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  5. SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths
 

SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths

Journal
EXPERIMENTAL ASTRONOMY  
Date Issued
2012
Author(s)
Boccaletti, Anthony
•
Schneider, Jean
•
Traub, Wes
•
Lagage, Pierre-Olivier
•
Stam, Daphne
•
GRATTON, Raffaele  
•
Trauger, John
•
Cahoy, Kerri
•
Snik, Frans
•
Baudoz, Pierre
•
Galicher, Raphael
•
Reess, Jean-Michel
•
Mawet, Dimitri
•
Augereau, Jean-Charles
•
Patience, Jenny
•
Kuchner, Marc
•
Wyatt, Mark
•
Pantin, Eric
•
Maire, Anne-Lise
•
Vérinaud, Christophe
•
Ronayette, Samuel
•
Dubreuil, Didier
•
Min, Michiel
•
Rodenhuis, Michiel
•
MESA, Dino  
•
Belikov, Russ
•
Guyon, Olivier
•
Tamura, Motohide
•
Murakami, Naoshi
•
Beerer, Ingrid Mary
•
SPICES Team
•
Mas, M.
•
Rouan, D.
•
Perrin, G.
•
Lacour, S.
•
Thébault, P.
•
Nguyen, N.
•
Ibgui, L.
•
Arenou, F.
•
Lestrade, J. F.
•
N'Diaye, M.
•
Dohlen, K.
•
FERRARI, MARCO  
•
Hugot, E.
•
Beuzit, J. -L.
•
Lagrange, A. -M.
•
Martinez, P.
•
Barthelemey, M.
•
Mugnier, L.
•
Keller, C.
•
Marley, M.
•
Kalas, P.
•
Stapelfeldt, K.
•
Brown, R.
•
Kane, S.
•
DESIDERA, Silvano  
•
SOZZETTI, Alessandro  
•
MURA, Alessandro  
•
Martin, E. L.
•
Bouy, H.
•
Allan, A.
•
King, R.
•
Vigan, A.
•
Churcher, L.
•
Udry, S.
•
Matsuo, T.
•
Nishikawa, J.
•
Hanot, C.
•
Wolf, S.
•
Kaltenegger, L.
•
Klahr, H.
•
Pilat-Lohinger, E.
DOI
10.1007/s10686-012-9290-5
Abstract
SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and characterize long-period extrasolar planets and circumstellar disks in the visible (450-900 nm) at a spectral resolution of about 40 using both spectroscopy and polarimetry. By 2020/2022, present and near-term instruments will have found several tens of planets that SPICES will be able to observe and study in detail. Equipped with a 1.5 m telescope, SPICES can preferentially access exoplanets located at several AUs (0.5-10 AU) from nearby stars (<25 pc) with masses ranging from a few Jupiter masses to Super Earths (∼2 Earth radii, ∼10 M⊕) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.
Volume
34
Issue
2
Start page
355
Uri
http://hdl.handle.net/20.500.12386/34760
Url
https://link.springer.com/article/10.1007/s10686-012-9290-5
https://api.elsevier.com/content/abstract/scopus_id/84866927948
Issn Identifier
0922-6435
Ads BibCode
2012ExA....34..355B
Rights
open.access
File(s)
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1203.0507.pdf

Description
postprint
Size

888.3 KB

Format

Adobe PDF

Checksum (MD5)

5e18a2baf8087abb19182c31398f98d3

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