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The EDdington Mission

Published online by Cambridge University Press:  26 May 2016

Ian Roxburgh
Affiliation:
Astronomy Unit, Queen Mary, University of London, E1 4NS, UK Observatoire de Paris, Place Jules Janssen, 92195 Meudon, France
Fabio Favata
Affiliation:
Astrophysics Division, ESTEC, ESA, Noordwijk, The Netherlands

Abstract

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The Eddington mission was given full approval by the European Space Agency on the 23rd May 2002, as part of the new “Cosmic Vision” Science programme, with launch scheduled for 2007. Its twin science objectives are asteroseismology and planet finding. In its current design it consists of 4 × 60 cm folded Schmidt telescopes, each with 5° × 5° field of view and its own CCD array camera. The current observing plan is to spend 2 years primarily devoted to asteroseismology with 1–3 months on different target fields monitoring up to 50,000 stars per field, and 3 years continuously on a single target field monitoring upwards of 100,000 stars as required for planet searching. The asteroseismic goal is to be able to detect oscillations frequencies with a precision 0.1–0.3 μHz.

Type
Session 3 Rotation, Solar and Stellar Physics
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Favata, F., Roxburgh, I. W. and Christensen-Dalsgaard, J. eds, 2000. with Aerts, C., Antonello, E., Catala, C., Deeg, H., Gimenez, A., Grenon, M., Pace, O., Penny, A., Schneider, J., Waltham, N., Eddington, A Mission to Map Stellar Evolution through Oscillations and to Find Habitable Planets, Report of Assessment Study, ESA-SCI(2000)8 Google Scholar
Roxburgh, I. W., Christensen Dalsgaard, J. and Favata, F., eds 2000. with Antonello, E., Baade, D., Badiali, M., Baglin, A., Bedding, T., Brown, T., Catala, C., Collier, A., Dziembowski, W., Gilmore, G., Gimenez, A., Gough, D., Horne, K., Kjelsden, H., Leger, A., Penny, A., Preite-Matinez, A., Rivinus, Th., Schneider, J., Stefl, Z., Sterken, C., Weiss, W. Eddington - A Stellar Physics and Planet Finder Explorer. Proposal submitted to ESA in response to the ESA F2/F3 call for proposals.Google Scholar