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Dielectric Permittivity Measurements of Geologic Samples at Venus Surface TemperaturesSynthetic-aperture radar (SAR) and radar sounding are two powerful remote sensing techniques used to examine the surface and subsurface of planets. Their value is critical in the case of Venus due to this planet’s global and visually opaque cloud layer. The recently selected VERITAS and EnVision orbital missions, slated to study the planet in the early 2030’s, employ radar instruments to image the surface (VERITAS and EnVision) and probe the subsurface (EnVision). For both techniques, the complex dielectric permittivity of the surface and subsurface materials control radar backscatter intensity and penetration depth.

Since the 1970’s, many studies have characterized the dielectric permittivity of geologic materials collected both on Earth and on the Moon to constrain the radar reflectivity and transparency at a variety of radar frequencies [e.g., 1]. Two consistent findings from those studies are that complex permittivity depends on both the density (or porosity) and the composition of the material. Denser materials and more metal-rich compositions tend to have higher permittivity values and to incur greater propagation path loss. Water content also elevates permittivity of otherwise dry rocks/soils/regolith [e.g., 2]. However, permittivity is independent of frequency for the 0.5-18 GHz range, within which SAR imaging commonly lies. The one aspect poorly explored thus far is the effect of elevated temperatures on dielectric permittivity. Previous work suggests that increased lattice vibrations and flow of free electrons associated with an increase in temperature elevate both the real (reflectivity) and imaginary (path loss) parts of the complex permittivity.

We are currently conducting a 3-year campaign to measure the complex dielectric permittivity of Venusrelevant geologic materials at Venus surface temperatures (380°C - 460°C) and with frequencies relevant to VERITAS, EnVision, and Magellan imaging synthetic aperture radars.
Document ID
20240000300
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
M Barmatz ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
D C Nunes
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
J Batres
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
M Gilmore ORCID
(Wesleyan University Middletown, Connecticut, United States)
D Steinfeld
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
J Filiberto ORCID
(Johnson Space Center Houston, United States)
Date Acquired
January 9, 2024
Publication Date
March 11, 2024
Publication Information
Publisher: Lunar and Planetary Institute
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 55th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 11, 2024
End Date: March 15, 2024
Sponsors: Lunar and Planetary Institute, National Aeronautics and Space Administration
Funding Number(s)
WBS: 811073
CONTRACT_GRANT: 80NM0018D0004
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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