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Opportunity's thousand-year-old crater
Posted By Emily Lakdawalla
2010/01/29 10:59 CST
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Since leaving Marquette Island on sol 2,122, Opportunity has been barreling southward on her journey toward Endeavour crater. On her horizon for the last several sols has been a very small but very fresh looking crater named Concepción. Here's how it looked after Tuesday's drive, sol 2,136:

NASA / JPL / mosaic by Emily Lakdawalla
Concepcion crater, Opportunity sol 2136
On sol 2,136 (January 26, 2010), Opportunity approached a small crater that is estimated to be roughly 1,000 years old.
NASA / JPL / mosaic by Emily Lakdawalla
Concepcion crater, Opportunity sol 2138
On sol 2138 (January 28, 2010), Opportunity had approached the small, fresh crater Concepcion close enough to peer into its dust-filled interior.But how old is "fresh?" A recent update on the JPL website said that Concepción is thought to be 1,000 years old. Which immediately makes you wonder -- how did they figure that out? Opportunity has no tools that could figure out the age of a rock from a distance, or, for that matter, in situ. Radiometric age dating is, sadly, something that cannot be done at all (yet) from a spacecraft. So how do we know this thing is 1,000 years old?
I had no idea, but Matt Golombek was kind enough to explain things to me. In an abstract that he and several coauthors will be presenting at this year's Lunar and Planetary Science Conference (here, in PDF format), he explains the process by which they arrived at the age of a different set of craters visited by Opportunity, the so-called "Resolution" cluster. This included craters referred to as Resolution, Adventure, Discovery, and Granbee, which Opportunity visited from sols 1,818 to 1,854. They used three different methods to estimate when the ripples in Meridiani last moved to be approximately 100,000 years ago; and the Resolution cluster is superposed on the ripples with no evidence of being deformed by ripple motion, so it's younger than 100,000 years old.

NASA / JPL / UA
The Resolution cluster of craters
A view from Mars Reconnaissance Orbiter HiRISE down onto the Resolution cluster of craters, which opportunity explored from sols 1820 to 1857. These craters' rays have vanished but the craters themselves are not covered by dunes (unlike the larger crater near the top of this image) so are probably old but not as old as the time when the dunes last moved, estimated to be around 100,000 years ago. The image covers an area 100 meters wide.
Concepcion crater from HiRISE
Concepcion crater is relatively fresh, because it still retains dark rays superimposed upon the Meridiani dunes. However, it is not as fresh as some craters in Meridiani, because it lacks bright rays. It is estimated to be roughly 1,000 years old. Opportunity approached it on sol 2,138. The image covers an area 100 meters square.A general rule for ages in planetary geology: geologists typically think about ages in terms of orders of magnitude, or sometimes even multiple orders of magnitude. When they speak of something that is 1000 years old, that is not to differentiate it from something that is 1,001 or 999 years old -- or even from something that is 2,000 or 500 years old. It is to differentiate it from something that is at least an order of magnitude older or younger, 10,000 or 100 years old. With anything but the Moon, even an order of magnitude is probably more detailed than we know the ages; two orders of magnitude, differentiating among things that are 10 versus 1000 versus 100,000 versus 10,000,000 years old is probably the best we can do.
If absolute age dates are inexact, relative ones aren't. We can use superposing relations of crater ejecta blankets, dune motion, river channel carving, volcanic eruptions, et cetera to determine a very detailed relative sequence of when things happened on Mars, or any other solid-surfaced world -- this flow happened before that crater, which happened before these dunes marched across, and so on. Our estimates of the exact ages of things may change over time as we get better data, but those changes won't (usually) affect our understanding of the relative timing of the events that shaped Mars' surface.
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