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Proceedings Paper

The satellite formation flying in lab: PROBA-3/ASPIICS metrology subsystems test-bed
Author(s): G. Capobianco; D. Loreggia; S. Fineschi; M. Focardi; A. Bemporad; M. Casti; V. Noce; F. Landini; C. Baccani; M. Pancrazzi; M. Romoli; G. Massone; G. Nicolini; S. Buckley; K. O'Neill; I. Cernica; M. Purica; E. Budianu; C. Thizy; J.-S. Servaye; I. Mechmech; Etienne Renotte
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Paper Abstract

Formation flying is one of the most promising techniques for the future of astronomy and astrophysics from the space. The capabilities of the rockets strongly affect the dimensions and the weights of telescopes and instrumentation to be launched. Telescopes composed by several smallest satellites in formation flying, could be the key for build big space telescopes. With this aim, the ESA PROBA-3 mission will demonstrate the capabilities of this technology, maintaining two satellites aligned within 1 mm (longitudinal) when the nominal distance between the two is of around 144m. The scientific objective of the mission is the observation of the solar corona down to 1.08 solar radii. The Coronagraph Spacecraft (CSC) will observe the Sun, when the second spacecraft, the Occulter Spacecraft (OSC) will work as an external occulter, eclipsing to the CSC the sun disk. The finest metrology sub-systems, the Shadow Position Sensors (SPS) and the Occulter Position Sensor Emitters (OPSE) identifying respectively the CSC-Sun axis and the formation flying (i.e., CSC-OSC) axis will be considered here. In particular, this paper is dedicated to the test-bed for the characterization, the performance analysis and the algorithms capabilities analysis of the both the metrology subsystems. The test-bed is able to simulate the different flight conditions of the two spacecraft and will give the opportunity to check the response of the subsystems in the conditions as close as possible to the flight ones.

Paper Details

Date Published: 29 July 2016
PDF: 6 pages
Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99046E (29 July 2016); doi: 10.1117/12.2233207
Show Author Affiliations
G. Capobianco, INAF - Astrophysical Observatory of Turin (Italy)
D. Loreggia, INAF - Astrophysical Observatory of Turin (Italy)
S. Fineschi, INAF - Astrophysical Observatory of Turin (Italy)
M. Focardi, INAF - OAA Arcetri Astrophysical Observatory (Italy)
A. Bemporad, INAF - Astrophysical Observatory of Turin (Italy)
M. Casti, ALTEC - Advanced Logistics Technology Engineering Ctr. (Italy)
V. Noce, INAF - OAA Arcetri Astrophysical Observatory (Italy)
F. Landini, INAF - OAA Arcetri Astrophysical Observatory (Italy)
C. Baccani, Univ. of Florence (Italy)
M. Pancrazzi, INAF - OAA Arcetri Astrophysical Observatory (Italy)
M. Romoli, Univ. of Florence (Italy)
G. Massone, INAF - Astrophysical Observatory of Turin (Italy)
G. Nicolini, INAF - Astrophysical Observatory of Turin (Italy)
S. Buckley, SensL (Ireland)
K. O'Neill, SensL (Ireland)
I. Cernica, National Institute for Research and Development in Microtechnologies (Romania)
M. Purica, National Institute for Research and Development in Microtechnologies (Romania)
E. Budianu, National Institute for Research and Development in Microtechnologies, (Romania)
C. Thizy, Ctr. Spatial de Liège (Belgium)
J.-S. Servaye, Ctr. Spatial de Liège (Belgium)
I. Mechmech, Ctr. Spatial de Liège (Belgium)
Etienne Renotte, Ctr. Spatial de Liège (Belgium)


Published in SPIE Proceedings Vol. 9904:
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Howard A. MacEwen; Giovanni G. Fazio; Makenzie Lystrup; Natalie Batalha; Nicholas Siegler; Edward C. Tong, Editor(s)

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