Paper published in a book (Scientific congresses and symposiums)
MAPLE: reflected light from exoplanets with a 50-cm diameter stratospheric balloon telescope
Marois, Christian; Bradley, Colin; Pazder, John et al.
2014In Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
 

Files


Full Text
marois-spie-maple.pdf
Author postprint (1.57 MB)
Download

Copyright 2015 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.


All documents in ORBi are protected by a user license.

Send to



Details



Abstract :
[en] Detecting light reflected from exoplanets by direct imaging is the next major milestone in the search for, and characterization of, an Earth twin. Due to the high-risk and cost associated with satellites and limitations imposed by the atmosphere for ground-based instruments, we propose a bottom-up approach to reach that ultimate goal with an endeavor named MAPLE. MAPLE first project is a stratospheric balloon experiment called MAPLE-50. MAPLE-50 consists of a 50 cm diameter off- axis telescope working in the near-UV. The advantages of the near-UV are a small inner working angle and an improved contrast for blue planets. Along with the sophisticated tracking system to mitigate balloon pointing errors, MAPLE-50 will have a deformable mirror, a vortex coronograph, and a self-coherent camera as a focal plane wavefront- sensor which employs an Electron Multiplying CCD (EMCCD) as the science detector. The EMCCD will allow photon counting at kHz rates, thereby closely tracking telescope and instrument-bench-induced aberrations as they evolve with time. In addition, the EMCCD will acquire the science data with almost no read noise penalty. To mitigate risk and lower costs, MAPLE-50 will at first have a single optical channel with a minimum of moving parts. The goal is to reach a few times 109 contrast in 25 h worth of flying time, allowing direct detection of Jovians around the nearest stars. Once the 50 cm infrastructure has been validated, the telescope diameter will then be increased to a 1.5 m diameter (MAPLE-150) to reach 10[SUP]10 [/SUP] contrast and have the capability to image another Earth. <P />
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Marois, Christian;  National Research Council Canada (Canada)
Bradley, Colin;  Univ. of Victoria (Canada)
Pazder, John;  National Research Council Canada (Canada)
Nash, Reston;  Univ. of Victoria (Canada)
Metchev, Stanimir;  Univ. of Western Ontartio (Canada)
Grandmont, Frédéric;  ABB Inc. (Canada)
Maire, Anne-Lise ;  INAF - Osservatorio Astronomico di Padova Vicolo dell’Osservatorio 5, 35122, Padova, Italy
Belikov, Ruslan;  NASA Ames Research Ctr. (United States)
Macintosh, Bruce;  Stanford Univ. (United States)
Currie, Thayne;  Univ. of Toronto (Canada)
Galicher, Raphaël;  LESIA, Observatoire de Paris, CNRS (France)
Marchis, Franck;  SETI Institute (United States)
Mawet, Dimitri;  European Southern Observatory (Chile)
Serabyn, Eugene;  Jet Propulsion Lab. (United States)
Steinbring, Eric;  National Research Council Canada (Canada))
More authors (5 more) Less
Language :
English
Title :
MAPLE: reflected light from exoplanets with a 50-cm diameter stratospheric balloon telescope
Publication date :
01 August 2014
Event name :
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Event date :
from 22-06-2014 to 27-06-2014
Main work title :
Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
Pages :
91432R
Commentary :
9143
Available on ORBi :
since 21 January 2020

Statistics


Number of views
30 (0 by ULiège)
Number of downloads
42 (1 by ULiège)

Scopus citations®
 
2
Scopus citations®
without self-citations
1
OpenCitations
 
0

Bibliography


Similar publications



Contact ORBi