Share Email Print

Proceedings Paper • Open Access

SIMBIOSYS-STC ready for launch: a technical recap
Author(s): Emanuele Simioni; Vania Da Deppo; Cristina Re; Maria Teresa Capria; Giampiero Naletto; Gianfranco Forlani; Leonardo Tommasi; Michele Dami; Donato Borrelli; Iacopo Ficai Veltroni; Matteo Massironi; Alessandra Slemer; Raffaele Mugnuolo; Francesco Longo; Gabriele Cremonese

Paper Abstract

BepiColombo is the first ambitious, multi-spacecraft mission of ESA/JAXA to Mercury. It will be launched in October 2018 from Kourou, French Guiana, starting a 7-year journey, which will bring its modules to the innermost planet of the solar system.

The Stereo Camera (STC) is part of the SIMBIO-SYS instrument, the Italian suite for imaging in visible and near infrared which is mounted on the BepiColombo European module, i.e. the Mercury Planetary Orbiter (MPO). STC represents the first push-frame stereo camera on board of an ESA satellite and its main objective is the global three-dimensional reconstruction of the Mercury surface.

The harsh environment around Mercury and the new stereo acquisition concept adopted for STC pushed our team to conceive a new design for the camera and to carry out specific calibration activities to validate its photogrammetric performance. Two divergent optical channels converging the collected light onto a unique optical head, consisting in an off-axis telescope, will provide images of the surface with an on-ground resolution at periherm of 58 m and a vertical precision of 80 m.

The observation strategies and operation procedures have been designed to optimize the data-volume and guarantee the global mapping considering the MPO orbit.

Multiple calibrations have been performed on-ground and they will be repeated during the mission to improve the instrument performance: the dark side of the planet will be exploited for dark calibrations while stellar fields will be acquired to perform geometrical and radiometric calibrations.

Paper Details

Date Published: 12 July 2019
PDF: 17 pages
Proc. SPIE 11180, International Conference on Space Optics — ICSO 2018, 1118042 (12 July 2019); doi: 10.1117/12.2536065
Show Author Affiliations
Emanuele Simioni, INAF – Osservatorio Astronomico di Padova (Italy)
Vania Da Deppo, INAF, CNR-Istituto di Fotonica e Nanotecnologie (Italy)
Cristina Re, INAF – Osservatorio Astronomico di Padova (Italy)
Maria Teresa Capria, INAF-IAPS (Italy)
Giampiero Naletto, Univ. of Padova, INAF, CNR (Italy)
Gianfranco Forlani, Dept. of Engineering and Architecture (Italy)
Leonardo Tommasi, Leonardo (Italy)
Michele Dami, Leonardo (Italy)
Donato Borrelli, Leonardo (Italy)
Iacopo Ficai Veltroni, Leonardo S.p.A. (Italy)
Matteo Massironi, Univ. of Padova (Italy)
Alessandra Slemer, CNR-Istituto di Fotonica e Nanotecnologie (Italy)
Raffaele Mugnuolo, Ctr. di Geodesia Spaziale (Italy)
Francesco Longo, ASI (Italy)
Gabriele Cremonese, INAF – Osservatorio Astronomico di Padova (Italy)

Published in SPIE Proceedings Vol. 11180:
International Conference on Space Optics — ICSO 2018
Zoran Sodnik; Nikos Karafolas; Bruno Cugny, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?