Proceedings Paper
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Paper Abstract
In June 2012, Euclid, ESA's Cosmology mission was approved for implementation. Afterwards the industrial contracts were signed for the payload module and the spacecraft prime, and the mission requirements consolidated. We present the status of the mission in the light of the design solutions adopted by the contractors. The performances of the spacecraft in its operation, the telescope assembly, the scientific instruments as well as the data-processing have been carefully budgeted to meet the demanding scientific requirements. We give an overview of the system and where necessary the key items for the interfaces between the subsystems.
Paper Details
Date Published: 2 August 2014
PDF: 8 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91430H (2 August 2014); doi: 10.1117/12.2054883
Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann Jr.; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)
PDF: 8 pages
Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 91430H (2 August 2014); doi: 10.1117/12.2054883
Show Author Affiliations
R. Laureijs, European Space Research and Technology Ctr. (Netherlands)
G. Racca, European Space Research and Technology Ctr. (Netherlands)
L. Stagnaro, European Space Research and Technology Ctr. (Netherlands)
J.-C. Salvignol, European Space Research and Technology Ctr. (Netherlands)
J. Lorenzo Alvarez, European Space Research and Technology Ctr. (Netherlands)
G. Saavedra Criado, European Space Research and Technology Ctr. (Netherlands)
L. Gaspar Venancio, European Space Research and Technology Ctr. (Netherlands)
A. Short, European Space Research and Technology Ctr. (Netherlands)
P. Strada, European Space Research and Technology Ctr. (Netherlands)
C. Colombo, European Space Research and Technology Ctr. (Netherlands)
G. Buenadicha, European Space Astronomy Ctr. (Spain)
J. Hoar, European Space Astronomy Ctr. (Spain)
R. Kohley, European Space Astronomy Ctr. (Spain)
R. Vavrek, European Space Astronomy Ctr. (Spain)
Y. Mellier, Institut d'Astrophysique de Paris (France)
CEA/Service d'Astrophysique (France)
M. Berthe, CEA/Service d’Astrophysique (France)
G. Racca, European Space Research and Technology Ctr. (Netherlands)
L. Stagnaro, European Space Research and Technology Ctr. (Netherlands)
J.-C. Salvignol, European Space Research and Technology Ctr. (Netherlands)
J. Lorenzo Alvarez, European Space Research and Technology Ctr. (Netherlands)
G. Saavedra Criado, European Space Research and Technology Ctr. (Netherlands)
L. Gaspar Venancio, European Space Research and Technology Ctr. (Netherlands)
A. Short, European Space Research and Technology Ctr. (Netherlands)
P. Strada, European Space Research and Technology Ctr. (Netherlands)
C. Colombo, European Space Research and Technology Ctr. (Netherlands)
G. Buenadicha, European Space Astronomy Ctr. (Spain)
J. Hoar, European Space Astronomy Ctr. (Spain)
R. Kohley, European Space Astronomy Ctr. (Spain)
R. Vavrek, European Space Astronomy Ctr. (Spain)
Y. Mellier, Institut d'Astrophysique de Paris (France)
CEA/Service d'Astrophysique (France)
M. Berthe, CEA/Service d’Astrophysique (France)
J. Amiaux, CEA/Service d’Astrophysique (France)
M. Cropper, Mullard Space Science Lab., Univ. College London (United Kingdom)
S. Niemi, Mullard Space Science Lab., Univ. College London (United Kingdom)
S. Pottinger, Mullard Space Science Lab., Univ. College London (United Kingdom)
A. Ealet, Lab. d'Astrophysique de Marseille (France)
K. Jahnke, Max-Planck-Institut für Astronomie (Germany)
T. Maciaszek, Observatoire Astronomique de Marseille-Provence (France)
F. Pasian, INAF - Osservatorio Astronomico di Trieste (Italy)
M. Sauvage, CEA/Service d’Astrophysique (France)
S. Wachter, Max-Planck-Institut für Astronomie (Germany)
U. Israelsson, Jet Propulsion Lab. (United States)
W. Holmes, Jet Propulsion Lab. (United States)
M. Seiffert, Jet Propulsion Lab. (United States)
V. Cazaubiel, Airbus Defence and Space (France)
A. Anselmi, Thales Alenia Space (Italy)
P. Musi, Thales Alenia Space (Italy)
M. Cropper, Mullard Space Science Lab., Univ. College London (United Kingdom)
S. Niemi, Mullard Space Science Lab., Univ. College London (United Kingdom)
S. Pottinger, Mullard Space Science Lab., Univ. College London (United Kingdom)
A. Ealet, Lab. d'Astrophysique de Marseille (France)
K. Jahnke, Max-Planck-Institut für Astronomie (Germany)
T. Maciaszek, Observatoire Astronomique de Marseille-Provence (France)
F. Pasian, INAF - Osservatorio Astronomico di Trieste (Italy)
M. Sauvage, CEA/Service d’Astrophysique (France)
S. Wachter, Max-Planck-Institut für Astronomie (Germany)
U. Israelsson, Jet Propulsion Lab. (United States)
W. Holmes, Jet Propulsion Lab. (United States)
M. Seiffert, Jet Propulsion Lab. (United States)
V. Cazaubiel, Airbus Defence and Space (France)
A. Anselmi, Thales Alenia Space (Italy)
P. Musi, Thales Alenia Space (Italy)
Published in SPIE Proceedings Vol. 9143:
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Jacobus M. Oschmann Jr.; Mark Clampin; Giovanni G. Fazio; Howard A. MacEwen, Editor(s)
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