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Mars 2020 Perseverance Rover Structure Components Functions Science Instrument of Mars 2020 Perseverance Rover

MEDA of the Mars 2020 Perseverance Rover – part 2

Radiation and Dust sensors

The radiation and dust sensor assembly for the Mars 2020 Perseverance Rover‘s MEDA is located on the top deck. Our 1:2 Perseverance Mars Rover Replica will perfectly replicate the appearance structure of the radiation and dust sensor assembly but they won’t be actual sensors.  This Mars 2020 Perseverance Rover‘s MEDA’s radiation and dust sensor assembly consists of photodetectors and a charge-coupled device, and the purpose is to study the characteristics of the Martian dust, such as its shape, size, or opacity. The Mars 2020 Perseverance Rover’s MEDA inherited a lot of features from previous space missions.

For example, from the Curiosity Rover mission, the rover environmental monitoring station (REMS) is applied on the Mars 2020 Perseverance Rover. It is a set of sensors that are designed to work and collect information on a low atmosphere, which includes air and ground temperature sensors, wind sensors, humidity and pressure sensors, and a photometer.

From the Mars MetNet Lander Mission, the solar irradiance sensor (MetSIS) is inherited. Mars is a cold planet compared to our Earth. Moreover, the entry, descent, and landing process for the Mars 2020 Perseverance Rover are extremely bumpy. Both harsh conditions could potentially affect the sensors. Therefore, this sensor is specially designed so that it can endure the landing impact and also operate normally at low temperatures. It consists of 32 detecting elements in 11 spectral bands. The sample rate and channels to be sample can both be manually and autonomously configured.

From the ExoMars 2016 Lander mission, DREAMS, which is short for Dust characterization, Risk assessment, and Environment Analyzer on the Martian Surface is inherited to the Mars 2020 Perseverance Rover. The Mars 2020 Perseverance Rover’s version of DREAMS has 7 detectors. These detectors are arranged so that a 360 ° azimuth is possible.

From the Mars Exploration Rover Misson and Mars Science Laboratory mission. the HazCams is applied to the Mars 2020 Perseverance Rover and now is renamed as SkyCam on the Mars 2020 Perseverance Rover.

Our Perseverance Mars Rover Replica will perfectly replicate the appearance structures of the REMS, MetSIS, DREAMS, and the HazCam, though they won’t have the functions as the real Mars 2020 Perseverance Rover.

The Mars 2020 Perseverance Rover’s MEDA’s radiation and dust sensors are the first set of sensors that are specially for studying the sun brightness and dust conditions. This will help scientists model the atmospheric conditions of Mars and prepare for human exploration in the future.