The Mars Environmental Dynamics Analyzer (MEDA) is an instrument on board the Mars 2020Perseverance rover that will characterize the dust size and morphology, as well as surface weather.[2][3] Specifically, the information obtained will help address future human exploration objectives, as dust sizes and shapes, daily weather report and information on the radiation and wind patterns on Mars, that are critical for proper design of in situ resource utilization systems.[2][3] MEDA is a follow-on project from REMS, of the Curiosity rover mission.[4] MEDA has an increased scope, with greater data collection on Mars dust which contributes to overall Mars program objectives and discovery goals.[4]
The instrument suite was developed and provided by the Spanish Astrobiology Center at the Spanish National Research Council in Madrid, Spain. On April 8, 2021, NASA reported the first MEDA weather report on Mars: for April 3–4, 2021, the high was "minus-7.6 degrees, and a low of minus-117.4 degrees ... [winds] gusting to ... 22 mph".[5]
Instituto Nacional de Tecnica Aeroespacial
Madrid, Spain
Pamela Conrad
NASA Goddard Space Flight Center
Greenbelt, Maryland
Miguel Ramos
Universidad de Alcala de Henares
Madrid, Spain
Javier Gomez-Elvira
Instituto Nacional de Tecnica Aeroespacial
Madrid, Spain
Alfonso Saiz-Lopez
Agencia Estatal Consejo Superior de Investigaciones Científicas
Instituto de Quimica Fisica Rocasolano
Madrid, Spain
Felipe Gomez-Gomez
Instituto Nacional de Tecnica Aeroespacial
Madrid, Spain
Agustin Sanchez-Lavega
Universidad del Pais Vasco UPV/EHU
Bilbao, Biscay, Spain
Ari-Matti Harri
Ilmatieteen Laitos
Helsinki, Finland
John SchofieldNASA Jet Propulsion Laboratory
Pasadena, California
Mark LemmonTexas A & M
College Station, Texas
Eduardo Sebastian
Instituto Nacional de Tecnica Aeroespacial
Madrid, Spain
German Martinez
University of Michigan
Ann Arbor, Michigan
Michael Smith
NASA Goddard Space Flight Center
Greenbelt, Maryland
Sara Navarro Lopez
Instituto Nacional de Tecnica Aeroespacial
Madrid, Spain
Leslie Tamppari
NASA Jet Propulsion Laboratory
Pasadena, California
Claire Newman
Aeolis Research
Pasadena, California
Overview
Dust dominates Mars' weather the way that water dominates Earth's weather. Martian weather cannot be predicted unless dust behavior is studied and understood in the weather context.[3][8] MEDA is a suite of environmental sensors designed to record dust optical properties and six atmospheric parameters: wind speed/direction, pressure, relative humidity, air temperature, ground temperature, and radiation (UV, visible, and IR ranges of the spectrum).[3][9]
The technology used on MEDA was inherited from the REMS package operating on the Curiosity rover and the TWINS package on InSight lander.[2] The sensors are located on the rover's mast and on the deck, front and interior of the rover's body. It records data whether the rover is active or not, at both day and night.[9] The instruments will collect data for 5 minutes every 30 minutes.[8]
^ abcThe Mars Environmental Dynamics Analyzer (MEDA): A Suite of Environmental Sensors for the Mars 2020 Rover. Tamppari, L.; Rodriguez-Manfredi, J. A.; de la Torre-Juárez, M.; Bridges, N.; Conrad, P. G.; Genzer, M.; Gomez, F.; Gomez-Elvira, J.; Harri, A. M.; Lemmon, M. T.; Martinez, G.; Navarro, S.; Newman, C. E.; Perez-Hoyos, S.; Prieto, O.; Ramos, M.; Saiz-Lopez, A.; Sanchez-Lavega, A.; Schofield, J. T.; Smith, M. D. American Geophysical Union, Fall Meeting 2015, abstract #P11B-2097