You are browsing the archive for ChemCam Archives - Page 2 of 16 - AGU Blogosphere.
20 June 2017
Curiosity continues to drive to the east-northeast around two small patches of dunes that are positioned just north of Vera Rubin Ridge. Once beyond this easternmost dune patch, the plan is for her to turn to the southeast and towards the location identified as the safest place for Curiosity to ascend the ridge.
18 June 2017
As this is my first time contributing to the Curiosity rover blog, I’d like to quickly introduce myself to you all. I’m Mark, an MSL Participating Scientist and a faculty member at Northern Arizona University, trained in geochemistry, spectroscopy, and remote sensing. I’m excited to help walk you all through the daily endeavors of this wonderful rover and mission!
16 June 2017
The drive on Sol 1728 was successful, and our weekend plan will be chock-full of activities. On the first sol, we will do some contact science on the rather colorful workspace that is currently in front of the Curiosity rover.
14 June 2017
After a busy day of contact science yesterday, today’s Curiosity rover plan was dedicated towards remote science and driving. As Mastcam PUL-1 today, I was fairly busy helping put together a suite of Mastcam images for Curiosity to take.
25 May 2017
After Curiosity’s 14.6 m drive, the GEO group decided against arm activities due to a lack of compelling targets and in deference to making the next drive longer. So GEO science activities relied on Mastcam and ChemCam. On Sol 1707, ChemCam will capture a raster of the ‘White Cap Mountain’ bedrock target (the white bedrock left of center in the bottom quarter of the above Navcam image), as well as a …
21 May 2017
The rover planners parked us in front of the one slab of outcrop – an island among ripples of sand – we could safely drive to from our Sol 1700 position, setting us up to continue our exploration of the Murray formation.
18 May 2017
Curiosity continues towards Vera Rubin Ridge with a 48 m drive. GEO decided for the touch-and-go option (instead of lengthening the drive like on Sol 1684) using APXS and MAHLI on “Ripple Pond,” a typical member of the Murray formation.
15 May 2017
The road to Vera Rubin Ridge, a feature believed to be enriched in the mineral hematite, is getting steeper, so we are stopping frequently to study the composition of the bedrock beneath our wheels.
14 May 2017
Curiosity continued her detailed investigation of the interesting suite of outcrops we have been picking our way across during the last week. As we climb up Mount Sharp, recently over slopes of 4-6 degrees, we have seen more varied outcrop structures and chemistries than the rest of the Murray formation, and such changes catch the collective eye of the team.
9 May 2017
After the drive on Sol 1691, the workspace in front of the Curiosity rover had plenty of interesting rocks in front of us to keep us busy.
Today we planned two sols, 1693 and 1694. On the first sol, we will conduct a suite of remote science observations before driving away and resuming our trek up Mount Sharp.
The weekend drive stopped a little bit short of the target, but that’s ok because it put the Curiosity rover in reach of some interesting cross-bedded rocks. We decided to do a “touch and go” plan for Sol 1691, quickly analyzing the rocks in front of us and then continuing on to the original drive destination.
8 May 2017
We’ve been getting some really interesting data down from our investigation of a large sand drift (megaripple), so we packed in many more observations to assess the full variability of the sandy materials before driving away and continuing our climb up Mt. Sharp.
3 May 2017
Continuing the steady march up Mt. Sharp, Curiosity drove 18.3 m to bring us closer to a series of features being called megaripples, which are darker and larger ripples than were seen on the Bagnold Dunes.
2 May 2017
Planning rover science activities is a dynamic process. Unlike yestersol’s plan, the Geology Theme Group decided to include an APXS and MAHLI “touch-and-go” in the plan, carrying out valuable contact science on the layered Murray bedrock.
30 April 2017
After a drive of almost 29 meters, we are parked at a site suitable for a busy plan full of contact science on the Murray formation. GEO focused mainly on characterizing nearby flagstone – “Duck Brook Bridge” was like the typical Murray formation that was tan in color, and “Cliffside Bridge” and “Waterfall Bridge” were more coarse-grained and gray.
27 April 2017
After a 30 meter drive on Sol 1679, we find ourselves near diverse outcrops of the Murray formation. We plan to drive on today across the Murray formation towards Vera Rubin Ridge.
25 April 2017
Our drive yestersol went as planned and added another 28.3 meters to Curiosity’s odometer. The science team was pleased to see that more interesting outcrop would be reachable by Curiosity’s arm from our new location, so we decided to plan contact science followed by an afternoon drive in the Sol 1679 plan.
Curiosity drove another 33 meters on Sol 1677, and again is surrounded by rocky outcrops partly covered by dark sand.
23 April 2017
This morning we woke up to fresh images from Curiosity that showed our surroundings after an ~17 m Sunday afternoon drive. I always really enjoy days like this because, even after 1,676 sols and just under 16.1 kilometers of driving, it still thrills me to look at images from unexplored areas of Mars.