CORONAGRAPH
Coronagraph specifications
A starlight suppression level of 10⁻¹⁰ or better will be reached at any separation between the specified inner and outer working angles (IWA/OWA) around the star of interest. The coronagraph instrument will be mostly used for exoplanet detection and orbit determination.
HABEX INSTRUMENTS SUITE
Workhorse Camera
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UV Spectrograph
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Coronagraph
Starshade
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Who To Contact
For Science, Press please contact:
Scott Gaudi: gaudi.1@osu.edu
Sara Seager: seager@mit.edu
Bertrand Mennesson: Bertrand.Mennesson@jpl.nasa.gov
Scott Gaudi: gaudi.1@osu.edu
Sara Seager: seager@mit.edu
Bertrand Mennesson: Bertrand.Mennesson@jpl.nasa.gov