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One of the main research topics of planetary exploration is the water cycle, but it is difficult to design a general, robust and scalable procedure, that allows to monitor the interaction of the atmosphere with the ground. Laboratory simulations can recreate the planetary atmospheres, surfaces and the interactions within. However, it comes with a challenge, from procuring necessary equipment to training personnel. This paper describes a protocol to design experiments to study the formation of brines under Martian conditions of temperature, relative humidity and carbon-dioxide atmosphere, and monitors the process with electrical conductivity measurements. We also provide a brief account of constructing a simple and inexpensive electrical conductivity measurement setup. The protocol may be adapted to design similar experiments in vacuum or other planetary atmospheres.
Importance of brine formation studies
Hygroscopic salts can absorb atmospheric water vapor to form liquid solutions in a process called deliquescence. This process creates brine under favorable conditions on the surface of Earth and Mars that is likely to exist in certain times and places. The reverse process called efflorescence is also possible when the brines dehydrate under unfavorable conditions. The plausible existence of brines on the surface or subsurface of Mars has several implications on the current terrestrial and Martian studies. Additionally, salts can hydrate, hold and release water molecules, which also affects the water cycle and the properties of the regolith.
There is an increasing international interest on determining the temperature, relative humidity and pressure conditions that are favorable for the formation of brines due to deliquescence of salts and salt mixtures, both for Earth and Mars. Field observations of the dark steep-sloped water tracks near Don Juan Pond (DJP) watershed and the formation of wet patches in the McMurdo Dry Valleys in Antarctica have been attributed to the brine formation in the calcium-chloride rich sediments1.
These results have also been validated with laboratory experiments simulating the low temperatures between -30 °C and 15 °C and a relative humidity between 20% and 40%2. Chloride-bearing evaporites in the Yungay region in the hyper-arid core of the Atacama Desert, Chile can absorb water and harbor microbial life3. The processes occurring in the DJP and the driest places on Earth such as the Atacama Desert may be analogous to several of the Martian studies suggesting that similar processes could be happening on the present-day Mars1,2,4,5,6,7,8,9,10,11,12,13,14,15,16. Recent remote sensing observations of the Salar de Uyuni (Bolivian Altiplano) have described a similar process to what is observed on Mars from orbit17. Despite harsh conditions, the deliquescence-driven brine formation process can sustain liquid water in quantities large enough to allow colonies of bacteria to thrive deep within the salt nodules3. This is of interest to astrobiologists and planetary scientists.
Diurnal absorption and desorption of the atmospheric moisture by the deliquescent salts in the Martian regolith has been reported4,5. The brine formation process of perchlorates existing on Mars have already been studied, observing the changes in phase or hydration state of individual salt particles1,9,18.Different brine related studies have also been performed under Mars-relevant conditions to determine the relative humidity values at which Mars relevant salts and salt mixtures will undergo deliquescence and efflorescence19,20,21. Others have used these experiment conditions to study the evaporation rates of brines at Martian temperature, relative humidity and carbon-dioxide atmosphere22.
Methods of brine formation detection and monitoring
Several methods exist to monitor the brine formation process. Visual observation and images in the visible wavelengths are the simplest. Weighing the salts to monitor the increase in mass could well be used23. Usually the environmental parameters such as temperature, relative humidity and pressure are monitored to properly interpret the observations. Some studies used a hygrometer. The hygroscopic properties of the salts can also be measured with differential mobility analyzers or electrodynamic balances, but their operation is not accurate enough beyond a relative humidity of90%24. In recent studies, transmission and scanning electron microscopes (TEM and SEM) have been widely utilized. Both these microscopes have environmental cells that enable studying the interaction of water with individual salt particles24. The phase changes and transitions in individual salt particles are generally detected with optical, infrared (IR) or Raman spectroscopy incorporated in the experimental setup8,13,19,20,25. Existing spectroscopic methods offer good observation limits and a clear detection of phase changes, but they are not compatible to monitor bulk salt samples and for the continuous monitoring of the brine formation process through the intermediate stages of phase transitions. Furthermore, the laser-based microscopic devices such as the 'Raman microscope' are expensive and may require a complex experimental setup.
We use electrical conductivity as the measurement technique. Measurements to determine the relative humidity at which the salts undergo deliquescence have been performed using electrical conductivity where the derived values were in good agreement with those determined using a standard hygrometer26. The time series of the brine formation process of the deliquescent salts has been studied using electrical conductivity earlier by Heinz et al.27. Here, they used a mixture of JSC Mars-1a simulant and perchlorates or chlorides. The electrical conductivity technique has also been used to detect liquid or frozen water in soils28,29. The advantage of this method is that, it can be applied both to small and medium-sized samples, as long as they are contained in the space between the two electrodes.
This protocol could be useful to design similar experiments that involves controlling the temperature and relative humidity in vacuum or simulating the extraterrestrial atmospheres such as Mars and others.

Figure 1: Construction of the experiment setup. A block diagram showing a simple electrical conductivity measurement setup comprising of the main components such as electrodes, measuring circuits and an Arduino. Please click here to view a larger version of this figure.
Electrical conductivity of brines can be measured with a simple inexpensive setup as shown in Figure 1. The specific products to construct the setup is given in Table of Materials. The setup primarily consists of a pair of metal electrodes of same dimensions separated by a known distance within which the salt or salt mixtures for the study are accommodated. A PT1000 resistance temperature detector can be used to measure the temperature of the salts. One of the flat ends of the electrodes can be soldered to each terminal of a shielded coaxial cable. Similarly, the two terminals of the sensor can be soldered to another shielded coaxial cable. The other ends of each of these coaxial cables can be connected to the circuits to measure electrical conductivity and temperature, respectively. An Arduino board and a simple serial data monitor can be used to retrieve the data and store it.
In the context of this experiment, we use the Engineering Qualification Model (EQM) of the HABIT/ExoMars 2022 instrument, the closest replica of the Flight Model (FM) that will be flown to Mars in 2022. HABIT stands for HabitAbility: Brines, Irradiation, and Temperature. It is one of the two European payloads in the ExoMars 2022 Surface Platform Kazachok and has the objective to study the habitability conditions at the landing site, Oxia planum, Mars. The Brine Observation Transition To Liquid Experiment (BOTTLE) is one of the components of HABIT instrument with a purpose to demonstrate the liquid water stability on Mars31. The protocol described here serves to calibrate the electrical conductivity measurements as a function of brine formation under Martian conditions of temperature, relative humidity and carbon-dioxide atmosphere31. This is applied to retrieve the calibrated electrical conductivity measurements of BOTTLE that aids with the detection of liquid brine formation process on Mars, which is one of its primary mission objectives18. By calibration, here we refer to experiment-level calibration. Instrument-level calibration is performed with determining the geometrical cell constants of each electrode pair and with calibration standards of known electrical conductivity31.