Scientific Colloquium
November 22, 2013

NOTE: BUILDING 34, ROOM W150


"Mars: Periglacial Morphology and Ice Stability"

At the Mars Phoenix landing site and in much of the martian northern plains, there is ice-cemented ground beneath a layer of dry permafrost. Unlike most permafrost on Earth, though, this ice is not liquid at anytime of year. However, in past epochs at higher obliquity the surface conditions during summer may have resulted in warmer conditions and possible melting. This situation indicates that the ice-cemented ground in the north polar plains is likely to be the most recently habitable place on Mars as near-surface ice likely provided adequate water activity ~5 Myr ago. The possibility of life on Mars is important both for Mars science (Science Mission Directorate (SMD) and Mars Exploration Program Analysis Group (MEPAG) goals and objectives) as well as preparation for human exploration (Human Exploration and Operations Mission Directorate (HEOMD) and Strategic Knowledge Gaps (SKGs) pertaining to biohazards and planetary protection).

The high elevation Dry Valleys of Antarctica provide the best analog on Earth of martian ground ice. These locations are the only places on Earth where ice-cemented ground is found beneath dry permafrost. The Dry Valleys are a hyper-arid polar desert environment and in locations above 1500 m elevation, such as University Valley, air temperatures do not exceed 0įC. Thus, similarly to Mars, liquid water is largely absent here and instead the hydrologic cycle is dominated by frozen ice and vapor phase processes such as sublimation. These conditions make the high elevation Dry Valleys a key Mars analog location where periglacial processes and geomorphic features can be studied in situ.
This talk will focus on studies of University Valley as a Mars analog for periglacial morphology and ice stability. We will discuss observations revealing a unique trend as the depth to ice-cemented ground varies linearly from near zero at the head of the valley to over 80 cm deep 1.5 km away at the valley mouth. This setting provides a natural gradient in physical permafrost properties, water vapor transport, and ice stability. We will also discuss geomorphic ramifications of this ground ice distribution as polygon size is shown to increase down the length of the valley and is correlated with increasing ice depth. Since polygons are long-lived landforms and observed characteristics indicate no major fluctuations in the ice-table depth during their development, the University Valley polygons have likely developed for at least 104 years to achieve their present mature-stage morphology, and the ice-table depth has been stable for a similar length of time. In addition, we will discuss geomorphic features (e.g., rock weathering and erosion, thermal contraction, sublimation till) as possible diagnostics for subsurface ice type. Finally, we will review a landing site selection study encompassing this information gleaned from the Antarctic terrestrial analog studies plus Mars spacecraft data analysis to identify candidate landing sites for a future mission to search for life on Mars.

About the speaker:

Dr. Jennifer Heldmann is currently a research scientist working in the Division of Space Sciences and Astrobiology at NASA Ames Research Center in Moffett Field, California. She has a Bachelorís degree in Astrogeophysics from Colgate University, a Masterís degree in Space Studies with a Minor in Geology, and a Ph.D. in Planetary Science from the University of Colorado at Boulder.

Heldmannís scientific research interests focus on studies of the Moon and Mars. Her Mars research focuses on studies of recent water on the Red Planet through spacecraft data analysis, numerical modeling, and fieldwork in Mars-analog environments such as the Outback of Australia, the Canadian High Arctic, the Atacama Desert, Spitsbergen, the Mojave Desert, and Antarctica. Water is especially important to understand climate, geology, and the potential for past and/or present life on Mars. She is also involved in planning for the future human exploration of Mars and has served on several MEPAG (Mars Exploration Program Analysis Group) special action teams for defining precursor activities needed to enable future human exploration of Mars. (e.g. Human Exploration of Mars Science Analysis Group, Mars-Forward Lunar Objectives Special Action Team, Analysis of the Precursor Measurements of Mars Needed to Reduce the Risk of the First Human Missions to Mars, Precursor Science Analysis Group).

Heldmann also studies the Moon with a focus on improving our understanding of lunar volatile deposits. Such studies are important scientifically in terms of Solar System evolution and also are relevant for planning future human exploration of the Moon through the identification of materials that can be used for in situ resource utilization (ISRU). She recently served on the Science Team, Payload Team, and as the Observation Campaign Coordinator for NASAís Lunar Crater Observation and Sensing Satellite (LCROSS) mission to study the permanently shadowed regions of the lunar poles. LCROSS successfully impacted the Cabeus crater at the lunar south pole and confirmed the presence of water ice as well as numerous other volatile species on our Moon. She is now working on the Resource Prospector Mission concept to send a rover to the Moon to investigate the distribution and nature of polar volatiles.

Heldmann has written numerous scientific papers and book chapters and is the recipient of numerous NASA Achievement Awards including a NASA Headquarters Special Act Award, NASA Ames Honor Award, and multiple NASA Group Achievement Awards. She has been featured in multiple public venues discussing Moon and Mars research (NPR, History Channel, National Geographic, etc). She is committed to education and public outreach and is keen to inspire the next generation of scientists and explorers by sharing the excitement of Solar System exploration with students, teachers, and the general public whenever possible.


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