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Coronagraphic Imaging of Debris Disks From a High Altitude Balloon Platform

Unwin, Stephen and Traub, Wesley and Bryden, Geoffrey and Brugarolas, Paul and Chen, Pin and Guyon, Olivier and Hillenbrand, Lynne and Krist, John and Macintosh, Bruce and Mawet, Dimitri and Mennesson, Bertrand and Moody, Dwight and Roberts, Lewis C., Jr. and Stapelfeldt, Karl and Stuchlik, David and Trauger, John and Vasisht, Gautam (2012) Coronagraphic Imaging of Debris Disks From a High Altitude Balloon Platform. In: Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave. Proceedings of SPIE. No.8442. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 84420G. ISBN 9780819491435. https://resolver.caltech.edu/CaltechAUTHORS:20150522-083914095

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Abstract

Debris disks around nearby stars are tracers of the planet formation process, and they are a key element of our understanding of the formation and evolution of extrasolar planetary systems. With multi-color images of a significant number of disks, we can probe important questions: can we learn about planetary system evolution; what materials are the disks made of; and can they reveal the presence of planets? Most disks are known to exist only through their infrared flux excesses as measured by the Spitzer Space Telescope, and through images measured by Herschel. The brightest, most extended disks have been imaged with HST, and a few, such as Fomalhaut, can be observed using ground-based telescopes. But the number of good images is still very small, and there are none of disks with densities as low as the disk associated with the asteroid belt and Edgeworth­ Kuiper belt in our own Solar System. Direct imaging of disks is a major observational challenge, demanding high angular resolution and extremely high dynamic range close to the parent star. The ultimate experiment requires a space-based platform, but demonstrating much of the needed technology, mitigating the technical risks of a space-based coronagraph, and performing valuable measurements of circumstellar debris disks, can be done from a high-altitude balloon platform. In this paper we present a balloon-borne telescope concept based on the Zodiac II design that could undertake compelling studies of a sample of debris disks.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.924175DOIArticle
ORCID:
AuthorORCID
Guyon, Olivier0000-0002-1097-9908
Macintosh, Bruce0000-0003-1212-7538
Mawet, Dimitri0000-0002-8895-4735
Mennesson, Bertrand0000-0003-4205-4800
Roberts, Lewis C., Jr.0000-0003-3892-2900
Stapelfeldt, Karl0000-0002-2805-7338
Vasisht, Gautam0000-0002-1871-6264
Additional Information:© 2012 Society of Photo-Optical Instrumentation Engineers (SPIE). August 22, 2012. Some of the research described in this publication was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:Suborbital, Coronagraph, Debris Disks, Exoplanets
Series Name:Proceedings of SPIE
Issue or Number:8442
DOI:10.1117/12.924175
Record Number:CaltechAUTHORS:20150522-083914095
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150522-083914095
Official Citation:Stephen Unwin ; Wesley Traub ; Geoffrey Bryden ; Paul Brugarolas ; Pin Chen, et al. " Coronagraphic imaging of debris disks from a high altitude balloon platform ", Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84420G (August 22, 2012); doi:10.1117/12.924175
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:57765
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:22 May 2015 20:32
Last Modified:10 Nov 2021 21:54

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