Microwave Thermal Mapping of the Stealth Region on Mars

Anton B. Ivanov, Duane O. Muhleman, Ashwin R. Vasavada

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)

Abstract

Mars was observed at 1.35 cm (22 GHz) with the Very Large Array (VLA) on February 19, 1995. We mapped the thermal emission from the martian surface in the Tharsis and Amazonis regions. Observed variations of microwave brightness temperature were compared with the results of a subsurface thermal model to derive the emissivity and dielectric constant of the soil. The results revealed a region with anomalously high values of emissivity (ε = 0.99 ± 0.01), which is approximately inversely proportional to the density of the material. We interpret this region as having a low density (ρ = 0.5 ± 0.3 gm cm-3) near the surface. It lies within the boundaries of Stealth - the echoless radar feature discovered by Muhleman's radar group in 1991 (Science253, 1508-1513). We suggest two hypotheses for the formation of Stealth. It may consist of ash flows from the nearby Tharsis volcanoes, or it might be an eolian deposit.

Original languageEnglish
Pages (from-to)163-173
Number of pages11
JournalIcarus
Volume133
Issue number2
DOIs
Publication statusPublished - Jun 1998
Externally publishedYes

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