I'm starting a map thread. It's hard to know what we will get but I expect a route map will emerge bit by bit. Maps showing the landing location will be easier to make initially.
Phil
Starting off with an overview of the site, with landing ellipses based on the work done at Hong Kong Polytechnic University. The initial site is indicated. The landing ellipse is about 60 by 20 km and if you center one at the initial site it contains two craters with rough ejecta blankets (bright in this image, which is Mars Odyssey THEMIS infrared with inverted shading). Two nearby ellipses were chosen to avoid the craters, and the western one was then moved a bit to avoid more rough terrain at its southern end. The landing site is very close to the center of that ellipse and about 40 km from the initial site.
Phil
Until higher-res imagery arrives, here's a crop at CTX full-res (5.67 m/px) with a circle roughly at the dot in Phil's ellipse map. (merge of 2 CTX tiffs - 1km squares for scale reference but not referring to any particular origin)
I think the distance from center to edge of the image, about 3.5km, is the horizon distance from about 1.7m height on Mars.
It's clear that following this mission will be tricky and maps will be tentative and only sporadically updated for a while.
But you have to start somewhere. This is a VERY tentative start. A HiRISE image will improve the basemap, and eventually a reprojected panorama can be laid over that.
What I show here is all I know at present. I will update it when we get news. Let me know if anything else appears! I am assuming landing day was sol 0 but that may not be correct.
Phil
The text accompanying the 'group photo' of the rover and lander together says that the camera was deployed 10 m south of the lander. Then the rover moved back towards the lander for the photo. I have illustrated that here (using a guess as to the locations of the camera and the rover during photography). All very uncertain of course. I don't think the date of the group photo was mentioned - before or after the Tianwen-1 orbiter image, so I can't add a date.
All this is subject to ongoing revision.
Phil
I'm a bit late to the game as I had other work, but it's finally time for me to catch up with all the events.
After the second HiRISE image appeared I have made some big changes to my map. I decided that the dark markings west of the bright streak are probably not tracks after all - especially if you overlay the two HiRISE images, which makes the tracks east of the streak easier to see and the others less distinct. I also changed my interpretation of the 'group photo' from the deployed camera. The foreground surface in that image is more red on the left side and middle, and darker and less red on the right. I was interpreting that as showing the surface from the west side of the streak but now I think it's from the east, and that seems to match the geometry of the lander better as well.
All that may still be wrong! A Chinese map would be very useful. Until we get one HiRISE may be our best guide.
Phil
Bit by bit a map takes shape. This uses the new panorama.
Phil
And an overview map - this will be the standard resolution for mapping.
Phil
And Zhurong is almost at the parachute... Would be nice to get a new Hirise.
Huge image with a recent path nice guess from here:
https://twitter.com/TheElegant055/status/1413594702054674432
Link to 50MB full resolution version:
https://drive.google.com/drive/folders/19PTSvxpEc0hlSnaGYTILuTgwRZE4Mk8E
So, those light-toned features are barchan-like dunes. Wonder if we can determine the composition of these dunes? Or what the source of this material is?
--Bill
The LIBS instrument will give composition - they were within LIBS range.
There are dark dunes on Mars (e.g. Bagnold Dunes in Gale Crater) and bright features like this, usually called drifts or ripples. The dark features are made of basaltic sand and they can indeed by barchans - see also the Greeley Dune Field inside Endeavour crater. These brighter features are made of finer material, silt to dust sized particles. The reason the dark and light don't just mix to form mid-toned deposits is that the wind sorts particles by size. That finer material is probably mixed globally and doesn't tell much about local geology.
(Continue discussion in the other thread)
Here is a very rough update to the map using the new information. A new HiRISE image would be very useful! (or a Chinese map)
Phil
https://news.cgtn.com/news/2021-07-11/China-s-Zhurong-rover-drives-for-over-410-meters-on-Mars-11OJM3iid5C/index.html
I believe, this means, we will get some parachute close-ups soon.
http://www.chinanews.com/gn/2021/07-11/9517522.shtml
"According to news from the National Space Administration, as of today (July 11) at 20 o'clock, the "Zhu Rong" rover has traveled a total of 410.025 meters and operating conditions are normal."
I updated my map with the parachute images. The sol dates might be one sol out depending on exact timing. The sol 56 marker is where I think the approach Hazcam image was taken, but only an approximate location.
Phil
You are doing some really nice work here - for all missions! Thanks.
Phil
Thanks Phil. Means a lot. In fact you just gave me an idea to add the fourth one. See Exomars thread post #570.
I just had an interesting and very welcome email from a reader of the forum who corrected me on my estimated sol numbers. I have updated my map with the corrected numbers and added an approximate location near the second dune - I am not sure which sol the rover arrived near that dune but we may know it after new images are released.
Corrections are always welcome - we really need as many eyes on this as possible.
Phil
The Chinese map I linked to in the main thread lets me improve my map.
Phil
My best guess for sol 75 would be right at the bottom of my map.
The query after 'c. 72' is for the date. The location is good.
Phil
New drive map from https://mp.weixin.qq.com/s/nneKWbj2Zyp0tJ_1-3cjmA.
I give them passing marks on autonomous driving (or for careful directed driving).
--Bill
You are right, it should be more like 30 km between dots. I don't remember where the 40 km came from but it doesn't match the map. I might have been quoting some other source or just put too much Baileys on my cornflakes that morning.
I think they want to use the ground-penetrating radar on a trough about 1700 m south of the current position, which would be an interesting thing to do. Then keep going that way and hope to reach a cone.
Phil
New drive map from https://twitter.com/CNSAWatcher/status/1432279954868350977.
This map is very useful, but I am intrigued to find that it does not overlay the new orbiter image of the track very precisely. I will wait until we have a new HiRISE image before updating my map. The orbiter image was taken on 24 August and this map matches that except for the last point, so this map was probably made with data up to 23 August, a week prior to release.
Phil
Amazing how detailed the orbiter get the track... a single track on Tianwen-1,.. Hirise will indeed be nice with its better resolution and seeing the 2 track path.
We have had no news on Tianwen-1 and Zhurong for a while. The rover at least, and probably the orbiter too, are entering a superior conjunction blackout period about now. Their blackout will be longer than NASA's, probably because it's the first time they have dealt with it and will want to be more conservative.
Meanwhile I wanted to show the difference between the existing map and the new Tianwen-1 orbiter image. My map is based on the published map with track and waypoints. The orbiter image shows tracks offset from it, with the offset increasing away from the lander (though the last point is close again). I suspect this is because of a small difference in the definitions of map projections between the projected orbiter image and the route map. (My coordinates are from HiRISE which opens the possibility of another offset, but in all cases I am matching to surface features using HiRISE as a standard). The maximum offset is about 10 m.
Phil
Agreed. The 'quiet spell' from Zhurong is not to be worried about. They don't have an as-established DSN infrastructure or as much experience with dealing with a faint, noisy signal.
I'm still impressed with their Rover's track. I don't know how on-course it is, but it doesn't seem to be bumping into things...
--Bill
Here is an update to my map (section 2) based on this site:
https://mp.weixin.qq.com/s/NImpyH43GAhMnF0dkpU1jA
(thanks to Andrew Jones for tweeting about it).
I have not yet corrected it to fit the tracks seen in orbital images. I will wait for a new HiRISE image to do that.
Phil
A very quick look at the end of year location. The new partial panorama is looking southeast and it leads to this position. I will post a proper map when I can get to it.
Phil
I assumed the partial panorama was from the end of year date, but if it is from sol 201 I will correct my map. I am still hoping for a new HiRISE image to guide my next map. There are small differences beteen the various sources we have.
Phil
Recent article characterizing first 60 sols of Zhurong traverse was published in https://www.nature.com/articles/s41561-022-00905-6.
While the article is sadly behind paywall it is possible to download supplemental files which include rover's track points.
Here is a comparison map of my version of traverse vs the new track points in red:
Zhurong traverse updated with track visible in new HiRise photo https://www.uahirise.org/ESP_073225_2055.
I also updated positions for sols 0-60 with date mentioned in previous post and manage to extend coverage to sol 75. Sols after that are approximate.
The Chinese data veers off course to the east when compared to track visible in HiRise photo, so I corrected its position to nearest point in the track.
Zhurong rover map update. There is not a lot of new info, just the drive from sol 297 position to the (final?) position.
This last segment of the drive did not leave rover tracks visible in HiRise imagery, so its course is a bit conjectural.
BW version:
Following on the discussion about maps in the main thread, I have tried to bring everything I have into one coherent set of locations. This is not yet the whole story and it will not agree with some sources but it is the best I can do at the moment.
Phil
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