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MEDA, THE NEW INSTRUMENT FOR MARS ENVIRONMENT ANALYSIS FOR THE MARS 2020 MISSION

机译:MEDA,火星2020任务的火星环境分析新仪器

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The Mars 2020 rover mission is part of NASA's MarsrnExploration Program, a long-term effort of roboticrnexploration of the red planet. Designed to advancernhigh-priority science goals for Mars exploration, thernmission will address key questions about the potentialrnfor life on Mars. The mission will also providernopportunities to gather knowledge and demonstraterntechnologies that address the challenges of futurernhuman expeditions to Mars.rnThe Mars Environmental Dynamics Analyzer (MEDA)rnis an integrated full suite of sensors designed to addressrnthe Mars 2020 mission objectives of characterization ofrndust size and morphology and surface weatherrnmeasurements.MEDA system consists of one control unit and 10rnseparated sensor enclosures distributed in differentrnpositions along the Mars 2020 rover. MEDA isrncomposed of an ARM-based control computer with itsrnflight software application, two wind sensors includingrnmixed ASICs inside, five air temperature sensors, onernsky pointing camera complemented with 16 photodetectorsrnlooking up and around, one thermal infraredrnsensor using five measurement bands, one relativernhumidity sensor, one pressure sensor and the harnessrnthat interconnects all of them. It is a complex systemrnintended to operate in one of the harshest environmentsrnpossible, the Mars surface, for many years to come.rnThis will become a short term reality thanks to therncombination of a strong international science teamrndriving the science and system requirements workingrntogether with a powerful industrial organization torndesign and build the instrument. The instrument isrnbeing built right now, with its Critical Design Reviewrnat the end of 2016, and the flight model to be providedrnin 2018.rnThis paper summarizes the main scientific objective ofrnthe MEDA instrument, the links between the Missionrnand the MEDA science objectives, and the challengingrnenvironmental Mars requirements. It will then focusrnon the engineered definition of the instrument, showingrnthe overall architecture of the instrument and itsrnsensors, including a discussion of the heritage from REMS.
机译:火星2020年火星探测器任务是美国宇航局MarsrnExploration计划的一部分,该计划是对红色星球进行机器人长期探索的一项长期努力。旨在推动火星探索的高优先科学目标,该任务将解决有关火星生命潜力的关键问题。该任务还将提供没有机会收集知识和演示技术,以应对人类未来对火星的挑战。火星环境动力学分析仪(MEDA)是一套完整的传感器组合,旨在解决2020年火星的任务目标,即表征尘埃大小,形态和表面气象测量系统.MEDA系统由一个控制单元和10个单独的传感器外壳组成,这些传感器外壳沿2020年火星探测器分布在不同的位置。 MEDA由基于ARM的控制计算机及其飞行软件应用程序组成,其中两个风传感器包括内部混合ASIC,五个空气温度传感器,onernsky指向摄像机以及16个向上和向周围的光电探测器,一个使用五个测量频带的热红外传感器,一个相对湿度传感器,一个压力传感器和相互连接的线束。它是一个复杂的系统,旨在在未来许多年内无法在最恶劣的环境之一火星表面上运行。这要归功于强大的国际科学团队的共同推动,这将推动科学和系统要求的结合以及强大的工业应用,这将成为短期现实。组织撕毁了设计并建造了仪器。该仪器目前正在建造中,将于2016年底进行关键设计评审,并于2018年提供飞行模型。本文概述了MEDA仪器的主要科学目标,Missionrn与MEDA科学目标之间的联系以及具有挑战性的环境。火星要求。然后,它将重点关注仪器的工程定义,显示仪器及其传感器的总体架构,包括对REMS的继承的讨论。

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    Airbus Defence and Space - Crisa, Calle Torres Quevedo 9, 28760 Tres Cantos (Madrid) Spain,Email: jose-francisco.moreno-avarez@airbus.com;

    Airbus Defence and Space - Crisa, Calle Torres Quevedo 9, 28760 Tres Cantos (Madrid) Spain,Email: antonio.pena-godino@airbus.com;

    Centro de Astrobiología (CSIC-INTA), Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz (Madrid) Spain,Email: manfredi@cab.inta-csic.es;

    Jet Propulsion Laboratory (NASA- JPL), 4800 Oak Grove Dr, Pasadena, CA 91109 USA,Email: Elizabeth.C.Cordoba@jpl.nasa.gov;

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