Category Archives: Mars Reconnaissance Orbiter

Tectonically Speaking

It Looks Like Mars Has Plates!

Remember back in geology class when we all learned about plate tectonics on Earth?  The continents and oceans of our planet ride along on crustal plates that jostle against each other like huge cracked regions in an eggshell, and in some places, dive under each other toward the mantle of our planet.  Those motions set off earthquakes, which you’ve probably heard about along such places as the San Andreas Fault in California.

The interior part of the Valles Marineris on Mars. Courtesy NASA.

Well, for the longest time, geologists and planetary scientists figured that Earth was the only planet we know about with plates.  Except now it turns out that Mars has a very primitive form of plate tectonics that are likely responsible for the formation of the huge Valles Marineris canyon system on the Red Planet.  UCLA scientist An Yin has discovered these plates by analyzing satellite images from the  THEMIS (Thermal Emission Imaging System), an instrument on board the Mars Odyssey spacecraft, and from the HIRISE (High Resolution Imaging Science Experiment) camera on the Mars Reconnaissance Orbiter.

Dr. Yin compared what has been found on Mars with studies done in the Himalayas and in California. There are striking similarities between the fault systems seen in these regions on Earth with canyons on Mars, which has a linear volcanic zone typical of plate tectonics.

In particular, the Valles Marineris region on Mars now appears to be an obvious product of plate tectonics, rather than just a crack opening up on the surface of the planet as scientists once thought. Yin suspects that this famous canyon system on the Red Planet is really a plate boundary that experiences horizontal motion. That’s similar to the motion along Earth’s San Andreas Fault, which periodically causes earthquakes.  The two plates divided by the Valles Marineris have moved approximately 93 miles horizontally relative to each other, according to Yin. By comparison, the San Andreas has moved about  twice as much, and the motions are comparable in type.

On Earth, the huge powerhouse of our core and mantle provide energy to move the plates around actively. Mars, on the other hand, doesn’t have as much activity at its core, which means that it likely has fewer plates and motions than Earth does.  This primitive state of Red Planet plate tectonics also means that Mars has quakes, just not as often as Earth does.

These days, Mars exploration is all the rage again, with the daily news and views from Curiosity, Opportunity, and the orbiters at the Red Planet sending back a constant flow of images and data. Discoveries of things like Martian plate tectonics are a natural outcome of all this Mars exploration. Not all discoveries get made overnight. Sometimes it takes years for scientists to get enough data and perspective to crystallize their findings. I’m excited to find out just what else we’re going to learn about Mars now and on into the future!

Speaking of exploring Mars, there’s a nifty 3D exploration of Mars that you can do right at your computer. Check out this view from Mars Day 2 from Curiosity.  I just spent some time playing with it, and I feel like I’ve just come back from a little Red Planet field trip.

 

 

It’s Windy on Mars!

Dust Devils Just Keep on Dancing Across Mars

Okay, a few weeks ago we had a week’s worth of high winds where I live, typical for Colorado in the late winter.  We call ’em Chinook winds, and they tend to dry things out as they blow at speeds upwards of 70 to 90 mph (112-144 km/hour) and gusts up above 100 (160 km/hr).  That’s all part of a weather pattern that occurs here, and in other parts of the world as the seasons change.  Right now, as we saw in Texas a few days ago, the winds and the associated weather patterns whip up twisters, tornadoes, dust devils.

The winds blow on Mars, too, and the Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) camera has been very good at spying out Martian dust devils.  Unlike a tornado which we see here on Earth, a dust devil typically forms on a clear day when the ground gets heated by the Sun. That warms the air just above the ground, and that air rises quickly through a small pocket of cooler air above it. If the conditions are just right, the air can start to rotate, and as it does, it picks up dust.  This is a  frequent occurrence on Mars.

HiRise view of a dust devil on Mars, taken March 14, 2012. Courtesy NASA/HiRise Team.

On March 14th, HiRISE caught sight of a Martian dust devil roughly 12 miles high (20 kilometers) whirling through a region called Amazonis Planitia.   The dust devil about (70 yards, or just about 70 meters across). The image was taken during late northern spring, two weeks short of the northern summer solstice, a time when the ground in the northern mid-latitudes heats up in the sunlight.

One of the cool things about these dust devils is that they scour the ground of dust, leaving behind a thin, sinuous little path. When those little paths were discovered, their appearance and cause was unknown. It didn’t take long for scientists to connect them with the appearances of dust devils. It appears that these dust devils are one mechanism by which dust gets redistributed around the Martian surface.

Check out the full story and a very cool animation showing what the dust devil might look like from the side at the NASA Mars Reconnaissance Orbiter page. It’s full of wooty Mars goodness!  And, if you experience winds and dust devils where YOU live on Earth, then you have a good idea of what it’s like on Mars when one goes twisting by!