Mars Polar Layered deposits. Observations from the THEMIS investigation Anton B. Ivanov, THEMIS team JPL HEND Workshop, IKI Марсианские полярные слоистые отложения. Спектральная съёмка камерой THEMIS. А. Б. Иванов, команда THEMIS Лаборатория Реактивного Движения HEND Workshop, ИКИ

Polar research and THEMIS*  What is the composition, structure and chronology expressed in the stratigraphy of the polar deposits? yThickness, extent, and continuity of layers. yComposition, structure, and ice- and dust-grain characteristics of layers. yHistory and origin of the re-entrant troughs ySeasonal behavior of surface seasonal and residual ice caps. *After results of the First Polar Conference (Clifford et al.[2000])

Polar caps – the MOLA view North Pole to 54NSouth Pole to 54S

Polar caps – the MOLA view

THEMIS Characteristics zTHEMIS as spectrometer y“usability” for polar observations, note cold spots yT11, T20, T25, (Kieffer/Titus (TES/IRTM), Forget (IRTM) ) zTHEMIS as a imager yTHEMIS context - MOC WA/Viking - THEMIS - MOC NA

THEMIS IR bands THEMIS Calibration report. Figure 7-6 THEMIS IR camera has 10 bands from 6.62 µ m to µm Band 9 (12.58) is the most useful for polar studies.

THEMIS sensitivity zThis graph illustrates change in degrees K per 1 DN at a range of surface temperatures Band 9 gain=8 offset =4

Mars South Pole - Overview

South pole - exposed water ice H. Kieffer, T. Titus (2002)

South pole - Swiss cheese note temperatures on the bottom of the depressions Temperature, K THEMIS VIS MOC-NA THEMIS IR

South polar layers North and South layered deposits North layers THEMIS VIS, 36 m/pixel, still covered by seasonal frost (early spring) MOC-NA, 5 m/pixel, not covered with frost. NP Summer

Matching layers. Figure shows 3 MOC images taken in various parts of the cap (~100km distance). It is possible to find matches for some layers. Work is currently under way to map these matches in 3D.

MGS/Odyssey data analysis. Excellent geometrical information allows us to register MOC-NA images together with THEMIS VIS images (see Figure). THEMIS gives a lot of coverage (e.g. we have already covered South 36 m/pixel), where as MOC-NA gives us phenomenal detail. We plan to have a more active campaign next Mars summer to cover more of the North Pole.

THEMIS IR at the Pole. Figure illustrates two THEMIS IR images taken on different orbits (~10 deg of Ls apart) of the same trough in the NPLD. Temperature of the layers of the trough changes at a different rate from the rest of ice. Measure of this rate is important to understand thermophysical properties of the layers.

Summary zTHEMIS contributes new types of data : IR at 100m/pix and VIS at 18m/pix zTHEMIS is capable of tracking changing properties of the water ice on the surface. zHypothesis : was the extent of the ancient ice cap similar to current or it was covering a much larger area. yJoint analysis of THEMIS VIS and MOC NA images allows to locate similar (same texture and position) layers in various places on the cap. yTracing 3D layer structure will show how the cap was developing with time.

Summary - cont. zTHEMIS IR has enough SNR to analyze rate of temperature change of layers in the trough. We are investigating possibility of calculating thermal inertia properties of the terrain. yThe amount of dust/ice ratio in the polar layered deposits is still unknown. yQuestion: Is it possible to use HEND/GRS data to constraint this ratio and obtain some bulk number for both north and south ice caps.