Hostname: page-component-7bb8b95d7b-lvwk9 Total loading time: 0 Render date: 2024-09-19T10:26:40.930Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectroscopy with the Terrestrial Planet Finder Coronagraph

Published online by Cambridge University Press:  02 May 2006

Sara R. Heap
Sara R. Heap
Affiliation:
Exploration of the Universe Division, Goddard Space Flight Center, Greenbelt MD, USA email: Sally.Heap@NASA.gov
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We describe the rationale and requirements for an integral-field spectrograph aboard NASA's Terrestrial Planet Finder Coronagraph.

Keywords

space vehicles: instruments(stars:) planetary systems(stars:) planetary systems: formation(stars:) planetary systems: protoplanetary disksinstrumentation: spectrographsinstrumentation: detectorstechniques: image processingplanets and satellites: generalastrobiology
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Colloquium C200: Direct Imaging of Exoplanets: Science & Techniques , October 2005 , pp. 529 - 534
Copyright
© 2006 International Astronomical Union