The Mars Phoenix Lander will be the next Martian probe to be land on the Red Planet. Real soon now. As in, on Sunday.

From the Phoenix Mars Mission homepage:
Mars is a cold desert planet with no liquid water on its surface. But in the Martian arctic, water ice lurks just below ground level. Discoveries made by the Mars Odyssey Orbiter in 2002 show large amounts of subsurface water ice in the northern arctic plain. The Phoenix lander targets this circumpolar region using a robotic arm to dig through the protective top soil layer to the water ice below and ultimately, to bring both soil and water ice to the lander platform for sophisticated scientific analysis.
The complement of the Phoenix spacecraft and its scientific instruments are ideally suited to uncover clues to the geologic history and biological potential of the Martian arctic. Phoenix will be the first mission to return data from either polar region providing an important contribution to the overall Mars science strategy “Follow the Water” and will be instrumental in achieving the four science goals of NASA’s long-term Mars Exploration Program.
One of the exciting things about this mission is the Canadian involvement. The Canadian Space Agency has contributed an important package – a weather station.
Canada’s contribution to Phoenix is a meteorological station that will record the daily weather of the Martian northern plains using temperature, wind and pressure sensors, as well as a light detection and ranging (lidar) instrument. The weather station will help improve models of the Martian climate and predict future weather processes, paving the way for future exploration missions. This information may also improve scientists’ understanding of Earth’s dynamic polar regions by comparison between the two planets. Resembling a brilliant green laser, the lidar will probe what is known as the “boundary layer” of the Martian atmosphere (the turbulent layer of the atmosphere about 7-10 km above the surface) and provide information about the structure, composition and optical properties of clouds, fog and dust in the lower atmosphere (up to 20km above the landing site).