Europlanet Science Congress 2021
Virtual meeting
13 – 24 September 2021
Europlanet Science Congress 2021
Virtual meeting
13 September – 24 September 2021
EPSC Abstracts
Vol. 15, EPSC2021-69, 2021
https://doi.org/10.5194/epsc2021-69
Europlanet Science Congress 2021
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

MiniPINS - Miniature Planetary In-situ Sensor Packages for Mars and Moon

Maria Genzer1, Harri Haukka1, Maria Hieta1, Antti Kestilä1, Ignacio Arruego2, Victor Apestigue2, Alejandro Gonzalo Melchor2, Cristina Ortega3, Carmen Camañes3, Manuel Dominiguez-Pumar4, Jose Antonio Rodriquez Manfredi5, Servando Espejo6, Héctor Guerrero7, Matti Palin1, Jarmo Kivekäs1, Petri Koskimaa1, Iina Jaakonaho1, Matias Meskanen1, and Matti Talvioja8
Maria Genzer et al.
  • 1Finnish Meteorological Institute, Space research and observation technologies, Helsinki, Finland (maria.genzer@fmi.fi)
  • 2Instituto Nacional de Técnica Aeroespacial (INTA), Torrejón de Ardoz, Madrid, Spain
  • 3Added value Solutions (AVS), Elgoibar, Spain
  • 4Universitat Politècnica de Catalunya (UPC), Barcelona, Spain
  • 5Centro de Astrobiología (CAB, CSIC-INTA), Madrid, Spain
  • 6Instituto de Microelectrónica de Sevilla (IMSE), Sevilla, Spain
  • 7IMDEA Nanociencia, Madrid, Spain
  • 8Talvioja Consulting Ltd, Helsinki, Finland

MiniPINS is an ESA study led by the Finnish Meteorological Institute to develop and prototype miniaturised surface sensor packages (SSPs) for Mars and the Moon. The study aims at miniaturising the scientific sensors and subsystems, as well as identifying and utilizing commonalities of the packages, allowing to optimise the design, cut costs and reduce the development time. MiniPINS mission passed its Mission Definition Review in 2020, and Preliminary Requirements Review in 2021. The mission is currently in phase B1. 

Mars SSP “MINS” is a penetrator with approx. 25 kg mass, piggy-backed by another Mars mission spacecraft to Mars and deployed either from the approach orbit or Mars orbit.  The design of MINS has significant heritage from FMI’s MetNet mission design [1]. 4 penetrators are planned to be released to different landing sites on Mars. The Entry, Descent and Landing sequence of MINS is completely autonomous and controlled by its on-board computer. In the Martian atmosphere the penetrators undergo aerodynamic braking with inflatable breaking units (IBUs) until they reach the target velocity of 60-80 m/s for entering the Martian surface. The penetration depth target is up to 0.5 m, depending on the hardness of the soil.

       

The geometry of MINS penetrator includes a thin section to improve penetrability to the soil, a medium section with 150 mm diameter to accommodate a 2U CubeSat structure inside, and a top section with a wider diameter to stop the penetration and avoid the top part to be buried inside the soil. The deployable boom is accommodated in the top section, together with some surface sensors. The subsystems of MINS are developed using two approaches: COTS with flight heritage and delta-qualification (mainly CubeSat systems) and in-house development.

MINS has an ambitious science program to study for example the Martian atmosphere, seismology, magnetic field and chemistry. Scientific measurements will be performed above, at and below the Martian surface. MINS nominal mission will last for 1 Martian year (2 Earth years) with another Martian year as an option.

Lunar SSP “LINS” is a miniature 7 kg station deployed on the Moon surface by a rover. The baseline carrier mission for LINS is European Large Logistics Lander (EL3). 4 LINS packages are deployed to different sites within the rover’s traveling perimeter by the rover’s robotic arm. Once placed, LINS will perform scientific measurements for a minimum of 2 years (nominal mission).

LINS thermal design enables its survival during 14-day long Lunar nights when the temperature drops down to -170°C. LINS consists of a double structure, with external separated from the internal by PEEK blocks. The bottom of LINS can be completely in contact with the lunar regolith, since it is isolated from the internal one, and the space between can accommodate additional thermal insulation. Additional heating power is provided by 3W RHU of European design.

 

LINS will characterize the local environment with context images, thermal sensors, magnetometer, seismometer and ionizing radiation sensor. Other scientific payload options were also studied, but they were left as optional choices due to mass and energy limitations of LINS. The subsystems of LINS have much synergy with MINS with many based on CubeSat systems.   

[1] Harri et al. (2017), The MetNet vehicle: a lander to deploy environmental stations for local and global investigations on Mars, Geosci. Instrum. Method. Data Syst., 6, 103-124

 

MiniPINS contract is carried out under a programme of and funded by the European Space Agency. The view expressed herein can in no way be taken to reflect the official opinion of the European Space Agency. 

How to cite: Genzer, M., Haukka, H., Hieta, M., Kestilä, A., Arruego, I., Apestigue, V., Gonzalo Melchor, A., Ortega, C., Camañes, C., Dominiguez-Pumar, M., Rodriquez Manfredi, J. A., Espejo, S., Guerrero, H., Palin, M., Kivekäs, J., Koskimaa, P., Jaakonaho, I., Meskanen, M., and Talvioja, M.: MiniPINS - Miniature Planetary In-situ Sensor Packages for Mars and Moon, Europlanet Science Congress 2021, online, 13–24 Sep 2021, EPSC2021-69, https://doi.org/10.5194/epsc2021-69, 2021.