Terrestrial Planet Finding with a Visible Light Coronagraph
@article{Kuchner2003TerrestrialPF, title={Terrestrial Planet Finding with a Visible Light Coronagraph}, author={Marc J. Kuchner and David N. Spergel}, journal={arXiv: Astrophysics}, year={2003} }
Directly imaging extrasolar planets using a monolithic optical telescope avoids many pitfalls of space interferometry and opens up the prospect of visible light studies of extrasolar planetary systems. Future astronomical missions may require interferometry for high spatial resolution, but given that the first direct imaging missions will probably fit into a single launch vehicle, the astrophysics of planet finding calls for a visible light coronagraph as the first space mission to search for…
Figures from this paper
7 Citations
The New Worlds Observer: a mission for high-resolution spectroscopy of extra-solar terrestrial planets
- PhysicsSPIE Astronomical Telescopes + Instrumentation
- 2004
The New Worlds Observer (NWO) is a proposed space mission to provide high resolution spectroscopy from the far UV to the near IR of extra-solar terrestrial sized planets. The design of NWO is based…
Optical coronagraph testbed requirements and design for exoplanet and star simulation
- Physics, GeologySPIE Astronomical Telescopes + Instrumentation
- 2004
The telescope for a Terrestrial Planet Finder (TPF) coronagraph has exceedingly stringent phase and amplitude requirements, especially for the large, monolithic primary mirror (possibly as large as 4…
Optical requirements for a Terrestrial Planet Finder optical coronagraph primary mirror
- PhysicsSPIE Optics + Photonics
- 2003
One possible implementation of an optical coronagraphic approach to finding exo-solar planets incorporates a large, monolithic primary mirror (PM) that is approximately 4 meters by 10 meters in size.…
Pupil Mapping in Two Dimensions for High-Contrast Imaging
- Physics
- 2005
Pupil mapping is a technique whereby a uniformly illuminated input pupil, such as from starlight, can be mapped into a nonuniformly illuminated exit pupil, such that the image formed from this pupil…
MEMS Deformable Mirrors for Adaptive Optics in Astronomical Imaging
- Physics
- 2006
We report on the development of micro-electromechanical (MEMS) deformable mirrors designed for ground and space-based astronomical instruments intended for imaging extra-solar planets. Three…
Astronomical imaging with EMCCDs using long exposures
- PhysicsAstronomical Telescopes and Instrumentation
- 2013
Astronomical imaging is always limited by the detection system signal-to-noise ratio (SNR). EMCCD cameras offer many advantages for low light applications, such as sub-electron read-out noise, and…
References
Biosignatures and Planetary Properties to be Investigated by the TPF Mission
- Physics, Geology
- 2002
Abstract iiiI. Basic Science Goals of TPF and the Broad Diversity of Terrestrial Planets 1II. Interpretation of Visible and IR Spectra of Terrestrial Planets 3Introduction 3General Discussion…