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Simulated Martian Conditions

The spectral characteristics of some geological samples were recorded and the effect of environmental parameter variations (such as gas pressure and temperature) on the spectral features were also acquired by using the in situ spectral sensors under various simulated Martian conditions.

A Mars Environment Chamber Coupled with Multiple In Situ Spectral Sensors for Mars Exploration

Simulated Martian Conditions

The ML-PENG generates sufficient power to operate five light-emitting diodes by harvesting biomechanical energy under simulated Martian conditions.

Polarization- and Electrode-Optimized Polyvinylidene Fluoride Films for Harsh Environmental Piezoelectric Nanogenerator Applications.

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10.1089/ast.2020.2329

Martian conditions that generate reactive oxygen species involve the decomposition of H2O2 at temperatures of around 278 K under relatively high doses of C-band ultraviolet radiation (UVC).

Reactive Oxygen Species in Emulated Martian Conditions and Their Effect on the Viability of the Unicellular Alga Scenedesmus dimorphus.

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10.3791/61217

This paper describes a protocol to design experiments to study the formation of brines under Martian conditions and monitor the process with electrical conductivity measurements.

Measuring Electrical Conductivity to Study the Formation of Brines Under Martian Conditions.

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10.1016/J.PSS.2021.105193

We considered scenarios analogous to Martian conditions and calculated the single and multiple scattering polarization for Martian dust, water ice and carbon dioxide ice with the help of a Radiative Transfer algorithm for Nadir and Limb spacecraft observation positions.

Polarization signatures of Mars dust and clouds: Prospects for future spacecraft observations

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10.1016/j.actaastro.2020.12.037

Our results reveal that unsteady lift enhancement mechanisms, such as delayed stall and rotational lift, are present in the bioinspired solutions for the scaled vehicles hovering in Martian conditions.

Data-driven CFD scaling of bioinspired Mars flight vehicles for hover

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10.1109/ACCESS.2021.3112107

To have low signal attenuation under Martian conditions, the device operating frequency is limited to 100 kHz.

Design, Development, and Characterization of a Low Frequency CMUT-Based Anemometer

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10.1016/J.PSS.2019.01.004

Through theoretical modeling, we predict the power spectrum of wind pressure fluctuations at the center of the dome under Martian conditions.

Porous domes as wind noise filters for infrasound sensing on Mars

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10.1089/ast.2018.2001

For this reason, the International Space Station (ISS) can be advantageously used to expose the same samples studied in the laboratory to UV radiation representative of martian conditions.

The Photochemistry on Space Station (PSS) Experiment: Organic Matter under Mars-like Surface UV Radiation Conditions in Low Earth Orbit.

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10.1099/ACMI.AC2019.PO0322

In order to better establish which of these are capable of supporting persistent growth under martian conditions, we performed a series of enrichments using four geological simulants for Mars: a global composition, an early and unaltered basaltic composition, a sulfur-rich composition, and a haematite-rich composition.

Viable metabolisms in a simulated martian chemical environment

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10.1017/S147355041800037X

Recently desert cyanobacteria were exposed to ground-based simulations of space and Martian conditions and to real space and Martian conditions simulated in low Earth orbit using facilities attached outside the International Space Station.

Desert cyanobacteria under space and planetary simulations: a tool for searching for life beyond Earth and supporting human space exploration

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Martian Conditions - Martian conditions that generate reactive oxygen species involve the decomposition of H2O2 at temperatures of around 278 K under relatively high doses of C-band ultraviolet radiation (UVC). [1] This paper describes a protocol to design experiments to study the formation of brines under Martian conditions and monitor the process with electrical conductivity measurements. [2] We considered scenarios analogous to Martian conditions and calculated the single and multiple scattering polarization for Martian dust, water ice and carbon dioxide ice with the help of a Radiative Transfer algorithm for Nadir and Limb spacecraft observation positions. [3] Our results reveal that unsteady lift enhancement mechanisms, such as delayed stall and rotational lift, are present in the bioinspired solutions for the scaled vehicles hovering in Martian conditions. [4] To have low signal attenuation under Martian conditions, the device operating frequency is limited to 100 kHz. [5] Through theoretical modeling, we predict the power spectrum of wind pressure fluctuations at the center of the dome under Martian conditions. [6] For this reason, the International Space Station (ISS) can be advantageously used to expose the same samples studied in the laboratory to UV radiation representative of martian conditions. [7] In order to better establish which of these are capable of supporting persistent growth under martian conditions, we performed a series of enrichments using four geological simulants for Mars: a global composition, an early and unaltered basaltic composition, a sulfur-rich composition, and a haematite-rich composition. [8] Recently desert cyanobacteria were exposed to ground-based simulations of space and Martian conditions and to real space and Martian conditions simulated in low Earth orbit using facilities attached outside the International Space Station. [9]

Simulated Martian Conditions

The spectral characteristics of some geological samples were recorded and the effect of environmental parameter variations (such as gas pressure and temperature) on the spectral features were also acquired by using the in situ spectral sensors under various simulated Martian conditions. [1] The ML-PENG generates sufficient power to operate five light-emitting diodes by harvesting biomechanical energy under simulated Martian conditions. [2] Here, the results of the SVTs, the last set of experiments, which were performed in ultraviolet radiation combined with simulated space vacuum or simulated martian conditions, are reported. [3] As all bacterial enzymes are encoded within the bacterium nucleic acids, we have designed experiments to study the ability of this microbe to survive, grow and metabolize under simulated Martian conditions of pressure, temperature and different concentrations of sulfate compounds. [4] , in space and simulated martian conditions for 531 days in low Earth orbit as part of the "Biofilm Organisms Surfing Space" (BOSS) experiments. [5]