The Bubble Lab is an experimental laboratory to study (a) fluids in hydrothermal terrain, and (b) volcano-tectonic processes. We simulate fluids and solids in two separate but closely related laboratories. First, we have an experimental laboratory for studying gas bubbles in hydrothermal and volcanic systems and an earthquake simulator. Second, we study the deformation and fracturing of scaled analog volcanoes and their intrusions. The goal of the Bubble & Volcano Lab is to study the …

Experimental tectonics is the branch of geosciences that uses so-called "analogue models" scaled down from nature to the laboratory to study tectonic processes in situ. Thanks to new materials, testing methods and monitoring techniques, which have been developed in the past two decades, anologue modelling nowadays provides quantitative tectonic oberservations across all relevant spatial and temporal scales. Please find an introductory texts to our lab and methods …

The groundwater monitoring is used to evaluate the local quality and quantity of the groundwater. These information are required to obtain important insights in the hydrochemical processes in the aquifer, as well as the origin and residence time of groundwater.
The Grundfos MP 1 submersible pump set with a connected, closed flow cell enables observations of the physicochemical parameters with digital IDS sensors (temperature, pH, electrical conductivity, redox potential, dissolved oxygen), …

The MSF-Lab, established in 2004, is part of the Department of Experimental Planetary Physics and is used for different astrobiological and physical experiments to simulate the key environmental conditions like pressure, temperature, radiation, gas composition, and primarily also the diurnally varying atmospheric humidity in a range from earth conditions to similar to those at the near-surface atmosphere of Martian mid- and low latitudes. A further part of the laboratory are tests with gas, …

The Planetary Analog Simulation Facility-Laboratory (PASLAB) at the DLR is used for different astrobiological, chemical and physical experiments to simulate variations in key environmental conditions like pressure, temperature, radiation and gas composition, under conditions ranging from Earth-like (including Early Earth) to the near-surface atmosphere of Martian mid- and low latitudes and exoplanets (e.g. temperature range between -70 °C to +20 °C, low pressures 6 to 10 mbar, etc.). The DLR …