The Haughton-Mars Project: Overview of science investigations at the Haughton impact structure and surrounding terrains, and relevance to planetary studies

The Haughton impact structure (23 km in diameter) on Devon Island, High Arctic, has been the subject of a number of scientific investigations since its identification as an impact structure in the early 1970s (see Grieve 1988 for a summary). Due to its near polar location (75.2°N, 89.5°W), Haughton...

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Bibliographic Details
Main Authors: Pascal Lee, Gordon R. Osinski
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
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Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.471.7911
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Summary:The Haughton impact structure (23 km in diameter) on Devon Island, High Arctic, has been the subject of a number of scientific investigations since its identification as an impact structure in the early 1970s (see Grieve 1988 for a summary). Due to its near polar location (75.2°N, 89.5°W), Haughton has experienced a predominantly cold and relatively dry climate throughout most of its history, and is for this reason exceptionally well preserved considering its age (~39 Ma). While by no means subject to environmental conditions as extreme as those encountered on Mars at present, the structure’s general climatic setting in a terrestrial polar desert (annual average temperature is –16 °C; annual precipitation is <13 mm)—including the implied continuous permafrost underlying its terrains—and the presence of a number of other geologic features at or near the crater that bear possible relevance to Mars, make the site attractive as a potential analog for Mars (Lee 1997). Haughton is the only terrestrial impact structure known to be set in a polar desert. In 1997, a pilot study was initiated to visit Haughton with an eye towards comparative planetary studies (with focus on Mars) and a small field party of four deployed to Devon