Keller, H.U. and Barberieri, C. and Lamy, P- and Rickman, H. and Rodrigo, R. and Wenzel, K.-P. and Sierks, H. and A´Hearn, M. F. and Angrilli, F. and Angulo, M. and Bailey, M. E. and Barthol, P. and Barucci, M. A. and Bertaux, J.-L. and Bianchini, G. and Boit, J.-L. and Brown, V. and Burns, J. A. and Büttner, I. and Castro, J. M. and Cremonese, G. and Curdt, W. and da Deppo, V. and Debei, S. and de Cecco, M. and Dohlen, K. and Fornasier, S. and Fulle, M. and Germerott, D. and Gliem, F. and Guizzo, G. P. and Hviid, S. F. and Ip, W.-H- and Jorda, L. and Koschny, D. and Kramm, J. R. and Kührt, E. and Küppers, M. and Lara, L.-M. and Llebaria, A. and Lopez, A. and Lopez-Jimenes, A. and Lopez-Moreno, J. and Meller, R. and Michalik, H. and Michelena, M. D. and Müller, R. and Naletto, G. and Origne, A. and Parzianello, G. and Pertile, M. and Quintana, C. and Ragazzoni, R. and Ramous, P. and Reiche, K.-U. and Reina, M. and Rodriguez, J. and Rousset, G. and Sabau, L. and Sanz, A. and Sivan, J.-P. and Stöckner, K. and Tabero, J. and Telljohann, U. and Thomas, N. and Timon, V. and Tomasch, G. and Wittrock, T. and Zaccariotto, U. (2006) OSIRIS - The Scientific Camera System Onboard Rosetta. Space Science Reviews, 128 (1/4), p. 433. DOI: 10.1007/s11214-006-9128-4.
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The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS is the scientific camerasystem onboard the Rosetta spacecraft. OSIRIS will detect 67P/Churyumov-Gerasimenko from a distance of more than 10<sup>6</sup> km,characterise the comet shape and volume, its rotational state and find a suitable landing spot for Philae, the Rosetta lander. OSIRIS will observe the nucleus, its activity and surroundings down to a scale of about 2 cm px<sup>-1</sup>. The observation will begin well before the onset of activity and will extend over month until the comet reaches perihelion. During the rendevous episode of the Rosetta mission, OSIRIS will provide key information about the nature of cometary nuclei and reveal the physics of cometary activity that leads to the gas and dust coma. OSIRIS comprises a high resolution Narrow Angel Camera unit and a Wide Angel Camera unit accompanied by three electronics boxes. The two units use identical shutter, filter wheel, front door, and detector systems. They are operated by a common Data Processing Unit. The OSIRIS instrument has a total mass of 35 kg and is provided by six European countries.
|Title:||OSIRIS - The Scientific Camera System Onboard Rosetta|
|Date:||24 March 2006|
|Journal or Publication Title:||Space Science Reviews|
|In ISI Web of Science:||Yes|
|Page Range:||p. 433|
|Keywords:||Rosetta, Osiris, camera system, comet|
|HGF - Research field:||Aeronautics, Space and Transport (old)|
|HGF - Program:||Space (old)|
|HGF - Program Themes:||W EW - Erforschung des Weltraums|
|DLR - Research area:||Space|
|DLR - Program:||W EW - Erforschung des Weltraums|
|DLR - Research theme (Project):||W - Projekt ROSETTA Instrumente (old)|
|Institutes and Institutions:||Institute of Planetary Research > Asteroids and Comets|
|Deposited By:||Dr.rer.nat. Ekkehard Kührt|
|Deposited On:||16 Jul 2007|
|Last Modified:||14 Jan 2010 23:16|
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