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The Planetary Society BlogBy Emily LakdawallaBringing MOLA altimetry tracks into Google MarsAug. 27, 2010 | 15:02 PDT | 22:02 UTC
I've had a fun morning of noodling around learning how to write KML files, and have produced one for Google Mars that shows you all of the Mars Orbiter Laser Altimeter tracks that cross the area Opportunity has driven through already, as well as the area of Endeavour crater. For the 5% of you who have any idea what I'm talking about and any understanding of why I would want to do this, here's a link to the KML file and a screen grab from Google Mars showing it in action. For the rest of you, I'll explain below what I did and why it was a worthwhile use of my time!
What are Mars Orbiter Laser Altimeter ground tracks? Mars Orbiter Laser Altimeter -- MOLA, for short -- was one of the science instruments on Mars Global Surveyor, which orbited Mars for nine years, from 1997 to 2006. It's a pretty simple experiment to explain: it consisted of a laser that fired flashes of light at the surface and watched for the reflected flash. By timing the delay between the initial and reflected flashes and multiplying by the speed of light and dividing by two, the MOLA team calculated the range to the planet. That information, combined with precise tracking data, permitted the MOLA team to compute Mars' global topography to very high precision. The altitude measured at each shot point was precise to within 37 centimeters, and shot points were separated along the spacecraft's orbital path by about 300 meters. Here's the resulting MOLA map of Mars:
Why do I want to bring the MOLA ground tracks into Google Mars? That global digital terrain model is really valuable for looking at the topography of vast landscapes, but when you really want to look at detailed topographic information for small-scale features -- like, say, the elevation changes encountered by the Mars Exploration Rover Opportunity during its kilometers-long traverse across Meridiani Planum -- this map is simply not good enough. You need to dig in to the original MOLA data, which consists of latitude, longitude, altitude triples. (Actually there's more information than that, but latitude, longitude, and altitude is the part of the data that I need.) If I zoom in on Opportunity's path, you can see why this is important. This screen cap shows Opportunity's path as mapped by Eduardo Tesheiner in red. In orange and yellow are Mars Global Surveyor ground tracks; some tracks were on the ascending branch of the circlar orbit and some were on the descending branch, which is why they cross. The ground tracks are labeled with the locations and altitudes of individual MOLA shot points. (The altitudes here are negative numbers; elevation is relative to Mars' mean, and the rovers were constrained to land at low-elevation locations to give them longer paths to decelerate through the atmosphere.) The shot points are mostly very evenly spaced along each track at 300 meters apart. But in the cross-track direction -- going from east to west -- the spacing is very uneven, and in some places the tracks are several kilometers apart. What you're looking at is MOLA's cross-track resolution at its worst. Mars Global Surveyor was a polar orbiter, so the ground tracks crossed near the poles. Near the equator (another constraint for the rovers was that they had to land near the equator, to maximize output of their solar panels), the tracks are spaced at their widest.
The first thing you have to do is to get the MOLA data. When I was in grad school and MOLA was active, this was a very tedious process. Now, though, it's very, very easy, thanks to the Geosciences Node of the Planetary Data System. To get MOLA data, the first thing you should do is figure out what part of Mars you want to get MOLA data for. That's most easily done in Google Mars. Identify a latitude/longitude box -- minimum and maximum latitudes and minimum and maximum longitudes. Then go to the Geosciences Node's Mars Orbital Data Explorer and click on "MOLA PEDR Query." The query tool is pretty self-explanatory. Put in your min and max latitude and longitude values in the "Step 1" dialog box; you may need to add 360 to longitudes determined from Google Mars, which measures longitude from -180 to 180 rather than 0 to 360. Skip Step 2. Then click the "Query Count" button under step 3. It'll let you know how many MOLA shots are in the latitude and longitude box you checked. Once you've done that, you can download the data by using one of the "Generate Files" buttons. I used CSV format, which opens readily in Excel, and it worked fine except that the column headers were messed up -- but that's easy to fix manually.
Nowadays, excellent stereo coverage by the Mars Reconnaissance Orbiter CTX and HiRise cameras are resulting in much more detailed topographic information for landing sites on Mars than even MOLA afforded. But even with beautifully detailed digital terrain models derived from those high-res cameras, MOLA will remain important, because its accuracy across all of Mars allows scientists to tie the high-res digital terrain models derived from single images, which only produce relative elevation information (elevation change within the image), into regional elevation maps with precise absolute altitude information.
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CommentsHoly MOLA, that crater is _deep_!
#1 - Torbjörn Larsson, OM - 08/27/2010 - 15:25
It is! That plot really helps give you a sense of the scale of it, thanks!
#2 - Tim - 08/28/2010 - 00:56
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