2009-03-20

Spirit Sol 76

Our downlink data is delayed by some kind of ground system glitch. The glitch clears up to show us a flattish, whitish rock just in front of us, and a much more interesting fishlike rock a few meters away. It reminds me of a coelacanth or something. So we're going to MI the nearby whitish rock, then drive to the coelacanth. This all fits neatly into one of the scientists' sol templates (a "D-type," or "dirt-type," sol).

The "coelacanth's" name is Mazatzal, which is the name of a group of mountains in Arizona. Nobody can get this name straight; all night, people keep calling it "Mazatlan," "Marzipan," etc., until it becomes a running joke. I really wanted them to call it "Coelacanth," but that would have been worse. I end up attaching a picture of a coelacanth to my uplink report anyway.

Our odometry total is 459m, plus the 25m or so we traversed today. Added to Opportunity's 115m, we are just under 600m combined.

The time the scientists save planning by using the new sol templates gives them a lot of time to sit around arguing. They must love them.

To kick off the discussion, Jeff Johnson shows a PANCAM spectrum of Bear Claw, the scuff I helped make when I was last on shift. It's a beautiful, beautiful picture, and the science information revealed by the scuff is no less interesting. The small rocks we see around us seem to be made mostly of the same stuff as Adirondack. The material inside the Serpent drift, the stuff revealed by the scuff, is something different -- they don't know what yet -- and the dark deposit on the far wall of the crater, with its "mystery feature," is something in between. That's surprising, since they expected Serpent's insides to look the same as the crater deposit. They haven't yet compared the data to the trench results -- "but that's a good idea," Jeff muses, "we should do that."

The scar, however, does show some evidence of the mystery feature, which is also surprising: why would the stuff (whatever it is) be in some of these identical-seeming drifts and not in others? At this point, there's no answer.

At the SOWG meeting, Art has some bad news: the rover appears to have lost one of its PRTs (a temperature sensor). But he compensates with good news. No, it's not that he just saved a bunch of money by switching his auto insurance to GEICO. It's that the ICFA is at 90% capacity. The ICFA, he explains, is the Ice Cream Freezer Assembly.

Today's IDD work is straightforward; it's the drive that's going to be a pain. Mazatzal is only a few meters away, but we have to do a little zig-zagging in order to get there from here. But that's not such a big deal; what makes this drive difficult is that we don't yet know how we're slipping in this terrain. So we can't be sure whether the drive will overshoot, and overshooting will be a problem, because the rock we're driving to is obstacle-sized: it wouldn't be safe to drive over it. And, because they naturally want to IDD the rock when we get there, we have to end up in a fairly narrow range: close enough to reach a range of targets with the arm, not so close that we can't even safely unstow the arm without whacking the rock -- or, worse, not so close that we actually drive onto the rock. Even if we had a good slip analysis, there would still be significant uncertainty, because that's just a probability; it changes based on how rocky the terrain is, for instance. We do the best we can.

On my way out I run into Ted Specht, who wrote some software we ended up not using. Back when that used to happen to me, I always used to wonder why. Why would people ask for things and then not use them once I delivered them? Now I know: on a flight project, things move so fast that you've got to keep moving with them. Ted's a multimission guy; if he'd been 100% on MER, we probably would have ended up using his stuff. But he had other obligations, and by the time he delivered his solution, we had other solutions in place. Fortunately, he's still glowing from his honeymoon in Croatia. I don't think he minds at all that we didn't end up using his code. Or even notices.






Courtesy NASA/JPL-Caltech. Mazatzal (above) totally looks like a coelacanth (below, c/o Wikimedia).



Courtesy Alberto Fernandez Fernandez. Image licensed under a Creative Commons Attribution ShareAlike 2.5 license.


2009-03-19

Spirit Sol 75

I'm off shift, which means I spend my time hacking on RoSE instead of doing the glamorous work.

We've traversed another 34.3m around the crater, which is a pretty good drive for this rocky terrain. They also scarred a drift as they drove by it -- driving along a drift such that the wheels on one side rode through it, periodically wiggling the wheels and correcting for yaw. They took pictures of the scar before moving on; this should make for some interesting science.

It's not clear how much farther we'll travel around the rim before heading for the hills. They're looking into what data we need to gather, via remote sensing, on the Columbia Hills before we have to pause exploring while they upload the new flight software.

It occurred to someone that autonav won't see a certain type of obstacle as a hazard: a tall, thin spike. Despite the fact that nobody has ever, ever observed such an object on Mars, we get an official directive not to plan autonav drives into an area unless we can rule out the existence of such a hazard. In most cases, if we could see that well into the area in question, we wouldn't rely on autonav; we'd use blind driving instead. The new directive is very stupid. I think Mark instigated the concern about it as a way to drive the project to install the updated flight software, which would detect Martian beanpoles as a hazard.

The best news of the day, I think, is that our big picture is back. I think somebody must have taken it to LPSC. In any case, Mars is outside my office door once again.

2009-03-18

Spirit Sol 74

Interestingly, the scuff-drive ended up driving the rover's right bogie to the hardstop. While climbing over one of the rocks as we backed up, the bogie (the rear part of the rocker-bogie suspension) was angled way up. No harm resulted to the vehicle, and as Rich Petras points out, this is something that rocker-bogie suspensions will do from time to time, and none of our modeling tools can predict it well. So I didn't do anything wrong. But it's a little freaky to see.

I finish implementing a new RoSE feature just in time to go to the downlink assessment meeting. I'm not really clear on how far they drove yestersol, if at all, but they did some remote sensing on White Elephant. Steve Ruff, reporting the MTES results, deadpans: "It looks like a dusty rock." The RAT guy, Steve Gorevan, says White Elephant looks "eminently RATtable," an important consideration for characterizing white rocks. Arvidson seems to want to skip White Elephant, though, feeling that it will slow us down too much. We're not really sure if the terrain is navigable (because we don't have terrain meshes yet), and he wants to put more meters on the wheels.

One thing they might want us to do while putting meters on the wheels is to deliberately drive one side of the rover along a drift, leaving a big scar for them to image. There are problems with doing this (it guarantees slippage, which means uncertainty in our positioning, and that uncertainty is multiplied for a longer drive). But it sounds like a cool thing to do.

Just before the meeting ends, Ray reports that "at LPSC, we were heroes." Steve Squyres stood up and got a huge round of applause before he even said anything. The room was packed wall to wall -- people were standing in the aisles and along the walls; you couldn't enter or leave. "I haven't seen such excitement since the Viking lander missions," he says. "Even grumpy old greybeards were ooh-ing and aah-ing."

2009-03-17

Spirit Sol 73

Once again I have a lousy night's (actually, day's) sleep. I keep waking up, thinking of ways the drive is going to fail. There are a lot of them. We didn't correct enough for slip. Or: did we really analyze the depression ahead and to the right of us? Could any nasty surprises be lurking there? Or: if we slip too much as we drive downhill, we'll end up climbing that 20cm rock ahead of us instead of stopping short of it, and if there's a depression on the far side, we could get high-centered on it -- with the rock scraping the rover's belly, and the rover unable to gain enough traction with any of its wheels to crawl back off. Of course, this would mean that our imaging was badly wrong, and our simulations were badly wrong, and our slip estimates are badly wrong. But apart from that, it's very likely.

I obsessively check the flight director's report while getting ready, and am considerably relieved to read that we drove the expected distance and have a scuff mark in front of us. Is it reachable from the IDD? Did we nail the mid-drive imaging? The report doesn't say. But when I get to work and see the results, I'm shocked.

It's perfect.

The scuff is nearly dead center from our final position, with good chunks of it in the IDD work volume. (In fact, maybe all of it is in the work volume; the tool that does the preliminary analysis has some limitations that the shape of the scuff might be exposing.) And the mid-drive NAVCAM, which is a bellwether for the other mid-drive imaging, couldn't be better. The main body of the scuff is right there in the middle of the image. While I'm gaping, John Grant says: "Let me be the first to congratulate you on a perfect drive." When he left last night, he just wanted us to end up somewhere near the scuff. And we executed perfectly. I don't know if it's relief or disbelief, but I can't stop looking at it.

I know I say this all the time, but seriously: I worry too damn much.

I'm not on shift today, Chris is, so it will be his job to IDD the scuff (which has been named "Bear Paw"; targets in it are getting names like "Panda" and "Grizzly"). So I get to wander around and unwind a little before the meetings. Because I didn't come in the usual door, it's not until now that I notice that the beautiful big picture they hung outside our office is gone. Nobody seems to know where it went. Only the tape remains.

But there are a couple of new things posted up in other areas. A copy of the Weekly World News, with its cover story of strange cat-like creatures detected by the Mars rovers, is a favorite. This has been posted in the SMSA (outside of camera range), next to some supermarket flyer advertising, among real items such as $1 calculators, "Mars Water" -- direct from Mars -- for the low, low price of $999,999.99 per gallon.

I take some time to catch up on the images from both rovers. Just as I finish, I manage to delete all the images I've saved for the last week or so. Fuck! I have to go back through the database, digging around for the images I'd liked enough to save. Fortunately, I still have the filenames in an open xterm, and I'd named the files descriptively enough that I'm able to find most of them again.

Correcting this stupid mistake makes me a little late for the downlink assessment meeting. It turns out that Serpent's inner material, while considerably darker than its exterior, is not the same stuff as in the crater after all, so there's little reason to stay. Although, after some debate, they do decide to do a touch-and-go here: they'll look at the inner material quickly and drive on in the afternoon. The target of the next drive, or set of drives, will be -- assuming they can get there from here -- one of the fabled white rocks. This one's been named "White Elephant," and I can't help thinking this is an expression of the attitude the non-members of the White Rock Mafia have toward their White Rock Mafia colleagues.

The composition of Serpent's interior was one surprise. Serpent's outer layer gives us another surprise. Serpent looks like a miniature sand dune (technically, a ripple); we expected it to be soft. But the outer layer is an indurated crust: it's composed of sand, but the sand is somehow cemented. I ask Craig Leff what could be causing that kind of effect; he doesn't know. On Earth, he says, something like that is usually the result of evaporating water. Here, nobody knows what could be causing it.






Courtesy NASA/JPL-Caltech. Holy smoke, it's perfect!






Courtesy NASA/JPL-Caltech. Rover's-eye view from our final position, with the Serpent scuff right in front of us, ready for us to IDD it.


2009-03-16

Spirit Sol 72

I wake up a couple of hours early, in a near panic. I had completely forgotten that our previous drive had timed out, which means we would have had a goal-error flag set. Mark didn't mention this in his hastily written downlink report, so we didn't clear the flag in this drive sequence, which means the drive won't happen. I dislodge Zenobia, log in from home, and check the telemetry -- only to find that the goal-error flag wasn't set after all. (Which must be the actual reason Mark didn't mention it: there was nothing to mention.) I don't understand this, but I'm so relieved that for the moment I don't care. I actually manage to get a little more sleep before I have to get up.

(It turns out later that there's a good explanation why there was no goal error. At the end of our last drive, the rover timed out because it was back-and-forthing, trying to find a safe path. It happened to time out after a backward move, which left a little extra space in front of it. The sequence cleared the timeout error, enabling the rover to complete the final stutter-step into the small safe zone, without producing a goal error. If there had been such an error, Mark would have mentioned it and we would have cleared it as a routine matter; we do that all the time. So everything was fine. You'd think my subconscious would have recognized this pattern by now, instead of waking me up all the goddamn time.)

My badge is working again. I stuck around for hours yesterday, just to find out that Security couldn't help me at all. The project sent them a list of people whose access was supposed to be revoked and mistakenly included my name on it; apparently, this kind of thing happens all the time. And I'm far from being the only person it happened to this time: I keep having to open the door for other people whose access was mistakenly revoked along with mine and hasn't been restored yet.

Today's drive didn't quite complete, but we got a heck of a lot closer than I expected. We made it to the far side of Serpent and turned to face the bedform; that's the good news. The bad news is that the rover saw a 10cm rock with a depression behind it, and interpreted this as a 30cm obstacle. (Not unreasonably, actually; the rover could actually end up in trouble if it tried to drive over this in just the wrong way.) This exceeds the maximum obstacle size, so the rover refused to perform the final approach. We ended up 85cm short of our destination. Considering all the things that might have gone wrong, this is not bad at all. And there wasn't anything we could have done about it in advance; from our starting location, we couldn't see this terrain well enough to have avoided the problem. Just one of those things.

While we're looking at this, John Grant comes by to alert us to the day's likely plan. It's always something new. They want us to drive up partway onto Serpent, make a big scuff mark (not really a trench, just enough to scrub off the outer dust layer), back up so they can PANCAM/MTES/NAVCAM the scuffed area, and then drive forward again so that the area they just imaged is in the IDD work volume.

What makes this interesting is that we have no idea how much we'll slip in the process. So we can't accurately correct for slippage in advance. Mark suggests using visual odometry, a feature where the rover watches how objects in its visual field change position as it moves, and updates its own internal position estimates based on the result. This is really how humans work: when you're "navigating" as you walk, you trust your eyes more than you trust your feet. The rover normally trusts its feet (wheels), because it thinks so slowly. But when you need precision and can't correct on the ground, visual odometry is the only way to go. We haven't done this on Spirit before, but Opportunity has used it to good effect.

The big news in the downlink assessment meeting is that we've achieved mission success. We were waiting to rack up 60 sols of science ops. That was delayed by the Bad Thing[1], but we've now hit the goal. From here on out, we're gold. More good news: Lutz reports that yestersol's MI images (the ones we took after the gunslinging) look fabulous -- judging from the thumbnails, at least; we'll get the full frames in the overnight pass.

The plan shapes up to be pretty much what John Grant said it would, but there's a lot of debate over exactly what we want the rover to do to Serpent before we poke at it. Do we just want to drive onto it, then drive back off? Or should we wiggle the wheels, or run one of the wheels in a trench-like operation to scoop material out of it? Do we want to make one track or two? John suggests that everyone who cares about the details discuss the matter with me after the meeting, then ends the meeting itself. I accumulate a group of about a dozen scientists, who debate amongst themselves for a while before deciding that anything I do that scrapes away the upper layer is fine. Since we're already more or less lined up with Serpent, we should be able to just drive almost straight ahead onto it -- this will roll the left wheels over the top of the bedform -- and drive straight back off. In order to IDD the resulting scuff mark, we'll have to shift the rover to the left, which there's no very good way to do -- because the middle wheels don't articulate, we have to turn and drive and turn, and this accumulates uncertainty. (This maneuver later becomes known as "The Translation Dance.") But it should be OK.

This is starting to look like a nice, straightforward plan. So naturally it goes to hell. I'm building the sequence in the SOWG meeting when I realize that if we carry out that plan, we'll end up with the rover straddling Serpent. Which in itself is fine; Serpent isn't that tall where we are. The problem will be that we won't be able to use the APXS. To use the APXS, you first have to open its dust doors, which you do by pressing the instrument against a hard surface; this triggers a switch that pops the doors open. Soil isn't firm enough to cause this to happen (and we'd get the instrument dirty anyway, if we tried), so when using the APXS on a soil target, we instead bring it underneath the rover and press it up against the rover's "chin" (technically, a calibration target called the CCT). But when doing this, the IDD needs a lot of clearance under the rover. And Serpent is too tall. If we try to open the APXS on the CCT while straddling Serpent, we'll end up dragging the RAT (the instrument opposite the APXS) through the dirt, which is Very Bad.

We can't fix it by backing off farther, because there's a rock of about the same size at Serpent's tip. If we back off farther than that, we can't reach Serpent any more. The scientists consider whether we can open the APXS before driving and just leave it open overnight, but this violates a flight rule and nobody feels very comfortable with it. We'll have to find another answer.

Fortunately, I paid attention to the earlier discussion and I know what their general goals are, so I have an alternative to suggest: drive around to the side of Serpent and scuff it from there instead. I'd previously rejected this idea because it made things too complex (the drive itself is not complex, but the more driving we do here, the more uncertainty we have about the results), but I no longer see an alternative. We go down to the sequencing room and I start planning it.

Now there's another problem. The instrument reps need to know where to point the cameras to get images of the scuff marks. But we don't really know where those are going to be, because, again, we don't know how we're going to slip. We don't know exactly where the rover is going to intersect with Serpent, and we don't know how it will yaw when scuffing, and we don't know how it will slip afterward. All of these problems combined make it impossible to pick a precise target in advance.

This leads to an overly complicated discussion, made worse by the fact that every time we get all of the participants up to speed, someone else overhears the content of the discussion and wants in, and we have to start over. I start to get really frustrated: time is running out, and there are too many people offering too many suggestions (often ones we've already dealt with, before that person came into the conversation).

At last I see the answer. It's one of those things that's easier to see if you're a programmer. We've all been thinking in terms of absolute positioning -- predicting the spot where Spirit will cross Serpent -- but the answer is relative positioning. "We don't have to know in advance where the scuff mark is going to be," I point out. "We just make the scuff mark wherever we make it, shift the rover over and reorient it so that we're facing along the scuff, and take the images from there."

This won't eliminate all of the uncertainty, but it'll eliminate more than enough, leaving only whatever we pick up during the last little bit of the drive. They'll instruct the cameras to take images of a position 85cm in front of the rover (this length is determined by properties of the rover and its instruments) -- wherever that happens to be -- and it'll be my responsibility to ensure that there's a scuff mark there. That won't be easy, but it also won't be excessively difficult; the post-scuff driving takes place on relatively flat ground, and we can help our chances by making a really long scuff.

They aren't immediately convinced; they normally target the same spot for pre- and post-disturbance observations. But, as a couple of them point out, the drift is likely to be compositionally uniform over its length; it won't matter if the pre- and post-disturbance observations are a few cm apart. And if they can give up that constraint, my suggestion will solve all of the rest of the problem. Chris helps by taking over the job of convincing them and working out the targeting while John Wright and I work on the drive.

There are more distractions. There are currently no IDD activities scheduled for tomorrow, but there's an MI observation in purgatory. A couple of the scientists keep pestering me for the sequence ID of the IDD sequence (which they need in order to deliver their own), but I don't want to deal with that unless the observation makes it into the final plan; otherwise it's wasted work. (Maybe I should have just given them a sequence ID; then they could have wasted their own time instead of mine, and I wouldn't have come across as uncooperative. Confusingly, this seems both right and evil at the same time.) The IDD stuff ends up not making it into the plan, so I don't have to deal with it after all.

Part of the reason the IDD stuff gets pushed out is that Jeff is planning using my original resource estimates, which included the overhead of visual odometry. Now that we've decided on relative targeting for the images, we don't need visodom any more, and we need far less time and energy than we had expected. Instead of taking an hour, we'll be done in 20 minutes, even though the drive itself is now more complicated. But it's too late to go back and change things now. I feel awful about pushing some science out of the plan, yet I'm philosophical about it: if they want us to work on a compressed schedule, this kind of thing is going to happen. Haste makes waste, or so I've heard.

I get the drive into very rough shape and hand over to John; we continue working on it together. One of the changes we make, to help ourselves out, is to broaden the scuff. We'd originally planned to step down the bedform in 10cm intervals, wiggling the wheel as we go; this would leave a scuff about the width of a single wheel. We change this to perform a small turn-in-place at 10cm intervals instead, so we'll cut a significantly broader swath out of the bedform. We've arranged the drive so that only one wheel is on the bedform while we do this, so we shouldn't slip much, and having a broader scuff means we can accommodate more uncertainty in the rover's final position. We're going to scuff the hell out of this thing. When we show the animation of the intricate drive at the walkthrough, Kevin Talley asks, "So, do the other bees know where the honey is now?"

Why are they so interested in Serpent? The dark deposit at the other end of Bonneville -- which we decided not to drive to -- contains a "mystery feature." It's a spectral signature that's not in the scientists' library, meaning there's some unknown combination of elements over there. Serpent and its neighboring bedforms were likely formed from that material, blown by the wind across the crater to settle here. So, effectively, we might be able to examine the far end of the crater by poking at this thing.

I end up staying so late past the end of my shift that I decide to stick around for the Command Approval Meeting. I've never been to one, and I might as well take the opportunity to do it now. While waiting, I get into a discussion of SEQGEN with Kevin Talley and Richard Kornfeld, who are terribly frustrated with it. So is Celina Garcia, who says she badly wants to just rewrite it.

"I've been more frustrated with SEQGEN than you've ever been with anything in your lives," I tell them. All the same, I find myself gently defending SEQGEN. It's not meant for this kind of environment, it's meant for cruise and orbital ops, which work on a very different timescale. The fact that we can use it at all, in a way so far removed from its original intent, is remarkable. In the same way, its developers and adapters aren't used to the pace of development we've pushed them into, because of MER's own highly accelerated development schedule. We were asking them for a final adaptation in less time than they normally have to develop a prototype.

I don't bring up this point, but there's also an us-versus-them aspect to it. I see a tendency among project people to treat anyone outside the project as an enemy. (Shamefully, I'm as guilty of this as anyone; and having been the outsider in this situation myself, I should know better. I choose to construe this as evidence of the trap's perniciousness.) If you're having trouble with software developed by someone on the project, you go to them and tell them there's a problem, and since their goals are your goals, they work with you. When it's a tool developed outside the project, we feel ourselves to be under attack. It doesn't help that you have different bureaucracies to work with in the two cases, increasing the perceived separation. And it doesn't help that people outside the project legitimately have different goals: they're not just worrying about your mission, they're also worrying about Cassini, Voyager, and who knows what else.

I spend some time thinking about this problem and don't come up with any answers I like. But I'm happy I can at least see the problem from this side now.

John has an idea for the extended mission. Why doesn't he become an RP-1 and I'll become an RP-2? That way, he can go back to vanpooling (which saves him a lot of money, apparently) and I won't have to get here at 7:00 every morning. I've been thinking along the same lines, I tell him. "I'm not looking forward to going back to Earth time," I confess. "You know how enthusiastic I am about this mission, but getting here at 7:00 every morning will suck that out of me in no time."[2] I don't really want to give up being an RP-1, though, since I think I prefer it to being an RP-2. So I temporize: "I'll think about it."

I'm not there much longer before I give up on the idea of waiting for the CAM. If I do become an RP-2, I'll see plenty of them in person, and if I don't, it's not a tragic loss. So I hold the door for some unlucky soul whose badge access still hasn't been restored, and I leave.




Footnotes:

[1] By which I mean the Sol 18 Anomaly, when we got stuck at Adirondack -- making no progress toward our official mission goals -- for what seemed like forever.

[2] Five years later, I'm still no morning person. However, I fully recognize how lucky I am that my one and only complaint about my job is that it starts earlier in the morning than my brain does, so I don't bitch too much. Don't get me wrong, I bitch. But not too much.

2009-03-15

Spirit Sol 71

During my pre-shift time, Frank, who's trying to stay awake until the CAM, comes down to hang out and shoot the breeze a little. He's not happy with his SpaceOps paper, he tells me. He wanted to write the definitive paper on how we're using RSVP to drive the rovers, and ended up with something much less than that. "But I'll write that paper later," he shrugs.

The world of "writing papers" still seems weird to me. I got so used to working on the kind of code you wouldn't bother to write a paper about. Necessary stuff, stuff JPL couldn't do without. But, let's face it, boring stuff. It's hard to compete with writing the software we use to drive Mars rovers.

Speaking of which ... "So, what are you planning to do when the project is over?" Frank asks. I don't really know. I've planned to go back to working on the stuff I was working on before, especially since that's what I've been promising John[1]. But I don't think I'd be happy with things just going back to the way they were. Something's going to have to change. I just don't know what it is.

Frank offers to arrange work for me -- graphics stuff, if I want it. Tempting, tempting. But I have promises to keep.

And meters to go before I sleep. Against expectations, we're driving today. Off in the drive direction is a long bedform named "Serpent." Serpent is too large to drive over, so we're going around it. The plan for tomorrow is to drive to its southern tip (this takes us away from the crater rim); we'll maybe poke at it with the IDD, then head on. We might also study some nearby rocks, since there are some white rocks near Serpent and this gives us a chance to get the fucking white rock business laid to rest once and for all. (That's not my characterization; Ray actually says "fucking." He wants to drive on in the worst way. I find this impatience endearing, as does Frank, who asks him to come upstairs and light a fire under Opportunity's scientists so they can get the hell out of their crater already.)

And we might get to do other stuff to Serpent, such as dragging the wheels over it to form a makeshift trench. We're going to show this little snake who's boss!

More surprising than the news that we're driving is the news that we're not going to drive into Bonneville after all. There's just nothing interesting in there -- nothing close enough for us to reach, anyway; we'd have to go all the way to the far wall for that, and that would mean kissing the Columbia Hills goodbye. Dave Des Marais asks for a traversability analysis at some point anyway, just so we'd know whether we could have gone in if we'd wanted to. But we don't want to.

Unfortunately, I'm not the only one who was surprised that we're driving. The project management was also surprised -- or would be, if they knew. They thought yestersol that we wouldn't be driving, so they've given the downlink teams the sol off. Which means nobody's here to do the usual traversability analysis and stuff. Fortunately, though, Frank happens to stumble onto Mark Maimone, who's here even though it's his day off (now, what kind of sick weirdo would do that?), and Mark takes care of it, kicking out a downlink report, INCONS file, and traversability analysis in no time.

Which means I get to relax and go to the downlink assessment meeting. Yestersol was the most complex sol we've ever sequenced (not for the rover drivers, but for the rest of the team; the day was very heavy on remote sensing). They broke records for the largest number of observations and the greatest number of different targets examined in one sol. "This is not necessarily a good thing," Ray says in admonishing the science team to trim its appetite. One price of our newly compressed schedule is that we can't do stuff like that any more. Which probably means we shouldn't have succeeded; it only encourages them. But Ray will fix that.

The meeting itself is mostly routine, though a White Rock Mafia member gives a presentation at the end -- Mysteries of the White Rocks -- that lays out their side of the argument. Some of it is Deep Geology, which means it goes over my head, but the crux of the argument is that it all depends on why the white rocks are white. It might just be dust adhering to the rocks from atmospheric settling, or deposited on them from below (as odd as that sounds) as part of the process of exhumation. But the exciting case would be that the white stuff is intrinsic to the rock, and we're sort of seeing it sweating out -- this would be exciting because the processes that cause the white stuff to get sealed in in the first place could be water-based. This would make the white rocks a smoking gun for past water in Gusev, and that is the reason we're here.

Not everyone is convinced, but I don't stay to watch the fight; I've discovered that we don't have the terrain meshes we're going to need to plan the drive, and that's something I need to take care of sooner rather than later. I go upstairs and get MIPL to kick off the process, and get a nasty surprise when I go back downstairs. All of a sudden, my badge doesn't work in the fucking badge reader. Ten minutes earlier, it was fine, and now it's declared me persona non grata. This is particularly inconvenient because the restrooms are in the non-secured area, which means you need badge access if you want to get back in.

Unless you're as pissed off as I am. Then you do what I do: you disable the fucking lock. I first try a couple of solutions that would disable the lock only when I'm on the outside of it, but I don't get them working quickly, and I have real work to do. So I just put tape over the hole. Jesus Tap-dancing Christ.

I call Security, but they can't help me over the phone. To get this sorted out, I'll have to go by the Security Office when it opens, several hours from now. This will mean sticking around well after my shift ends. Oh, goody. I'm sure to be in a real good mood, then.

The Serpent drive turns out to be trickier than it looked initially. The terrain between us and Serpent is reasonably flat, so it would be a snap to just drive to there, but there are more constraints than that: we have to be pointed at 60 degrees for communication reasons[2], which will leave us aimed away from Serpent and thus unable to IDD it. So we have to drive to the other side, then turn around to 60 degrees and come back to it. And there's an obstacle-sized rock near the tip -- there's enough room to fit the rover through there, but we're not sure how far we're going to slip in this terrain, especially since we're heading downhill. We can't just drive over it, either; we're not sure how badly we'll slip if we try, it's too high in most spots, and the scientists don't want us to disturb the soil yet anyway.

So we pull an old trick out of our bag: drive the rover as close to the gap between Serpent's tip and the rock as we feel is safe, then autonav between Scylla and Charybdis. Every time we use autonav, we add a set of reasons the drive might fail -- but then again, we can't risk not using it. I warn Ray that there's a lot of uncertainty and list all of the reasons I can think of that the drive might fail. He shrugs and says, "Sounds like an interesting experiment." So we're good to go.

Having worked out the approach, the drive itself isn't too hard to implement, even with the IDD work they want us to do first. The IDD sequence turns out to be pretty cool, actually: we bring the APXS up in front of the left front HAZCAM to get a confirmation that its doors are closed (Opportunity's APXS doors didn't fully close recently, and they want to explore this) -- that's something we haven't done before -- then place the MI on a target near the right front wheel. What's fun about this is that the IDD turret and wrist perform beautiful, complex spins and twists as part of the motions. This reminds more than one observer of a gunslinger: Ray suggests that the rover should have had a holster.

The mood tonight is more relaxed. The place is emptier. Justin Maki suggests that people are finding the mission routine: there were plenty of people here on sol 1, and for other big events. But I think it's probably just that many of the scientists are at the Lunar and Planetary Science Conference.

Both rovers are working well, and Art says we'll keep running them forever. But Robin Fergason points out that this might not be up to us. They're talking about turning off MGS, even though it's still going strong -- and playing an important role in this mission, acting as one of our liaisons to the rovers. Why would they turn it off? Because operating it costs $8 million per year. By space exploration standards, that's nothing. Hell, we spend that much on -- well -- ice cream.[3]

Um.

Well, maybe they'll let us work on the next rover, Art says. I tell him that exploring Mars is like sex and pinball: the reward for doing it well is that you get to do it again.





[1] John Louie, my group supervisor.

[2] Our UHF antenna is theoretically omnidirectional, so it's not supposed to matter what heading we end up at. In practice, however, it's not so: the rover mast and other features on the deck act as obstructions that factor into the antenna's actual performance. For a particular comm pass -- with Odyssey at a particular location in the sky -- we'll get better results with Spirit at some headings than at others. Thisol we determined that the best heading was 60 degrees (headings are measured clockwise from due north).

[3] Just in case anyone without a sense of humor reads this: yes, that's a joke.

2009-03-14

Spirit Sol 70

It's starting already: at least temporarily, they're moving the downlink teams to Earth time. Sigh.

I've decided to keep coming in at my regular time, even though I could be coming in 90 minutes later (like everyone else), so that I can get more work done. Sigh. But maybe this will mean I'll be able to work less on my days off. (Fat chance.)

They've taken another image of the backshell -- or whatever it is -- which have failed to fully clarify the situation. There are several Spongebob Squarepants fans on the project, who have decided that that's what it is. I guess that counts as finding life on other planets.

At the downlink assessment meeting, they have a beautiful color image of the color crater panorama on the big screens. I'm really getting spoiled by the big screens. When the project is over, I'm going to have to buy a 3200x1200 projection monitor.

Anyway, the plan from here is to work the rim. We'll be here for about 3 weeks (later they say 18-22 sols), inspecting rocks, soils, ripples, deposits, etc., as we crawl along, and that will take us to the end of the nominal mission. The extended mission will be the drive to Columbia Hills.

The guy defending this plan puts up a presentation with a picture of Opportunity's crater; there's a round of good-natured booing. But the point of showing the image is to set a context: in its crater, Opportunity found the interesting stuff (bedrock) just below the rim. We can expect something similar here -- we may, for example, not need to clamber all the way down to the bottom of the crater; exploring the rim and upper slopes may do everything we need.

At Bonneville, though, there is no evident outcrop (which everyone was hoping for). Still, there's significant value in being here. You tend to get more weathering on slopes, since they present a broad face to the wind and allow the weathered material to "escape" (by running downhill), so we'll see fresh material just beneath us. For the same reason, coatings and non-basalt rock types that don't weather as fast as basalts will also be exposed here. So even though we don't see bedrock, we should see plenty of geologically interesting stuff.

One thing we'll need to do is analyze the crater slopes. The angles we're seeing, 20-25 degrees, are on the edge of what we're able to traverse, but there's a worse problem: on those slopes, we're likely to see 100% slippage. This makes it a rover trap, where we can get in but find ourselves unable to get back out. I have the image of a sort of hungry robotic ant lion, lying patiently in wait at the bottom of Bonneville for millions of years, ready for the moment an unwary robotic explorer from another planet should wander in ....

And Ray notes the other end of it: 100% slippage would mean that we could slide all the way down, unable to brake. "I don't want to try to traverse one meter down and the next thing we see is the dunes at the bottom," he tells me. Just think how I'd feel about it!

Ray also has a more serious, and pointed, question. Suppose remote sensing shows more of the same -- more of what we've already seen here. Do we even have to go in? There's a lot of discussion about this, but I think the short answer is: no.

One other note from Ray: we're big news in Baker, CA -- population 392. Don't ask me what Ray was doing there; maybe it's because Baker is the home of the world's tallest thermometer. But he was, and he tells us that people kept coming up to him and saying, "Hey, I heard you made it to that crater!" So if we're news there, I guess we're news everywhere.

Today's sequencing is just a little IDD work; I could do it in my sleep. I'm done with it and hand off to Bob practically the minute he comes in. Once again, I leave on time. This could become a habit.

2009-03-13

Spirit Sol 69

I wake up about an hour early so I can deal with the paperwork for my SpaceOps paper. It turns out there are no problems: the JPL guy faxed me the forms I need to sign, just as I'd asked, so all I have to do is sign them and fax them to the SpaceOps people. (Oh, yeah, and send them the paper itself.) But as a result, I'm about an hour early. So I go ahead and go to work -- and catch up on the latest images before my shift even starts.

Ahhhh, that's better.

Moreover, they're on a new schedule -- the meetings start 90 minutes later now, so I could have come in that much later. They were testing this schedule a few days back, and it looks like it's going to be permanent. And, as it turns out, we're sitting still for at least one more sol -- no driving, no IDD. So I have practically nothing to do today, except hang around and catch up on work.

Now that we've gotten a better look at the backshell, it doesn't look like the backshell any more. Whatever it is, it's angular, not round. It might be a broken chunk; they're going to take more images to find out for sure. In the meantime, there's a lot of joking about our having found an alien artifact -- job security, here we come!

75% of the legacy panorama is now on the ground -- good news, since they've got another one coming (just in time for their conference, of course). And they're showing a movie of the Deimos transit: eight frames, ten seconds apart. (It's not clear to me whether this is the movie Opportunity took, or whether we got our own; it sounds like the latter.) The PUL says that the transit was a little earlier, and a little closer to the center of the sun, than was expected. There's some uncertainty about Phobos's and Deimos's orbits -- because they're so small, they're hard to observe -- which our observations will help to eliminate.

And our odometer is practically a blur: we've already gone 402m, total. Someone also discovered that we've been a little wrong about one of the mission success criteria. With a tau (atmospheric opacity) of over 0.5, we have to operate the rover for only 60 sols, not 90, to declare success. The time we spent sitting at Adirondack doesn't count, so we reach the minimum success level in only 3 more sols -- not 21 more sols, as we had all thought. Our thanks go out to the global dust storm that preceded our arrival.

The dark deposit we see inside Bonneville crater is of uncertain composition. Its spectral characteristics seem to be more like Gusev-area rock than soil, but no rocks are visible in the area of the deposit itself. It's just possible we'll have to go down there and see for ourselves, though the default plan is just to crawl along the rim for a while instead.

I do actually have a little bit of work to do, as it turns out. We're trying to characterize how the rover slipped in driving up the last few meters of the crater rim, so that we can do a better job of driving it in this area. To do that, we need to know precisely how far it actually moved, as opposed to what we commanded. And to do that, we need to take pictures of the wheel tracks -- specifically, the locations where the rover started and ended each leg of the traverse.

This is harder than it sounds, because we don't know exactly where those locations are (if we knew that, we wouldn't have to take the pictures). Making matters worse, the rover reset its position -- as commanded -- when it was done with the drive, so the numbers we have for the commanded positions no longer mean what we want them to mean to the rover. The MI PUL (Alex) and I have to fix this by coregistering images by hand. We identify the same rocks in both the pre-drive and post-drive images, compare their positions, and use the difference to compute the actual offsets we need to use to aim the cameras at the drive locations. We must have done a good job, though -- when we check the pointing afterward in RSVP's camera view, it looks like we nailed them. We'll see when we get the actual images. After that, I hack on RoSE for a while -- mainly for fun. I have real work to do, but it can wait a day.

Andy stayed on Mars time longer than I thought, but tonight actually is his last night. Everyone signs the "Now Planning Sol 69" sheet for him, and he gets a round of applause. He's making a big mistake, though -- by which I mean, giving up his best excuse to just let things fall behind.





Courtesy NASA/JPL/Texas A&M/Cornell/SSI. A reduced-size version of Spirit's Deimos transit animation, taken on sol 68.


2009-03-12

Spirit Sol 68

I don't stay long. And I make a mistake I don't intend to make again: I save catching up on pictures for last, and run out of time to look at them. To hell with that: I don't mind coming in on my off days, but if I need to do that to catch up on my work, I'm putting myself first. This I vow!

Until next week, when I'll doubtless revert to my usual self-denying habits.

2009-03-11

Spirit Sol 67

The downlink assessment meeting has its share of happy news. They got a cool animation of Phobos transiting the sun. It's a crude animation -- only two or three frames -- but it's something that's never been seen before. That is, it's the first time we've seen Phobos transit the sun; the first transit by Deimos was snapped by Opportunity a sol or two ago. Phobos is larger and closer to Mars, so it obscures more of the sun; Deimos is just a tiny speck, but Phobos took a good bite out of that sucker.

Mark Adler reports that the sequence timings were a little messed up, so the traverse didn't complete. We're still a couple of meters short of the edge. But it turns out that this might be fortuitous: at this point, we lose elevation as we get closer to the rim, so we're getting a better view from where we ended up. Still, because of the way the drive ended, we don't have images of the terrain immediately under the rover. Thus we can't be sure it's safe to deploy the IDD; this limits what we can do tomorrow.

Our view of the crater itself has never been better. "In a sense, we've just found a new universe," Golombek says as a way of kicking off the "what's next" discussion. It falls to Dave Des Marais to re-frame the question in the terms I suspect are on everyone's mind: "What're we gonna do for LPSC?" (The Lunar and Planetary Science Conference is the conference they've been building up to; it occurs next week.) We'll probably just scoot forward 2m or so and take a legacy panorama. This will likely be at least 180 degrees or so, in color, and should look absolutely spectacular. And when will they need to have this done? "What day are the talks?"

I have a lot of work to do, but most of it I can do at home. I came in mainly to do a favor for Bob Deen, who (like me) is writing a paper for the Space Ops conference. (I wrote mine last night, after realizing the deadline was 10 days earlier than I thought. Most people, it turns out, are even later than I am: Frank, Jeng, and Brian, at least, haven't done theirs yet.) He needs some screen shots of Spirit exploring the trench, since he's particularly proud of the trench mesh and is going to discuss it in the paper. I put the screen shots together for him quickly, and he more than repays the favor by showing me a beautifully clear 3-D view of the crater, looking over the rim into the enormous bowl.

I spend some time catching up on my email, the backlog of which has grown to scandalous proportions. Andy sees me and asks the usual question: "So are there any days you don't come in?" I explain that I originally came in on my off days to catch up on the pictures, but I don't have much time for that any more; now I use my off days to catch up on all the work that piles up when I'm on shift. He tells me his strategy for dealing with it: "I just let things fall behind."

My email contains one more piece of good news: the free ice cream is back! Through the end of the nominal mission, anyway, which means until April-ish. Someone will have to go out each week and buy about $1000 worth of ice cream with his own money, then get reimbursed by the project. Mike Adler has already done it for this week. I seriously want to do this just once, for one simple reason: I want to see the look on the cashier's face when I show up at the checkout line with $1000 worth of ice cream.

The only thing funnier would be to throw in one box of tampons.





Courtesy NASA/JPL-Caltech. Phobos transits the sun.


2009-03-10

Spirit Sol 66

My new distance record didn't last very long. Today they put about 40m on the wheels, although the autonav got spooked again. So they ended up making about 30m of progress, or 25m after accounting for slip (we're now heading up the outer slope of the rim). We didn't make it to the rim; we have another 25m or so still to go before we reach the target point.

Still, that was enough to enable us to see significantly more of the crater. We can see a good chunk of the crater's inner slope and floor. And we can see the backshell, which landed inside the crater, near the top of the far wall.

We're interplanetary litterbugs!





Courtesy NASA/JPL-Caltech. A post-drive NAVCAM image looking across the rim of Bonneville. On the far side, in the upper right of this image, the sun glints off of the backshell -- part of the spacecraft Spirit rode to Mars.


2009-03-09

Spirit Sol 65

The rover got a little confused. The last 12m of the drive were supposed to be handled by autonav, because it involved traversing a region we couldn't see well enough to plan the drive ourselves. It turns out the region contains a hollow, which spooked the autonav. So the rover drove about 12m, but only progressed 5m towards the goal before stumbling onto the hollow; the remaining 7m was spent shuffling back and forth, trying to find a safe path out. As it happens, the rover found a safe path just at the end -- but too late; the time-of-day limit hit.

Well, I warned them yestersol that something like this might happen. But I'm still kind of bummed. As it happens, the scientists are happy anyway: the rover's back-and-forthing dug a shallow hole in the loose soil of the hollow -- "spontaneous trenching," someone calls it. Picking up on the theme, the deep tracks we just created are dubbed "Serendipity Trench" and becomes the focus of science observations. Sow's ear, silk purse.

The big news is that, even before we reached the hollow, we met mission success: our odometry now stands at 313m, comfortably exceeding the 300m NASA required us to achieve. All we have to do now is not break the rover before sol 90, which I think we can handle. Since Opportunity has just been shuffling around inside its crater, its total so far is only about 55m, so we might end up driving extra to make up the difference (the two rovers combined are supposed to reach 600m). Well, if they insist.

I'm still feeling bad that the drive didn't reach its goal, but the downlink assessment meeting makes me feel better. The scientists are happy with Serendipity Trench, and they're even happier about the odometry total. They announce the new total (now revised upward to 314m), and there was much rejoicing.

Matt Golombek is the SOWG chair again, and he states bluntly that we'll be driving. "I'm here for three sols and I want to be at the rim before I'm off." There's little, if any, opposition to this goal, but some of them underestimate Matt's eagerness. In discussing the long-term plan, a scientist says offhandedly that the rim is about two 15m drives away, and Matt quickly corrects him: "One 30m drive, thanks!"

Where exactly on the rim do we want to be? Ahead of us and a little to the right, on the very lip of the crater, we can see two largish rocks that might be very interesting science targets. One of them appears to be black (though this may just be shadowing), and is jokingly dubbed "Darth Vader." So the other, lighter-colored rock is tentatively named "Luke Skywalker." The plan tomorrow is to drive Spirit up to the rim between Darth and Luke, which are easily far enough apart for this. On subsequent sols, we'll look into the crater from that position, do remote sensing on both rocks, and then probably pick one of them for more focused study.

Since I'm shadowing today, I get to slack off. (What this actually means: I do other work, not rover-driving work.) I also get to attend the end-of-sol science discussion, which today is about the rim traverse plan. We'll reach the crater rim at its southwest edge and traverse the southern rim from the southwest area to the southeast or east. We won't go all the way around (this would be about 750m), as our next destination is the Columbia Hills to the east. When we reach the eastern edge of the crater, we'll literally head for the hills.

But will we enter the crater first? There's a lot of support for this, but we won't know whether we can do it until we reach the rim: if it's too steep, or the sand is too lose -- or there's just nothing of interest -- we'll skip it. We should know in a sol or two.





Courtesy NASA/JPL-Caltech. Final front HAZCAM image showing Serendipity Trench, the terrain we disturbed by our back-and-forth "roverdancing" at the end of the drive.


2009-03-08

Spirit Sol 64

Yestersol went damn near perfectly. 35.33m -- a new traverse record! The record-setting drives aren't exciting people as much as they used to, but I'm still happy about it. So is John Grant, who tells me enthusiastically that I did a great job. John also warns me that the NAVCAMs seem to show less benign terrain ahead. Here be hollows.

The big screens in the SMSA are showing the automatically generated "movie" of the autonav portion of the drive. (These are small images, taken 1m apart, showing what the rover saw as it navigated through the terrain.) The cool part is when the rover decides to drive over a sizable rock in its path. It looks like the rock is just under the obstacle size, and Spirit blithely climbs right over that sucker. It's big enough to show up in the ACS data as well; the rover changed pitch significantly while climbing the rock. Bob talked me into doing this last segment of the drive on autonav -- I was going to do it blind, for speed -- but he was right. The terrain is safe, but it was a better decision to have autonav on through here. If only for the movie.

Art wants us to cover another 30m tomorrow. We won't be able to do a two-drive day (the so-called "megadrive" approach), because we don't have comm passes at the right times. But it will be a decent-length drive all the same. Art tries to get me to promise him 30m, but I haven't looked at the data yet, so I don't. He tries again. I still won't promise him, and the second time he gets the message. "See what you can do," he says. Will do.

I guess the scientists' field trip was a short one, because the downlink assessment meeting is full again. LTP (in the person of Dave Des Marais) is enthusiastic about the success of the drive -- "especially in this terrain" (it's rocky out there) -- and has some real praise for the rover drivers. (I can't help it, I'm kvelling.) But they might want to pick a spot to settle down for some IDD work. "We may have to rein in the stallions a little bit," as he puts it. The good news from LTP is that our odometry total now stands at 286m, out of 300m needed to declare success. We'll make it tomorrow!

Tomorrow they plan to do an "air-lite" sol; a downlink-limited day, it will be dominated by a few atmospheric observations plus some driving. Because we're downlink-limited, we'll cut back on the autonav movie, taking an image only every 3m instead of every 1m. Some people would like to cut the movie altogether, but it has an engineering purpose: if the rover errors out during the drive, the movie can be an invaluable forensic tool. The rover has an on-board "fault image queue" that's supposed to be used for this purpose, but Mark Maimone doesn't agree that it's been tested well enough to rely on it yet. So taking the images only every 3m is our compromise, for now.

Since I know what the sol's plan is, at least as far as it concerns me, I leave the meeting and sit down with today's Mobility/IDD guy to analyze traversability. This entails running the navigation images through some of Mark's software, which colors it: green for very safe, yellow and orange for moderately safe, red for hazards. Then you plan the longest safe path you can. I see two good paths in the direction we want to go (northeast) -- one a little more to the north, one a little more to the east. The first path ends up growing on me, because even though it's less direct, it's simpler and safer overall, and we can do the whole thing with the much faster blind driving. The second path is the more obvious choice but has some drawbacks; for instance, near the limit of the NAVCAM data, we'll need some tight maneuvering between a couple of hazards. We'll probably have to leave that to the autonav, and that will eat into the drive time significantly.

Mark calls to see how it's going, and I talk to him about this on the phone; he follows along using a copy of the traversability map he's generated from home. He tells me he doesn't see my preferred path (which I've taken to calling the Northwest Passage), which puzzles both of us. He goes off and looks into it for a while, then calls back with the solution. The person who generated the traversability map I've been looking at did it with the wrong data. The real map has obstacles right where we were going to send the rover. I no longer wonder why Mark works all the time. "You can't turn your back for a second, can you?" I tease him. Of course, we'd have caught the error later in the planning cycle anyway, even without him -- one hopes.

At the SOWG meeting, both Art and John Grant say they're surly. In Art's case, it's because tomorrow's resource picture doesn't look as good as he thought. In John's case, it's because he somehow pissed off a bunch of the scientists -- I think I missed some fireworks by leaving the downlink assessment meeting early today. They needed to cut back on the science observations because they won't have much room in the downlink.

In any case, for planning purposes, everything except the drive is "in purgatory" -- a now-standard phrase meaning that it will make it into the plan if there's room, but you'd better not count on it. John is more blunt than usual about this: "Convince us your observation is crucial for tomorrow, or it's out."

Nearly everything ends up out.

This leads to some acrimony, considerably more than usual for this meeting. One of the scientists tries to persuade the room that it doesn't matter how much data we generate tomorrow, what matters is keeping our overall average below the overall downlink budget. So it's OK if we go over the line tomorrow; we'll make it up on the next day. The rest of the room finally seems to be wising up about this frequently practiced bit of self-delusion, though -- the problem is that they always overspend today, promising to make up for it tomorrow, and somehow tomorrow never comes. The argument doesn't want to go away, until another scientist sardonically calls for a filibuster. "If we talk long enough, it will be too late to put anything in the plan," he says. The rest of them get the message and manage to work together, but the issue clearly isn't laid to rest. After the meeting ends, a couple of pockets of people remain behind, each faction rehearsing its argument for friendly ears.

Since all I have to do is plan the drive, sequencing is relatively easy. I decide to finish before Bob comes in, and to my surprise I succeed -- with a few minutes to socialize, to boot.

And time to eavesdrop, as well. While I'm doing a mindless part of the work, I listen in as a couple of the scientists argue about our general approach to the crater. One of them is pressing Doug Ming's point that we're rushing to the rim, saying that we should be conducting a more gradual, systematic study of the soil and rocks along the way. The other strongly disagrees: "If you were out there, the first thing you'd do is run to the edge of the crater and look in," he says, and that seems to settle it.

Bill Dias has been out for a week or more, and it turns out that he's left the project. More than that, he's left JPL, after 14 years. Nobody seems to know why, or what happened. But he sent email titled "Change is good ...." That change is disconcerting. Bill was cranky, pessimistic and sarcastic (which is probably why we ended up getting along so well -- rim shot, please). He could also be very funny and likable when he wanted to be. I'll miss him.

Shortly before I leave, Jim Bell shows us the latest PANCAM image. It's a picture of the Earth from Mars, taken by Spirit, the one she woke up to take the other night. The Earth is just a tiny dot in the center of the image, a handful of faint pixels -- almost drowned out by the twilight in the unenhanced version. Looking at this picture, I feel an unaccountable mix of pride and something else I can't quite put my finger on -- sadness, I think, or maybe loneliness. Spirit is very far from home, and she will never make it back. Others seem to find the image mostly awe-inspiring. Art compares the picture to the famous Apollo photo of Earthrise as seen from the moon -- "Well," he says, "maybe their picture was better." I think this one is better, because it's ours. But Jim Bell sums it up when he says quietly, "Don't think for one second that there aren't millions of people who would die to be us right now."





Courtesy NASA/JPL-Caltech. Five years on, the rovers have sent more than 200,000 images to Earth. This one is my favorite.


Courtesy NASA/JPL-Caltech. Same image, with "You Are Here" text. Funny, but I think the version without that is much more profound.


Another iconic, beautiful, inspiring image of the Earth from space -- from Apollo.


2009-03-07

Spirit Sol 63

I wake up feeling the usual absolute sick certainty that I've destroyed the rover. At the very least, I should have nudged the final waypoint a little to the southwest, to leave room for the final northeast-oriented "stutter-step" short leg of the drive; this portion is done using autonav, so the rover will keep itself safe, but they might miss out on some science data. I check the downlink reports two or three times before even leaving home, but in vain. The pass hasn't happened yet, so there's nothing to report.

Of course, everything went perfectly. The final part of the drive timed out, but that wasn't unexpected. We're now 88m from the crater rim.

So I worry too much.

Most of the scientists are off today, on a field trip to Amboy Crater (where they did some of the Sojourner field testing). Steve Collins suggests freaking them out by getting out there ahead of them and putting the testbed rover in the crater, drilling RAT holes in various rocks, and so on. "Fooled you!"

John Grant, who's back to being the SOWG chair again, spots me looking over the drive data with the Mobility/IDD folks. "You da man!" he tells me. Their tentative plan is to shoot for another 20-30m tomorrow, then maybe a megadrive toward Bonneville. We'll be maybe 10m from the rim at that point, almost close enough to reach out and touch it. With our robotic arm.

With the scientists on a field trip, the downlink assessment meeting is sparsely attended -- only about 20 people in the room, less than half the usual number. It's also much more informal and jocular than usual. Everybody can sit more or less within earshot of each other, so they don't really need the mikes, and the room takes on a much different dynamic.

The group's already bouyant mood is only helped along by LTP's welcome observation that we've now traversed about 250m of the 300m required for Spirit to claim full success; everything else NASA requires of us is done. ("Ah, let's just do the 50 meters tomorrow and finish it up," I suggest. In this crowd I find lots of approval.) For the near future, we'll be alternating "dirt sols" (examining soil or rocks, as we will tomorrow) with "aerosols" (studying the atmosphere).

It so happens that there's a smooth, long, flat rock just in front of our left wheel. They've named this rock "Plank," and the debate du jour is whether to IDD the rock or the soil -- or to skip it and just dedicate the day to driving. The case for IDDing the rock is strengthened if it's one of the so-called "white rocks" we've seen around us occasionally. The White Rock Mafia is all at Amboy, so nobody's here to argue vociferously for examining Plank (if it qualifies as a "white rock" at all), but a few of the scientists try to represent them in absentia. They end up deciding that Plank is not a white rock, but when the vote comes, the scientists decide that the rock is of more interest than the soil (by 11-3, a runaway). So we're going to try to IDD it if possible. (The conclusion was helped along by a great compromise idea from John Grant: whether we vote for the rock or the soil to be the favored target, also choose a backup target from the other area; if we can't reach the favored target for whatever reason, we'll do the other instead.)

John floats the idea of doing a megadrive on the following sol. Preliminary opinion favors this, but with some dissent. Some of the dissenters seem to be swayed by Jim Bell's observation that we want the sols leading up to the crater rim to minimize data generation, so that we can clear out the flash -- when we get up to the rim, we'll be taking picture after picture, of the crater and the surrounding terrain, and we'll need somewhere to put them. On the other hand, as Doug Ming points out, we're rushing through a rich target area right now; we have a responsibility to study the terrain systematically as we go, not just blow through it. John cuts off the discussion shortly after that, as they need to discuss it with the full group anyway, and I go off to see if the IDD can reach the targets they've chosen.

It can't. Or maybe it can, but this will take careful sequencing, and I'll have a lot of driving to plan as well as the IDD work. Doug Ming saves me by finding another target on the rock that turns out to be a snap to reach. This makes my life much, much easier. (I probably could have saved myself a lot of trouble on other sols by telling them that they should choose different targets, but I hate to push back on science. I need to consider the fact that it can be better for them if I do that sometimes. And usually they don't care about the particular target anyway; they just want measurements of the rock, not of this particular point on it. Live and learn.)

As a result, I'm done sequencing the IDD work by the end of the SOWG meeting (though Bob will tweak it later, as he always does). It's gratifying to realize how far I've come: doing a multi-sequence, three-instrument placement used to be at the limit of what I could handle in my shift. This one I get done in maybe half an hour, leaving plenty of time to work on the drive.

So I have plenty of time to check out the crater rim. Some of the scientists, looking carefully at today's post-drive PANCAMs, have noticed that you can just barely see the far rim of the crater. We're looking through a dip in the near side of the rim, seeing the inside of the Bonneville, on its far side. "I'm reminded, once in a while, of why we do this," Andy remarks.

Even before seeing the crater rim, Andy was in a good mood, possibly because this is his last day on Mars time. He's returning to a strategic shift (which means: normal Earthling-type hours) in order to help design the extended mission. Julie Townsend is going to take his place, after she finishes training her own replacement (Saina Ghandchi).

Those aren't the only personnel changes. Lots of people are leaving the project altogether, including, to my surprise, Rob Manning. He's going to work on some other project that needs him more. Pete Theisinger is long gone, of course. The rovers themselves are going strong, but the team is breaking up and fading away.





Courtesy NASA/JPL-Caltech. I believe this is the PANCAM image I was looking at, where you can just spot the far rim of Bonneville through a sort of notch in the near rim.


Courtesy NASA/JPL-Caltech. The long, flat rock next to the left front wheel is Plank.


2009-03-06

Spirit Sol 62

I'm back on shift today. We're planning only one sol, sol 62, but the two-sol plan that ended yestersol seems to have gone very well. Yestersol, in particular, they did an excellent drive: as I'm sitting in the SMSA watching the data come in, they report 29.283m!

It turns out to have been a little farther than that, incidentally: at the downlink assessment meeting, having gotten more complete data, they report 31m, to a round of applause.

The other news at the downlink assessment meeting is slightly more bleak. They're going to have to curb their appetite for data for a while. The legacy panorama is finished (which news also brings a round of applause), but it used up a huge amount of their available data volume. As Dave Des Marais memorably puts it, they're now like a snake that's just swallowed a pig. It doesn't help that we're not doing the best job of managing the data we've gotten -- we're just now getting some PANCAM images that were intended for drive decisions several sols ago. So not only are we not getting this data when we need it, but it ends up blocking other data that is now more relevant. Oops.

LTP reports that we've now driven 226m, total, of 300m needed for minimum mission success. For once, we've climbed above the red minimum-success line on Dave's chart. We're still unsure exactly how far we have left to reach the rim, but we should get there in another six sols or so. There's growing support among the scientists to reach the rim, not only because we need the mileage for mission success, but also because some conference is coming up and they want crater images to show off. Well, whatever it takes ....

We probably will not drive into Bonneville crater when we get there, at least according to Matt Golombek. If it's as they expect, the inner crater walls will be too steep for us to drive down. And even if we get in, the same slopes might well keep us from being able to get back out. Not good. So we'll probably have to creep around the rim, peeping inside when we can. (Hey, that's a good name for this: "creep and peep.")

Tomorrow's plan is a simple one: unstow the IDD just long enough to MI the soil, then restow and drive. It gets even easier when they later cut the MI observation (for data-volume reasons) and it turns into a plain drive.

Nothing much is going to happen until the SOWG, but I need to know how far we can drive tomorrow using the data we've got. The data was still being received when the meeting started, so I leave early to go look at it with Mark and Rich. It's rocky off to our right, and our left doesn't look much better. Straight ahead is relatively smooth sailing, except for a depression we can't see into. For safety's sake, we have to treat the depression as an obstacle -- even though we could almost certainly drive safely through it -- so we're going to have to take the long way around, zig-zagging between some hazards to the northeast of us.

On the trek to the rim, they won't do much IDD work (maybe every other sol, and not much of it on any given sol), so it's a perfect time for them to do atmospheric studies. They're planning more of that over the next few sols, including, tomorrow, the long-awaited Earth image. In the middle of the bitterly cold Martian night, they're going to wake up and look up at the sky. If they get lucky, they'll catch a glimpse of a pale blue dot the rovers once called home.

"Everyone needs to go outside at 2:30AM and wave tomorrow," someone says. They're kidding, obviously, and anyway, as seen from Pasadena, Mars will be below the horizon when the time comes. Spirit might see Earth, but she won't see our part of it -- her hometown. The next night, when 2:30 comes, I go outside and wave to the stars anyway.




Courtesy NASA/JPL-Caltech. A rover's-eye view of the way to Bonneville.

2009-03-05

Spirit Sol 61

The big picture of the "smoky" RAT hole is on the wall in the downlink assessment meeting. The scientists are trying the two-sol planning experiment, planning sols 61 and 62 today. The basic idea is to IDD the rock on sol 61 (possibly with a short afternoon drive), then drive toward Bonneville on sol 62. They also want to take a "legacy panorama" -- another panorama like the mission success pan they took on the lander, this one from so far away that the lander is no longer visible. We're that far away already.

From here until we reach the crater rim (which Ray pushes hard for, again -- my hero!), we'll mostly have touch-and-go sols, IDDing a rock if one happens to be in the IDD work volume, and otherwise examining the soil. The drives will be structured the way they normally are, blind driving until the limit of our data, stopping for localization imagery, then autonav until the time-of-day limit. Then we take drive-direction imagery so we can drive efficiently the next sol, and shut down for the evening. We're going to try to reach the rim in 10 more sols.

I don't hang around Building 264[1] long, just enough for a quick pix fix. Instead of leaving, I take Rafi's suggestion and go to Thursday Quality Time.[2] Which turns out to be very nice. Everyone wants to talk to me about the mission, so I feel like a local celebrity. But mainly it's just nice to hang out with these people. I've missed them.




Footnotes:

[1] The JPL building from which we drive the rovers. It's so nice how they name the buildings creatively like that.

[2] Rafi Solomon is a fellow member of the group I officially work for -- I supposedly develop software for processing telemetry, but I haven't actually done much of that for the last few years. "Thursday Quality Time" is the affectionate name for our weekly group meeting, which should give you a clue as to why I really do like those people and miss spending time with them.

2009-03-04

Spirit Sol 60

The project continues to work on extended ops scenarios. Since the rover drivers are under the most time pressure most days, we'll be among those most affected by the outcome, so they've asked the rover drivers who aren't on shift -- including me -- to come in for a meeting to discuss it. I listen and try to give useful feedback, but I realize in the meeting that I don't care that much about which option they select. Either way, it's not going to be the same any more. It will still be very cool, but I don't think it will be the same.

I also realize that surface ops has changed my life. I haven't been in a meeting like this in a long time, and I sure as hell haven't missed it. A bunch of people sitting around a table, most of them typing at their laptops, droning on and on, not getting anything accomplished. My life used to have a lot of this. Surface ops forces people to move, to waste no time, to think fast, to be efficient, to get things done. Surface ops is institutionalized impatience, and with good reason: there's a deadline every day. This must be a little bit like what some people feel when they leave the military.

One of the presenters also says that "people are getting tired of Mars time." I look around, surprised to realize that it's true. Everyone in the meeting -- everyone who's working Mars time, at least, and that's most of them -- looks exhausted. "I love Mars time," I say, thinking: "you wimps."

I also feel a very petty satisfaction in seeing how tired they look. Most people who have trouble with Mars time have trouble because they're morning people. I've been in meetings with some of these people at 7:30AM more times than I can count, and I felt every bit as haggard as they look now. Well, now they know how I always feel! Score one for night people!

I have a lot of work to do, but I can do most of it at home with a cat on my lap. So I don't stick around long. But before I leave I talk to Art Thompson a little bit. Art is almost as enthusiastic as I am about the mission, I think. "How often do you get a chance to do something like this?" he's always asking. As a Pathfinder veteran, he's had the chance twice; I will probably never do this again.

On my way out, I see a beautiful picture on the wall in the SMSA: the second try at RATting the rock worked, leaving a 2mm-deep hole ringed by a mess of debris. I congratulate the RAT folks, who are looking happy and relieved, and go home to work.




Courtesy NASA/JPL-Caltech. The successful RAT hole on Humphrey.

2009-03-03

Spirit Sol 59

Opportunity found unmistakable signs of water, it turns out. It's even on the news, despite the fact that it's an election day. As I'm showering, they're having the press conference. I picked the wrong day to sleep in.

The RATting didn't go as planned yestersol. It's not hard to predict my reaction: this must be my fault. But it isn't; Jeng assures me that the IDD sequence was fine. The likely cause is that the RAT team picked particularly aggressive settings for the drilling operation, expecting the rock to be very hard, and this led to terminating the drilling after only 20 minutes. So they're trying again tomorrow.

The ops teams continue to think about the extended mission, and in fact they're going to try a little of it. A couple of sols from now, they're going to try planning two sols in a single day, which is probably what we'll be doing in extended ops. This should be interesting.

Since I'm not on shift, I relax a little and catch up on the images I've missed. I listen in as Jennifer Trosper laments that Opportunity is getting all the glory; she seems to think it's been that way for some time. Some people seem to have assumed that we never recovered from the anomaly. She relates a question someone recently asked her: "Why don't we hear anything about Spirit? Is Spirit dead now?"

I sigh deeply.

2009-03-02

Spirit Sol 58

Today Ray Arvidson gives the science lecture. He paints it as a justification -- an apologetic one -- for staying at Humphrey for so long. The MTES shows a nice clean basaltic signature on this rock (and lots of others around here). In particular, the MTES shows olivine in Humphrey, but for some reason it's not showing any other basaltic minerals. Maybe they're just being blocked by the dust somehow, but we needed to confirm that by brushing off the dust and looking again. When they did that, the MTES showed exactly the same results. So the next hypothesis was that the layer beneath the dust may be a "rind" -- an indurated surface formed by water vapor, which will block the layers beneath. The next step, then, is the one we're doing now -- drill deeply enough that we'll get through the rind (if there is one) and look again. "This process is not being done just to cause Mickey Mouse signatures," he concludes, "though that was kind of cool ...."

We get the MI images back, and they're not showing what we expected. We had targeted two locations, one a little below and to the right of the Mickey head, and one at the bottom of Mickey's right (stage-right) ear. The images we've gotten back so far show part of a circle in the lower left of the image, as if we were looking at the right-ear image but the arm had drooped more than expected, moving down the rock face to show the right-hand side of Mickey's face instead. This is more droop than we should have seen, so either something is wrong with the arm or something was wrong with the sequencing (which would make it my fault, just to put a point on it).

It's not the worst thing in the world from a science perspective, since the point of the right-ear observation was to see some unbrushed surface, and we do. But it's not nearly as much as we expected: we were expecting more than half of the image to be brushed surface, and this is maybe a tenth. And worse than that, it means that we can't target the instruments correctly because the arm is behaving in ways we don't understand (or it means I really screwed something up, which is bad in a different way).

The scientists are planning a big day for tomorrow. Energy permitting, they'll first RAT the reachable spot, then MB, APXS, and MI that spot -- the entire suite. They start discussing what they'll cut first if energy proves to be a limitation (which won't be surprising: when grinding, the RAT runs for a long time and draws a lot of energy). While they're discussing it, Art Thompson (the TUL for today) comes in to say that we're precluded from using the IDD at all until we fully understand what happened. He promises we'll analyze it and have an answer -- one way or the other -- by the SOWG. I know what this means for me, and hustle to the Mobility/IDD station. As I'm leaving, I hear Art telling them some good news to go along with the bad news: we've changed the way we model power, so we should be able to model more accurately. This will help enormously, because we've had to be more conservative than necessary in our plans as the available daily power budget has decreased.

Jeng is the Mobility/IDD guy for the day, and he fills me in on his concerns. First, there's the MI image that doesn't look like we expected. Second, the joint angles the IDD is reporting don't match up very well with the predictions. It's normal for there to be a difference of less than one degree, due to minor uncertainties in the position of the vehicle, inaccuracies in the terrain mesh, and so on. But the differences he's seeing exceed two degrees.

The first problem already has an answer, which one of the scientists (Doug Ming) and I were working out when Art came in with the bad news. It turns out that it isn't a right-ear image, it's an image from the other placement. The reason we're seeing Mickey's face in it is that the MI field of view is a little wider than we thought: we had thought that it would show unbrushed area only, but when we model it in RSVP and look through the MI, we see almost exactly what's showing up in the real image. So at least as far as that's concerned, we've gone from thinking that the IDD was way off to thinking that it's spot on, and it was only our expectations that were wrong.

The second problem is more troublesome, but yields to analysis in the end. Jeng and Chris and I stare at it for a little while, then we realize that the predicted angles themselves might be wrong. The predictions come out of simulating the sequence in RSVP and recording the angles the simulated rover reaches. But RSVP doesn't model the interaction of the rover and the rock surface -- it cheerfully lets the instruments pass through solid rock. And because of the inherent measurement uncertainties, we always command a slight overdrive, telling the rover to push the instrument to a point that lies inside the rock. (It actually stops moving earlier than that, when switches mounted on the instrument report contact with a solid surface.) Normally, the difference doesn't amount to much, but the IDD happens to be in an unusual pose, in which it takes a lot of shoulder movement to make a small change in the actual position of the instrument tip. When we redo the simulation without an overdrive, the differences subside into the expected range. Again, the IDD was performing splendidly, and only our expectations were wrong.

We breathe a collective sigh of relief, but we repeat the experiment with a couple of other positions just to make sure. In each case the non-overdrive prediction compares well with the actuals. We tell Mark Adler, who looks very, very relieved.

So it turns out to be just one of those things. There happened to be nothing wrong, but what if Jeng had been right? We might have caused severe damage to the vehicle if he hadn't raised the alarm. Being on the downlink team is a tough job: you don't want to panic unnecessarily, but you don't want to ignore real problems, either. Every time anything unusual happens, you get to roll those dice.

With the IDD concerns addressed, the SOWG is free to ratchet up the complexity. Tomorrow, we RAT the rock, then MB and APXS the RATted spot. The following sol, we'll MI it and MB it again (presumably for longer the second time). This will be straightforward, so I start sequencing in the meeting, with the goal of finishing before it ends. But it turns out to be the shortest SOWG meeting ever, at a mere 23 minutes. Oh, well.

I continue sequencing downstairs. Relatively speaking, it's an easy night. We got very amusing email from the staffing office, of all places. Some guy in New Hampshire says he can see spider-like creatures in the Spirit images, at 600x magnification (since the images are 1024x1024, this would be about 1 or 2 pixels). For some odd reason, nobody seems to have replied to his email on the subject. My favorite response to people like this is to tell them that they're absolutely right, and not to let anyone tell them otherwise. (Not that I've ever done this, but I'm always SO tempted.) There's a lot of support for this idea. Art rags on the MI PUL: "If you'd been doing your job, you'd have found this!" He adds that if he'd seen the email earlier, he'd have had the entire SOWG call this guy (whose phone number was included in the email). That would have been some SOWG meeting.

Since it's a slow night, several of us fall to chatting. Art tells a few MER and Pathfinder war stories, as well as some from his Shuttle days. One reason the engineer-scientist relationship on MER is so good, he says, is that Squyres enforced some flight discipline on the scientists from the get-go, so that they have some idea of what the engineering situation is. The scientists normally take a more academic perspective, without taking into account what needs to be done in order for things to work. (Of course, he adds in fairness, this is the engineer's perspective; the scientists would tell the story another way.) On one Shuttle mission, the science team came in and swapped out some circuit boards in one of their experiments without telling anyone. When this was discovered, it caused them to fail a review. They didn't fly that experiment. This is the sort of thing that wasn't allowed on MER, Art says, and it's one reason the scientists understand us better: they know more about what constraints we're under, and that there's a good reason when we tell them no.

Art discloses another interesting MER fact: Justin Maki wanted to put a mirror on the lander, so that the rover could take a picture of itself. They just weren't able to find the right spot, and the idea was eventually abandoned.

Art also mentions, in passing, that some people are talking about a 150-sol total mission (90 nominal, 60 extended). Holy cow! It makes me wonder again whether I'll get to participate in the extended mission.

Word comes that there are a couple of astronauts on the floor. ("Good ones?" I ask. "Or just Shuttle astronauts?" This gets a laugh, but I'm ashamed of it. Well, maybe a little ashamed.[1]) The astronauts attend our activity plan approval meeting, dressed in their blue uniforms. It turns out that Albert Haldemann, one of the scientists, knows one of them -- because he was with them at one point, trying out for the astronaut program. Albert didn't make it, obviously, but he says working on MER is the next best thing.

They discuss tomorrow's big announcement, the water news. Albert jokes: "How many times can we discover water on Mars before people get fed up with us?" I guess we'll find out tomorrow.




Courtesy NASA/JPL-Caltech.






Footnotes:

[1] We're just jealous. You can see how much we love our jobs, but I still doubt you could find three people on MER who wouldn't have instantly dropped everything we were doing in exchange for a single Shuttle flight.

2009-03-01

Spirit Sol 57

I arrive before the downlink data does, beating it by about an hour, so I don't have a lot to do. I help Mark out with something minor and listen to the afternoon science talk, which is discussing "my" trench results. It's nothing I haven't heard by now, though.

When the data does arrive, there's an unpleasant surprise hidden in it: we didn't make it all the way back to the rock, possibly falling short as much as 10 or 15cm. This has the potential to be very bad. The IDD placement was already tricky where we started out, and we knew we were smack in the middle of a 9cm zone that would be favorable for RATting. This means that at a minimum, we needed to return to within 4.5cm of our original position, which shouldn't have been a problem.

Except we'd slipped on the previous sol's drive, probably while backing away from the rock. The mobility/IDD person on shift had noticed this late and put it into his report late -- after I'd read it already, so I didn't account for it in the drive. Which would have been perfectly easy to do, if only I'd known. We slipped about 6cm, which will leave us outside the RAT sweet spot. We yawed a little, too, which may mean that we're in an even worse position for IDDing this rock.

This is going to suck. This was already our second chance, our recovery action. The RAT guys were very concerned about this drive, because they don't think the rest of the science teams will want to hang out here for another sol as we do another bump-drive. So if we've messed this up, there's going to be some bad blood.

To make matters worse, it'll take time to find out. Maybe we're fine, maybe there will be a Congressional investigation. We don't know yet. The ground tools have to process the data for a while, and then humans get involved, and then the ground tools think some more.

Andy reports that the scientists don't want to RAT tomorrow anyway; they want to APXS and maybe MB the area they're going to RAT first. This is for a combination of power, thermal, and science reasons. The placement of these instruments is somewhat less sensitive, so that might be good news: if we need an adjustment drive after all, we might be able to do it late in the day, after the instrument placements. It will mean they won't get an overnight MB, but maybe they can live with that.

I find myself hovering, waiting for things to get to the point where I can evaluate the situation. This isn't going to help, so I join the downlink assessment meeting "already in progress," as they say. They're exploring a lot of possibilities, but they all involve staying put for now -- no Bonneville drives for at least a couple more sols. Ray is eager to know whether we're within RAT range, since this will drive all of their decisions. I start to explain that I was watching that pot and it wasn't boiling, and even as I'm saying this, Mark arrives to say we've got all the data. Ray asks for a definitive answer in time for the SOWG meeting, about an hour away.

We still don't have the terrain meshes I need for planning, but we've got enough for the RAT guys to select a target. They do this. We've lucked out: there's one spot on the rock that should be reachable, and on which we can apply enough preload to get a solid RAT grind. They give me the coordinates of the target, but since we don't have a terrain mesh yet, it's just a point (actually a point/normal) hanging in space. It's enough for me to get started, though, and I start to convince myself that it's all going to work out.

I won't really know until I get the terrain mesh, and that's not showing up. It's probably fine, already in progress, but I have no visibility into MIPL's process for producing them, so I can't say. I don't want to bug MIPL about it, but the RAT guy points out that we had a data dropout early in the pass, in one of the HAZCAM images, and this might screw up the data product and therefore MIPL's automatic pipeline. So I go see if the mesh is in progress, and it turns out it's a good thing I did so. They were waiting for some other data to show up before they started, but I tell them I don't need it and ask for them to start on the HAZCAM mesh, which they do.

(Incidentally. MIPL has a news article posted on the wall; it's the recent AP story that quotes John Wright's description of the rover's traverse behavior: "We go, stop, go, stop, go, stop." They've even blown up the quote and put it next to the article. I think this is a good description, but somehow it's becoming an in-joke. At one point, Andy addresses me in this wise: "O Mighty Rover Planner, Who Goes and Stops and Goes and Stops." I'm pretty stressed at that point, but I can't help it, this makes me laugh.)

The mesh shows up just in time for me to verify (with Frank's help) before the SOWG meeting starts that the sequencing is likely to work with the desired target: we can reach it with all of our instruments, and that's all we really need. Despite the focus on the eventual RATting of this rock, the short term is another matter; tomorrow is dedicated to a pre-RAT APXS and MB. I spend most of the SOWG meeting roughing out the arm motions to make sure I haven't missed anything, but it seems to be OK.

My stress level is slowly dropping, and the sequencing is going well. I brought in cookies as a snack, and now I put them out on the table for everyone; Scott Doudrick does the same with some kind of yummy fudge snack. The consensus is that this is vitally necessary, in order to make up for the sudden recent lack of free ice cream, and both snacks start to disappear.

I finish sequencing and walk around a little to unwind. I hang out with Ashitey for a few minutes, and he tells me he's at last getting a chance to really play with RoSE and thinks it's awesome. "You should get an award," he says. "Seriously. You should get an award." I give him a cookie.