Overview of Technologies for Direct Optical Imaging of Exoplanets
Creators
Abstract
The execution of a mission as ambitious and challenging as finding indications of life on planets around other stars requires careful evaluation of potential technological approaches. Following the strong endorsement from the last decadal survey on Astronomy and Astrophysics for the New Millennium (2001), NASA pursued a vigorous TPF program with nearly $150M community investment over the last decade in science, technology and mission studies. After a 3-year head-to-head comparison of exoplanet missions using direct optical imaging and mid-infra red (mid-IR) interferometry, NASA endorsed a visible imaging coronagraphic concept as the first of its exoplanet characterization missions in 2004.
Additional Information
© 2009. The work described in this report was performed at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.Attached Files
Published - Levine_Visible_Planet_Imaging_TEC_EOS.pdf
Files
Levine_Visible_Planet_Imaging_TEC_EOS.pdf
Additional details
Identifiers
- Eprint ID
- 57854
- Resolver ID
- CaltechAUTHORS:20150527-103313767
Related works
- Describes
- http://adsabs.harvard.edu//abs/2009astro2010T..37L (URL)
Funding
- NASA/JPL/Caltech
Dates
- Created
-
2015-05-27Created from EPrint's datestamp field
- Updated
-
2021-08-20Created from EPrint's last_modified field
Caltech Custom Metadata
- Series Name
- Technology Development Papers
- Series Volume or Issue Number
- 37