H2O at the Phoenix Landing Site

Phoenix Ascending The Phoenix mission landed on Mars in March 2008 with the goal of studying the ice-rich soil of the planet's northern arctic region. Phoenix included a robotic arm, with a camera attached to it, with the capacity to excavate through the soil to the ice layer beneath it, scoop up soil and water ice samples, and deliver them to a combination of other instruments—including a wet chemistry lab and a high-temperature oven combined with a mass spectrometer—for chemical and geological analysis. Using this setup, Smith et al. (p. 58) found a layer of ice at depths of 5 to 15 centimeters, Boynton et al. (p. 61) found evidence for the presence of calcium carbonate in the soil, and Hecht et al. (p. 64) found that most of the soluble chlorine at the surface is in the form of perchlorate. Together these results suggest that the soil at the Phoenix landing site must have suffered alteration through the action of liquid water in geologically the recent past. The analysis revealed an alkaline environment, in contrast to that found by the Mars Exploration Rovers, indicating that many different environments have existed on Mars. Phoenix also carried a lidar, an instrument that sends laser light upward into the atmosphere and detects the light scattered back by clouds and dust. An analysis of the data by Whiteway et al. (p. 68) showed that clouds of ice crystals that precipitated back to the surface formed on a daily basis, providing a mechanism to place ice at the surface. A water ice layer was found 5 to 15 centimeters beneath the soil of the north polar region of Mars. The Phoenix mission investigated patterned ground and weather in the northern arctic region of Mars for 5 months starting 25 May 2008 (solar longitude between 76.5° and 148°). A shallow ice table was uncovered by the robotic arm in the center and edge of a nearby polygon at depths of 5 to 18 centimeters. In late summer, snowfall and frost blanketed the surface at night; H2O ice and vapor constantly interacted with the soil. The soil was alkaline (pH = 7.7) and contained CaCO3, aqueous minerals, and salts up to several weight percent in the indurated surface soil. Their formation likely required the presence of water.

[1]  F. Daerden,et al.  Mars Water-Ice Clouds and Precipitation , 2009, Science.

[2]  D. Ming,et al.  Detection of Perchlorate and the Soluble Chemistry of Martian Soil at the Phoenix Lander Site , 2009, Science.

[3]  D. Ming,et al.  Evidence for Calcium Carbonate at the Mars Phoenix Landing Site , 2009, Science.

[4]  A. Zent A historical search for habitable ice at the Phoenix landing site , 2008 .

[5]  R. Morris,et al.  Geomorphologic and mineralogic characterization of the northern plains of Mars at the Phoenix Mission candidate landing sites , 2008 .

[6]  M. Mellon,et al.  A prelanding assessment of the ice table depth and ground ice characteristics in Martian permafrost at the Phoenix landing site , 2008 .

[7]  Allan I. Carswell,et al.  Lidar on the Phoenix mission to Mars , 2008 .

[8]  Paul S. Smith,et al.  Mars Exploration Program 2007 Phoenix landing site selection and characteristics , 2008 .

[9]  M. Mellon,et al.  Periglacial landforms at the Phoenix landing site and the northern plains of Mars , 2008 .

[10]  Raymond E. Arvidson,et al.  NASA Mars 2007 Phoenix Lander Robotic Arm and Icy Soil Acquisition Device , 2008 .

[11]  Carol R. Stoker,et al.  Introduction to special section on the Phoenix Mission: Landing Site Characterization Experiments, Mission Overviews, and Expected Science , 2008 .

[12]  M. Mellon,et al.  Vertical distribution of hydrogen at high northern latitudes on Mars: The Mars Odyssey Neutron Spectrometer , 2007 .

[13]  D. Fisher A process to make massive ice in the martian regolith using long-term diffusion and thermal cracking , 2005 .

[14]  Jacques Laskar,et al.  Long term evolution and chaotic diffusion of the insolation quantities of Mars , 2004 .

[15]  M. Zuber,et al.  CO2 Snow Depth and Subsurface Water-Ice Abundance in the Northern Hemisphere of Mars , 2003, Science.

[16]  Robert M. Haberle,et al.  Orbital change experiments with a Mars general circulation model , 2003 .

[17]  Robert L. Tokar,et al.  Global Distribution of Neutrons from Mars: Results from Mars Odyssey , 2002, Science.

[18]  P. A. J. Englert,et al.  Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits , 2002, Science.

[19]  Bruce M. Jakosky,et al.  The distribution and behavior of Martian ground ice during past and present epochs , 1995 .

[20]  B. Murray,et al.  Behavior of Carbon Dioxide and Other Volatiles on Mars , 1966, Science.