Mars' south polar Ar enhancement: A tracer for south polar seasonal meridional mixing

A. L. Sprague, W. V. Boynton, K. E. Kerry, D. M. Janes, D. M. Hunten, K. J. Kim, R. C. Reedy, A. E. Metzger

Research output: Contribution to journalArticle

51 Scopus citations

Abstract

The gamma ray spectrometer on the Mars Odyssey spacecraft measured an enhancement of atmospheric argon over southern high latitudes during autumn followed by dissipation during winter and spring. Argon does not freeze at temperatures normal for southern winter (∼145 kelvin) and is left in the atmosphere, enriched relative to carbon dioxide (CO2), as the southern seasonal cap of CO2 frost accumulates. Calculations of seasonal transport of argon into and out of southern high latitudes point to meridional (north-south) mixing throughout southern winter and spring.

Original languageEnglish (US)
Pages (from-to)1364-1367
Number of pages4
JournalScience
Volume306
Issue number5700
DOIs
StatePublished - Nov 19 2004

ASJC Scopus subject areas

  • General

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    Sprague, A. L., Boynton, W. V., Kerry, K. E., Janes, D. M., Hunten, D. M., Kim, K. J., Reedy, R. C., & Metzger, A. E. (2004). Mars' south polar Ar enhancement: A tracer for south polar seasonal meridional mixing. Science, 306(5700), 1364-1367. https://doi.org/10.1126/science.1098496