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Friday

Schedule

id
date time
PM2
16:20
Abstract
The instrument HABIT (HabitAbility, Brine Irradiation and Temperature) on the ExoMars 2022 platform
Friday

Abstract details

id
Current and future Mars missions
Date Submitted
2021-04-30 10:54:00
Javier
Martin-Torres
University of Aberdeen
Contributed
The instrument HABIT (HabitAbility, Brine Irradiation and Temperature) on the ExoMars 2022 platform
J. Martin-Torres (University of Aberdeen, UK), M.P. Zorzano (University of Aberdeen, UK) and the HABIT Team
HABIT (HabitAbility, Brine Irradiation and Temperature) is an edge-breaking and multipurpose instrument, managed by the University of Aberdeen, UK, that will be part of the ExoMars 2022 mission.

It is a surface station devoted to evaluating the habitability of Mars, but also will be the first European In-situ Resource Utilization instrument for future Mars exploration.

The HABIT (HAbitability, Brine Irradiation and Temperature) instrument is dedicated to investigating the habitability on present-day Mars by quantifying the availability of liquid water, the thermal ranges and UV doses. It includes the BOTTLE (Brine Observation Transition To Liquid Experiment) compartment to capture at night-time atmospheric water by deliquescence of four different types of salts: calcium perchlorate, magnesium perchlorate, sodium perchlorate and calcium chloride, and 3 environmental sensors devoted to monitoring the full diurnal and seasonal variations of the ground and air temperature, and the UV irradiance. These three sensors shall complement the existing environmental package of the spacecraft, which has Pressure and Relative Humidity sensors. HABIT measurements will allow constraining the habitability at the landing site in terms of metabolic and reproduction temperature, calculating the heat-flux and the UV biological dose, providing the Relative Humidity of the ground and air, to study the atmosphere/surface water interchange, provide information about winds (which shall be useful also for the rover drilling and sampling operations), and about thermal inertia and subsurface thermal profile and hydration level complementing the studies of the other platform and rover instruments. It will also provide the concentration of the atmospheric trace gas ozone (complementing orbiter observations from NOMAD-Trace Gas Orbiter) and atmospheric UV opacity (providing continuous monitoring of the dust cycle).

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