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Fourier-Kelvin stellar interferometer (FKSI): a progress report and preliminary results from our nulling testbed

Barry, R. K. and Danchi, W. C. and Chambers, V. J. and Rajagopal, J. and Richardson, L. J. and Martino, A. and Deming, D. and Kuchner, M. and Linfield, R. and Millan-Gabet, R. and Lee, L. A. and Monnier, J. D. and Mundy, L. G. and Noecker, C. and Seager, S. and Wallace, D. J. and Allen, R. J. and Traub, W. A. and Ford, H. C. (2005) Fourier-Kelvin stellar interferometer (FKSI): a progress report and preliminary results from our nulling testbed. In: Techniques and Instrumentation for Detection of Exoplanets II. Proceedings of SPIE. No.5905. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 59050Z. ISBN 9780819459107. https://resolver.caltech.edu/CaltechAUTHORS:20190122-075634496

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Abstract

The Fourier-Kelvin Stellar Interferometer (FKSI) is a mission concept for an imaging and nulling interferometer for the near infrared to mid-infrared spectral region (3-8 microns). FKSI is a scientific and technological pathfinder to TPF/DARWIN as well as SPIRIT, SPECS, and SAFIR. It will also be a high angular resolution system complementary to JWST. There are four key scientific issues the FKSI mission is designed to address. First, we plan to characterize the atmospheres of the known extra-solar giant planets. Second, we will explore the morphology of debris disks to look for resonant structures to find and characterize extrasolar planets. Third, we will observe young stellar systems to understand their evolution and planet forming potential, and study circumstellar material around a variety of stellar types to better understand their evolutionary state. Finally, we plan to measure detailed structures inside active galactic nuclei. We report results of simulation studies of the imaging capabilities of the FKSI with various configurations of two to five telescopes including the effects of thermal noise and local and exozodiacal dust emission. We also report preliminary results from our symmetric Mach-Zehnder nulling testbed.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.627827DOIArticle
ORCID:
AuthorORCID
Deming, D.0000-0001-5727-4094
Kuchner, M.0000-0002-2387-5489
Millan-Gabet, R.0000-0003-0447-5866
Monnier, J. D.0000-0002-3380-3307
Noecker, C.0000-0003-1417-2383
Seager, S.0000-0002-6892-6948
Additional Information:© 2005 Society of Photo-optical Instrumentation Engineers (SPIE). This work was supported in part by NASA Goddard Space Flight Center’s Internal Research and Development (IRAD) and Director’s Discretionary Fund (DDF) programs.
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Subject Keywords:nulling interferometer, symmetric Mach-Zehnder nuller, extrasolar planets, giant planets, planet formation, debris disk, habitable zone
Series Name:Proceedings of SPIE
Issue or Number:5905
Record Number:CaltechAUTHORS:20190122-075634496
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190122-075634496
Official Citation:R. K. Barry, W. C. Danchi, V. J. Chambers, J. Rajagopal, L. J. Richardson, A. Martino, D. Deming, M. Kuchner, R. Linfield, R. Millan-Gabet, L. A. Lee, J. D. Monnier, L. G. Mundy, C. Noecker, S. Seager, D. J. Wallace, R. J. Allen, W. A. Traub, H. C. Ford, "The Fourier-Kelvin Stellar Interferometer (FKSI): a progress report and preliminary results from our nulling testbed," Proc. SPIE 5905, Techniques and Instrumentation for Detection of Exoplanets II, 59050Z (14 September 2005); doi: 10.1117/12.627827
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92386
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:22 Jan 2019 20:13
Last Modified:28 Oct 2019 23:51

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