Paper
24 July 1998 Terrestrial Planet Finder: the search for life-bearing planets around other stars
Author Affiliations +
Abstract
The Terrestrial Planet Finder (TPF) will detect and characterize Earth-like planets around nearby stars. NASA is currently funding a number of small studies to look at trade-offs in the design of TPF. The possible trade-offs include orbit location (1 to 5 AU), aperture size (4 to 2 m), and physically connected baselines vs. separated spacecraft flying in close formation. The performance of TPF depends critically on the brightness of the local zodiacal dust cloud at the observing site, and on the brightness and degree of structure in the zodiacal dust cloud around other stars. Sensitivity calculations indicate that TPF could accomplish its goals using 4-5 m telescopes operating at 1 AU. Such a mission would have many advantages relative to a mission operating smaller telescopes in lower background conditions at 5 AU.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Charles A. Beichman "Terrestrial Planet Finder: the search for life-bearing planets around other stars", Proc. SPIE 3350, Astronomical Interferometry, (24 July 1998); https://doi.org/10.1117/12.317137
Lens.org Logo
CITATIONS
Cited by 40 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Planets

Stars

Space telescopes

Telescopes

Clouds

Solar system

Interferometers

RELATED CONTENT

Darwin interferometer
Proceedings of SPIE (July 24 1998)
New Worlds Observer: Minotaur to Ares V
Proceedings of SPIE (July 12 2008)
A roadmap for NASA's search for other Earths
Proceedings of SPIE (August 31 2005)
SIM Lite Astrometric Observatory progress report
Proceedings of SPIE (July 21 2010)

Back to Top