TNA1: Planetary Field Analogues

TNA 1 coordinator: Felipe Gomez

TNA1 Planetary Field Analogues offers access to 5 well-characterized terrestrial field sites that have been selected so as to provide the most realistic analogues of surfaces of Mars, Europa and Titan, to which planetary missions have either recently been directed or are planned. The five sites are:

Rio Tinto a 100 km long acidic aqueous river environment located in the Huelva province in South West Spain. Rio Tinto is a unique site in Europe in which a rock-water-biology interaction produces river water with a pH that averages 2. The site also supports a unique ecosystem making it a desirable site for studying possible habitats for life on other planetary bodies. The very low pH of the water and production of hydrated mineral precipitation (jarosite, goethite) represents a distinctive geological environment that will allow assessment of the relative role of biological and inorganic processes in the production of geology comparable to that found on the surface of Mars by the Mars Environmental Rover Opportunity (e.g. Jarosite).

Tunisian Chott, located in South West Tunisia is a seasonal lake that is completely dry most of the year. The surface of the lake is covered with a hard NaCl crust covering underground water. From the astrobiology point of view it is extremely interesting to examine the biological cycles at such low and salty water levels. Future new space missions are expected to take advantage of remote testing facilities such as Tunisian Chott El Jerid to fully validate their instrumentation. This field analogue will be fully characterised using field, geophysical and microbiological methodology in 2009-2010 so will only be open to access from 2011.

Ny-Ålesund, Svalbard archipelago. Ny-Ålesund is the world's northernmost permanent settlement situated on the island of Spitsbergen in the Svalbard archipelago, only 1,200 km from the North Pole. It includes areas in front of two glaciers that are very well suited for testing instruments for ground ice and permafrost mapping. In addition, there are locations that include large amounts of buried glacier covered by layers of sediments that comprise mixtures of silicate minerals and organic material. The study area is also within a region of permanent permafrost. The growing interest in physical conditions of the icy moons of the outer planets and the possibility that they may host life forms has led to a major increase in the research undertaken on Spitsbergen and access to this site is therefore highly competitive, in Europlanet access will be provided for a field campaign in 2010.

Ibn Battuta Centre near Marrakech in Morocco is a desert field facility. This extreme environment is used to test rover, landing systems, instruments dedicated to the Mars exploration and to perform scientific analysis of Mars analogues. Desert environments in the region provide a wide variety of field analogues including sand dunes, rocky desert, regoliths, evaporates and other environments and geological and geomorphological features such as flash flood drainage. Ongoing geological analysis of the region aims to quantitatively understand the origin of environments such as mud volcanoes, evaporitic deposits, the recent stratigraphy of aeolian sediments and deflation surfaces that appear remarkable comparable to those reported from Mars. Astrobiology research is also examining potential habitats and energy sources within ancient mud volcanoes and evaporates with the goal of establishing how specific endolithic communities and arid bacterial niches function.

The Kamchatka Peninsula in Siberia Russia is one of four regions in the world with extensive geyser activity allowing a study of the complex inter-relationship between volcanism and landform development, highly relevant to some planetary bodies, whilst the hot springs are also the habitat of diverse microbiology. The microorganisms living in these springs survive in extreme conditions both in terms of temperature and water composition (e.g. highly acidic).The site is therefore both a possible analogue of prebiotic conditions but may form an analogue to some of the surfaces of Jovian and Saturnian moons (e.g Europa and Titan).The Kamchatka region also offers Mars analogue terrains and was used in the Soviet/Russian space programme for testing of Mars rovers for Mars-96 mission.

 

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Last updated:19 May 2009