ESP_013948_1410, the kind of data we can't wait to get more of!

We are now returning to our normal mode of operations after several long months of being in safe mode. The anomaly on August 26th was the last in a series of computer glitches on board the MRO spacecraft that caused a reboot. The engineering teams have been working incredibly hard to get the anomaly figured out and prevent a possible side-effect from causing really serious problems. While they may not understand the original problem, and there is a chance it may happen again, they’re confident that at least it will not threaten the mission, so they’ve given us the go-ahead to resume normal operations.

Safe mode is a way of running the spacecraft where all of the science instruments are turned off and quiet. We still receive engineering telemetry so we can monitor temperatures and voltages. There are also “survival” heaters that prevent HiRISE from getting too cold in this mode.

During this time, the uplink operations staff has gotten a little restless. (more…)

Ice excavated from the subsurface, by a crater 6m (20 feet) in diameter, sublimates away over the course of the martian summer. Each of these HiRISE images are 35m (115 feet) across and were taken in October 2008 and January 2009.
Image credit: NASA/JPL-Caltech/University of Arizona

An exciting new paper came out in yesterday’s issue of Science magazine, with HiRISE team member Shane Byrne as the lead author. Water ice has been discovered being exposed by fresh Martian craters!

This is exciting for several reasons: first, these are very tiny craters – only a few meters (yards) across. This means they’re not excavating very deep into the crust of Mars. So the ice has to be really shallow – less than a few feet below the surface! Secondly, the location of these craters is surprising – they’re between 40-55 degrees north latitude. This is far from the polar regions, where we’d expect to find ice (for example, where the Phoenix mission landed at 68 degrees north, ice was found by digging down into the dirt).

The third exciting aspect of this ice is its purity. We’d expect this ice to be mixed in with dirt and dust and rock. Instead, we found that it’s 99% pure ice! (Only 1% is dirt mixed in.) This can be measured because we watched the ice disappear over time. By taking repeated images of the same spot, HiRISE got a time sequence as the ice slowly faded. It faded so slowly that it has to be almost all ice – a dirtier mixture would have faded much faster as it sublimated (went directly from a solid to a gas) in Mars’s extremely dry atmosphere.

Speaking of dry atmospheres, this also has interesting implications about the history of the Martian climate – there had to have been more water vapor in the atmosphere in the recent past than we previously thought. We still have lots of questions about how this ice formed, how much of it there is, and how many more of these craters we’ll find. Luckily, we’ve got a long mission ahead of us to explore these issues!

This discovery is also a great example of how the instruments on MRO work together. CTX initially detected these new craters as “dark spots,” and HiRISE followed up to confirm that they’re really impact craters. Some of those HiRISE images revealed some very bright white material, and then CRISM confirmed that material really is water ice. The instruments worked together to accomplish the best combined science. Go team! ☺

Here are some more detailed stories, images, and multi-media:

• Really nice movie with Shane Byrne talking about the discovery and excellent animations showing the locations of the craters and the time-evolution of the ice disappearing: NASA multimedia – then go to “Video Gallery” on the right, and click on “Mars – Exposed”.

• NASA press release, and all of the images and materials from the press conference

• UA news story

We’ve seen many more news stories & blogs – thanks for the interest, everyone! It’s great that everyone thinks this is as exciting as we do! ☺

The HiRISE team met up this summer in Whitefish, Montana. In between meetings, we were also able to take several geologic field trips and hikes. Glacier National Park has many cool (haha) glacial features, of course, and we also learned about some interesting sedimentology that occurred in the ancient geologic past. The patterns we saw in the sedimentary rocks are similar to those discovered by the Mars Opportunity Rover – cross-bedding and festooned ripples that form when sand is laid down under a body of water. The shape and direction of the ripples can tell you how much water was present, how fast it was flowing, and whether it was a river, a lake, or an ocean. These are important questions we’d like to answer about the history of water on Mars.

The park also has wonderful examples of glacial geology. HiRISE has taken images of many features thought to be related to glaciers, so it’s important to understand the terrestrial analogs that lead scientists to think these are evidence of flowing ice on Mars. For example, we hiked along a moraine composed of jumbled rocks the Grinnell Glacier left behind as it flowed downhill. In addition to the remains of the (rapidly disappearing) glacier itself, we also saw typical glacial erosional structures such as U-shaped valleys, hanging valleys, and cirques. For a HiRISE image of cirque-like features, see PSP_005730_1405.

On one of our field trips, we were accompanied by reporter Michael Jamison of The Missoulian. This story was on the front page of the paper the following day:

I thought the story was really good – a quirky (but so are we!) description of why we would want to stare at the rocks in such a magnificent setting, and their relevance to our mission to Mars. We all thought it was funny when he called Alfred McEwen, our Principle Investigator, a “Marsman”!

HiRISE Team in Glacier National Park, in front of a classic U-shaped valley carved by glacial erosion.

Here are a few excerpts from yesterday’s University of Arizona story about our PDS release:

The HiRISE team has so far released a total 26.9 terabytes of data…. That amounts to more data than has been released by all previous deep space missions combined.

“If I showed each HiRISE image for 10 seconds, it would take me about 4 years to show them all,” said UA’s Alfred McEwen, HiRISE principal investigator.

…

Spacecraft motion pushes this electronic array so that it records the view down to Mars’ surface at a ground speed of about 3.2 kilometers per second, or about 7,000 miles per hour.

Skeptics doubted that a technique called “time integration delay,” needed to compensate for extremely short exposure times – about one ten-thousandth of a second per pixel – could produce sharp, unsmeared images.

But the technique has worked “wonderfully well,” thanks to accurate spacecraft pointing and stability and precise exposure time calculations, McEwen said.

Click here for full story.

It seems the landslides in PSP_007338_2640 have caught a lot of attention!

There has been a lot of online and print news coverage: CNN, Time, Fox News, Astronomy, Space.com, New Scientist, National Geographic, and our local Arizona Daily Star, among many others. The New York Times made a really nice slide show that includes the avalanche, the Earth-Moon image, as well as other great images from our big PDS release. Blogs are talking about it (Cumbrian Sky and the Bad Astronomy Blog, to name just two). People over at unmannedspaceflight.com are discussing the avalanches a lot, too. (I’m sure there are tons I’ve missed – apologies – if you feel left out, post it in a comment below!)

A co-worker heard NPR’s Wait, Wait, Don’t Tell Me featured a question about the avalanches on Saturday. It was even the Astronomy Picture of the Day yesterday!

I’ve talked personally to a lot of people about it, too. It’s amazing how it’s caught everyone’s interest. I think most people who see it for the first time have the same “Holy crap!” reaction that we all had when we first saw it here at HiROC. Then they start trying to figure out what’s going on, what caused it, what it means, how we can take more data and look at past images to narrow down different hypotheses… which is exactly the process that scientists go through!

The best part of the story, I think, is how the landslide was serendipitously captured in an image, and then accidentally noticed! HiRISE has sent back such an incredible volume of highly detailed data, no one person has time to study it all in full resolution. We’ve released 17 Terabytes, thousands of images, and it’s very likely that more surprises like this are waiting to be discovered in them. So go look at more HiRISE images; let us know what you find! We can’t wait to see how Mars can surprise us further.

Thanks for being as excited about HiRISE and Mars as we are!

Saturday’s front-page of the Arizona Daily Star featured a good article about HiRISE with a humorous photo of Chris S. shoulder surfing as Anjani P. worked.

This is of course a typical scene as these images are coming down. Someone will be “driving”, so to speak: browsing, “surfing”, zooming, panning, contrast stretching and more, using the amazing image processing tools that our partners at the USGS in Flagstaff have developed. And someone else (or two, or three, or a dozen) will be standing over their shoulders, watching and collaborating. Or in Chris’s case, probably making jokingly snide comments.

But it makes for a world of difference between what you, out there, the public, experience and what we experience. Bridging that gap is a challenge for our public outreach team as the mission continues. We’ve got the benefit of having the brightest minds in planetary geology offering live commentary and analysis using the finest tools and top-of-the-line workstations. The experience of seeing the image is very dynamic; jumping between resolutions, zooming in to dunes and boulders and rocky outcrops, “stretching” the image to pull out detail hidden in dark shadow or blended in on bright surfaces.

I guess what I’m trying to say is that while our excitement is evident from the posts here, communicating exactly why we’re excited is much more difficult. Unless you could be here shoulder surfing….