title: Surface energy budget and thermal inertia at Gale Crater: Calculations from ground-based measurements.
abstract: The analysis of the surface energy budget (SEB) yields insights into soil-atmosphere interactions and local climates, while the analysis of the thermal inertia (I) of shallow subsurfaces provides context for evaluating geological features. Mars orbital data have been used to determine thermal inertias at horizontal scales of ∼104m2to ∼107m2. Here we use measurements of ground temperature and atmospheric variables by Curiosity to calculate thermal inertias at Gale Crater at horizontal scales of ∼102m2. We analyze three sols representing distinct environmental conditions and soil properties, sol 82 at Rocknest (RCK), sol 112 at Point Lake (PL), and sol 139 at Yellowknife Bay (YKB). Our results indicate that the largest thermal inertiaI= 452 J m-2K-1s-1/2(SI units used throughout this article) is found at YKB followed by PL withI= 306 and RCK withI= 295. These values are consistent with the expected thermal inertias for the types of terrain imaged by Mastcam and with previous satellite estimations at Gale Crater. We also calculate the SEB using data from measurements by Curiosity's Rover Environmental Monitoring Station and dust opacity values derived from measurements by Mastcam. The knowledge of the SEB and thermal inertia has the potential to enhance our understanding of the climate, the geology, and the habitability of Mars.
authors.affiliation: Department of Atmospheric, Oceanic and Space Sciences, University of Michigan Ann Arbor, Michigan, USA.
authors.forename: G M
authors.initials: GM
authors.lastname: Martínez
authors.affiliation: Department of Atmospheric, Oceanic and Space Sciences, University of Michigan Ann Arbor, Michigan, USA.
authors.forename: N
authors.initials: N
authors.lastname: Rennó
authors.affiliation: Department of Atmospheric, Oceanic and Space Sciences, University of Michigan Ann Arbor, Michigan, USA.
authors.forename: E
authors.initials: E
authors.lastname: Fischer
authors.affiliation: Department of Atmospheric, Oceanic and Space Sciences, University of Michigan Ann Arbor, Michigan, USA.
authors.forename: C S
authors.initials: CS
authors.lastname: Borlina
authors.affiliation: Department of Earth and Space Sciences, University of Washington Seattle, Washington, USA.
authors.forename: B
authors.initials: B
authors.lastname: Hallet
authors.affiliation: Jet Propulsion Laboratory Pasadena, California, USA.
authors.forename: M
authors.initials: M
authors.lastname: de la Torre Juárez
authors.affiliation: Jet Propulsion Laboratory Pasadena, California, USA.
authors.forename: A R
authors.initials: AR
authors.lastname: Vasavada
authors.affiliation: Departamento de Física, Universidad de Alcalá de Henares Madrid, Spain.
authors.forename: M
authors.initials: M
authors.lastname: Ramos
authors.affiliation: Department of Space Studies, Southwest Research Institute Boulder, Colorado, USA.
authors.forename: V
authors.initials: V
authors.lastname: Hamilton
authors.affiliation: Centro de Astrobiología Madrid, Spain.
authors.forename: J
authors.initials: J
authors.lastname: Gomez-Elvira
authors.affiliation: Space Science Division, NASA Ames Research Center Moffett Field, California, USA.
authors.forename: R M
authors.initials: RM
authors.lastname: Haberle
keywords: MSL; Mars; REMS; surface energy budget; thermal inertia