Welcome to the Astrobiology Research Group!

The focus of our research is planetary habitability and astrobiology. Our goal is to understand habitable environments on Earth and beyond, and to develop life detection instrumentation for past and present life. Our research group is led by Prof. Dr. Dirk Schulze-Makuch and our project group leaders Dr. Janosch Schirmack, Dr. Jacob Heinz, Max Riekeles, Felix Arens, and Christof Sager.

For further information on our research, please check out the descriptions of our recent subprojects BRINES, BALMAC and Microbial Motility, as well as our publication list.


Latest Research

Schulze-Makuch, D. (2021) The Case (or Not) for Life in the Venusian Clouds. Life, 11, 255, doi:10.3390/life11030255.
C. Sager, A. Airo, F. Arens and D. Schulze-Makuch (2021) New types of sand wedge polygons in the salt cemented soils in the hyper-arid Atacama Desert. Geomorphology, Volume 373, doi:10.1016/j.geomorph.2020.107481
M. Riekeles, J. Schirmack, D. Schulze-Makuch (2021) Machine Learning Algorithms Applied to Identify Microbial Species by Their Motility. Life 2021, 11, 44. doi:https://doi.org/10.3390/life11010044
A.C. Waajen, J. Heinz, A. Airo, and D. Schulze-Makuch (2020) Physicochemical salt solution parameters limit the survival of Planococcus halocryophilus in Martian cryobrines. Front Microbiol, 11:1284, doi: 10.3389/fmicb.2020.01284
J. Heinz, T. Krahn, and D. Schulze-Makuch (2020) A New Record for Microbial Perchlorate Tolerance: Fungal Growth in NaClO4 Brines and its Implications for Putative Life on Mars. Life, 10 (5), doi: 10.3390/life10050053
J. Heinz, and D. Schulze-Makuch (2020) Thiophenes on Mars: Biotic or Abiotic Origin? Astrobiology, 20 (4), doi: 10.1089/ast.2019.2139
D. Maus, J. Heinz, J. Schirmack, A. Airo, S.P. Kounaves, D. Wagner, and D. Schulze-Makuch (2020) Methanogenic Archaea Can Produce Methane in Deliquescence-Driven Mars Analog Environments. Scientific Reports, 10 (6); doi: 10.1038/s41598-019-56267-4
J. Heinz, A.C. Waajen, A. Airo, A. Alibrandi, J. Schirmack, and D. Schulze-Makuch (2019) Bacterial Growth in Chloride and Perchlorate Brines: Halotolerances and Salt Stress Responses of Planococcus halocryophilus. Astrobiology, 19 (11) 1377-1387, doi: 10.1089/ast.2019.2069
D. Schulze-Makuch, D. Wagner, S. P. Kounaves, […] J. Heinz, [45 co-authors in total] (2018) Transitory microbial habitat in the hyperarid Atacama Desert. PNAS, 115 (11) 2670-2675; doi: 10.1073/pnas.1714341115
J. Heinz, J. Schirmack, A. Airo, S.P. Kounaves, and D. Schulze-Makuch (2018) Enhanced Microbial Survivability in Subzero Brines. Astrobiology, 18 (9) 1171–1180, doi: 10.1089/ast.2017.1805
Full publication list here

Habitability of Martian Environments (HOME) [2014-2019]

textThe low average temperature and low water activity of the Martian near-surface environment makes it challenging for living organisms to persist and propagate. Nonetheless, recent mission results indicate that environmental conditions exceed locally and temporarily the lower thresholds for life to exist. Furthermore, specific soil minerals, or combinations thereof, appear to provide a suitable habitat for microbial life, especially if associated with low-temperature brines or hygroscopic salts. Thus, a quantitative understanding of the habitability potential of the Martian near-surface environment, past and present, is very much needed and the focus of HOME.

To achieve this objective, it is planned to test different types of soils and some of Earth’s hardiest organisms, using them as models (‘Mars-analogues’), to see if they can survive and perhaps even grow under the various environmental stresses known to exist on Mars.

A major tool of the laboratory investigations will be the experimentally proven state-of-the-art Mars Simulation Chamber at the German Aero Space Center, to which various soils materials and microorganisms will be exposed. The planned experimental investigations and models will be concurrently updated by analyzed mission data, particularly from landers and rovers (e.g., Curiosity Rover), to adjust this work to the newest Martian geochemical and environmental data available. Results from the HOME-related work will timely provide critical scientific knowledge to interpret incoming data from ESA’s ExoMars mission, which is scheduled for launch in 2016/2022. As one important deliverable of this work will also be to construct a Mars Soil Analyzer, an instrument which will be designed for a future mission to Mars with the objective to achieve Technology Readiness Level 6 at the completion of the proposed study.


The Atacama Project

The Atacama Project is one of the subprojects of HOME. This project is a collaborative and international investigation with the objective to investigate the dry limit of life. The Atacama Desert is one of the best analog sites to test for habitable environments on Mars. In April 2015 we conducted our first field season investigating a moisture-transect in the Atacama Desert and some specialized habitats that are known to exist near some of the driest sites. Samples were collected from selected sites, which are currently analyzed using a variety of geochemical, mineralogical, physical and microbiological methods. The investigations are conducted by a consortium of research groups from Europe, North America, and South America. In June 2015 we installed sensors at some of these sites for long-term monitoring of relative humidity and meteorological parameters, and in March 2016 we collected additional samples.

Fig.1: Sampling in the Yungay Area of the Atacama Desert, Chile.


supported by ERC Advanced Grant 339231


  • Qries
  • This project has received funding from the European Union’s Seventh Framework Programme for research, technological development and demonstration under grant agreement no 339231.






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