Title of article
Optical performance of the New Worlds Occulter
Author/Authors
David Arenberg، نويسنده , , Jonathan W. and Lo، نويسنده , , Amy S. and Glassman، نويسنده , , Tiffany M. and Cash، نويسنده , , Webster، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2007
Pages
10
From page
438
To page
447
Abstract
The New Worlds Observer (NWO) is a multiple spacecraft mission that is capable of detecting and characterizing extra-solar planets and planetary systems. NWO consists of an external occulter and a generic space telescope, flying in tandem. The external occulter has specific requirements on its shape and size, while the telescope needs no special modification beyond that required to do high-quality astrophysical observations. The occulter is a petal-shaped, opaque screen that creates a high-suppression shadow large enough to accommodate the telescope. This article reports on the optical performance of the novel New Worlds occulter design. It also introduces two new aspects of its optical performance which enhance the detectability of extra-solar planets. We also include a brief discussion of the buildability and the tolerances of the occulter. It is also shown that an occulter design can be found for any set of science requirements. We show that NWO is a viable mission concept for the study of extra-solar planets. To cite this article: J.W. Arenberg et al., C. R. Physique 8 (2007).
Keywords
Tolerancing , Contrast ratio , Tolérance , Occulter , Exoplanet detection , New Worlds Observer , New Worlds Observer , Inner working angle , Occulteur , Détection des exoplanètes , Rapport de contrast
Journal title
Comptes Rendus Physique
Serial Year
2007
Journal title
Comptes Rendus Physique
Record number
2283839
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