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Proceedings Article

Status of the terrestrial planet finder interferometer (TPF-I)

[+] Author Affiliations
Charles Beichman

Michelson Science Ctr., California Institute of Technology

Peter Lawson, Oliver Lay, Asif Ahmed, Steve Unwin

Jet Propulsion Lab.

K. Johnston

U.S. Naval Observatory

Proc. SPIE 6268, Advances in Stellar Interferometry, 62680S (June 27, 2006); doi:10.1117/12.673583
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From Conference Volume 6268

  • Advances in Stellar Interferometry
  • John D. Monnier; Markus Schöller; William C. Danchi
  • Orlando, Florida , USA | May 24, 2006

abstract

The interferometric version of the Terrestrial Planet Finder (TPF-I) has the potential to find and characterize earth-sized planets in the habitable zones of over 250 nearby stars and to search for life using biomarkers in the atmospheres of any planets found. The scientific case for such a mission continues to be strengthened by on-going progress in the detection of planets via indirect means. This paper summarizes the status of TPF-I, illustrative scientific requirements for the mission, and its enabling technologies.

© (2006) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Charles Beichman ; Peter Lawson ; Oliver Lay ; Asif Ahmed ; Steve Unwin, et al.
"Status of the terrestrial planet finder interferometer (TPF-I)", Proc. SPIE 6268, Advances in Stellar Interferometry, 62680S (June 27, 2006); doi:10.1117/12.673583; http://dx.doi.org/10.1117/12.673583


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