Add to ORKGIn this study, four new simulants have been developed, and their associated fluid chemistries have been derived for use in a series of microbiological simulation experiments. These experiments will determine if aqueous environments on Mars, past or present, could potentially support microbial life and identify any key geochemical biosignatures that may arise as a result of that life
The identification of geochemical bio-signatures is important for assessing whether life existed on ...
We developed scenarios for shallow and deep subsurface cryptic niches for microbial life on Mars. Su...
Planet Mars past environmental conditions were similar to the early Earth, but nowadays they are sim...
Today the martian surface is unable to sustain liquid water. However, there is evidence on the surfa...
Water present on early Mars is often assumed to have been habitable. In this study, experiments were...
Microbes have multiple ways of producing energy. Which of these methods are possible depends on the ...
There is evidence that water may exist on Mars as brines in the subsurface. The chemistries of these...
There is evidence that water may currently exist on Mars as brines. The chemistries of these brines...
We report on new analogue materials to simulate Martian rocks and soils, especially under realistic ...
Methane was first observed in the martian atmosphere in 2003. This organic molecule has an expected...
The martian surface cannot sustain liquid water today, but there is evidence water was present durin...
The first step in finding potential extant, and/or extinct, life on Mars is to understand the potent...
There is evidence that water may exist on Mars in the form of brines. The chemistries of these brin...
The waters that were present on early Mars may have been habitable. Characterising environments anal...
A selection of the core questions in astrobiology deal with the origin of life on Earth, life in ext...
The identification of geochemical bio-signatures is important for assessing whether life existed on ...
We developed scenarios for shallow and deep subsurface cryptic niches for microbial life on Mars. Su...
Planet Mars past environmental conditions were similar to the early Earth, but nowadays they are sim...
Today the martian surface is unable to sustain liquid water. However, there is evidence on the surfa...
Water present on early Mars is often assumed to have been habitable. In this study, experiments were...
Microbes have multiple ways of producing energy. Which of these methods are possible depends on the ...
There is evidence that water may exist on Mars as brines in the subsurface. The chemistries of these...
There is evidence that water may currently exist on Mars as brines. The chemistries of these brines...
We report on new analogue materials to simulate Martian rocks and soils, especially under realistic ...
Methane was first observed in the martian atmosphere in 2003. This organic molecule has an expected...
The martian surface cannot sustain liquid water today, but there is evidence water was present durin...
The first step in finding potential extant, and/or extinct, life on Mars is to understand the potent...
There is evidence that water may exist on Mars in the form of brines. The chemistries of these brin...
The waters that were present on early Mars may have been habitable. Characterising environments anal...
A selection of the core questions in astrobiology deal with the origin of life on Earth, life in ext...
The identification of geochemical bio-signatures is important for assessing whether life existed on ...
We developed scenarios for shallow and deep subsurface cryptic niches for microbial life on Mars. Su...
Planet Mars past environmental conditions were similar to the early Earth, but nowadays they are sim...