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Mars Environmental Dynamics Analyzer

From Wikipedia, the free encyclopedia
Environmental instrument on the Perseverance rover
Mars Environmental Dynamics Analyzer
OperatorSpanish National Research Council
ManufacturerSpanish Astrobiology Center (CSIC-INTA)
Instrument typeSuite of environmental sensors
FunctionMeasure dust size, morphology, weather
Mission duration1 Mars year[1]
Properties
Mass5.5 kg (12 lb)
Power consumption17 watts
Host spacecraft
SpacecraftMars 2020Perseverance rover
Launch dateJuly 30, 2020
RocketAtlas V 541
Launch siteCape CanaveralSLC-41
REMS instrument on Mars

TheMars Environmental Dynamics Analyzer (MEDA) is an instrument on board theMars 2020Perseverance rover designed to characterize dust size and morphology, as well as surface weather.[2][3] This information is intended to inform future human exploration objectives, as dust sizes and shapes, daily weather reports, and information on radiation and wind patterns on Mars are critical for proper design ofin situ resource utilization systems.[2][3] MEDA is a follow-on project from REMS of theCuriosity rover mission,[4] with a larger scope.[4]

The instrument suite was developed and provided by theSpanish Astrobiology Center at theSpanish National Research Council inMadrid, 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]

Scientific team members

[edit]

The Principal Investigator isJosé Antonio Rodríguez Manfredi and the Deputy Principal Investigator is Manuel de la Torre Juarez (JPL-NASA).[6][7]

List of coinvestigators and their affiliations:[7]

Nathan Bridges

Johns Hopkins University/Applied Physics LaboratoryLaurel, Maryland

Olga Prieto-Ballesteros

Instituto Nacional de Tecnica AeroespacialMadrid, Spain

Pamela Conrad

NASA Goddard Space Flight CenterGreenbelt, Maryland

Miguel Ramos

Universidad de Alcala de HenaresMadrid, Spain

Javier Gomez-Elvira

Instituto Nacional de Tecnica AeroespacialMadrid, Spain

Alfonso Saiz-Lopez

Agencia Estatal Consejo Superior de Investigaciones CientíficasInstituto de Quimica Fisica RocasolanoMadrid, Spain

Felipe Gomez-Gomez

Instituto Nacional de Tecnica AeroespacialMadrid, Spain

Agustin Sanchez-Lavega

Universidad del Pais Vasco UPV/EHUBilbao, Biscay, Spain

Ari-Matti Harri

Ilmatieteen LaitosHelsinki, Finland

John SchofieldNASA Jet Propulsion Laboratory

Pasadena, California

Mark LemmonTexas A & M

College Station, Texas

Eduardo Sebastian

Instituto Nacional de Tecnica AeroespacialMadrid, Spain

German Martinez

University of MichiganAnn Arbor, Michigan

Michael Smith

NASA Goddard Space Flight CenterGreenbelt, Maryland

Sara Navarro Lopez

Instituto Nacional de Tecnica AeroespacialMadrid, Spain

Leslie Tamppari

NASA Jet Propulsion LaboratoryPasadena, California

Claire Newman

Aeolis ResearchPasadena, California

Overview

[edit]

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, relativehumidity, airtemperature, ground temperature, andradiation (UV, visible, and IR ranges of the spectrum).[3][9]

The technology used on MEDA was inherited from theREMS package operating on theCuriosity rover and the TWINS package onInSight 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][needs update]

ParameterPerformance/units[3][9]
Mass5.5 kg (12 lb)
PowerMax 17 watts
Data return≈11 megabytes
Temperatureaccuracy: 5K
resolution: 0.1 K
Relative humidityaccuracy of 10%
in the 200-323 K range
PressureRange: 1 to 1150 Pa
accuracy: 20 Pa
resolution: 0.5 Pa
Radiationeight upward looking photodiodes:

• 255 +/– 5 nm for the O3
• 295 +/– 5 nm for the O3
• 250–400 nm for totalUV
• 450±40 nm for MastCam-Z cross-calibration
• 650 +/– 25 nm for SuperCam cross-calibration
• 880 +/–5 nm for MastCam-Z cross-calibration
• 950 +/– 50 nm forNIR
• one panchromatic (300-1000 nm) filter

Windaccuracy: 2 m/sec
resolution: 0.5 m/sec

Components

[edit]
Various components of MEDA highlighted in this graphic of planned devices for thePerseverance rover

See also

[edit]

References

[edit]
  1. ^"Mission: Overview". NASA. RetrievedMarch 7, 2015.
  2. ^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
  3. ^abcdeMars 2020 - MEDA Specifications. NASA, 2016.
  4. ^ab"MEDA: An Environmental and Meteorological Package for Mars 2020"(PDF).45th Lunar and Planetary Science Conference (2014). RetrievedNovember 12, 2022.
  5. ^Cappucci, Matthew (April 8, 2021)."NASA receives first weather reports from Perseverance rover on Mars at Jezero Crater - The weather data is crucial as the first flight of Ingenuity draws near".The Washington Post. RetrievedApril 8, 2021.
  6. ^Juarez, Manuel de la Torre."JPL Science: Manuel de la Torre Juarez".science.jpl.nasa.gov. Retrieved2021-02-19.
  7. ^ab"MEDA Team Members - NASA Mars". 2020-07-17. Archived fromthe original on 2020-07-17. Retrieved2021-02-19.
  8. ^abMEDA, THE ENVIRONMENTAL DYNAMICS ANALYZER FOR MARS 2020 (PDF). J. A. Rodriguez-Manfredi,M. de la Torre, J. S. Boland, et al. 3rd International Workshop on Instrumentation for Planetary Missions (2016).
  9. ^abcMars Environmental Dynamics Analyzer (MEDA).Mars 2020 Rover, NASA. 2015.

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