Perseverance MEDA Atmospheric Pressure Observations—Initial Results

Author:

Harri Ari‐Matti1ORCID,Paton Mark1,Hieta Maria1ORCID,Polkko Jouni1ORCID,Newman Claire2ORCID,Pla‐Garcia Jorge3ORCID,Leino Joonas1ORCID,Mäkinen Terhi1,Kauhanen Janne1ORCID,Jaakonaho Iina1ORCID,Sánchez‐Lavega Agustin4ORCID,Hueso Ricardo4ORCID,Genzer Maria1,Lorenz Ralph5ORCID,Lemmon Mark6ORCID,Vicente‐Retortillo Alvaro3ORCID,Tamppari Leslie K.7ORCID,Viudez‐Moreiras Daniel3ORCID,Torre‐Juarez Manuel de la7ORCID,Savijärvi Hannu1ORCID,Rodríguez‐Manfredi Javier A.3,Martinez German8ORCID

Affiliation:

1. Finnish Meteorological Institute Helsinki Finland

2. Aeolis Research Chandler AZ USA

3. Centro de Astrobiología (INTA‐CSIC) Madrid Spain

4. UPV/EHU Bilbao Spain

5. Johns Hopkins Applied Physics Laboratory Laurel MD USA

6. Space Science Institute College Station TX USA

7. Jet Propulsion Laboratory/California Institute of Technology Pasadena CA USA

8. Lunar and Planetary Institute Houston TX USA

Abstract

AbstractThe Mars2020 Perseverance Rover landed successfully on the Martian surface on the Jezero Crater floor (18.44°N, 77.45°E) at Martian solar longitude, Ls, ∼5° in February 2021. Since then, it has produced highly valuable environmental measurements with a versatile scientific payload including the MEDA (Mars Environmental Dynamics Analyzer) suite of environmental sensors. One of the MEDA systems is the PS pressure sensor system, which weighs 40 g and has an estimated absolute accuracy of better than 3.5 Pa and a resolution of 0.13 Pa. We present initial results from the first 414 sols of Martian atmospheric surface pressure observations by the PS, whose performance was found to meet its specifications. Observed sol‐averaged atmospheric pressures follow an anticipated pattern of pressure variation in the course of the advancing season and are consistent with data from other landing missions. The observed daily pressure amplitude varies by ∼2%–5 % of the sol‐averaged pressure, with absolute amplitude 10–35 Pa in an approximately direct relationship with airborne dust. During a regional dust storm, which began at Ls ∼ 135°, the daily pressure amplitude roughly doubled. The daily pressure variations were found to be remarkably sensitive to the seasonal evolution of the atmosphere. In particular, analysis of the daily pressure signature revealed diagnostic information likely related to the regional scale structure of the atmosphere. Comparison of Perseverance pressure observations with data from other landers reveals the global scale seasonal behavior of Mars' atmosphere.

Funder

Suomalainen Tiedeakatemia

Eusko Jaurlaritza

Publisher

American Geophysical Union (AGU)

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