dc.contributor.author |
Beichman, Charles |
en_US |
dc.date.accessioned |
2004-09-26 |
|
dc.date.available |
2004-09-26 |
|
dc.date.issued |
1997-04-24 |
en_US |
dc.identifier.citation |
Blois, France |
en_US |
dc.identifier.clearanceno |
97-0506 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/22058 |
|
dc.description.abstract |
The Terrestrial Planet Finder (TPF) missions has as its goal the detection and characterization of earth-like planets around nearby stars. NASA is currently funding a number of small studies to look at the trade-offs in the design of TPF. The possible trade-offs include orbit location (1 to 5 AU), aperture size (6 to 1.5m), physically connected baselines or separated spacecraft flying in close formation. |
en_US |
dc.format.extent |
10341 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
Planet Finder earth-like planets zodiacal dust cloud |
en_US |
dc.title |
The Terrestrial Planet Finder |
en_US |