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Pebbles before mountains

Written by  Tuesday, 18 January 2022 06:02
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Pasadena CA (JPL) Jan 14, 2022
NASA's Mars 2020 mission team has been working methodically and thoroughly, making good progress on understanding the best path forward to remove the uninvited pebbles from Perseverance's bit carousel. Over the previous weekend, and earlier this week, operational sequences were developed and tested to remove these rocky interlopers. With terrestrial experimentation complete, we have begun

NASA's Mars 2020 mission team has been working methodically and thoroughly, making good progress on understanding the best path forward to remove the uninvited pebbles from Perseverance's bit carousel. Over the previous weekend, and earlier this week, operational sequences were developed and tested to remove these rocky interlopers.

With terrestrial experimentation complete, we have begun executing our mitigation strategy on Mars. On Jan. 12 we did a detailed image survey of the ground below Perseverance. This was done so we would have a good idea what rocks and pebbles already exist down there before some more - from our bit carousel - join them in the not-so-distant future.

With this below-chassis, preliminary imaging, in hand, the team embarked on a maneuver with our robotic arm I never imagined we would perform - ever. Simply put, we are returning the remaining contents of Sample Tube 261 (our latest cored-rock sample) back to its planet of origin. Although this scenario was never designed or planned for prior to launch, it turns out dumping a core from an open tube is a fairly straightforward process (at least during Earth testing). We sent commands up yesterday, and later on today the rover's robotic arm will simply point the open end of the sample tube toward the surface of Mars and let gravity do the rest.

I imagine your next question is, "Why are you dumping out the contents of the sample tube?" The answer is that, at present, we are not certain how much cored rock continues to reside in Tube 261. And while this rock will never make my holiday card list, the science team really seems to like it. So if our plans go well with our pebble mitigation (see below), we may very well attempt to core "Issole" (the rock from which this sample was taken) again.

Which brings me to next steps in our pebble mitigation strategy: we're sending up commands to the rover later today, ordering it to do two rotation tests of the bit carousel. These tests (the first, a small rotation; the second, larger) will execute this weekend. Our expectations are that these rotations - and any subsequent pebble movement - will help guide our team, providing them the necessary information on how to proceed. Still, to be thorough, we are also commanding the rover to take a second set of under-chassis images, just in case one or more pebbles happen to pop free.

We expect the data and imagery from these two rotation tests to be sent to Earth by next Tuesday, Jan. 18. From there, we'll analyze and further refine our plans. If I had to ballpark it, I would estimate we'll be at our current location another week or so - or even more if we decide to re-sample Issole.

So there you have it. The Perseverance team is exploring every facet of the issue to ensure that we not only get rid of this rocky debris but also prevent a similar reoccurrence during future sampling. Essentially, we are leaving no rock unturned in the pursuit of these four pebbles.


Related Links
Perseverance Mars 2020
Mars News and Information at MarsDaily.com
Lunar Dreams and more

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MARSDAILY
Perseverance set to exit Seitah area
Pasadena CA (JPL) Jan 10, 2022
While many reflect on the past and bid it farewell, there's a lot of exciting science to come in the next year. While many were enjoying the days between the Christmas and New Year holidays in the US, at JPL we were working to finish up sampling activities at Issole. We'll soon bid an Auld Lang Syne to the Seitah region. As lead Mapping Specialist, I get enjoy looking at the road ahead for the rover. We'll start be looping back around Seitah east, following our path back towards the Octavia E. But ... read more


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