EGU23-16660, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-16660
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Martian Atmospheric Pressure Measurement from Space

Joel Campbell, Zhaoyan Liu, Bing Lin, Jirong Yu, and Shibin Jiang
Joel Campbell et al.
  • NASA Langley Research Center, Hampton, VA, USA, Joel.f.campbell@nasa.gov

In order to facilitate human exploration on Mars, a need exists to study weather patterns and atmospheric conditions on Mars. Mars has colder weather than Earth, is known for its dust storms, and has a very thin atmosphere, yet its atmosphere and climate are more like Earth's than any other planet in our solar system. Despite these challenges, NASA scientists believe that Mars is the most promising planet for exploration and habitation. We are developing a new measurement concept that uses differential absorption Lidar system in the 2-μm CO2 absorption band to measure atmospheric CO2 and pressure on Mars. By selecting two or more closely spaced wavelengths, one can eliminate the effects of other gases and surface reflections, allowing us to accurately measure CO2 absorption and determine CO2 levels and air pressure on Mars. Our simulations show that this system will be able to measure air pressure with 1 Pa precision up to 5 km away, even in the presence of moderate dust, and measure CO2 and pressure profiles from the surface up to 13 km with a horizontal resolution of 100 km and a vertical resolution of 100 m (400 m during the day). These measurements will improve weather and climate modeling and prediction on Mars.

How to cite: Campbell, J., Liu, Z., Lin, B., Yu, J., and Jiang, S.: Martian Atmospheric Pressure Measurement from Space, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-16660, https://doi.org/10.5194/egusphere-egu23-16660, 2023.