We recently calculated the cost of building and running HiRISE since its inception, and it comes to ~70 million dollars over the last seven years. That sounds like a lot of money to me, but it works out to only 22 CENTS per American! What a bargain! I admit, I’m a little biased, but I think HiRISE’s amazing images, exciting science, and advances in exploration are well worth that investment. The return on that investment isn’t just a matter of the data we get back from Mars – that money goes toward employing engineers, scientists, students, and operations staffers like me. I counted almost 100 people on our team roster that are at least partially supported by HiRISE funds.

Ideally, we’d reach far more than 1,000 people – as “the people’s camera,” we’d love to give every person their 22 cents’ worth. Of course, not everyone uses Twitter, so we try to do other things, like this blog, our website, facebook, on-line learning & activities, and in-person tours and talks.

What else could we be doing? What kinds of things would you like to see us do more of? What’s worth 22 cents to you?

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! ☺

UA job posting website

If you live in Tucson, you might be interested to know that we’re looking for a new HiRISE Targeting Specialist (HiTS) here at HiROC!

Our faithful blog readers are probably already familiar with some of what the HiTS do, but for the rest of you, here are some past entries related to different aspects of the job:

• Welcome, Newbies! – Training other new HiTS
• ESP so far – In the extended mission, things are (supposedly!) easier…
• How big are our feet? – Planning software HiTS use, HiPlan
• High data rate and HiTemp – Some of the challenges of planning images
• Looking Back – Special sequence commanding

I’ve found it to be an exciting and rewarding job, but it’s not an easy one. You need to be the type of person who thrives under pressure; can deal with firm deadlines, but is also creative and self-motivated in between deadlines; pays attention to small details, but can also “see the big picture” (so to speak ). You need to be able to communicate with, and translate between, people with diverse backgrounds and experience, from researchers on the science team to NASA engineers. Ideally, you’d have some relevant scientific background (planetary science, astronomy, or geology, for example), be familiar with UNIX and some programming, and most importantly, be excited about exploring Mars!

To view the complete job description, requirements, and apply online, click this link to the University of Arizona job listing. If you have any questions about the job, please leave them in the comments below!

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.

Artist's rendition of Mars Polar Lander in 3-D

The Unmanned Spaceflight forums have a long discussion on the previous search efforts. Many candidates were proposed, and the community’s discussion about them is quite enlightening.

Emily Lakdawalla at the Planetary Society also started a coordinated search effort last year. I don’t know if that effort is still ongoing, but her page on how to use HiRISE images in the search is still a great resource. It includes examples of known hardware, cosmic ray hits and other artifacts, and more tips on searching.

In addition to the list of images on the previous blog entry, these new images have been released: (we’ll try to keep this list up to date as more are released)

• ESP_013368_1035
• ESP_013078_1030
• ESP_013223_1025
• ESP_013289_1035
• ESP_013566_1025
• ESP_013500_1035
• ESP_013711_1030
• ESP_013724_1030
• ESP_013935_1030
• ESP_013790_1035
• ESP_014001_1040
• ESP_014080_1040

Thanks for all your interest, and good luck searching!

9/2/09: ETA new images released in September PDS release.

It appears that a recent Java patch causes problems launching the IAS Viewer client and other Java-based software launched via Java Web Start. The update changed the location of the Java Web Start application so that the system opens the downloaded JNLP file as a text file, most likely with something called Dashcode. One of our system administrators found a solution on an Apple support discussion archive. You should only have to do this once to fix the problem:

1. Find any *.jnlp file in the Finder. These may be on your Desktop, or in a download folder, depending on how your web browser is configured.
2. Highlight the file by clicking on it, then select ‘Get Info’ from the File menu.
3. In the Open with: section, click on the popup menu and select ‘Other…’.
4. In the file chooser window that pops up, under Devices, pick the hard disk icon that corresponds to the name of your system hard disk (probably has the same name as your computer).
5. From there, select the System folder, then Library, then CoreServices, and scroll down to find the Java Web Start application, select it and click the ‘Add’ button. (Note, the location of Java Web Start application may differ on your system.)
6. Back in the Get Info window, click the button that says change all to apply this change to all of your JNLP files, then close the Get Info window.

When something tries to open a .jnlp file now, it should be properly handled by Java Web Start, launching the corresponding application.

Thanks to one of our twitter followers, @doug_ellison, for pointing out that many of you are having this problem!

Please note, we offer this for informative purposes, and you should make changes at your own discretion.

Governor Janet Napolitano visits the HiROC lobby in February 2006

My favorite part is when people have questions for us – even when I don’t know the answers. Because, honestly, that’s what science is – we don’t always have the answers, but that’s what makes it exciting! It’s also fun to find out which aspects of the mission inspire other people, and I get a different perspective on what they think is interesting (versus just what I think is interesting!). Some of the questions are really good, too! We were talking with some middle-school students from El Paso, Texas, and their questions were so astute. One girl asked, “Does Mars have plate tectonics?” Another good question was, “How do we know about the interior of Mars?” These are great questions, and HiRISE is helping scientists to answer these and other questions, along with data from many other instruments studying Mars.

In case you were curious about these particular questions, like these kids were, here are some short answers and references for more information:

• Does Mars have plate tectonics?

  It doesn’t now, but it might have in the past. The crust of Mars is thicker and stronger than that of Earth, so it’s more difficult to break it apart into plates and start subducting them below one another. However, there is some evidence that Mars may have had active plate tectonics early in its history. Maybe the presence of water in the crust weakened the rock enough to allow plate tectonics. HiRISE is investigating evidence of water in the Martian past, which may help illuminate this issue.

  For more reading:

  1. “Plate Tectonics . . . on Mars” Science News Magazine Volume 155, Number 18 (May 1, 1999) (article)
  2. Sleep, N.H. 1994. Martian plate tectonics. Journal of Geophysical Research 99, 5639. (scientific paper)
  3. Nimmo, F., Stevenson, D.J. 2000. Influence of early plate tectonics on the thermal evolution and magnetic field of Mars. Journal of Geophysical Research 105, 11969-11980. (scientific paper)
• How do we know about the interior of Mars?

  HiRISE and other cameras can only take pictures of the surface of Mars. So how do we know so much about what’s inside the planet? For example, we know that Mars has an upper crust, a mantle, and a dense core, like the Earth.

  One way to see beneath the surface is to use impact craters – they punch holes through the crust and expose deeper rocks. HiRISE has imaged a lot of craters! There is also an instrument on the MRO spacecraft with HiRISE called SHARAD, which uses radar to see buried layers of rock and ice. We know about the deeper interior of the planet from spacecraft that have been orbiting Mars for decades and measuring how gravity, heat flow, and the magnetic field vary over different areas. We can also measure the elevation of different features, and that tells us something about what’s underneath. For example, a tall mountain may have very deep roots that extend into the mantle. Scientists also make theoretical models of the planet based on what we know about the physics and chemistry of how it formed and has evolved. There is still a lot of work to be done in this area, and scientists hope future missions will tell us more about the Martian interior. For example, a seismic

  For more reading:

  1. “Martian Interior” (2007) European Space Agency. (article)
  2. Zuber, M.T. 2001. The crust and mantle of Mars. Nature 412, 220-227. (scientific paper)
  3. Planetary Interiors by W. Hubbard (book, general to all planets)

This is my neighborhood as HiRISE would see it: (Look at all those pools! Tucson is not nearly as dry as Mars )

These are 11×17 PDFs showing cutouts of new releases, so you can print your own posters. Currently these are available for weekly releases starting 3/25/09 – look for more with each week’s new images!

They’re all available on this page. There are also links to the flyers on the individual image pages such as this one: http://hirise.lpl.arizona.edu/ESP_011425_1775 (Look for the “HiFLYER” link in the lower right hand side.)

Enjoy!