TY - GEN
T1 - The wide field cameras on-board the emirates lunar mission's rashid rover
AU - Virmontois, C.
AU - Els, S. G.
AU - Almarzooqi, Hamad
AU - Khoory, M. S.
AU - Kumar, S.
AU - Belal, A. S.
AU - Ioannou, Z.
N1 - Publisher Copyright:
© 2021 International Astronautical Federation, IAF. All rights reserved.
PY - 2021
Y1 - 2021
N2 - Optical wide field imaging cameras are the core components of any planetary surface mission. They provide the necessary surface view to support decision taking in operations, as well as deliver data to perform surface navigation of highest precision, and to identify worthwhile scientific targets for up-close investigation. Very importantly, optical images are the lasting public legacy of any robotic surface mission, and thus represent crucial products for public outreach. The cameras on-board small rover missions are usually a compromise of the performances required to reach the operational and scientific goals, and the mass and complexity and cost envelopes. For example, scientific high performance camera systems would employ sets of filters to obtain images in different wavelengths to obtain the spectrophotometric data. However, the involved mechanical complexity of such a system is often prohibitive for small missions. The use of three band (RGB) color sensors is a compromise as it allows to obtain at least some basic spectral resolution, while maintaining system complexity at a low level. To discuss the various trade-offs, this paper presents the imaging system of the Rashid rover of the Emirates Lunar Mission. This camera system consists of two identical cameras, one of which acts as prime and one as secondary camera. The component identity is beneficial in view of minimizing system and development complexity, as well as suitable orientation on the rover provides operational redundancy. As these cameras are based on the same design as the Navcam cameras of the MMX Rover mission, these cameras exploit synergies between different planetary mission concepts. This paper discusses the considered use cases, operations scenarios, the thus deduced requirements, and their weighing in view of the different design goals for the imaging system. The camera system design parameters are shown, and how these fit in the overall mission concept, and the anticipated usage, and mission boundaries.
AB - Optical wide field imaging cameras are the core components of any planetary surface mission. They provide the necessary surface view to support decision taking in operations, as well as deliver data to perform surface navigation of highest precision, and to identify worthwhile scientific targets for up-close investigation. Very importantly, optical images are the lasting public legacy of any robotic surface mission, and thus represent crucial products for public outreach. The cameras on-board small rover missions are usually a compromise of the performances required to reach the operational and scientific goals, and the mass and complexity and cost envelopes. For example, scientific high performance camera systems would employ sets of filters to obtain images in different wavelengths to obtain the spectrophotometric data. However, the involved mechanical complexity of such a system is often prohibitive for small missions. The use of three band (RGB) color sensors is a compromise as it allows to obtain at least some basic spectral resolution, while maintaining system complexity at a low level. To discuss the various trade-offs, this paper presents the imaging system of the Rashid rover of the Emirates Lunar Mission. This camera system consists of two identical cameras, one of which acts as prime and one as secondary camera. The component identity is beneficial in view of minimizing system and development complexity, as well as suitable orientation on the rover provides operational redundancy. As these cameras are based on the same design as the Navcam cameras of the MMX Rover mission, these cameras exploit synergies between different planetary mission concepts. This paper discusses the considered use cases, operations scenarios, the thus deduced requirements, and their weighing in view of the different design goals for the imaging system. The camera system design parameters are shown, and how these fit in the overall mission concept, and the anticipated usage, and mission boundaries.
KW - Camera
KW - Image sensor
KW - Moon
KW - Rover
KW - Space
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M3 - Conference contribution
AN - SCOPUS:85127265634
T3 - Proceedings of the International Astronautical Congress, IAC
BT - IAF Space Exploration Symposium 2021 - Held at the 72nd International Astronautical Congress, IAC 2021
PB - International Astronautical Federation, IAF
T2 - IAF Space Exploration Symposium 2021 at the 72nd International Astronautical Congress, IAC 2021
Y2 - 25 October 2021 through 29 October 2021
ER -