Home > Research > Publications & Outputs > SIMBIO-SYS

Links

Text available via DOI:

View graph of relations

SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission. / Cremonese, G.; Capaccioni, F.; Capria, M.T. et al.
In: Space Science Reviews, Vol. 216, No. 5, 75, 17.06.2020.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Cremonese, G, Capaccioni, F, Capria, MT, Doressoundiram, A, Palumbo, P, Vincendon, M, Massironi, M, Debei, S, Zusi, M, Altieri, F, Amoroso, M, Aroldi, G, Baroni, M, Barucci, A, Bellucci, G, Benkhoff, J, Besse, S, Bettanini, C, Blecka, M, Borrelli, D, Brucato, JR, Carli, C, Carlier, V, Cerroni, P, Cicchetti, A, Colangeli, L, Dami, M, Da Deppo, V, Della Corte, V, De Sanctis, MC, Erard, S, Esposito, F, Fantinel, D, Ferranti, L, Ferri, F, Ficai Veltroni, I, Filacchione, G, Flamini, E, Forlani, G, Fornasier, S, Forni, O, Fulchignoni, M, Galluzzi, V, Gwinner, K, Ip, W, Jorda, L, Langevin, Y, Lara, L, Leblanc, F, Leyrat, C, Li, Y, Marchi, S, Marinangeli, L, Marzari, F, Mazzotta Epifani, E, Mendillo, M, Mennella, V, Mugnuolo, R, Muinonen, K, Naletto, G, Noschese, R, Palomba, E, Paolinetti, R, Perna, D, Piccioni, G, Politi, R, Poulet, F, Ragazzoni, R, Re, C, Rossi, M, Rotundi, A, Salemi, G, Sgavetti, M, Simioni, E, Thomas, N, Tommasi, L, Turella, A, Van Hoolst, T, Wilson, L, Zambon, F, Aboudan, A, Barraud, O, Bott, N, Borin, P, Colombatti, G, El Yazidi, M, Ferrari, S, Flahaut, J, Giacomini, L, Guzzetta, L, Lucchetti, A, Martellato, E, Pajola, M, Slemer, A, Tognon, G & Turrini, D 2020, 'SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission', Space Science Reviews, vol. 216, no. 5, 75. https://doi.org/10.1007/s11214-020-00704-8

APA

Cremonese, G., Capaccioni, F., Capria, M. T., Doressoundiram, A., Palumbo, P., Vincendon, M., Massironi, M., Debei, S., Zusi, M., Altieri, F., Amoroso, M., Aroldi, G., Baroni, M., Barucci, A., Bellucci, G., Benkhoff, J., Besse, S., Bettanini, C., Blecka, M., ... Turrini, D. (2020). SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission. Space Science Reviews, 216(5), Article 75. https://doi.org/10.1007/s11214-020-00704-8

Vancouver

Cremonese G, Capaccioni F, Capria MT, Doressoundiram A, Palumbo P, Vincendon M et al. SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission. Space Science Reviews. 2020 Jun 17;216(5):75. doi: 10.1007/s11214-020-00704-8

Author

Cremonese, G. ; Capaccioni, F. ; Capria, M.T. et al. / SIMBIO-SYS : Scientific Cameras and Spectrometer for the BepiColombo Mission. In: Space Science Reviews. 2020 ; Vol. 216, No. 5.

Bibtex

@article{b115b6ff4b9a4082b66ff5d8a7569b5f,
title = "SIMBIO-SYS: Scientific Cameras and Spectrometer for the BepiColombo Mission",
abstract = "The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well.",
keywords = "BepiColombo, Mercury, Cameras, Hyperspectral imaging, Image resolution, Infrared devices, Interplanetary flight, Ionosphere, Maps, Morphology, Orbits, Photomapping, Spectral resolution, Spectrometers, Spectroscopy, Sulfur compounds, Digital terrain model, European Space Agency, High spatial resolution, High spectral resolution, High-resolution imaging, Instrument performance, Mercury planetary orbiters, Visible and near infrared, Stereo image processing",
author = "G. Cremonese and F. Capaccioni and M.T. Capria and A. Doressoundiram and P. Palumbo and M. Vincendon and M. Massironi and S. Debei and M. Zusi and F. Altieri and M. Amoroso and G. Aroldi and M. Baroni and A. Barucci and G. Bellucci and J. Benkhoff and S. Besse and C. Bettanini and M. Blecka and D. Borrelli and J.R. Brucato and C. Carli and V. Carlier and P. Cerroni and A. Cicchetti and L. Colangeli and M. Dami and {Da Deppo}, V. and {Della Corte}, V. and {De Sanctis}, M.C. and S. Erard and F. Esposito and D. Fantinel and L. Ferranti and F. Ferri and I. Ficai Veltroni and G. Filacchione and E. Flamini and G. Forlani and S. Fornasier and O. Forni and M. Fulchignoni and V. Galluzzi and K. Gwinner and W. Ip and L. Jorda and Y. Langevin and L. Lara and F. Leblanc and C. Leyrat and Y. Li and S. Marchi and L. Marinangeli and F. Marzari and E. Mazzotta Epifani and M. Mendillo and V. Mennella and R. Mugnuolo and K. Muinonen and G. Naletto and R. Noschese and E. Palomba and R. Paolinetti and D. Perna and G. Piccioni and R. Politi and F. Poulet and R. Ragazzoni and C. Re and M. Rossi and A. Rotundi and G. Salemi and M. Sgavetti and E. Simioni and N. Thomas and L. Tommasi and A. Turella and {Van Hoolst}, T. and L. Wilson and F. Zambon and A. Aboudan and O. Barraud and N. Bott and P. Borin and G. Colombatti and M. El Yazidi and S. Ferrari and J. Flahaut and L. Giacomini and L. Guzzetta and A. Lucchetti and E. Martellato and M. Pajola and A. Slemer and G. Tognon and D. Turrini",
year = "2020",
month = jun,
day = "17",
doi = "10.1007/s11214-020-00704-8",
language = "English",
volume = "216",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Netherlands",
number = "5",

}

RIS

TY - JOUR

T1 - SIMBIO-SYS

T2 - Scientific Cameras and Spectrometer for the BepiColombo Mission

AU - Cremonese, G.

AU - Capaccioni, F.

AU - Capria, M.T.

AU - Doressoundiram, A.

AU - Palumbo, P.

AU - Vincendon, M.

AU - Massironi, M.

AU - Debei, S.

AU - Zusi, M.

AU - Altieri, F.

AU - Amoroso, M.

AU - Aroldi, G.

AU - Baroni, M.

AU - Barucci, A.

AU - Bellucci, G.

AU - Benkhoff, J.

AU - Besse, S.

AU - Bettanini, C.

AU - Blecka, M.

AU - Borrelli, D.

AU - Brucato, J.R.

AU - Carli, C.

AU - Carlier, V.

AU - Cerroni, P.

AU - Cicchetti, A.

AU - Colangeli, L.

AU - Dami, M.

AU - Da Deppo, V.

AU - Della Corte, V.

AU - De Sanctis, M.C.

AU - Erard, S.

AU - Esposito, F.

AU - Fantinel, D.

AU - Ferranti, L.

AU - Ferri, F.

AU - Ficai Veltroni, I.

AU - Filacchione, G.

AU - Flamini, E.

AU - Forlani, G.

AU - Fornasier, S.

AU - Forni, O.

AU - Fulchignoni, M.

AU - Galluzzi, V.

AU - Gwinner, K.

AU - Ip, W.

AU - Jorda, L.

AU - Langevin, Y.

AU - Lara, L.

AU - Leblanc, F.

AU - Leyrat, C.

AU - Li, Y.

AU - Marchi, S.

AU - Marinangeli, L.

AU - Marzari, F.

AU - Mazzotta Epifani, E.

AU - Mendillo, M.

AU - Mennella, V.

AU - Mugnuolo, R.

AU - Muinonen, K.

AU - Naletto, G.

AU - Noschese, R.

AU - Palomba, E.

AU - Paolinetti, R.

AU - Perna, D.

AU - Piccioni, G.

AU - Politi, R.

AU - Poulet, F.

AU - Ragazzoni, R.

AU - Re, C.

AU - Rossi, M.

AU - Rotundi, A.

AU - Salemi, G.

AU - Sgavetti, M.

AU - Simioni, E.

AU - Thomas, N.

AU - Tommasi, L.

AU - Turella, A.

AU - Van Hoolst, T.

AU - Wilson, L.

AU - Zambon, F.

AU - Aboudan, A.

AU - Barraud, O.

AU - Bott, N.

AU - Borin, P.

AU - Colombatti, G.

AU - El Yazidi, M.

AU - Ferrari, S.

AU - Flahaut, J.

AU - Giacomini, L.

AU - Guzzetta, L.

AU - Lucchetti, A.

AU - Martellato, E.

AU - Pajola, M.

AU - Slemer, A.

AU - Tognon, G.

AU - Turrini, D.

PY - 2020/6/17

Y1 - 2020/6/17

N2 - The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well.

AB - The SIMBIO-SYS (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) is a complex instrument suite part of the scientific payload of the Mercury Planetary Orbiter for the BepiColombo mission, the last of the cornerstone missions of the European Space Agency (ESA) Horizon + science program. The SIMBIO-SYS instrument will provide all the science imaging capability of the BepiColombo MPO spacecraft. It consists of three channels: the STereo imaging Channel (STC), with a broad spectral band in the 400-950 nm range and medium spatial resolution (at best 58 m/px), that will provide Digital Terrain Model of the entire surface of the planet with an accuracy better than 80 m; the High Resolution Imaging Channel (HRIC), with broad spectral bands in the 400-900 nm range and high spatial resolution (at best 6 m/px), that will provide high-resolution images of about 20% of the surface, and the Visible and near-Infrared Hyperspectral Imaging channel (VIHI), with high spectral resolution (6 nm at finest) in the 400-2000 nm range and spatial resolution reaching 120 m/px, it will provide global coverage at 480 m/px with the spectral information, assuming the first orbit around Mercury with periherm at 480 km from the surface. SIMBIO-SYS will provide high-resolution images, the Digital Terrain Model of the entire surface, and the surface composition using a wide spectral range, as for instance detecting sulphides or material derived by sulphur and carbon oxidation, at resolutions and coverage higher than the MESSENGER mission with a full co-alignment of the three channels. All the data that will be acquired will allow to cover a wide range of scientific objectives, from the surface processes and cartography up to the internal structure, contributing to the libration experiment, and the surface-exosphere interaction. The global 3D and spectral mapping will allow to study the morphology and the composition of any surface feature. In this work, we describe the on-ground calibrations and the results obtained, providing an important overview of the instrument performances. The calibrations have been performed at channel and at system levels, utilizing specific setup in most of the cases realized for SIMBIO-SYS. In the case of the stereo camera (STC), it has been necessary to have a validation of the new stereo concept adopted, based on the push-frame. This work describes also the results of the Near-Earth Commissioning Phase performed few weeks after the Launch (20 October 2018). According to the calibration results and the first commissioning the three channels are working very well.

KW - BepiColombo

KW - Mercury

KW - Cameras

KW - Hyperspectral imaging

KW - Image resolution

KW - Infrared devices

KW - Interplanetary flight

KW - Ionosphere

KW - Maps

KW - Morphology

KW - Orbits

KW - Photomapping

KW - Spectral resolution

KW - Spectrometers

KW - Spectroscopy

KW - Sulfur compounds

KW - Digital terrain model

KW - European Space Agency

KW - High spatial resolution

KW - High spectral resolution

KW - High-resolution imaging

KW - Instrument performance

KW - Mercury planetary orbiters

KW - Visible and near infrared

KW - Stereo image processing

U2 - 10.1007/s11214-020-00704-8

DO - 10.1007/s11214-020-00704-8

M3 - Journal article

VL - 216

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

IS - 5

M1 - 75

ER -