The Phoenix Mars Lander carrying the Canadian meteorological station (also known as MET) and the lidar instrument landed in the Martian North Pole on May 25, 2008, after a journey almost ten-month long. The first mission ever to land in the Martian Arctic region revealed the presence of water ice on the Red Planet and also provided scientists with a complete set of meteorological data. One year later, atmospheric scientists are still analyzing all the data beamed back by Phoenix. We caught up with Dr. Vicky Hipkin, MET mission scientist for the Canadian Space Agency, who is now working with her colleagues on the Canadian science team using MET data to improve atmospheric models of the Mars water cycle.
We were mostly interested in pressure and temperature measurements, which would indicate seasonal trends. So far, there had been very few meteorological measurements made on Mars. Phoenix was only the fourth Martian weather station, and it was the first one in the Arctic. We were looking for anything new and some confirmation of phenomena we had noticed before like the formation of clouds.
The detection of snow is the MET's major discovery. Thanks to the Canadian lidar instrument, we were able to observe snowfall above Phoenix's landing site. We also discovered that Martian clouds do form much closer to the ground than we expected. The lidar also gave wonderful data about the height and the thickness of these low clouds.
We are still investigating the seasonal changes, and we have got a lot of new experiments to look at in our data interpretation. Given this new information and these new discoveries, we are now working on new models of Mars' atmosphere. We are testing these models and making sure that they correspond with the newly acquired data. We can then look at the impact of these results on our past climate predictions. In fact, the data gathered on the formation of clouds does affect our models in regards to the distribution of water on Mars. It is still very early to talk about any results. We are currently working on an article that will be published in a scientific journal this summer.
The more we discover, the more interesting Mars becomes! We've been exploring Mars with the goals of understanding its climate and searching for life. We have made encouraging discoveries that hint at the possibility of Mars being able to support microbial life. The kinds of things we're seeing with the discovery of methane, habitable properties of the soil and the finding of new ice reservoirs towards the middle latitudes can only help making it a friendlier environment for biology. Upcoming missions will most certainly build up on Phoenix's discoveries. We're advancing the story, but it just makes Mars more interesting!
Following a rapid descent, the three legs of the Phoenix Lander touched down on the soil of the Martian arctic. Just hours after landing, the lander began to relay images to Earth via MRO. After a few days of testing and calibration, Phoenix began to use its laboratories and the Canadian weather station. (Photo: NASA/JPL/CalTech)
In this mosaic of images, the weather MET mast is almost at the centre with the lidar to its left. The two Canadian instruments deployed on Phoenix are at work gathering meteorological data. (Photo: NASA/JPL/CalTech)
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Phoenix's Canadian-built lidar shot rapid pulses of light into the atmosphere, which bounced off the passing clouds and dust overhead. The data now helps determine the composition, movement, height and size of the clouds and particles above the lander. Note that the lidar is wrapped in its white thermal blankets bearing the Canada wordmark. (Photo: NASA/JPL/CalTech)
Phoenix took this picture of its underbelly using the camera mounted on its robotic arm. It discovered a white substance that was found to be ice-water. The white patch was uncovered when the surface soil was blown away during Phoenix's landing. The discovery of ice-water on Mars was one of the key goals of the Phoenix Mars Lander mission. (Photo: NASA/JPL/CalTech)
Phoenix opened its eyes and sent us the first live images from the Martian arctic. The soil is marked by polygon-shaped fissures that could be linked to the past presence of water. An increase in temperature would have caused the fissuring of the soil by evaporating the water it contained. These polygon-shaped structures are similar to those seen in certain parts of the western Canadian Arctic, which are primarily caused by the freeze/thaw cycle. (Photo: NASA/JPL/CalTech)