds and the Weathering Rinds on rock surfaces. Or so my creaky memory sez.
I've been going through and organizing the images better and categorize everything in a searchable relational database. Been putting this Herculean task off for years, though I do have the work on some some sites started. But now that I've "discovered" Midnight Planets ( http://www.midnightplanets.com/index.html ), it will make this organizationizing (is that a word??) much easier. Thanks, Mike Howard!!!!
Currently, I'm focused on the "Meridiani Onlap", that critical contact between the Meridiani Burns Formation and the earlier weathered Endeavour ejecta apron. We have many images of that zone from the Cape York approach and many from the Cape York exit.
So much to do, so little time.
Thanks for the Espernace RAT images, Mike. I've been waiting on images to come dribbling in on that area (the usual post-conjunction logjam). Time to move _that_ off'n the back burner, too...
BTW, in the data pipeline today (?) we have a series of MIs of the soil at Knobby's Head and Pancams of a new site named "Gnarlaroo". On my Wish List at this site? Those dunes on the eastern side of the Knobby Bench... an opportunity to sample wind-transported material from inside Endeavour Crater. Both the light-toned longitudinal dunes and the dark-toned pre-barchans.
Stay tuned...
--Bill
On the road North to Nobbys Head (Sol 3330)
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3330_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3330_pancam.jpg
(Tosol we are Sol 3333, all the same numbers )
This is what our Intrepid Explorer is up to:
First is a crop of the HiRISE image ESP_018701_1775_RED.JP2 showing the northern part of Knobby's Head. It is inverted so that South is up so that it can be viewed in context with the next Pancam pan. The "*" shows the guesstimated location of Oppy on Sol-3330 and the arrow shows the approximate look direction. Those tasty dunes I mentioned earlier are in the upper left of this image, but I'll s'pose that the drive direction will be towards upper right.
And next is a panorama of the leftmost two images of the Pancam "next-drive" image set, cropped and exaggerated 3x. View is to the Southwest.
And so it goes...
--Bill
Back a few sols, on Sol 3308, Oppy has imaged her tracks in color :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3308_pancam2.jpg
Sol-657, Dec 2005, has it been that long? And that Mogollon Thread, as well as the Mogollon and Olympia and Payson, et al, sites are well worth a read, well worth the review.
And I'll note that the "attached image" is by MMB. Thanks, Mike, again.
I got a chuckle. One response to your post was "Here we are, kneeling on this wonderful outcrop, can't find the handlens or scratch plate, and the carpal tunnel is acting up... ain't life wonderful", and the author of that reply didn't have corrective surgery until 2012.
Check MMB/MP. Another installment of imagery-- looks like Oppy is on the move, and going on the West side of the rim outcrop at Knobby.
--Bill
Talk of purple layers in sandstone has triggered a childhood memory. Digging through the white sands of beaches in the west highlands of Scotland I used to encounter discrete purple layers. Somebody told me at the time these were due to staining by iodine from the seaweed. Thinking back I would have to question this and consider the alternative possibility of gravitational sorting of haematite grains by wave action. On Mars the processes must be totally different but the same colour raises the same questions. Iodine, haematite or something else altogether?
Maybe not Romans but Phoenicians . .
We're getting our first good pancam views of the far rim in a while, as part of the long-baseline Nobby sequence. Here's a spectacular view that shouted out "anaglyph me!":
Here are two L257 Pamcam images from panoramas made on Sol-3325 at Sutherland Point.
The first is titled "Sutherland contact" and the second is titled "Sutherland outcrop". Both sites have intriguing lithologies and textures.
--Bill
Sol 3333 panoramics are down
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3333_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3333_pancam.jpg
Very cool to be roving again! A nice 3D pano to be had from Sol 3334:
Here is another "Vertical Exaggeration" panorama (aka "Philovision") of the Navcam pan from Sol-3333. The Central Mound of Endeavour is on the left, Cape Tribulatin in center with the summit of Knobbys Head on the right. You can still orient via the inverted HiRISE image in my post #148.
Interesting oblique view of the downhill wasting process here.
--Bill
Very nice! And here is a reduced-scale version of it with an arrow pointing to a possible new dust devil. That white streak seems to be missing in older images.
Phil
Indeed, the DD does show better in the vertically exaggerated image. It was fairly broad and diffuse and doesn't stand out in the "raw" image. I wonder if this is a new undocumented feature of Philovision or if it is something that we (or some of us) just forgot about?
Anyways, good catch...
--Bill
On this post-Cape_York leg of the Traverse there is a program called the "color clast survey", which appears to be an extension of the (apparently) defunct "systematic foreground..." program. This is really a good idea to characterize of the soil along the Traverse route. But they need to make sure that parts of the Rover chassis do not reflect into the camera because this can wreak havoc with the Auto-exposure and make processing the image challenging.
--Bill
"it does seem to turn a gusty thing into a DD-like thing."
Maybe you're right - it should be thought of as a little puff of dust raised by the wind rather than an actual dust devil, and the stretched image would be misleading. After all, that technique would make ground cover look like a forest (or the Viking 2 site look like a Christmas tree farm).
As for documentation, I never read it so I'm not going to start writing it!
Phil
May well be, but I'm thinking it'll affect the the total exposure of the frame. We'll see what it looks like in 6 mos when it hits PDS...
Yikes, it's like the fountains at Versailles!
Phil
The @n0m@lists would have a field day with those.
Dust devils? Cool, but possiby a touch passé. The probable gypsum veins in this remnant of the rim are more interesting. The rim has overrun by plains material, which means that there was massive erosion of the NW edge of Endeavour prior to that event. But was the gypsum formed within the rim which implies that these veins predate the plains material deposition and associated liquid water. Or are they the product of the same water event that is evidenced by Opportunity's observations of the plains material? I find it a touch disappointing that there seems to have been little correlation (at least in published articles) between Opportunity's limited area investigations and Endeavour crater as a whole. The hematite signature of the internal mound raises a lot of questions about how there was sufficient groundwater to form berries (assuming they are the hematite source in that area) unless the crater were filled with water.
Wonderful shot of Nobby's Head on Sol 3335, with our goal in the distance:
Yes Walfy. So much imagery this sol
A color portion of a bigger panorama, I think :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3335_pancam3.jpg
The bigger panorama, in greyscale for now :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3335_pancam2.jpg
The navcam shot, after a quick drive. Lovely ripples there :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3335_pano.jpg
And the drive direction :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3335_pancam.jpg
If I'm reading correctly, two 6x1 colour mosaics were shot on sol 3335. This is the second one, taken (almost) at the end-of-drive. The first one is still on the downlink queue and was shot before the drive, 35m to the NE.
Sol 3335, wider Navcam panorama :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3335_pano2.jpg
I have a question about 'contouring'. Walking in the hills it's not uncommon to follow a contour to avoid losing height. How much does this come into play in rover operations? I note that we have gone round the top side of Nobby's Head and so kept on the level.
The slopes are pretty subtle here and I think they could have done a direct route if they chose to. I think the approach to Nobby is mainly to do stereo imaging in case they need to use it for winter.
Also, they talked about possibly driving around and approaching from the west side of Solander, which would be easier than driving up from the east or north.
Hot off the wire... the central portion of an L257 Pancam panorama of Nobbys Head on Sol-3335:
--Bill
On the road again:
http://www.midnightplanets.com/web/MERB/image/03339/1F424617048EFFC1SDP1205R0M1.html
Phil
This is also a good hint:
A 3D pano from Sol 3339. Looks like we're south of Nobby's Head already, and rough plains ahead!
Solander Point is already showing a touch of parallax! Or am I imagining things. Viewable in http://imgbox.com/adfQ2Qy7.
Here's a smaller version:
Thanks for the nice stereo pan, walfy. I think we'd have to be almost sitting on top of Solander before we could see parallax with pancam...
Navcam and Pancam for this Sol 3339 :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3339_pano.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3339_pancam.jpg
Nothing seems to be between us and Solander Point now
I'm going to propose that this old degrated crater:
Looks like you're right. I guess we will skirt the edge of it.
Phil
This shot renders nicely in 3D, thought I'd share it, overlooking the swale atop Nobby's Head, Sol 3339 still:
Here's a navcam mosaic taken at the current site. It was shot during sol 3342 after driving about 54m SSE from the previous position.
Nature has an interesting story on the distance travelled by Lunokhod 1 and 2 on the Moon.
The scientists from MIIGAiK in Moscow now seem to have finished their analysis using DEM data (see earlier in the thread).
Lunokhod 1: 9.93 km (instead of 10.54 as recorded in the logs)
Lonokhod 2: 42.1 to 42.2 km (instead of 37 km as recorded in the logs)
http://www.nature.com/news/space-rovers-in-record-race-1.13229
So it really seems that Oppy is still quite a long way from breaking the distance record...
Michael
Here is a parting shot of Nobby's Head by Oppy on Sol-3442. A 2x1 Navcam panorama, 3x vertical exaggeration, looking back to the North.
--Bill
Added: Here is a HiRISE image of the site, with the approximate Sol-3442 location of Oppy shown along with the sight margins of the above Navcam pano.
Just something I put together
http://www.flickr.com/photos/43581439@N08/9088077807/
An L257 Pancam of the site "Numbat", Sol-3342, presumably located on the Bench at Nobby's Head. Along with the corresponding R721 Pancam, there is the suggestion of a change in composition of the underlying soil unit.
--Bill
Sol 3343 - looks like we just turned east for a short drive up to the southernmost hill of Nobby's Head.
Phil
If I'm reading the data correctly, Phil, there was no drive on 3343 but there's one planned for 3344.
Oh... OK... I was looking at this 3343 image and thinking it had to be where my lines show it here.
Phil
Tis possible-- you;re thinking that the light-toned fragments to the South (Navcam) are that low hill to the South (HiRISE)? The relief is so subdued here it's hard to tell. We have a Navcam Albedo pan on the table (with one bad frame), that would be ideal to polar project for Location. Expecting that last image just anytime...
--Bill
I think your position is correct too, Phil. The drive direction images on sol 3342 were facing east, so perhaps she's not done photographing Nobby's Head. Here's an anaglyph view.
This is half of a circular pan from sol 3339. The low hills where we are at present (3342) are visible to the southeast of this location.
Phil
The "missing piece" of the Albedo Pan hasn;t arrived so I did a quick cylindrical pan and reprojected it as a Polar pan.
Sol-3342, p2297, L2 Albedo Pan. North approx up:
--Bill
Practicing a bit with polars, here is a 3x1 Navcam from Sol-3442. North approximately up.
And we have several interesting Pancam sequences in the pipeline...
--Bill
My best "TLAR" guesstimate of where Oppy is on Sol-3345:
--Bill
I think the last two sites, 3342 and 3344, are slightly south of those positions. Here're the two vertical projections I just made to update my route map.
My take on this Sol 2244 & 2245 full 360 Navcam pan
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3344_pano.jpg
Nice pan - here's my circular version. Let's see if we can locate those names on it. (we had a Numbat 2 sols ago, and a Berrio crater near Whim Creek... seems a bit odd)
Phil
Right. The "Berrio Crater" (and -Bench) were Sol-3044. Those hid nicely in the Sol-3344 image list...
--Bill
It's not that bad. There are some 20 post-Esperance named sites and of these 8-9 are the current crop. The problem is keeping up with things in the long run.
--Bill
Wowsers! Looks like we're down on the plains again:
http://www.midnightplanets.com/web/MERB/image/03346/1N425235632EFFC2LMP0703L0M1.html
Phil
Looks like she's folded her tent and is headed Southwardish.
And we never found out about Gibber_Earless...
--Bill
"There are some 20 post-Esperance named sites and of these 8-9 are the current crop. The problem is keeping up with things in the long run."
That's what I am trying to do, to record, maybe not all these names, but as many as is feasible, and locate them on maps. Earlier ones come out of the Analyst's Notebook, but I try to keep up with current ones as well. But it's a lot of work!
Phil
It is a lot of work. Not only the identifying the named sites, but also locating them on polar reprojections of Nav- and PanCam panoramas (if available) and thence to HiRISE images and HiRISE-derived maps. As you well know. The BIG problem is not so much the named sites, but the multitude of "Foreground Quarter" and "Clast Survey"and "one-shot drive-by" images. Even innocuous images like FHazCam and RHazCam shots are useful for soil texture info.
It never ends. Thank goodness...
--Bill
Here is a best guesstimate of where Oppy was on Sols-3342-3344-3346:
The graben-- fault block-- that she passed East of on exiting Nobbys Head bench may show up on the azimuth 270* partial Navcam pan.
--Bill
Here is a 5x1 pano of that Sol-3346 Navcam sequence with a cropped and rotated portion of the above location image, showing the suspected graben/fault block. Note especially the unusual textures of the weathered rock in the "fault plane".
--Bill
Added: A 4x1 pano of the above sequence (left the fifth "northmost" panel off) showing the suspected fault (but not as well as I'd hoped).
--b
Sol 3346 panoramics :
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3346_pancam.jpg
http://www.db-prods.net/marsroversimages/Opportunity/2013/Sol3346_pano.jpg
Now these sites are going to be interesting:
Gibber Earless
http://www.midnightplanets.com/web/MERB/image/03346/1P425226706ESFC2B3P2597R2M1.html
Signal Head
http://www.midnightplanets.com/web/MERB/image/03346/1P425226858EFFC2B3P2391R2M1.html
Got stereo pairs, waiting for the color imagery.
--Bill
This is a cleaned-up view of Solander Point (and Cape Tribulation peeking over its shoulder) - cleaned up by merging the two most recent pancam images to improve signal to noise (mostly JPEG artifacts). There should be plenty of interesting things to look at - I like the long continuous light-toned stratum at the top of the brighter area. (Hopefully it's not just a big dust drift!)
EDIT - see following post - Bill's right of course - looks like the Meridiani plains, AKA Burns Formation, slope upwards a bit where they are plastered onto the tip of the point. But we presumably have to go higher up to get the slopes we need plus the old Endeavour rim material.
Phil
The bright area is the usual Meridiani Overlap/Bench that crops up at the foot of the hills and the continuous stratum may be simply outcrops superimposed along the line of sight. Here is a cropped and inverted ("North" is down) HiRISE image of the target area:
--Bill
It's very nice to have the view ahead and the view from overhead consecutively in the last two posts. Even better would be if someone could identify a few key points in both images to help the rest of us get our bearings. I have to admit I'm struggling a bit to find sure identifications when it comes to the details.
Good idea. It's hard to tell "Who's on First or What's on Second" without a scorecard.
First: An annotated and clarified image from Arvidson, et al.
Second: Phil's "solander_cleaned" image and a HiRISE image, shamelessly annotated.
"HTH"
--Bill
Special treat today: at least part of the sol 3348 drive direction mosaic is in stereo color (L27R12).
And the big filled crater is smiling benignly down on us as we go by.
Phil
"Hello and goodbye. I missed the chance to swallow you but never mind."
Here is a registered and merged combination of the L2 and R2 Drive Direction images from Sol-3350. This shows the Eastern slope of Solander in the vicinity of the "Bluffs" that I identified earlier in Post#223. In the foreground is the light-toned, and blocky, Meridiani Onlap unit. Above it can be seen distinct layers and even ledges of the basal part of the Endeavour Rim unit. This low part of the section has a good chance of having been weathered under wet and warm conditions (say "clay").
Don't zoom in beyond 150%, I didn't do a lot of work here prettyfying it...
--Bill
Very interesting. Is there any way you could combine red and blue? I ask for purely selfish reasons, because false-color drive direction stereo pairs are pretty much my favorite thing ever
Likely yes but now with a shoestring budget any development is tough to justify. Whenever we can we use both when we assess the terrain in front of us but manually, there is no automation behind it.
Paolo
Bill, post 228. It sure looks like strata but we have been fooled by Endeavour many times and Solander is almost certainly as big a dog's breakfast as Cape York. I think we are still in a 'suck it and see scenario'.
May well be Pareidolia in action. There are so many wild-eroded flutes on that surface that they may be looking like lineations at this low viewing angle.
We'll see what we see when we see it...
--Bill
According to metadata, Opportunity drove almost 120m south on sol 3351. Nice!
Nice email sent to the Opportunity team from John Callas after the Sol 3348 drive.
Definitely. And I would like to highlight his sentence "Clearly this rover and mission are in the Pantheon of great missions of exploration".
Part of the current HiRISE image of the Oppy route between Nobbys Head and Solander suggests a set of N-S lineations that appears to be offset at a point midway between the two sites. I wonder what the nature of these lineations is? And what is the nature of the area where they are apparently offset?
Another of the Mysteries of Mars...
--Bill
Inward slumping of parts of the crater rim are evident on the far side of Endeavour crater so perhaps this is the eroded remains of something like that? The Noachian layers seem to be dipping downward into Endeavour. Was that the case before the Endeavour impact or is it a product of that impact in some way? Questions, questions . .
Endeavour is pretty much on the threshold size for a complex crater so the eastern rim features could be where final crater marginal collapse zones caused terracing with associated faulting. The original rim would have been many hundreds of meters high so there could also have been some rebound, slumping and fracturing. The Endeavour rim is so worn down and over-run that it is difficult to determine an accurate footprint of the final crater.
What impresses me is that the Meridiani-age sediments (which we are now presumably traversing) were deposited long after the Endeavour event with the crater rim eroded down to a nubbins and the ejecta blanket eroded away or covered. The idea that the crater rim could still be structurally (tectonically??) active after all these aeons is almost incomprehensible. Not only do we have the lineations in the Meridiani-age sediments we also have that offset at the central point which implies faulting or slumping. And the term "Meridiani-age sediments" may be open to reinterpretation-- they may be the basal Burns Formation or even earlier. The gross characteristics are similar to the Burns: thinly-laminated to massive, fine-grained with concretions. We are not sure if the concretions are Blueberries, Newberries or Boysenberries.
A mystery that could be wrapped up in a enigma...
--Bill
Speculation: If the older buried rock along the rim has a lot of clays, expansion and contraction due to variable moisture content at some depth could generate large-scale cracking -- a periodic wetting and dessication cycle. The rock type boundaries of the rim would entrain the cracks.
Montmorillanite on Mars?
At Endeavour we are trying to interpret events that took place roughly 4 Ga ago in a far more energetic environment. The dating is rubbery and the elapsed time between the Endeavour impact and the Meridiani sediment event is unknown. While we have come to love the traverse surface of laminated sulphate sandstone littered with hematite concretion lag can we make any correlation to the Burnes formation which is defined as the 7 odd meter stratigraphic section explored in Eagle crater and Endurance? The big crater roadcuts of Endureance, Erebus and Victoria were at the top of a mound and we have descended a fair way with limited analysis of the couple of crater roadcuts we passed on the way. The Botany Bay surface looks different, but does this reflect enhanced erosion from channelling of wind from the crater or something else entirely?
Amen, brother. The surface started to look different when we rolled off of the Cape York bench and continues to provide much amazement. I see that we are still getting the "clast survey" and the "systematic foreground" sporadically in the daily offerings but we'll need to go mine the PDS in a few months. Still, the surface is fascinating to look at as we roll along.
Here is a crop of a HiRISE RED channel image of the Western Rim of Endeavour. This is just off the possible route of Oppy and in in the general vicinity of the supposed offset of the lineations that I noted a couple of days ago. Scale is 25cm/pixel and I've added a scale bar. Take a look and see what you can see. Bear this in mind: this is a red channel image, so reddish areas will show as light-toned, and bluish (ie, basaltic or hematitic signatures) will show up as dark-toned.
Have fun...
EDIT:Oops. Got a decimal off on the scale bar-- should be 50m, not 5.0
--Bill
Looks like another drive on sol 3353 - don't know how far yet, but we are covering the distance pretty fast now.
Phil
30m, according to the metadata.
Perhaps we shouldn't put too much emphasis on the orientation. There are similar features just to the east of Cape York visible in the attached image with varying orientation. As far as I know we don't have a real consensus on the cause of Anatolia Trough do we?
I've been admiring that terrain East of CY for years now.
The orientation and alignment of the lineations with the (remnant) structural features of the Endeavour rim is too strong to be considered casual. My intuition says that there may be a connection, but I'm always looking for another interpretation.
I don't know what current thought is on the Anatolia features. I feel that years ago the interpretation was karst: solution of the soluble keiserite-cemented sandstone along fractures and joint systems. And that is my continuing interpretation. I remember that Phil Stooke has some polar projections of MER-B Pancam panoramas of the type Anatolia feature near Eagle (Fram??) crater from the early Sols of Oppy.
Anyways, here is an annotated image of the Eagle-Endurance Crater region, with the Anatolia features delineated in Red, and the boundary between the Smooth sandy plains and the Rippled sandy plains to the South. I did this in 2005-2006 and the image is named "MER_DIMES_anatolia"; I don't recall where I got that base image.
--Bill
As the file name suggests, that is one of the three images taken by the descent image camera to measure horizontal motion and allow it to be cancelled out during the final stages of descent.
Phil
Ah, "Descent Image Motion Estimation System", intuitive once it's deacronym'd. PIA05146. And now I've gotten a proper non-jpeg'd TIFF.
Hmmm, you don't suppose that the shadow in a hotspot to the left of Endurance Cr really is a hotspot and shadow???
At any rate, here is a ground-truth demo comparing a crop from the DIMES image 3 and one of the MER-B polar Pancam panoramas (although one of my source/ working images is labeled "MOC" instead of "DIMES").
You can see that there is a preferred orientation to these things, even several kilometers away.
--Bill
The enduring legacy of MER...
I found this interesting thread:
http://www.unmannedspaceflight.com/index.php?showtopic=195&hl=dimes
--Bill
Back to 2013! This is the current position, a comparison of HiRISE and the 3353 Navcam partial pan in circular projection. A red spot shows the current location. Since they have made such good progress, maybe there will be a brief examination of the bedrock just ahead over the upcoming holiday.
The dark streaks in HiRISE are seen in the Navcams to be dust drifts.
Phil
Any idea where site Tawny is located?
No - what's it from? The latest Pancam targets?
Phil
I think it's important to note that the cracks back in the pre-Victoria days are on the surface of a sedimentary stack hundreds of meters thick, while the cracks around Endeavour's rim are in a relatively thin layer of sediments covering the rim -- perhaps only a few meters thick in some spots. The near underlying rock in both cases is totally different, so the processes resulting in the cracks on the surface is likely different as well.
For example, the karst explanation may work well for the earlier terrain while the cause of the Endeavour rim cracks could more likely be the result of slumping of the underlying crater rim or differential expansion/contraction of the thin sulfate surface layer and the underlying rock of the rim.
Just my meagerly informed musings.
Oh, agreed wholeheartedly. The Anatolia features seen early on and these lineations seen here are of the products vastly different ages, processes and Mars'es (climates). Especially intriguing is the terrain to the east within Endeavour which has many AnatoliaFeature-like characteristics but with a different genesis.
And doubly especially the thin, persistent (over a few kilometers at least) unit of the Meridiani Onlap which represents an unconformable contact between the old weathered and reworked impactites of the"Endeavour formation" and the newer sedimentary clastics of the basal Meridiani formation. This is a unique instant in geological time and we need to be looking at the ground under our boots to hear it's story...
--Bill
At the scale of a HiRISE image Tawny can be located a bit more precisely than that, Bill! It was within reach of the arm on sol 3352, and Opportunity was driving backwards with its arm on its north side at the time, so Tawny is a pixel or two on the north side of the sol 3351 location. It's at the scale of the rover camera mapping that we don't yet know where it is
Phil
But without FHazcams w/ the IDD deployed or the Pancam sequence we won't know exactly where Tawny is.
I guess it may be in this locale
http://www.midnightplanets.com/data/MERBRawJPG/03353/1F425859620EFFC3R9P1205L0M1.JPG
and zooming in on the HiRISE image I can pick out which of several rocks it might be, but not exactly. But I'll guess when we do get a peek at it, it'll be almost earthshaking...
--Bill
As Phil says, "Tawny" is near the sol 3351 marker (assuming that's in the right place), facing SW from the rover. This sol 3351 Front Hazcam image should show it: http://www.midnightplanets.com/web/MERB/image/03351/1F425685490EFFC3NLP1214L0M1.html.
But I'm not sure "Tawny" was much of anything; they might just have been checking out the arm after this potentiometer issue mentioned in the http://marsrovers.jpl.nasa.gov/mission/status.html#opportunity.
The feature you're interested in (post-drive on 3353) doesn't have a name yet, that I'm aware of. (Well it might have a name that we don't know about, but you know what I mean: there are no Pancam images of it the metadata yet.)
Yes... I guess... we're just going to have to wait.
<MOD HAT ON> Very funny, all, but let's try to stay a bit focused, eh?
The opstempo right now is a bit (well, quite a bit) more leisurely than previously. So, we're gettin' a little bored in the long intervals between new events. Understandable & natural.
Unfortunately that means that the SNR of this thread is decreasing thereby. I don't think it's intentional at all, but nevertheless it's happening.
So...just a gentle (and I do mean that) reminder to try to focus a bit more on the observations & the science. That's all.
</MOD>
Not totally clear what happened on 3335 - we have http://qt.exploratorium.edu/mars/opportunity/rear_hazcam/2013-07-02/1R426043435EFFC400P1311R0M1.JPG?sol3355 but no fhaz down. The latest blog entry at the end of http://www.nmnaturalhistory.org/rover-field-reports-from-mars.html says
That one rear hazcam must have been good though; they drove another 25m on it on sol 3356 (with autonav). That's after over 116m on sol 3355, plus taking a bunch of images along the way.
Bill and Phil: the crumbly rock on sol 3353 is now named http://en.wikipedia.org/wiki/Lake_Eyre. They got an L257R2 of it before zooming off.
The layers at the sol 3356 site (176/0158) are beautiful. Here are very quick Navcam and Pancam anaglyph views.
Yes! Lake Eyre.
And tosol's (Sol-3356) Drive Dir Pancams show the wonderfully delicate remnant bedding underfoot (-wheel). We may start seeing significant changes in the outcrops over the next few drives.
One of those Pancams in your anaglyph, for reference:
http://www.midnightplanets.com/data/MERBRawJPG/03356/1P426122443EFFC4BMP2401L2M1.JPG
--Bill
I like this view because it has the horizon (almost) horizontal. This is in spite of the rover being on a hillside. I presume the surface is quite bumpy and here we are luckily levelled by one of the bumps. Solander point has appeared on recent images as if it were a considerable hill, whereas like Cape York it is more like a shelf on a sloping surface. The top of it is about ten metres above plains outside the crater, useful perhaps for spotting distant horizons but not really much of a hill.
http://qt.exploratorium.edu/mars/opportunity/navcam/2013-07-03/1N426122294EFFC4BMP0702L0M1.JPG
That's great! I always like driving gifs.
Phil
There's some real parallax going on with with Solander Point and the distant ridge behind it, as I suspected a week or so back. It's quite clear now. We're getting so close to our winter hangout!
A.J.S. Rayl's new Planetary Society monthly update on Oppy is online.
http://www.planetary.org/explore/space-topics/space-missions/mer-updates/2013/06-mer-update-opportunity-continues-sprint-to-solander-point.html
Here is the Sol-3355 drive direction 3x1 Pancam, cropped and reprojected in a polar format. This was cropped to show the fore- and mid-ground. It is oriented in the drive direction, with South approximately up. Note the wonderful texture of the outcrop, especially in the foreground.
--Bill
Wow, Oppy's 10 year launch anniversary is coming up! IIRC the launch date slipped a couple of times and there were suggestions that if it was pushed forward much further it could have to wait until the '05 opportunity.
Here is the Sol-3356 drive direction 3x1 Pancam, cropped and reprojected in a polar format. This was cropped to show the fore- and mid-ground. It is oriented in the drive direction, with South approximately up. Note the wonderful texture of the outcrop in the foreground and midground, and the bedding in the midground.
--Bill
It would be nice to know whether Tawny was targeted or happenstance. Actually it looks kind of interesting. Rounded, sorted grains, texture reminiscent of lower Overgaard and a change from most of the laminated sedimentary surface. Pity in a way that priorities and winter deadlines have precluded any in depth investigation of the approach to Cape York or Botany Bay since a high water table at the top of the mound would imply at least some level of surface flow could have been expected in Botany Bay. Anyway, with the Solander slope hopefully Opportunity will be able to do a bit of roaming and investigation this winter.
The MI that came down today was not "Tawny". Today's MI is p2935 and the named site is p2530. Good sleuthing, though. And a good description of the victim.
As far as I've been able to prognosticate, this MI was taken after the FHazcam IDD check subframe made on Sol-3551 at Site-175/0589. The MI was made on Sol-3552 and is of the corner of one of the ubiquitous flatrocks of the area. This, AFAIK, was made after the IDD arm went C R E A K and they did a diagnostic on the spot.
Attached is a location image with some enhancement. This rock, which I am informally naming Ferd, was a surprise to me. It is more coarsely clastic than I would have expected. But this is a completely different area (and era) that what we have studied before, so it certainly falls within my expectations. I wish we had a better understanding of the Meridiani Onlap.
Anyway, this MI of today is the first of a series p'haps 20 MIs to look forward to.
--Bill
NOTE: Serpens was right, this site is "Tawny". Corrections and apologies made...
No - the MI and the fhaz subframe are indeed "Tawny". p2935 isn't a site code, it's a command sequence number.
(For reference, the Pancam images of Tawny were taken on sol 3353 at site 175/0591, after backing up from site 175/0589 where the arm work was done. The image ids for the Pancam images are 1P425857332ETHC3NNP2530L2M1 through 1P425857701ETHC3NNP2530R7M1; the site code is 'C3NN'; C3 = 175 and NN = 0591. This will all get much easier once the images actually come down.)
Correct, and I apologize to Brian for poo-poohing his location ID.
I have gotten into the habit (shortcut ??) of using the command sequence number (an action) to identify a location. I guess I started doing this since I use the Pancam Tracking Database to keep track of what, where and when was done. This works most of the time, but sometimes doesn't.
Ferd is now known as "Tawny".
And we do have a Phobos image upcoming:
03359 p2739.01 0 0 0 0 0 0 pancam_phobos_deimos_prepoint_L1R4
--Bill
Check out "Latest Images", new MIs of "Tawny" as well as a stereo pair of "Lake Eyre":
http://www.midnightplanets.com/web/MERB/latestImages.html
Yay.
Here is a cropped x-eyed stereo pair of "Lake Eyre". That is one rotten, weathered rock.
--Bill
Is it my imagination or are the blueberries around Cape York and in Botany Bay more misshapen and elongated than the near perfect spherules from earlier in the mission? While the nice round examples imply a static groundwater environment, more elongated concretions would support groundwater flow. I have always had difficulty reconciling the clear evidence of a long lasting water table at the top of the mound around Victoria, Erebus and Endurance and the hematite concretion signature from the Endeavour crater infill , with the seeming lack of evidence of water flow in the sulphate sandstone around Cape York and Botany Bay. Can anyone point me towards any papers or articles that address or correlate the probable groundwater effects over the area of the traverse?
We've been climbing a bit as we go south - this image looks back at Cape York (mosaic of 2 Navcam images on sol 3354). Below is a roughly x6 vertical stretch. The nearer object is Nobby's Head, with Sutherland Point almost hidden behind it. The farther object is Cape York, with a few dark spots at the left end being rocks at Odyssey crater. Everything tilts in towards Endeavour. Pancams of this area from Solander should be quite impressive.
Phil
Serpens, the Berries seen post-Cape York do appear to be differently-shaped, less perfect-spheroidal, but I can't call them "elongated" . But yes, they are different. I've been holding off, awaiting more of the "color clast survey" and "systematic foreground" and MI imagery before looking more closely. I may go ahead and pull together some type examples of the Berries we see on this leg of the Traverse just to get started and finisah up when the data hits the PDS.
Good idea, though. My thoughts are that on low-transmissivity, low gradient aquifers, as we have here, the groundwater velocity will be so exceedingly slow as to preclude streamlined concretions. I don't know of anything in the literature. Maybe Mr Don Burt would know.
Anyways, attached are two Berries cropped from MIs of the site Tawny on Sol 3352. My first thought is that these look etched or corroded.
--Bill
Oh, OK, I was thinking that because we now had a view back slightly above the plane of the Nobby's Head pavement - my image above shows the pavement looping around the Head, not just projected as a straight line. But that could occur through different geometries, I guess. I was thinking of climbing a bit from just after Nobby, not all the way from Cape York, but I was probably wrong anyway, it's just the way Nobby is tilted, I think.
Nice topo map!
Phil
Yes, a "lookback of where we was" is always of nostalgic interest. I remember one we did just as we departed Erebus Crater, looking back to Endurance over the Purgatorian Sea of Sand.
That map is a quickie "browse" DTM map from http://hirise.lpl.arizona.edu/dtm/dtm.php?ID=ESP_018701_1775 . The really nice .JP2 HiVIEW images have 600MB filesizes, much to much for me on Dialup. I need to go to our Public hi-speed 'Net connection at the Library with a Thumbdrive and do some DTM shopping. I'm sure that the .JP2 has "scalable" elevation scaling so one can get better resolution for a specific area. A contour map would be spiffy.
Maybe one of our local DTM mavens can work something up. Ditto on the upcoming project are at Solander.
/hint
--Bill
ps-- and in the FWIW dept:
03360 p2740.01 0 0 0 0 0 0 pancam_phobos_deimos_L1
for tomorrow.
--b
There is a nice contoured perspective view on p.51 of this PDF:
http://www.google.co.uk/url?sa=t&rct=j&q=&esrc=s&source=web&cd=1&ved=0CC8QFjAA&url=http%3A%2F%2Fshoreline.eng.ohio-state.edu%2Fpublications%2F10thesis_karahayit.pdf&ei=NhPZUcDRIIOl0AXx4IGgDQ&usg=AFQjCNEgkfkCQhVZL0749YOZ_rszrYoEpw&bvm=bv.48705608,d.d2k&cad=rja
Nice. I knew bits-and-pieces of how-we-did-it, and this thesis is a good summary of all that.
Ah, to have access to GIS and DTM software and databases...
--Bill
And here is a mosaic of Tawny, the MI target of Sol 3352. Not a great job, there are always problems with mixed shadows
and full sunlight.
--Bill
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